13573_An Introduction to Mechanics of Solids
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Transcript of 13573_An Introduction to Mechanics of Solids
1
An Introduction to Mechanics of
Materials
©
Vijay Gupta
Lovely Professional University, Punjab
2
Table of Contents
1 STRUCTURES, LOADS AND STRESSES 4 1.1 Mechanics of material 4 1.2 Deformation and resisting forces 4 1.3 Other loadings, stresses and strains 5 1.4 The concept of stress at a point 7 1.5 Stress on oblique planes 11 1.6 Notation for stress: double-index notation 12 1.7 Equivalence of shear stresses on complementary planes 13 1.8 Stresses in a thin circular pressure vessel 14 1.9 Summary 15
2 DEFORMATIONS, STRAINS AND MATERIAL PROPERTIES 17 2.1 Fundamental strategy of mechanics of deformable mechanics 17 2.2 Statically indeterminate problems 20 2.3 Lateral strain: Poisson ratio 23 2.4 Shear strain 25 2.5 Thermal Strains 27 2.6 Tensile test 28 2.7 Idealized stress-strain curves 30 2.8 Pre-stressing 32 2.9 Strain energy in an axially loaded members 33 2.10 Calculating deflections by energy methods: Castigliano theorem 33 2.11 Strain energy in an elastic body 38 Summary 39
3 TORSION OF CIRCULAR SHAFTS 41 3.1 Introduction 41 3.2 Relating angle of twist to twisting moment 41 3.3 Stresses and strain in a circular shaft 43 3.4 Hollow shaft 46 3.5 Statically indeterminate shafts 47 3.6 Composite shaft 49 3.7 Torsion of thin-walled tubes 50 3.8 Plastic deformation in torsion 51 3.9 Limit Torque 52 3.10 Strain energy in torsion 53
Summary 54
4 FORCES AND MOMENTS IN BEAMS 56 4.1 Introduction 56 4.2 Sign convention 57 4.3 Loads and supports 58 4.4 Determining shear forces and bending moments 59 4.5 General procedure for drawing shear force and bending moment diagrams by method of sections 61 4.6 The area method of drawing the SFDs and BMDs 64 Summary 69
5 STRESSES IN BEAMS 71 5.1 Introduction 71 5.2 Relating curvature of the beam to the bending moment 72 5.3 Composite beams 78 5.4 Stresses in beams carrying shear forces 82 5.5 Relating shear stresses to the shear force in a beam 83 5.6 Shear flow in beams 86 5.7 Shear centre 88 5.8 Plastic deformations in beams 88 5.9 Strain energy in bending 89 Summary 90
APPENDIX B PROPERTIES OF AREAS 93 B.1 First moments of area and centroid 93 B.2 Second moments of area 93 B.3 Parallel axes theorem 94 B.4 Perpendicular axes theorem 96
3
4
1 Structures, loads and stresses
1.1 Mechanics of material
The subject matter of a course on mechanics of materials deals with structures. A
table or a chair is a structure. A building is a structure. A bridge is a structure. A
TV tower is a structure. So is a printed circuit board, the casing of a fax machine,
or the body of a car. Among the many purposes of the various structures, one
common purpose is to resist and/or transmit forces acting on it. By resisting a
force we mean that the structure would not break under the force. The structure
of a building is designed to resist the loads which include the weight of the
people and things occupying it, the forces of wind acting on it in a storm, even
the load imposed by an earthquake, and the self-load of the building itself. The
structure of an aeroplane resists the aerodynamic loads, the weight of its
occupants (including the dynamic loads during acceleration and deceleration),
the load imposed by the thrust produced by the engines, and of course the weight
of the structure itself.
How does a structure resist loads?
Consider a simple case of a cantilever beam loaded as shown in Fig. 1.1. If the
beam is in equilibrium, the net force or moment on the beam or on any part of it
must be zero. Let us consider the part of the beam within the dashed-line box
shown. This is known as a free-body diagram (FBD).
Clearly, this part of the beam is not in equilibrium with just the external force, P.
We need additional external (i.e., external to this part of the beam) forces and/or
moments. The open arrows in Fig. 1.1b show the external force and moment
required to balance the applied load P. We will for the time being refer to these
as the reaction forces and the moments.
Where do these forces and
moment come from?
As we apply the force P to
the beam and if these
reactions do not kick in,
the beam will tend to
shear from the stump built
into the wall at the left-
end. The distortion of the
beam so produced results
in generation of material
forces within the beam
that resist this shearing action. When we consider the part of the beam shown in
the free body of Fig. 1.1b, these material forces appear as external forces (and
moments) on the beam. Of course, there are equal and opposite reaction on the
stump of the beam built in the wall.
We can summarize the above as:
The external forces acting on a structure result in deformation of the
structural members.
The deformation so caused result in resisting forces within the material
of the members.
When we consider the equilibrium of a part of the member, these
internal forces come into play as external forces and balance the applied
forces or moments.
1.2 Deformation and resisting forces
Consider a vertical rod anchored as shown in Fig. 1.2. It is common knowledge
that when you apply a longitudinal force P to this rod, it elongated a definite
amount (depending on its dimensions and its material). Consider a portion of the
rod enclosed by the broken line rectangle. The free body diagram (FBD) of this
part is shown in Fig. 1.1b. Since the rod is in equilibrium after the elongation,
there must be a force that balances the applied force P. Where does that force
come from? Clearly, there are internal forces which are holding this part from
running away from the rest of the member. These internal forces as seen in the
previous section are the consequence of the distortion produced in the bar. Now
5
more the force we apply, more is the
elongation, suggesting that the resisting
force that develops in the rod depends
on the elongation. Robert Hooke, a
British scientist is credited to be the first
to explore the relationship between the
resisting force and the elongation. He
found out in 1678 that for a given
material, the resisting force does not
depend on the elongation but on the
relative elongation produced. He
introduced the term strain to denote the
elongation relative to the original length
of the bar. If l denotes the original
length, and δ the elongation, the strain is
defined by
Strain, (1.1)
Strain is dimensionless and has no units.
Hooke also found out that it is not the force, but the intensity of force measured
as the force per unit area that needs to be considered. He called it stress. If A is
the area of cross-section of the bar, the stress is defined as the resisting force P
divided by A.
Stress, (1.2)
Stress has the dimensions of force per unit area (hydraulic pressure, too, has the
same dimensions) and has SI units of Newton per meter squared (M/m2) which is
termed as Pascal and abbreviated as Pa.
He further found that the stress and strain, in a large part, have a simple linear
relation for bars made of the same material:
Stress Strain, or, (1.3)
The constant of proportionately, E, is termed as the elastic modulus, and depends
on the material of the bar. Strain being dimensionless, the dimensions (and
units) of E are the same as those of stress.
Combining Eqs. 1.1 -1.3, we get:
(1.4)
The value of the elastic modulus E for most construction materials is quite high,
denoting that it takes fairly large forces to produce small elongations. Table B.1
in Appendix B gives the values of the elastic modulus for some common
materials. Steel has about the largest value of the elastic modulus of about 200
GPa1. Cast Iron has about half this value. Aluminium is still lower at 70 GPa.
The summary statements of the previous section can now be recast as:
The external forces acting on a structure result in strains in the structural
members.
The strains so produced result in stresses within the material of the
members.
The stresses, for the most part, are proportional to the strains produced.
The constant of proportionality is termed as the modulus of elasticity.
1.3 Other loadings, stresses and strains
We had in the previous section considered one kind of load that tends to elongate
a member, leading to one type of strain (longitudinal) and one type of stress
(tensile). It is possible to load members in various other ways. Compression
load is a familiar example. Compression results when two bodies are pressed
together. Columns that support elevated highways (Fig. 1.3), water tanks or roofs
are all compression members. A compression member shrinks in length because
of the load, resulting in compressive strains and stresses. The footing of a
machine is also under a compressive load. So also is the boom of the crane.
Compression also results in the situation shown in Fig. 1.4. Here two plates are
riveted together. As a force is applied to the plates that tends to pull them apart,
the rivet compresses the plates at the rivet holes as shown. The compressive
stresses so produced in the plates are also termed as the bearing stresses.
1 A GPa is 10
9 Pa, or 10
9 N/m
2
Fig 1.3. The columns supporting a highway deck, the boom of a
crane and a foundation block are all structural members in
compression
Fig. 1.2 A bar loaded
longitudinally
6
Fig 1.6 Twisting of a shaft. The shear stresses in the cross-section of the shaft
give rise to a resisting twisting moment.
Another type of load is the shear load. Consider a block of rubber glued to a
table on one side and a board on the other (Fig. 1.5). If we apply a load P as
shown, the block of rubber will undergo distortion and it will tend to slide off the
table. The distortion results in what are termed as shear strains, which, in turn,
result in shear stresses in the material.
Shear stress and shear strain is also produced in the rivet of Fig. 1.4. As the force
is applied the rivet has a tendency to shear at the middle. Shear stresses develop
to counter this action and keep each half the rivet in equilibrium.
Shear strain and shear stresses are also produced when a shaft is twisted as in Fig
1.6. If we consider the shaft as an assembly of thin slices stacked together, the
twisting action of the shaft tends to make the slices slip on one another. Internal
forces develop which resist these motions. These internal resisting forces are the
shear stresses and the resultant of these is a moment, termed as the twisting
moment.
Another type of distortion occurs when a moment is applied to a bar which tends
to bend it. As shown in Fig. 1.7, the upper fibres of the beam tend to shorten
from their original length, introducing compressive strain and resulting in
compressive stresses therein, while the lower fibres elongate introducing tensile
strain and tensile stresses therein.
The magnitude of these compressive and tensile stresses is such that they
integrate out to zero, which they must, since there is no applied force on the bar.
But the resultant moment is non-zero as is required to resist the applied bending
moment and ensuring equilibrium.
Let us summarize what was learnt in this section:
Forces that tend to reduce the size of a structural member produce
compressive strains which, in turn, produce compressive stresses.
Within limits, the magnitude of compressive stresses vary linearly with
the compressive strain, the constant of proportionality being the same as
the modulus of elasticity, E introduced in the last section with tensile
stresses and strains.
Fig. 1.7 Bending of a beam.
Fig 1.5 Shear in a block of rubber
Fig. 1.4 Riveted plates
Bearing stresses in
the plate
Shear stresses in
the rivet
PP
7
Forces that tend to distort the shape of a member, as in Fig. 1.5, produce
shear strains which in turn produce shear stresses. The more the shear
strain, the more is the shear stress.
A twisting moment applied to a shaft produces shear strains in the shaft.
These shear strains give rise to shear stresses across the cross-section of
the shaft, which result in a moment which balances the external twisting
moment. The more the external moment, more is the strain, more the
stress, and more the resisting moment.
A moment tending to bend a member as in Fig. 1.7, produces both
compressive and tensile strains and stresses in the beam. These stresses
give rise to a resisting moment which balances the bending moment.
1.4 The concept of stress at a point
In Section 1.2 we were dealing with a very simplistic case of a straight bar of
area A with a longitudinal load P and we defined stress simply as load per unit
area. This assumes a uniform distribution of stresses – a very severe
assumption. In practice, the deformations due to load and, consequently, the
strains and stresses will vary from point to point. It is, therefore, convenient to
define stress as the intensity of force at a point.
Consider a gear which is meshing with another gear which applies a force P on a
tooth (Fig. 1.8). Let us consider the equilibrium of this tooth. Fig 1.8b shows the
part of the tooth as a separate free body. The force that balances the external
force F is the force which was binding this tooth to the rest of the gear. This is
an external force that arises because of the loading of the gear and its consequent
straining. Let us imagine this straining and the internal forces are not distributed
uniformly on this material. Consider an elemental area2 δA on a face of a
structure exposed by making a cut at that location. Let δF represent the force
that the material that has been removed was applying at the elemental area δA.
This force arises from the deformation of the material under whatever external
load is being applied to the structure.
The stress at a point is defined as the intensity of the internal force of
deformation at this point:
Stress vector on this face at this point is t
The stress vector t depends upon the location as well as the direction of the
surface. If we had made the cut (at the same point) with a different inclination
(i.e., with the outward normal in some other direction), the stress vector would
have been different as is shown in Fig. 1.9
We can take the component of this vector along the normal to the surface and
along the surface:
The component of the stress vector normal to the surface is termed as the normal stress and is denoted by the Greek letter ζ. The component of the stress
vector along the surface is termed as the shear stress and is denoted by the Greek
letter η. As noted before, the dimensions of stress are Force/Area, or FL-2
, or ML-
1T
-2, and its SI unit is N/m
2 or Pascal, Pa. A Pascal is a very small unit and it is
common to have stresses in kPa or MPa.
Fig. 1.10a shows a bar loaded uniformly in tension as shown. Because of this
load the bar elongates setting up axial strains and stresses along any cross
section. Fig. 1.10b shows the resulting free body. It stands to reason that if we
take a section of this bar at any level, the resulting distribution of stresses must
be the same. However, if the loading is not uniform but concentrated at a point in
2 Area is a vector quantity, its direction denoted by the direction of the outward
normal to the surface.
(a) A gear (b) A cut-out portion of the tooth
Fig. 1.8 Stress at a point
(a) A solid object (b) Section through X along bb (c) Section through X along cc
Fig. 1.9 Stress depends on the direction of the cut
FFF
FArea δA
δF FFArea δA
δF
8
the bar as shown in Fig. 1.11a the story
changes. There is no reason to expect that
the stress distribution at a section is
uniform. In fact, it is not. Moreover, it
changes as we move from section to
section. If we take a section at different
heights along planes b, c, or d, the
resulting free bodies are shown in Fig.
1.11b, c and d. There total of the internal
forces or stresses at each of these sections
must be equal to P to balance the applied
force. But the distribution of these
stresses is quite different at the three
sections. The distribution of stresses becomes more uniform as we move
upwards, away from the point of application of the force P.
In fact, there is a principle known as St. Venant principle, named after a
nineteenth century French theoretician, which lays down this behaviour:
The difference between the stresses caused by statically equivalent load systems
is insignificant at distances greater than the largest dimension of the area over
which the loads are acting.
The loading in Figs. 1.10 and 1.11 are statically equivalent since they result in
the same net force and moments on the structure. The stresses in Fig. 1.10 (with
distributed loading) is uniform everywhere, and therefore, far away from the
point of concentrated loading in Fig. 1.11, we can take the stresses to be
uniformly distributed.
We shall, in this elementary text, will routinely make the assumption of uniform
stresses across sections, unless the context of the problem forbids it.
Example 1.1 Bearing stresses in foundations
Consider a wooden column (Fig. 1.12) resting on a concrete footing. Determine the maximum value of the load P if the maximum permissible stress in concrete is 60 MPa and in wood is 25 MPa.
Solution:
We assume that the stresses at any cross-section are
distributed uniformly. If P is the external load, the
stress in the wooden column is P (N)/ [π× (0.010 m)
2] = 3,183 P (N/m
2 or Pa). Similarly, the stress in
the concrete footing is P (N)/ [(0.030 m) 2
] = 1,111
P (N/m2 or Pa). Equating these stresses to 25 MPa
and 60 MPa, respectively, we find the value of P
from the first as 7.85 kN, and from the second as 54
kN.
Clearly, the maximum permissible load will be the
lesser of the two, i.e., 7.85 N. This suggests that we
can reduce the footing size drastically, if bearing
this load is the only design consideration.
Further we have considered only the compressive
stresses. Thin columns may buckle under
compressive load much earlier than they fail in compression. We will need to
check that too. We shall deal with this in a later chapter.
P P P P
(a) (b) (c) (d)
Fig. 1.11 The stress distribution becomes uniform as
we move away from the point of loading
d
c
b
(a) (b)
Fig. 1.10 The stress distribution
on a uniformly loaded bar
Fig. 1.12
9
Example 1.2 A truss
A truss structure is a load bearing structure assembled such that its members carry only axial loads, either tension or compression. It is made up of straight, two-force members3 joined together by frictionless pins. All the loads are applied at only the joints. Further, there are no external moments applied to such structure.
A truss is a gross approximation to an actual structure. There are no practical
frictionless pins, and most members carry some bending loads as well. But the
advantage of considering only two-force members (in simplifying calculations) is
so enormous that we make the truss approximation wherever feasible.
Fig. 1.13 shows a pinned structure consisting of two bars AB and BC from which a weight P hangs as shown. If the diameter of each bar is 6 mm and the permissible stress in the bar is 80 MPa, find the value of the maximum load P.
Solution:
Consider the
FBD of point B
where the load P
is being applied.
Since AB is a
pinned member,
and hence a two-
force member
there can only be
tension along it. Let us call it TBA. Similarly, there will be tension TBC along the
member BC.
The equilibrium of a body requires that the vector sum of forces and moments
should vanish:
∑ ∑ (1.5)
We need to apply only the force equations here. Taking the component-wise
sum of the forces, we get
3 A member on which external forces act only at two distinct points (and there is
no external torque acting on it) is termed as a two-force member. The forces
acting on a two-force member are collinear and opposed.
∑ (a)
∑ (b)
Solving the two simultaneously, we get
TBA = 0.51P, and TBC = 0.78P
The stresses in the bars are obtained by dividing the
above load by the cross-sectional area (assuming
uniform stress distribution), which is π× (0.003 m) 2
= 2.83×10-5
m2. The stress along BC will be the
limiting stress, since it is higher. Thus,
This gives the maximum load P as 2.9 kN
Example 1.3 A truss with roller support
Consider a structure shown in Fig. 1.14. If the members of the structure are mild steel with a radius of 20 mm, find the stresses in members AB, BC and AC.
Solution:
The support at point A is termed as a hinged support. This means that the support
cannot apply any moment at this point to the structure and the structure can
articulate at this point. The only possible external reactions (from the support) at
this point is a force with components both along and normal to the surface.
There is no reaction moment at this point. The support at point B is termed as a
roller support. A roller support, besides permitting rotation of the structure,
permits translation of structure along the supporting surface. This means that not
only is the reaction moment zero, but the force component along the support
surface is also zero. The only reaction possible at such a support is a force
component normal to the surface.
Fig. 1.13
Fig. 1.14
20kN
1 m
1 m
A
C
B
10
To find the stresses in the members, we need to determine the forces on them by
doing a statical analysis. The first step in solving this problem consists of
determining the reactions at the supports A and B.
The reactions at support are found by considering the equilibrium of the FBD of
the whole structure as drawn in Fig. 1.15a. Here all the external forces have
been shown: the applied load of 20 kN, the horizontal and vertical reactions RAx
and RAy at the pinned support A, and the horizontal reaction RBx at the roller
support B. The structure should be in equilibrium under the action of these
forces. There are two conditions for equilibrium: vector sum of all the forces as
well as all the moments must be zero.
Writing the sum of horizontal and vertical forces as zero gives us:
∑ (a)
∑ N (b)
Eq. (b) gives RAy = 20 kN. There is only one equation to determine the other two
unknowns. We need one more equation. That we get from the moment balance.
We can take the moments of forces about any convenient point. Here we take it
about the point A (because then the two force components at this point contribute
no moment):
∑ ( ) ( ) ( ) (c)
This gives = 20 kN, and, then Eq. (a) gives 20 kN, that is, 20 kN in
a direction opposite to that shown on the FBD in Fig. 1.15a, or 20 kN towards
left.
Fig. 1.15b shows the forces on the member AC. It is clearly that the net force on
the member is along the length4 of the member, tensile, and equal in magnitude
to √( ) ( ) The member BC is under a compression
of 20 kN.
Further, since at point B
there is no vertical force,
there cannot be any
force5 in member AB.
The stress in the two
members can be found
by dividing the forces
with the respective cross-
sectional areas. Thus,
the stress in member AC
is 28.3 (kN)/(π/4)(15×10-
3 m)
2 = 160.1 MPa, tensile, and that in member BC it is − 20 (kN)/(π/4)(15×10
- 3
m)2 = 113.2 MPa, compressive.
Example 1.4 Key
Consider the transmission of power by belt and pulleys. Fig. 1.16 shows a pulley
being driven clockwise by a belt. If the pulley is turning at 100 RPM and if the
power transmitted is 1 kW, what is the shear stress in the key? The shaft dia. is
20 mm, and the dimensions of the key are 4 mm × 4 mm and a length of 25 mm.
Solution:
A key is a common device used to couple a pulley with a shaft, so that as the
pulley rotates the shaft rotates with it. It is a metal piece inserted so that a part of
it is inside the shaft (in a slot termed as a keyway), and a part is within the pulley.
As the pulley turns, the key moves with it. The pulley applies a force on the key
towards the right as shown in Fig. 1.16b. The key whose lower part is enmeshed
with the slot within the shaft makes applies a force on the shaft to make it turn
with the pulley. As the key pushes the shaft, the shaft, in turn, pushes the key
back towards the left.
4 This should have been obvious without the calculations since members AC and
BC are two-force members. The forces acting on a two-force member are
collinear and opposed. 5 This is quite interesting. If there is no force in member AB, we really do not
need that member. Can the structure survive without the member AB? The
answer is: yes, if we are concerned only with the equilibrium, and no, if we
worry about the stability.
(a) FBD whole structure (b) Force along member AC
Fig. 1.15 (a) (b) (c)
Fig. 1.16 Shear stresses in a key
(a) (b) (c)
Fig. 1.16 Shear stresses in a key
20kN
1 m
RAx
CRBx
RAy
20kN
1 m
RAx
CRBx
RAyA
C
20 kN
20 kN
20kN
20kN
A
C
20 kN
20 kN
20kN
20kN
A
C
20 kN
20 kN
20kN
20kN
11
Now, if we look at Fig. 1.16b, we notice that the upper part of the key is being
pushed to the right while the lower part of the key is being pushed to the left.
We may say that the key will have a tendency to shear in the middle. Fig. 1.16c
shows the FBDs of the lower and the upper parts of the key. The internal shear
stresses acting on each half balance the externally applied forces.
Since the power transmitted is I kW, and the RPM is 100, the torque is 1000 W/
(2π r d/rev×100 rev/min/ 60 s/min) = 95.5 N.m. The force acting on the key (at
a radius of 10 mm) which transmits this torque is obtained as 95.5 Nm/0.01 m =
9,550 N
The total shear force
acting on the key (the
lower or the upper part)
is, thus, 9,550 N. The
area on which it acts is 4
mm × 25 mm and,
therefore, the shear stress
is 9,550 N/(4×10-3
m ×
25×10-3
m) = 95.5 MPa.
As an aside, note that the
applied load is producing
compressive or bearing
stresses as well. The
area on which the
compressive force (9,550
N) acts is 2 mm × 25 mm
and, therefore, the bearing stress is 9,550 N/(2×10-3
m × 25×10-3
m) = 190.1
MPa.
Example 1.5 Riveted lap joint
Consider two steel plates 2 mm thick joined together as shown in Fig. 1.16(a)
and (b) by two rivets of 10 mm diameter. The centres of rivets are 10 mm from
the edge of the plates. Determine the stresses in the rivets if a force of 2 kN is
applied to the plates trying to pull them apart.
Solution:
As was discussed earlier, the pull force tends to shear the rivets as shown in Fig.
1.17c. Since there are two rivets, we can assume at each rivet sustains half the
total force, i.e., 1 kN. This is the shear force in each rivet acting on the cross-
section l re of π× (0.005 m)2 = 7.85×10
-5 m
2. Therefore, the shear stress in
rivet shanks is 1 kN/7.85×10-5
m2 = 12.7 kPa.
Further, the pull force will tend to shear the plates as shown in Fig. 1.16d. This
shearing action acts on a total area of 2×(10 mm × 2 mm) = 4×10-5
m2
for the
force in each rivet, which is 1 kN. Thus, the shear stress in the plates will be 1
kN/4×10-5
m2 = 25 MPa.
Further the pull force will tend to crush the area of the plate as shown in Fig
1.16e, causing compressive or bearing stresses in the area in immediate contact
of the rivet. Surely these will not be distributed uniformly over the area. But if
we make the assumption that they are, the resulting bearing stresses will be 1
kN/(2 mm × 10 mm) = 50 MPa.
1.5 Stress on oblique planes
Consider again a bar of area A loaded axially as shown in Fig. 1.18a. Let us look
at the stresses on an oblique plane b inclined at an angle6 θ. It is clear that if we
draw the FBD of the lower portion of this bar as in (b), the total internal force
acting on this section is P as shown. But what is the stress here?
The area on which this force acts in not A but larger than A, equal to A/cosθ. If
we assume, as before, that the stress is distributed uniformly over the area (which
shall be quite true if the plane is not to close to the point of application of the
load) the stress vector here will be P divided by ( ) , or t = Pcosθ/A. We
can resolve this stress vector in two components (Fig. 1.18c), one normal to the
oblique area, and the other along it. The normal component is the tensile stress:
( ) ( ) (1.6)
This is also termed as the normal stress. The tangential component is a shear
6 The ngle θ is lso the ngle between the norm ls to the new pl ne nd the
original plane.
Fig. 1.17 Lap joint
P(a) (b) (c) (d) (e)
Fig. 1.18 Stresses on an oblique plane
P
Pθ
b
ζη ζ-η
η-η
12
stress:
( ) ( ) . (1.7)
Clearly, the value of the tensile and shear stresses at a location in the bar varies
with the angle of inclination θ of the plane being considered. The maximum
tensile stress occurs when θ is zero, i.e., the cut is perpendicular to the axis of the
bar, and reduces continuously as θ increases. But the behaviour of shear stress is
quite interesting. If we note that cosθ sinθ is (1/2)sin2θ, we see that the shear
stress η first increases as θ increases, attains a maximum value (equal to P/2A,
i.e., half the maximum value of the tensile stress) when θ is π/4, and then
decreases back to zero as θ increases to π/4. Also note that if the sectioning
plane is inclined in the other sense (with negative values of θ), the shear stress
on it has a reversed sense too. This is also obtained from the expression for η
given above since θ now is negative.
Two planes, one at angle θ, and the other at angle - θ are termed as
complementary planes. Shear stress on complementary planes have same
magnitude but opposite sense.
Please note that the equations obtained above are valid only for the special case
of axial loading of a straight uniform bar. If the geometry or loading were
different, these would no longer be valid.
Example 1.6 A Cardboard tube
A cardboard tube of diameter 70 mm is made from a strip of width 60 mm and
thickness 2 mm wound spirally with the edges glued together as shown in Fig.
1.19a. The cylinder is subjected to an axial load of 100 N, determine the shear
stress in the
glued joint.
Solution:
The angle of
the spiral can
be obtained by
imagining that
as the
cardboard strip
is wound up,
the strip should
advance in the
axial direction
a distance
equal to the
width of the strip as we go around the tube through one circumference, 2πR as
shown in Fig. 1.19b. This angle θ is, therefore,
.
The compressive stress in the cardboard tube along the axial direction is 100 N/
[2π(35×10-3
m)2×(2×10
-3 m)] = 227 kPa.
We can now use the Eq. 1.7 to determine the shear stress along the seam, which
is a surface with the normal in the direction as shown in the figure. It can be
seen that the angle θ here is the same as the angle in Eq. 1.7 (the angle between
the normals to the axial plane and the new plane on which stresses are to be
determined). Therefore,
( ) ( ) = 57.7 kPa
This is the shear stress along the glued seam. The seam would rip if the glue
cannot sustain this level of shear stress.
1.6 Notation for stress: double-index notation
As is clear from the
discussion above, the stress
vector at a point depends on
the orientation of the
surface under consideration.
We can, at the same point,
consider many differently
inclined surfaces. The
orientation of a surface is
denoted by the direction of the outward normal to the surface. Therefore, we
must specify the direction of the normal to the surface whenever we talk of stress
at a point.
We shall see later (in Chapter 6) that if we know the stress vectors on three
mutually perpendicular planes we can determine the stress vector on any other
plane. We, therefore, need to specify stresses on three such planes. Figure 1.20
shows stresses on three mutually perpendicular planes, with normals in x, y, and
z directions. We have shown here, the components of stress vectors on each of
these three planes. The tensile (or the compressive) components are represented
by the symbol ζ, and shear stress components by the symbol η. We use here a
double-index notation, with the first index of a stress component denoting the
plane on which it acts, and the second index denoting the coordinate direction of
Fig. 1.20 Specification of stress components
13
a component itself. Thus, ηxy is a component of shear stress acting on a plane
with the normal in the x coordinate direction, the component itself being in the y
coordinate direction. Similarly, ηzy is a shear stress component acting on a plane
with the normal in the z coordinate direction, the component being in the y
coordinate direction, and ζzz is a tensile stress component in the z direction acting
on a plane with normal in the z direction. It should be apparent that there are:
three tensile components, ζxx, ζyy, and ζzz, one each on the three faces
(note that the indices are repeated in each of them),
six shear stress components: two on each face, ηxy and ηxz on the x-face,
ηyx and ηyz on the y-face, and ηzx and ηzy on the z-face. We shall soon see
that three of them are equal to the other three, so that there are only
three independent shear stresses at a point (see section 1.7).
Sign convention: It is convenient to use the following sign convention:
We first define a face to be positive or negative: a face with the outward normal
in the direction of the positive coordinate axis is termed as a positive face; else it
is termed as a negative face. When a positively directed force acts on a positive
face or a negatively directed force acts on a negative face, the stress is assigned a
positive sign. And when a negatively directed force acts on a positive face or a
positively directed force acts on a negative face, the stress component is assigned
a negative sign.
A stress component is considered positive when a positively directed force acts
on a positive face, or a negatively directed force acts on a negative face7.
In other words, if both the sign of the force and the face are the same, positive or
negative, the resulting stress is a positive and if the two signs differ, the stress is
negative. This is summarised in Table 1.1 below:
Table 1.1 Sign convention for stress
Direction of normal Direction of force Sign of stress
In positive coordinate
direction (+)
In positive coordinate
direction(+)
Positive(+)
In negative coordinate
direction (−)
In positive coordinate
direction(+)
Positive(+)
In positive coordinate
direction(+)
In negative coordinate
direction(−)
Neg tive(−)
In negative coordinate
direction(−)
In negative coordinate
direction(−)
Neg tive(−)
7 This sign convention follows from the consideration of action and reaction
having the same sign.
It may be verified that all the stress components shown in Fig. 1.20 are positive.
Example 1.7 Nomenclature and signs of stresses
Fig. 1.21 shows stress
components on some faces
labelled (a) to (d). Name
these planes on which the
stresses have been shown.
Name the stresses and
determine their signs
according to the sign
convention outlined
above.
Solution:
Plane a is an x-plane, b a y-plane, c a z-plane and d is an x-plane (with the normal
in –ve x direction. The nomenclature and signs of the stresses are tabulated
below8:
Stress Index
of
plane
Index for
force
component
Symbol
for stress
Sign
of
plane
Sign of force
component
Sign
of
stress
1 x x ζxx + ve − ve − ve
2 x z ηxz + ve − ve − ve
3 x y ηxy + ve + ve + ve
4 z x ηzx + ve − ve − ve
5 z z ζzz + ve − ve − ve
6 z y ηzy + ve + ve + ve
7 y z ηyz + ve − ve − ve
8 y y ηxz + ve + ve + ve
9 y x ζzz + ve − ve − ve
10 x x ζxx − ve + ve − ve
11 x z ηxz − ve − ve − ve
12 x y ηxy − ve − ve + ve
1.7 Equivalence of shear stresses on complementary planes
8 Note that the signs of stresses on opposite faces a and d are identical, as they
should be. In fact, the sign convention has been designed to ensure this.
x
y
z
Face a
1
3 2
Face b
4
6
5
Face c9
8 7
Fig. 1.21
Face d
10
12
11
x
y
z
x
y
z
Face a
1
3 2
Face b
4
6
5
Face c9
8 7
Fig. 1.21
Face d
10
12
11
14
Consider a small two-dimensional element of dimensions δx and δy and of unit
depth as shown in Fig.1.22. We have
drawn the stress components on the
four faces of the element. We assume
a two-dimensional state of stress, i.e.,
we assume that there is no loading and,
hence, no stress component in the third
direction. We shall now consider the
equilibrium of the element under the
action of the forces due to these
stresses:
Face
(identified by the
direction of
outward normal)
Area
assume unit
depth
Force
x-component x-component
x δy•1 ζxx• δy ηxy• δy
− x δy•1 −ζxx• δy −ηxy• δy
y δx•1 ζyy• δx ηyx• δx
− y δx•1 −ζyy• δx −ηyx• δx
When we consider the force balance, we verify that there is no net force on the
element: the sum of x- and y- forces sum out to zero independently. We next take
the sum of the moments about the centre point of the element. Note that the
tensile forces produce no moment about that point. However, the shear forces
do. The shear forces on opposite faces are equal in magnitude but opposite in
sign and, therefore, constitute two couples, one anticlockwise (positive) and the
other clockwise (negative). The moments of the two couples are found by
multiplying the magnitudes of the forces and the perpendicular distance between
the two lines of action. The moment balance equation gives:
( ) ( ) ,
which on simplification gives = .
This is an important result and establishes that the shear-stress components on
adjacent (orthogonal) faces are equal in magnitude. We can, similarly, show that
= and = . As much was stated in Section 1.6 without proof. We
reiterate what was stated there:
The state of stress at a point can be established with six components of stresses:
three tensile components, ζxx, ζyy, and ζzz, one each on the three
orthogonal faces, and
three shear stress components ηxy, ηyx and ηzx.
We shall show in Chapter 6 that we can, from these six components on three
orthogonal planes through a point, determine the stress vector on any plane
through that point.
1.8 Stresses in a thin circular pressure vessel
Consider a thin9 cylindrical pressure
vessel of length L, radius R, and wall
thickness t. Fig. 1.23 shows the
cylinder with end plate removed. A
cylindrical polar co-ordinate system
with r, θ, and z coordinates is ideal for
this geometry. Let the internal excess
pressure be p. Under the action of
these forces, stresses will be set up in
the cylindrical vessel. Following the
development of the previous sections,
there will be six stress components
required to describe the state of stress
in the vessel walls: three tensile
components: ζrr, ζθθ, and ζzz, and three shear stress components: ζrθ, ζθz, and ζzr.
Let us first consider the tensile stress component ζθθ. As indicated by the first
subscript, θ, it acts on a plane with normal in the θ direction. This stress is
exposed (or m de ‘extern l’) by taking a section as shown by a diametrical
cutting plane as shown. Figure 1.24a shows the FBD of the lower half of the
cylinder (ends removed). We can determine the stress component ζθθ by
considering the equilibrium of the vertical component of all forces.
The total vertical force due to the tensile stresses is ζθθ times the area on which
these stresses act, which is 2×(L×t). Therefore, this force is 2ζθθLt. This force is
being balanced by the vertical component of the pressure forces acting on the
inside the half-shell. The integration of the vertical component of pressure forces
acting on this half of cylindrical shell is not straightforward. But it can be
determined quite easily by resorting to a frequently used trick. The pressure force
acting on the shell is equal and opposite to the pressure forces acting on the gas at
the shell wall (the principle of action and reaction). Consider the ‘FBD’ of the
‘g s’ cont ined in this h lf shell s shown in Fig. 1.24b. The vertic l net pressure
forces on the curved surface this FBD (which is the same and opposite to the
9 ‘Thin’ refers to the condition th t the w ll thickness t is much less than the
radius R.
Fig. 1.22 A 2-D infinitesimal element
Fig 1.23 A thin cylindrical vessel with
end plate removed
ζxxζxx
ζyy
ζyy
ηyx
ηyx
ηxy
ηxy
•
δy
δx
x
y
ζxxζxx
ζyy
ζyy
ηyx
ηyx
ηxy
ηxy
•
δy
δx
ζxxζxx
ζyy
ζyy
ηyx
ηyx
ηxy
ηxy
•
δy
δx
x
y
L
R
tz
θr
L
R
tz
θr
15
pressure forces of Fig. 1.24a) is balanced by, and hence equal to the pressure
force on the diametrical plane of this FBD. This is p(2RL). Therefore, the
integrated pressure force on the curved surface of the FBD of Fig. 1.24a is 2pRL.
2 ζθθLt = 2pRL, or,
(1.8)
This tensile stress in the circumferential direction is also termed as the hoop
stress.
We next consider the tensile stress ζzz which is the stress on the plane with
normal in the axial
direction. Such a
face is exposed when
we cut the cylinder
with a r-θ plane
parallel to the ends
as shown in Fig. 1.25
which shows the
FBD of one part of
the vessel so
exposed. The
external forces in the
z-direction acting on
this FBD are due to the tensile stress ζzz acting on area which can be
approximated by 2πRt, and the pressure p acting on the end plate area of πR2. The
z-force equilibrium, then, gives: ζzz×2πRt - p× πR2. This gives:
(1.9)
The third tensile stress is ζrr in the radial direction. Note that on the inner
curved surface the pressure p acts radially and,
therefore, is the stress ζrr at that point. But on
the outer curved surface, the pressure is zero, so
the stress ζrr is zero. Therefore, ζrr varies from
0 to p across the thickness of the cylinder. In
any case, since r >> t, the value of ζrr (between
0 and r) is much less than ζzz or ζθθ. Therefore,
in comparison to the other tensile stresses in the
cylindrical shell, it is common to neglect ζrr,
(1.10)
Let us next consider the shear stresses. We first
discuss ηθr. We shall use a very interesting
class of arguments termed as the symmetry arguments. Consider the two halves
of the cylinder as shown in Fig. 1.26. We have shown the shear stress
components ηθr on the upper half. Note that on the left-hand side, the plane has a
normal in the +ve θ direction (being counter-clockwise), and the stress is in the
+ve r direction. Therefore, the stress is ηθr and is +ve. On the right-hand side of
the upper half, both the signs are negative and therefore the stress is +ve again.
The two stresses having opposite sense is correct, since the horizontal forces
acting on this FBD should some out to zero (the sum of the horizontal component
of uniform pressure forces can safely be assumed to be zero).
Now on the lower half, the Newton third law (the
principle of action and reaction) dictates that the
stresses should have a sense opposite to that on the upper half. This is as shown.
But here we run into a problem. The stresses are both outwards on the upper
half, and both inwards on the lower half. This violates symmetry. It is easy to see
that it is not possible to distinguish between the upper and the lower halves of the
cylinder. If somebody came and switched the two halves while a reader was
away, there is no way by which the reader can tell which is which. This
symmetry requires that the state of stress on the two halves must be the same,
either both inwards or both outwards. Thus, the requirements of third law and
that of symmetry are in contradiction, and the both must hold! The resolution
this contradiction is possible only if the stress ηθr vanishes. This is a sufficient
proof. We can construct similar symmetry arguments to show that the other two
shear components ηrz and ηzθ too must vanish. Thus,
ηθr = ηrz = ηzθ = 0 (1.11)
1.9 Summary
The external forces acting on a structure result in strains in the structural
members. The strains so produced result in stresses within the material
of the members. The stresses, for the most part, are proportional to the
strains produced.
The constant of proportionality is termed as the modulus of elasticity
which is a property of the material of which the structural member is
made.
In general, the stresses vary from point to point, but the use of the St.
Venant principle permits us in many simple situations to assume
uniform stress distribution across a section. This is a useful particularly
at sections fairly distant from the points of application of loads.
Stress vector at a point describes the intensity of internal forces that
develop within a material in response to distortions that are produced
under the application of external loads.
(a) (b)
Fig 1.24 FBD of one half of thin cylinder exposing ζθθ
Fig. 1.25 FBD for determining ζzz
pσθθ
σθθ
ppσθθ
σθθ
ζZZ
p
ζZZ
p
16
The stress vector at a point depends on the orientation of the surface on
which the stress acts. Eqs. 1.6 and 1.7 describe the formula for
calculating the tensile and shear stresses on an oblique plane in the case
of longitudinal loading of a bar.
The stress at a point can be described by stating the stress vectors on
three mutually perpendicular planes with a total of three tensile
components and six shear components.
A double index notation is used to designate stress components, the first
index representing the direction of the outward normal to the surface,
and the second index the direction of the component itself.
A stress component is considered positive when a positively directed
force acts on a positive face, or a negatively directed force acts on a
negative face.
Equilibrium of forces require that the shear stress components occur in
pairs, so that the shear stresses on complementary planes are equal:
= , = and = . Thus, there are only three independent
shear-stress components.
We showed by symmetry arguments that the shear stress components in
a thin walled cylindrical pressure vessels all vanish.
17
2 Deformations, strains and material properties
2.1 Fundamental strategy of mechanics of deformable mechanics
All structures resist loads by deforming. A structure deforms as a load is applied
to it. As it deforms, the stresses build up within the structure to resist the applied
load. More the load more is the deformation and more are the stresses. The
deformation increases till the resulting stresses are sufficient to balance the
applied load.
We had considered in Sec. 1.2 the
deformation of a uniform bar under a
longitudinal load. If we take bars of
various cross-sectional areas and of
various lengths and plot the variations
of deformation with the loads, we
obtain plots as shown in Fig. 2.1b.
The variations are largely linear with
slopes that are different for different
bars. We had seen earlier that if we
convert the load to stress (stress, ζ =
load, P/cross-sectional area, A) and
deform tion to str in (str in, ε = elong tion, δ /original length, L), the lines with
different slopes collapse into one line, as long as the material of the various bars
is the s me. This f ct w s st ted s Hooke’s l w (Eq. 1.3), , where the
constant of proportionately E is termed as the elastic modulus, and is the
property of the material of the bar.
The above discussion can be seen in a slightly different light. The deformation
produced in the bar depends upon the load, the geometry of the bar and its
material. So does elongation. But the geometry of the bar is absent from Eq.
1.3. Once you convert the load to stress and deformation to strain, the
geometry of the structure becomes irrelevant.
The above is a very powerful insight and forms the basis of the fundamental
strategy of analysis in mechanics of deformable materials. This strategy can be
stated in the following manner: To determine deformations in a structure under a
given loading, we first convert the loading to stresses using equilibrium
considerations, convert stresses to strains using the material properties, and the
use the geometry of the structure to determine deformations from the strains so
calculated. This is also stated as a formula: macro to micro, conversion at micro
level, and then micro to macro. Loading is macro, stress and strain are micro
level, and deformation is macro level.
We may, at time, need to go in the reverse direction. We may be given the total
deformation from which we need to determine the loading: we calculate strains
from deformation, convert strains to stress using material properties, and the
integrate stress to find the loading. The strategy here too is macro to micro to
micro to macro.
Example 2.1 Tug of war
Consider a tug of war in which 6 young men are pulling on a manila rope (cross-
sectional area: 6 cm2) with forces as shown. Find the net elongation of the rope.
(a) (b) (c)
Fig. 2.1 Elongation of bars with loads
P
δ
ζ =P/A
ε=
δ/L
Area A
l
δ
P P
δ
ζ =P/A
ε=
δ/L
Area A
l
δ
P
Area A
l
δ
P
18
Solution:
Each section of the rope has a different tension, resulting in different stresses,
strains and elongations. Let us take the four steps of our strategy in sequence.
Loading to stresses:
To find the stresses, we first need to determine the tension in each section of the
rope. There are five distinct sections carrying tensions. (The sections at either
end do not have any tension, and, therefore, do not need any consideration.) This
is done by making appropriate FBDs which will make the required tension force
an external force. Fig. 2.3 shows a sequence of FBDs drawn for this purpose.
The first of these has externalised the tension TAB in the section AB of the rope.
By simple balance of forces we obtain TAB as 250 N. Similarly, from the other
FBDs we get TBC = 500 N, TCD = 800 N, TDE = 550 N, and TEF = 300 N.
If we assume a uniform distribution of stresses, which will be quite true away
from the points where loads are applied (St. Venant principle), we can find the
stresses in each section by dividing its tension by the cross-sectional area of the
rope. Thus, the stress in section AB is ζ = 250 N/0.0006 m2 = 416.7 kPa. The
stresses in other sections can be determined in a similar manner and are given in
column 3 of Table 2.1 below.
Stresses to strain:
Stresses nd str ins re rel ted by Hooke’s l w: ζ =Eε, where E is the elastic
modulus of the material. A search of literature reveals significant variations in
the value of E for manila ropes. A value of 100 MPa appears to be a good
approximation10
. We get the strains by dividing the stress values by this value of
E as shown in column 4 of Table 2.1.
Table 2.1 Calculation of elongation of the rope of Example 2.1
Strain to deformation:
Once the strains are calculated, we can determine the elongation in each section
by multiplying the strains with the length of the respective section. This has been
shown in column 6 of the table. The total elongation is 66.74×10- 3
m, or 6.67
cm.
Example 2.2 A hanging cable
Consider a cable of uniform section hanging as shown in Fig. 2.4. A steel cable
hangs from a roof under its own weight. It is important to see that the tension
along the length of the cable is not constant, but varies. This can be seen by
considering two sections, one at level b, and the other at level c. We have, in Fig.
2.4b, drawn the FBD of the cable up to level b. The tension T1 is clearly equal to
weight W1. The weight W2 in the FBD of Fig. 2.4c is no doubt greater than W1,
and therefore, T2 is greater than T1. Thus, the tension, and hence the stress along
10
The value of E for the rope accounts also for its unraveling as it stretches.
(1)
Section
(2)
Tension, N (3)
Stress, kPa
(4)
Strain
(5)
Length, m
(6)
Elongation, m
AB 250 416.7 4.16×10- 3
1.5 6.24×10- 3
BC 500 833.3 8.35×10- 3
2.0 16.70×10- 3
CD 800 1333.3 13.33×10- 3
1.5 20.02×10- 3
DE 550 916.7 9.20×10- 3
1.5 13.78×10- 3
EF 300 500.0 5.00×10- 3
2.0 10.00×10- 3
Fig 2.2 Tug of war
Fig. 2.3 FBDs for determining tensions in the rope
19
the cable increases from bottom to top.
The diameter of the cable is dictated by
the maximum stress in the cable. There is
a considerable wastage of material, since
the material near the bottom is not loaded
to its capacity.
In situations where the material costs are
heavy, it often pays to reduce the cable
diameter as we go down from the top.
Fig. 2.5 shows a cable where it has been
done. Its diameter at x = 0 is Do, and at x
= L is D1. The variation in diameter is
such that the stress at any given location
is constant equal to ζo. Find the
differential equation governing the
variation of diameter with x. Also set up an equation to determine the total
extension of the cable as a
function of the various
parameters involved.
Solution:
What is important to realize in
the problem is the fact that the
tension at any location varies
with x, the distance from the
roof. The weight supported by
the section at x reduces as x
decreases. We first determine
the tension as a function of x.
To determine the tension at x,
we take a slice of thickness dx of the cable at x, and draw its FBD. This FBD has
three forces, the upward tension T at x, the downward tension T + dT at x + dx,
and the weight dW of this slice of the cable. Clearly equilibrium requires that the
algebraic sum of the three be equal to zero. If the variable diameter of the cable
is denoted by D as a function of x, the tension T is easily estimated in terms of
the stress ζo as ( ), the stress being given as constant throughout.
The weight dW is easily estimated as ( ) , where ρ is the density of
the cable material and g the acceleration due to gravity. To determine the tension
T + dT, we have to note that the area at the bottom of the FBD is different from
that at the top. The tension here is thus,
[ . .
/ /
]
.
/ , neglecting terms of second
order in dx.
The force balance will then give, on simplification:
, where the negative sign indicates that diameter D decreases
as x increases. Using the boundary condition that the diameter D = D0 at x = 0,
we can solve this to get11
How would we now calculate the total elongation of the cable?
We first convert the stress at each section to the strain at that section. Since the
stress everywhere is the same, equal to , the strain is also the same everywhere
equal to , where E is the elastic modulus. And, therefore, the total
elongation is easily determined as .
Example 2.3 Deflection in an elementary truss
Consider again the truss with a roller support (Fig. 2.6) discussed previously as
Example 1.3, where the forces and stresses in the various members AC, BC and
AB were determined. It was shown that there is no force in AB, a tension of 28.3
kN in member AC, and a compressive force of 20 kN in the member BC. The
respective stresses were found to be 0, 160.1 MPa, and 113.2 MPa. Determine
the displacement of point C where the load of 20 kN is applied. All members are
made of steel (E = 210 GPa).
Solution:
The equilibrium part has already been solved. So also the stress determination.
We now need to find the displacement of point C to C1.
For this purpose, we first find the elongation (or shortening) of members AC and
BC. The stresses in the two members have already been calculated. The strains
are now calculated as stress/E. Thus,
εAC = 160.1 MPa/ 210 GPa = 0.76×10-3
, and
εBC = − 113.2 / 210 G = − 0.54×10-3
,
11
What about the second boundary condition: D = D1 at x = L? There is no other
constant to determine. Or is there not? The resolution of this question lies in the
fact that the constant stress ζ0 cannot be specified independently of D1 and L.
How would you determine ζ0 in terms of the other parameters?
Fig. 2.5 Cable of variable diameter
(a) (b) (c)
Fig. 2.4 A hanging cable
20
the negative sign
indicating that the
strain is compressive.
We convert the strains
into elongations. The
lengths of the two bars
are 1.41 m and 1 m,
respectively, and the
member AC elongates
by δAC = (0.76×10-
3)×1.41 m = 1.07×10
-3
m (or 1.07 mm), and
the member BC by δBC
= − (0.54×10-3
)×1.0 m
= − 0.54×10-3
m (or
0.54 mm).
To find the new location of point C, we use the following strategy: We change
the lengths to the rod to their new length and make them rotate in arcs about their
pivot points A and B, respectively. The point where the two arcs intersect is the
deflected location of point C.
Fig. 2.6b shows the geometric construction for determining the displaced location
C1 of point C. Bar AC has been shown elongated to AD (with CD being equal to
δAC =1.07 mm. We draw an arc with centre at A and AD as radius. The
displaced point C should be on this arc. Similarly, we displace point C to E by
an amount δBC = − 0.54 mm. We dr w n arc with centre at B and BE as radius.
The displaced point C should be on this arc as well. The point of intersection of
the two arcs then represents the new location C1 of C.
Determining the intersection
point of two arcs is a fairly
lengthy process. Fortunately,
since the changes in lengths are
very small fractions of the
lengths of the rods, and
therefore the angles of swing
are quite small, we can adopt an
approximate procedure wherein
we replace the arcs by the
tangents to the arc. We draw a
perpendicular to AD at D (to
represent the tangent to the arc
through D. Similarly, we draw
a perpendicular to AC at E (to represent the tangent to the arc through E. The
point where the two perpendiculars meet is the location of C1. We express the
new location by specifying the x- and y- displacement of the point C. The x-
displacement is easy to determine. It is nothing but EC, which is δBC = 0.54 mm.
We note that the y-displacement is EC1 = EF + FC1 = CG + FC1. But, CG =
CD/sin 45o = 1.07 mm/ 0.707 = 1.52 mm. we also see that FC1 = FG = 0.54 mm.
Thus, the y-displacement of the point C is 1.25 mm.
The procedure outlined here is quite a standard procedure for determining the
displacement in pinned structures like this truss.
2.2 Statically indeterminate problems
In the examples solved above
we first obtained loads and
stresses in the members
before moving to the next
step of determining strains
and stresses. There are,
however, problems where we
cannot determine the forces
in members without bringing
in the considerations of
deformation.
Consider as an example a
beam supported on two ends
as shown in Fig. 2.8. Since
the be m’s deflection is
excessive, it is propped up in
the middle by a column. Also shown is the FBD of the beam. There are now
three unknown reactions and only two equations (vertical force balance and
moment balance) to determine them. The problem is, therefore, statically
indeterminate.
It is easy to see that the reaction from the central prop depends on the rigidity of
the beam. If the beam is quite rigid, the beam may not even touch the central
prop and there will then be no reaction there. But as the rigidity of the beam
decreases, the load borne by the central prop increases. Therefore, it is necessary
to bring in the considerations of deformation even to solve the problem of
equilibrium.
The general strategy for solving the problems of the mechanics of deformable
bodies consists of three major steps:
Fig. 2.8 A propped beam
Fig. 2.6 Determining displacement in a truss
Fig. 2.7
20kN
1 m
1 m
A
CB
A
B
D
E C
C1
(a) (b)
21
Consideration of static equilibrium and determination of loads,
Consideration of relations between loads and deformations, (first converting
loads to stresses, then transforming stresses to strain using the properties
of the material, and then converting strains to deformations), and
Considerations of the conditions of geometric compatibility.
In statically indeterminate problems we cannot take these steps in a linear
sequence, because there are not enough equations of equilibrium to solve for all
the unknown loads. We have to consider simultaneously all three steps, even if
we were interested in only one, say, in determining the forces in the system, as in
the problem above.
We illustrate this strategy first with a simple example involving springs, and then
with a little more involved problems.
Example 2.3 A spring board
Fig. 2.9a shows a rigid board mounted on two similar springs, each of spring
constant12
k, and length h. A man with weight P walks out on the board till he
reaches a point a distance x from the second spring when the tip of the board
touches the foundation platform as shown in Fig. 2.9b. What is the value of x in
terms of P, L, h and k? Neglect the weight of the platform.
Solution:
It is clear from the
geometry of the
problem that as the
man walks out, the first
spring elongates
applying on the board a
downward force, while
the second spring
compresses applying an
upward force on the
board. Let the first
spring elongate by an
amount δ1 and let its
tension be R1. Let the
second spring shorten
by δ2 and the upward
12
Spring constant k is defined as the force required for producing a unit
deflection in a spring. Thus, if a force F produces an extension (or a
compression) of δ, the spring constant is given by k = P/δ. Its unit is N/m.
force it applies on the board be R2. Fig 2.7c shows the resulting FBD of the
board.
Equilibrium analysis
There are two unknown forces R1 and R2 in this problem. There is also the
unknown distance x that is to be determined. The equations of equilibrium give:
∑ : (a)
∑ ( ) (b)
The moments have been taken about the location of the first support. There is no
other equation of equilibrium. We cannot solve for three unknowns from these
two equations. This is why this problem is statically indeterminate. We
nonetheless move on.
Load deflection equations
Using the spring constant k:
(c)
(d)
This introduces two more equ tions, but two more unknowns, δ1 nd δ2 as well.
Geometric compatibility
From the geometry of the similar triangles in Fig. 2.9b, we can conclude that the
length of the first spring after deformation will be twice that of the second spring
after deformation.
( ) (e)
The problem is solvable now. There are five equations and five unknowns, R1,
R2, δ1, δ2, and x, the distance to be determined.
Writing R1 in term of R2 from Eq. (a), calculating δ1 and δ2 from Eqs. (c) and (d)
in terms of R2 only, and then substituting for δ1 and δ2 in Eq. (e), we can solve
for R2 to obtain
And then from (a):
Using these values of R1 and R2 in Eq. (c) we get the desired result,
Fig. 2.9 A spring board
22
Example 2.4 A bolt and a sleeve
A brass sleeve of length 50 mm (ID: 14
mm, OD: 18 mm) is held between a nut
and the head of a steel bolt of dia 10 mm
(Fig. 2.10). The nut is brought flush with
the sleeve and then tightened one quarter-
turn. If the pitch of the bolt is 0.7 mm,
determine the tension in the bolt.
Solution:
This is a statically indeterminate problem.
As we tighten the nut, a compressive
force builds up in the sleeve which
shortens in length. Simultaneously, a
tension is built up in the bolt which
elongates. Even though we are interested only in calculating a force, we cannot
do so without bringing in the considerations of stress, strain and elongation.
Equilibrium analysis
This is simple. If a compressive force P builds up in the sleeve, the tension in the
bolt is P.
Force deformation analysis
The force deformation analysis is done using the macro-micro-micro-macro
strategy developed in the previous section. To find the contraction in the length
of the sleeve in terms of the compressive force P, we first find the stress ζ = P/A,
the convert it into the strain ε = ζ/E = P/AE. The total contraction then is δ1 = εL
= PL1/A1E1. The elongation of steel bolt is, similarly, δ2 = PL2/A2E2.
Geometric compatibility
The nut moves through a total distance of ¼ of 0.7 mm, or 1.75×10-4
mm. If the
steel bolt did not elongate at all, this would be the magnitude of δ1. But the bolt
elongates through δ2. This means that the contraction of the sleeve would
decrease by an amount equal to δ2: Thus,
δ1 = 1.75×10-4
m − δ2.
Substituting the values of δ1 and δ2 in this condition, we get:
PL1/A1E1 = 1.75×10-4
m – PL2/A2E2
Here, A1 = π[(18×10-4
m)2 − 14×10
-4 m)
2]/4 = 1.00×10
-6 m
2,
A2 = π(10×10-4
m)2/4 = 0.78×10
-6 m
2,
L1 = L2 =5×10-2
m,
E1 = 110 GPa (for brass), and E2 = 200 GPa for steel.
Using these values, we get P = 225 N.
The resulting stresses will be 225 MPa in brass sleeve, and 282 MPa in the steel
bolt. Please note that these stresses are about the maximum that the sleeve and
the bolt can sustain. Any more tightening would result in failure of either or
both.
Example 2.5 A kinky spring
Fig. 2.11 shows an elementary design of a spring which has one spring constant
for the initial deflection (till the load is compressing only the inner aluminium
tube), and then it increases when the
load plate touches the outer brass
cylinder so that the load deflection
curve looks like that shown in the
figure. For the inner tube of 40 mm
dia and 2 mm wall thickness and the
outer tube of 50 mm dia and 2 mm
wall thickness, find the two spring
constants.
Solution:
Till the load is borne only by the
inner aluminium cylinder
For a load P the stress in the cylinder is obtained by dividing the load by its
cross-sectional area, which is πDt = π(40×10- 3
m)(2×10- 3
m) = 2.5×10- 4
m2.
Therefore, the stress is P/2.5×10- 4
Pa (compressive).
We convert this stress into strain by dividing it by the elastic modulus for
aluminium, which is about 70 GPa. Therefore, the strain is (P/2.5×10- 4
Pa)/70×109 Pa = 5.71×10
- 8 P (compressive).
For a length of 300 mm, this strain results in a shortening of the cylinder by ζ×L
= (5.71×10- 8
P)×(300×10- 3
m) = 1.71×10- 8
P m.
The spring constant13
is load per unit deflection, i.e., P/(1.71×10- 8
P) = 58.3
MN/m
13
One can find the spring constant quite directly by noting that the stress is P/A,
strain is stress/E, or P/AE. Deformation, then, is δ = PL/AE. The spring
Fig. 2.11 Kinky spring
Fig. 2.10 A bolt, sleeve and nut
23
The spring constant changes when the compression exceeds 0.1 mm, or when the
load exceeds (58.3×106 N/m)×(0.1×10
- 3 m) = 5.83 kN
After the outer cylinder kicks in
After the outer brass cylinder also starts bearing the load, the nature of the
problem changing drastically. We no longer can use equilibrium alone to
determine the loads borne by the two cylinders independently. It is a statically
indeterminate problem where considerations of equilibrium are interwoven with
the consideration of deflections.
Equilibrium of forces
Let us assume that after the total deflection exceeds 0.1 mm, the load borne by
the inner cylinder is F1 and that by the outer cylinder is F2. Clearly, the
equilibrium requires that:
P = F1 + F2 (a)
There is no other equation of equilibrium that can help us determine the two
forces.
Force deformation considerations
Let us move ahead and determine the stresses in the two cylinders, which are
F1/A1 and F2/A2, respectively, where A1 and A2 are the two areas.
The corresponding strains will be F1/A1E1 and F2/A2E2, both compressive, where
E1 and E2 are the two elastic moduli. The contractions will be:
δ1 = F1L1/A1E1 and δ2 =F2L2/A2E2. (b)
We have taken all steps according to the procedure outlined in Sec. 2.1 and
illustrated in the examples there: load (macro) to stress (micro) to strain (micro)
to deformation (macro).
Geometric compatibility
We know that the contraction of outer cylinder begins only when the inner
cylinder has compressed by a full 0.1 mm. Thus, the geometric compatibility
requires that:
(c)
The values of the various parameters are: L1 = L2 = 0.3 m, A1 = 2.5×10- 4
m2, A2 =
3.1×10- 4
m2, E1 = 70 GPa, and E2 = 110 GPa. We have used a value of E for
constant, therefore, is k = P/δ = AE/L. Plugging in the values of L, A and E we
obtain the same value as above.
brass as 110 GPa, which is about in the middle of the range of values given in
handbooks for brass or bronze as between 100 and 125 GPa.
Putting in the values of the parameters in Eq. (c), we obtain:
1.71×10- 8
F1 = 8.80×10- 9
F2 + or,
F1 = 0.51F2 + (d)
Eqs. (a) and (d) can be solved simultaneously to obtain14
and
. (e)
Finding the spring constant for this part is a little tricky. Note that we should
subtract 0.1 mm from the deflection δ and 5.83 kN from the load P to obtain the
slope of the second part of the load deflection curve of Fig. 2.11. We note that
. The spring constant after the kink is given
by:
The value of δ2 in terms of F2 is given obtained from Eq. (b) as δ2 = 8.80×10-
9F2. Eq. (e) gives F2 in terms of P. Thus, we obtain
( ), or
( )
,
This is more than three times the value when only the aluminium cylinder was
being deformed.
2.3 Lateral strain: Poisson ratio
Consider a bar of length L subjected to an axial load P as shown in Fig. 2.12.
Under the action of this load, the bar elongates by an amount δL so that an axial
strain is set up equal to . From our experience with elastic materials
like rubber bands we expect that as the bar elongates its cross-sectional area
decreases, i.e., transverse strains εyy and εzz are also set up. Simeon Poisson, a
French mathematician in the early 19th
century proposed that the strain in a
14 One can verify this result by using P = 5.83 kN, the value where the
brass cylinder just kick in and finding that and as it
should be.
24
transverse direction is a fixed
(negative) proportion of the strain in
the axial direction. Thus,
(2.1)
where ν is termed as the Poisson ratio
and is a property of the material15
.
Next, consider the case where a
second normal stress ζyy is also
present. Because the stress–strain
relation is linear, the additional
strains produced due to ζyy will
simply be superposed on the strains
due to ζxx. Further, since the properties of the material are independent of the
direction (termed as the property of isotropy), the strains due to ζyy are:
Similarly, the strains due to ζzz are:
.
Since these three strains in the three directions due to three different stresses are
all additive, the total strains in the three directions will be:
( ), (2.2)
( ), and (2.3)
( ). (2.4)
15
It is interesting to explore what change in volume results when a uniaxial load
is applied. Consider a small cuboidal element of dimensions δx, δy, and δz in the
x-, y-, and z-directions. If it is subjected to a load that causes an x-direction strain
equal to εxx, the resulting y- and z-str ins re − νεxx each. The new dimensions of
the elements now are, δx(1 + εxx), δy(1 − νεxx), and δz(1 − νεxx). Therefore, the
deformed volume is δx•δy•δz• (1 + εxx)•(1 − νεxx)•(1 − νεxx) ≈ δx•δy•δz•(1 + εxx −
νεxx − νεxx) = δx•δy•δz•[1 + (1 − 2ν) εxx], neglecting terms of higher order in ε. The
fractional change in volume is, thus, (1 − 2ν) εxx]. If the material is
incompressible, the v lue of ν, the oisson r tion must be ½.
These are the tensile (or compressive, if the algebraic sign is negative) strains on
the material due to tensile stresses. We can show using symmetry arguments that
shear stresses do not cause any tensile strain. Therefore, Eqs. 2.2-2.4 can be used
to convert stresses into strain. These relations can be taken as extensions of
Hooke law for uniaxial stress, and collectively are known as generalized Hooke
law.
Example 2.6 Compression of a block of rubber
A block of rubber 50 mm×50 mm×30 mm is placed in a cavity and compressed
with a force of 1 kN (Fig. 2.13). Determine the decrease in the thickness of the
block.
Solution:
As the rubber block is confined within a
cavity, its transverse dimensions will not
change and therefore there will be no strain
in the y- and z-directions. The (negative)
stress in the x-direction produces a (positive)
strain in the transverse directions. The walls
of the cavity prevent the rubber from
expanding in that direction, and as a
consequence, compressive stresses in y- and
z- directions result. This is, thus, a multi-
axial loading situation and the generalized
Hooke law (Eq. 2.2-2.4) applies. Clearly, ζyy
and ζzz re equ l (= ζ, s y) bec use of
symmetry. (we cannot distinguish between
y- and z- directions. The stress ζxx is equ l to (−1 kN)/ (50 mm× 50 mm) = −400
kPa, the negative sign indicating that it is a compressive stress. The value of E
for rubber is about 500 kPa with the value of Poisson ratio ν of 0.5 (note that this
value indicates that the rubber is essentially incompressible!). The three
equations then give:
-
( ), (a)
( ) (b)
( ) (c)
Eqs. (b) and (c) are identical (as expected, because of symmetry), and from these
we obtain ζ = −400 k . Using this v lue in Eq. ( ), we get
εxx = 0, i.e., no strain at all.
Fig. 2.13 Compressing a rubber
block
Fig. 2.12 Transverse strain under axial
load
L
P
P
x
zy
L
P
P
LL
P
P
x
zy
x
zy
25
What is going on?
This strange result is the consequence of the value of Poisson ratio being taken as
0.5, which is the same thing as assuming the material to be incompressible (see
footnote 5). Clearly, no strain can be produced in an incompressible material
confined in a cavity!
Let us redo this problem with a different material. Let us assume that the value
of E is 500 kPa and that of ν is 0.4, the other conditions remaining the same. The
three equations now are:
-
( ), (d)
( ) (e)
( ) (f)
As before, Eqs. (e) and (f) are identical, and from these we obtain ζ = −266.7
kPa. Using this value in Eq. (d), we get εxx = -0.37, a very large strain. The
thickness of the block will reduce by 37%.
Example 2.7 A confined pressure vessel
A long thin-walled cylindrical tank is snugly fitted between two rigid walls as
shown in Fig. 2.14. It is
then pressurised to an
excess pressure of p. If
radius of the cylinder is R
and its wall thickness t,
determine the compressive
force exerted by the wall on
the cylinder.
Solution:
The length of the
pressurized unrestrained
cylinder increases because
of the combined action of
the axial and the hoop stresses. This results in the cylinder trying to push the
walls outward, which in turn apply a compressive force F on the cylinder. We
can determine this force by noting that the net strain in the cylinder in the z-
direction should be zero.
There are two sources of axial stress ζzz in the cylinder: one is due to the internal
excess pressure ( ⁄ from Eq. 1.9), and the other is the axial force
applied by the walls on the cylinder. The compressive stress due to this force F
is obtained by dividing it by the cross-sectional area of the cylinder which
sustains this load, i.e., 2 . The two stresses are superposed, and the net stress
in the axial direction is given by
(a)
The negative sign is because the force F causes compressive stresses. The hoop
stress is given by Eq. 1.8 as:
(b)
The force F makes no contribution to the hoop stress.
The strain in the axial direction is given by Eq. 2.4 as
( )
Where ν is the Poisson ratio. Using the above values and the fact that ζrr is of
order p and, therefore, negligible, we get
( )
The value of ν is always less than 0.5.
2.4 Shear strain
A material subjected to shear stresses deforms in
shape. Fig. 2.15 shows an element of a material
that is under the action of a shear stress. We have
seen earlier that shear stresses occur in pairs: If on
the x-faces of an element there is are stresses ηxy
giving rise to a counter-clockwise couple as
shown, there must occur on the complementary y-
faces stress components that result in a clockwise
couple. Please note that all the stresses shown here have the same +ve signs16
. If
the direction of one of the stresses was changed, the direction of all the
components will be changed.
Though the element is under equilibrium under the action of these four types of
stresses and the consequent couples, the element deforms in shape. It can be
shown by some very interesting symmetry arguments17
that these stresses cannot
16
In fact, we have deliberately defined our sign convention for stresses to ensure
this very situation. 17
The reader is referred to Crandall, Dahl, Lardner, Mechanics of Solids,
McGraw-Hill, 2nd
SI edition, Section 5.4 for these fascinating arguments.
Fig. 2.14 A cylindrical tank between two walls
Fig. 2.15 Shear strain
26
result in any linear (tensile or compressive) strains: the linear dimensions of the
element will not change. It is only the shape that changes in this case. The
change in shape is manifested in the change in the included angle between two
lines which were parallel to the axes. Thus, angle at A reduces to α. We define
the shear strain in the element at this point to be the change in angle, i.e., (π/2 –
α), for an infinitesimal element in the limit that the dimensions of the element
tend to zero. The symbol used for the shear strain in the x-y plane is γxy, the
Greek letter gamma. Thus,
.
/ (2.5)
This is dimensionless as the linear strains were. The angles are measured in
radians
As for the tensile stress and strain, shear stress too is linearly related to the shear
strain.
, (2.6)
where G is termed as the shear modulus of the material. The shear modulus has
the dimensions of force/area or ML- 1
T- 2
. It has the same unit as E has, namely
Pascal, Pa. Table B.1 in Appendix B gives some representative values of shear
moduli and Poisson ratios of some common materials. Steel has a Poisson ratio
of about 0.27. Aluminium and brass have a little higher values of 0.32 and 0.35,
respectively. Soft rubber has a value of about 0.5, signifying that its volume does
not change appreciably as it stretches.
The shear modulus of most materials is about a third of their elastic modulus18
.
Shear stress in a plane depends on the shear strain in that plane alone, and not on
any other component of strain, shear or tensile. Similarly,
and (2.7)
Eqs. 2.6 and 2.7, together with Eqs. 2.2 – 2.4 form the complete set of strain-
stress relations.
Example 2.8 Calculating strains and stresses
Fig. 2.16 shows a small element of a steel structure after deformation. The
undeformed element was aligned with the axes and its dimensions were 0.2 mm
× 0.2 mm. The coordinates of its vertices A, B and D after deformation are given
as (in mm): A(0,0), B(0.194, 0.013), and D(−0.012, 0.196). C lcul te the v rious
strains and stresses.
18
It will be shown in Chapter 6 that E, G and ν are related: ( )
Solution:
From the given coordinates, the length of the line
AB is √( ) ( ) . The
original length of this line aligned with x-axis was
0.20 mm. This gives a contraction of 0.006 mm,
or a strain εxx of – 0.006 mm/0.2 mm = − 0.03 or −
3%.
Similarly, the length of line AD is
√( ) ( ) . The original
length of this line aligned with y-axis was also 0.20 mm. This gives a contraction
of 0.004 mm, or a strain εyy of – 0.004 mm/0.2 mm = − 0.02 or − 2%.
To calculate the shear strain γxy we determine the angle DAB. That is obtained by
subtracting from π/2 the angle the line AB makes with the x axis
(
) and adding to it the angle the line AD
makes with the y axis (
). Thus,
The shear strain, then, is
This is the shear strain in the material.
We next calculate the shear stress. From Eq. 2.6,
(- ) , or −150 , where
we have used 26 GPa for the value of G for steel.
We next calculate the linear stresses from Eqs. 2.2 and 2.3:
( ):
( ):
Solving these two simultaneously, we get ζxx = −5.57 G , nd ζyy = −2.70 G .
The negative signs indicate that both these stresses are compressive.
Example 2.9 A vibration isolator using rubber in shear
Figure 2.17 shows the schematic of a vibration isolator. The machine whose
vibrations are to be isolated is mounted on the central steel block and applies a
vertical load of 8,000 N as shown. It is suspended from two vertical walls
through two rubber pads of height 12 cm and cross-sectional area of 10 cm ×10
cm. The two rubber pads act as shear springs. Determine the total deflection of
the central post under the load and the effective spring constant of the two pads
taken together.
Fig. 2.16 Calculating strains
27
Solution:
Fig. 2.18 shows a pad in deflected
configuration. It shares the total load of 8,000
N with the other pad, and therefore, carries
4,000 N as a shear load. This load acts on an
area which is 12 cm×10 cm, or, 0.012 m2. The
she r stress is −4,000 N/0.012 m2, or,
. With G for rubber as 1.0 GPa, the
shear train is = −333.3 k /1.0
G = −0.33. The tot l line r deflection,
then, is −0.33×10 cm = −3.3 cm.
Since a load of 8,000 N produces a vertical
deflection of 3.3 cm, the spring constant of
the two pads taken together is 8,000 N/0.033
m = 242.4 kN/m.
2.5 Thermal Strains
As the temperature of a body changes so
does its dimensions. The change of length
with temperature is generally quite linear
with changes in temperature of several
hundred degrees Celsius. If we heat a rod of
length L through a temperature change of ∆T, its length changes as ,
where α is termed as the coefficient of thermal expansion. This can be seen as
producing a strain εT given by
(2.8)
The unit of α is per . Representative values of α for some materials are given
in Table B.1 in Appendix B. It should be noted that temperature changes do not
produce any shear strains.
These thermal strains are superposed on the elastic strains produced by loading of
members. The total strain produced in the presence of elastic strain is obtained
simply by adding the two strains. Thus, using Eqs. 2.2-2.4, and Eq. 2.8, we get:
( ) (2.9)
( ) , and (2.10)
( ) (2.11)
There is no change in shear strain because of thermal expansion, i.e., a shear
strain arises only due to the respective shear stress component.
If the structure in not permitted free expansion due to geometrical constraints,
stresses may be setup in the structure. Such stresses are frequently termed as
thermal stresses.
In examples below we illustrate how the thermal and elastic strains can be
combined.
Example 2.10 Thermal stresses
Fig. 2.19 shows a 20 cm long 3 cm dia steel
rod held between two rigid supports. The
temperature of steel rod is raised by 100 0C.
What is the force in the bar?
Solution:
The increase in temperature will tend to
increase the length of the rod. But the rigid
supports will prevent it from elongating.
This results in an axial force. If F is the compressive axial force acting on the rod
because of the walls, the stress ζxx = F/A = F/7.06×10−4
m2. Since there is
nothing that is applying a force in the other two directions, ζyy and ζzz are both
absent. Also, since there is no net change in the length of the bar, the axial strain
εxx is 0. Using these values in Eq. 2.9, we get:
, or .
Here α for steel is about 11×10- 6/ 0C, E = 210 GPa, and ∆T = 100
0C. The stress is
( - ) ( ) ( ), or 231 MPa,
compressive. By multiplying this stress with the area of the bar (7.06×10−4
m2), we get
the axial force F as 163 kN, a fairly large force.
Example 2.11 Residual stresses in electroplating
The corrosion resistance of steel is
improved by electroplating it with a
thin layer of copper, usually only a
few hundred microns thick. For bright
electroplating the bath temperature
should be around 50 0C. After
electroplating when the plated steel
returns to the room temperature, say
20 0C, the higher coefficient of thermal
expansion of copper compared to that of steel results in copper tending to
Fig. 2.17 Schematic of a
vibration isolator
Fig. 2.19
Fig. 2.20 Copper plating on steel
Fig. 2.18
Wall
8,000 N
Wall
Rubber blocks
Wall
8,000 N
Wall
Rubber blocks
28
contract more than that what the steel does. The bonding between steel and
copper prevents this, and as a result steel does not let the copper layer contract
more than it does itself. Steel layer ends up applying a tension to the copper
layer, and the copper layer pulls the steel inwards, the total tension force in
copper being equal to the compressive force in steel. However, since the steel
layer is an order of magnitude thicker than the copper layer, the stress in steel
will be negligible compared to that in copper.
Thus, there is a residual tensile stress19
in the copper layer. Estimate this residual
tensile stress.
Solution:
There is no stress at 50 0C. When the temperature decreases to 25
0C (∆T = −25
0C) the net strain in the copper layer will be exactly the same as the net strain in
the steel plate. The steel plate will have only the thermal strain, since we can
assume that the thickness of the steel plate is so large (compared to that of copper
film) that the same force in the two layers (equilibrium requirement) will result in
negligible stress in steel. Thus,
.
/
( )
Using the property values: 11×10- 6/ 0C; 16×10- 6/
0C; and
, we get:
( ) ( )
= ( ) (11 – 16) ×10- 6/ 0C×(− 25
0C)
= 15 MPa (tensile), not an insignificant stress
Example 2.12 Shrink fit
A steel shaft (20 mm dia) is to be fitted with a
steel sleeve (20 mm long, OD 26 mm). In
order to tightly fit the sleeve, its internal
diameter is made as 19.9 mm. It is fitted on to
the shaft by heating it till its internal diameter
is larger than 20 mm, slipping on, and then
letting it cool. As the sleeve shrinks, it presses
on to the shaft creating an interfacial pressure
which results in a good bond. Determine (a) the temperature beyond which the
19
This residual tension can be very detrimental when the structure is subjected to
tensile (or bending) load. The copper layer would crack and the corrosion
resistance will be lost.
sleeve should be heated for fitting, and (b) the resulting interfacial pressure on
cooling.
Solution:
It is convenient to work in the cylindrical polar coordinates, r, θ, and z, as shown.
The relevant equations for strains and stresses are obtained by simply substituting
r, θ, and z for x, y, and z in the equations developed so far20
.
To determine the temperature beyond which the sleeve should be heated for
fitting, we use Eq. 2.8 with εT = 0.1 mm/20 mm = 0.005, and αsteel = 11×10- 6/
0C,
to get
( - ) 455 0C
The sleeve has to be heated through a range of more than 455 0C to slip it on the
shaft without forcing it.
Now on cooling, the ID of the sleeve must be equal to the dia of the shaft. Let us
look first at the stress and strain in the shaft. If the interfacial pressure is p, the
radial stresses in the shaft are of order p. There is no other stress in the shaft. On
the other hand, the sleeve will be subjected to a radial stress of the order of p and
a hoop stress (radial stress ζθθ (refer to Section 1.8). The hoop stress is given by
Eq. 1.8 as pR/t. Since R >> t, the hoop stress, and consequently, hoop
strain are much larger than the compressive strain of the shaft. We can, thus,
neglect the compression of the shaft diameter in comparison to the increase in the
ID of the sleeve. Therefore, we can take the final dia of the shaft to be 20 mm
itself, and the final ID of the sleeve too as 20 mm. As the dia of the sleeve
increases from 19.9 mm to 20 mm, its circumference increases from π×19.9 mm
to π×20.0 mm, giving a hoop strain of 0.005. Since the axial stress is absent,
and the radial stress is of order p, much less than , we get 0.005 = /E.
Using the value of E as 210 GPa, and expressing as pR/t, we get p, the
interfacial pressure as 157.5 MPa
2.6 Tensile test
Tensile test is one of the primary tests that are used to determine experimentally
the properties of matter. A standardized specimen (Fig. 2.22) which uses a strip
or a rod of uniform cross-section between two enlarged ends is gripped and a
20
This is possible since none of the equations we have developed so far has
partial derivatives of physical quantities with respect to x, y, and z. Since θ does
not have the dimension of length, we cannot simply replace derivatives with
respect to y by those with respect to θ, and the equations that have partial
derivatives change in a more complex manner.
Fig. 2.21 A shaft with shrink-
fitted sleeve
29
tension force is applied. An extensometer
(Fig. 2.23) is used to measure how the length
between two specified points on the uniform
portion changes as the tension is increased.
The tension is converted into stress ζ by
dividing it with Ao, the cross-sectional area21
,
and the elongation is converted to linear
strain ε by dividing the elongation by Lo, the
gauge length (the undeformed distance
between the two points on the specimen). On plotting the two we get a graph
like that shown in Fig. 2.24 for ductile materials like steel. The initial part of the
curve is a straight line and
represents the linear elastic
range22
of the material. If a
material is loaded to point A
within this range as shown,
and then unloaded, the
material will return to its
unloaded state (strain will
return to zero). We say that
if the material is loaded and
unloaded within the elastic
range, the material exhibits
no permanent set. The slope
of the stress-strain curve in
the linear elastic range is E, the elastic modulus of the material.
The stress level up to which the linear elastic range extends is termed as the
proportional limit.
As the stress is increased, non-linearity comes into play, but the material still
shows elastic behaviour, i.e., on unloading the material exhibits no permanent
set. The stress level up to which the elastic range (linear or non-linear) extends is
21
Note that the stress here is only a nominal stress since we are not accounting
for the changed cross-sectional area as the specimen elongates. This is not
significantly different from the true stress till the strain becomes quite large. In
fact, the decrease in the stress at very large strains as shown in Fig 2.23 arises
only because we are not using the true stresses. The load does not decrease as
strain increases. 22
The linearity and elasticity are two different phenomena. The elasticity refers
to the fact that there is no permanent set, i.e., the material on unloading returns to
the original unloaded state, along the same curve it followed while loading. This
may or may not be linear. In fact, a rubber band is largely non-linear elastic.
termed as the elastic limit. It is not
possible to determine either the
proportional limit or the elastic limit
with any degree of accuracy.
The strains in the elastic region are
very small, quite insensible without
instruments to amplify their
magnitude. That is why extensometers
are used which amplify the strain,
either mechanically or optically.
When the stress in steel is of the order
of 400 MPa, the relative displacement
of two points originally 100 mm apart
would be of order of 0.2 mm. Strains
in most structural materials are of the order of a few tenths of a percent at most.
As the load is increased further the material stops showing the elastic behaviour,
that is to say that if the material is loaded beyond a certain point and then
unloaded, it will not return to its original unloaded state. We say that the
material now has a permanent set. In Fig. 2.25, the material is loaded up to point
Y. When the load is now decreased, the material follows the straight line path
downwards as shown. The straight line has the same slope E as the original
linear elastic line, but now it meets the strain axis at a point left of origin,
signifying that there is now a strain even when the loading and stress have been
reduced to zero. The material is said to have yielded and undergone plastic
deformation.
It is quite difficult to decide
experimentally the point at which the
plastic deformation begins. It is for
this reason that we, quite arbitrarily,
designate the point Y, where the
permanent set (the residual strain when
unloaded after loading to that point) is
0.2%, (or a strain of 0.002) as the yield
point of the material. The
corresponding stress ζY is termed as
the yield strength of the material.
Consider a material that is loaded
beyond the yield point Y to a stress
level Y1 (> Y). If the material is
unloaded now, it will follow a straight line down from Y1 with a slope of E to
point B, and there will be a permanent set as shown in Fig. 2.26. If, after this
Fig. 2.25 Yielding and permanent set
Fig. 2.24 Typical stress-strain curve for
a ductile material
Fig. 2.23 Schematic of an extensometer used in a
tensile test
Fig. 2.22 Tensile test specimens
30
initial yielding and unloading, the
material is loaded yet again, it will
follow the straight line up from
point B (with the slope E). This
material is now not going to yield
again till it reaches the stress level
of Y1, higher than Y. Thus by
loading the material to a level
higher than the yield strength Y,
we have been able to raise the
effective yield strength of the
material (in subsequent loadings)
to Y1. This phenomenon is known
as strain hardening and is
frequently employed to increase the wear resistance on materials. Shot peening
and sand blasting are examples of processes employed to strain harden structures.
Cold rolling of structural steel also produces usable work hardening.
Loading of the bar beyond the yield strength produces large deflections with
small increases in the stress. The maximum stress that the material is able to
attain is termed as the ultimate stress.
When a material is strained beyond the ultimate stress, the stress appears to be
decreasing as strains increases. As noted
earlier this is a false impression, since what we
are plotting here is the nominal stress obtained
by dividing the load by the initial area Ao. The
area of a ductile specimen decreases
significantly when it undergoes plastic
deformation. This is, usually, a local
phenomenon. The area of cross-section of the specimen suddenly starts
decreasing at some point where there are imbedded dislocations in the material.
This is termed as necking (Fig. 2.27). As the necking progresses, the true stress at
the section increases and the specimen fractures.
We summarize here the sequence of major events in the tensile test of a ductile
specimen:
Linear elastic deformation till the proportional limit: .
Non-linear elastic deformation till elastic limit.
Yield point, where the permanent set is 0.2%.
If we unload the material beyond yield point, and then reload it, the
yield strength increases. This is termed as strain hardening.
As the material undergoes plastic deformation, the stress level increase
up to ultimate stress.
Beyond ultimate stress, a neck develops in the specimen; the area
decreases locally while the nominal stress decreases.
Ultimately, the fracture takes place at the neck.
We have discussed so far the stress-strain curve for a ductile material. The
corresponding curve for a brittle material is significantly different from that for a
ductile material. Glass, cast iron, concrete, carbon fibre, and Perspex are some of
the brittle materials. Many material ductile at room temperature may be brittle at
low temperatures.
Most of the differences between the behaviour of ductile and brittle material
arises from the fact that there is little plastic deformation in a brittle material. Fig.
2.28 shows the stress-strain curves for glass and cast iron.
The first thing to
note is that both
these materials
undergo fracture
at very little
strain, much less
than that for a
ductile material.
Glass, for
example, shows
no plastic
deformation at
all.
Another feature
to note is that the
strength to fracture is much larger in compression than in tension. This is a usual
characteristic of brittle materials.
2.7 Idealized stress-strain curves
The stress-strain curves for the various materials do not admit any simple
mathematical description. However, we do need such descriptions for analysis of
structures. It is for this convenience that we model the materials into a few
classes and use simple stress-strain relations to model the actual behaviour.
Most problems of high school mechanics are solved by assuming the structural
members to be rigid. This means that there is zero strain for any level of loading.
Fig. 2.29a depicts the stress-strain curve for a rigid material.
Fig. 2.26 Strain hardening
Fig. 2.27 Necking of ductile
materials
Fig. 2.28 Stress-strain curves for some brittle materials
31
The stress-strain curve for a perfectly elastic material is as shown in Fig. 2.29b, a
sloping straight line whose slope is the value of the elastic modulus E. We have
used this idealization of materials in this book so far. This is a very useful model
and is used extensively in most structural analysis, because most structures are
designed to work within the elastic range.
Another commonly used idealized model is the elastic-perfectly plastic one
shown in Fig. 2.29c. in this, we assume that once the material yields, the stress
remains constants at the yield strength level. We shall have occasion to use this
in a few problems.
Fig. 2.29d shows the
behaviour of a
perfectly plastic
material. In such a
material there is no
strain till the stress
reaches a critical
level, after which
there is no increase
in stress as the
material deforms.
This idealization
may be used when
there are very large
plastic deflections,
so that the elastic-strain region of the stress-strain curve can be neglected.
The strain hardening model is shown in Fig. 2.29e. Note that the elastic-perfectly
plastic graph of Fig. 2.29c cannot model the strain hardening phenomena, since
the slope of the plastic part is zero. Reloading the material after unloading
following some plastic deformation will not increase the yield strength. But the
non-zero slope of the plastic part of the curve of Fig 2.29e ensures that the yield
strength increases on re-loading after the material has been de-stressed after it has
undergone some plastic deformation.
Example 2.13 Fitting an idealized curve
The solid line in Fig. 2.30 shows the stress-strain curve of cold-rolled 1020 mild
steel. Find a simple mathematical relation for load vs. elongation of a 20 cm
long 20 mm × 20 mm cross-section bar.
Solution:
A look at the actual stress-strain curve suggests that though the material exhibits
a bit of strain hardening, adopting an elastic-perfectly plastic idealization will not
be bad at all. We first determine the yield strength of this material by drawing a
line parallel to the elastic portion of the curve from a permanent set value of
0.2% or from strain ε = 0.002. The light broken line so drawn meets the curve at
a stress of about 580 MPa, which may be taken as the value of yield stress ζY for
this material. Therefore, the idealized curve looks like the broken heavy line
shown in the figure. In other words, we may model 1020 CR mild steel as elastic
up to a stress level of 580 MPa with a value of E = 580 MPa/ 0.003 = 193.3 GPa
(0.003 being the strain at the yield point). Thereafter, the steel may be taken to
deform perfectly plastically.
A stress of 580 MPa
corresponds to a load of
580 MPa×(20×10-3
m)2,
or 232 kN. In this
region, the elongation
will be δ = PL/AE =
P×0.2 m/(20×10-3
m)2
×
(193.3 GPa) = 2.59×10-
9P m, where P is the load
in Newton. We draw a
line through the origin
up to the yield point with
P = 232 kN. After this,
the deflection increases
without any increases in
the load. Fig. 2.31 graphs this load vs. elongation behaviour.
Fig. 2.29 Idealized stress strain curves
Fig. 2.31 Load-deflection curve
Fig. 2.30 Stress-strain curve for cold rolled 1020 mild steel
32
2.8 Pre-stressing
Many brittle materials have much higher yield strengths in compression than in
tension. For example, concrete has a tensile strength of only 10-15 % of its
compressive strength. It is
common to use
reinforcement in concrete to
give it increased strength in
tension. This is used quite
effectively in the design of
beams. We had seen in
Section 1.3 that in a beam
subjected to bending under
vertical loads, its upper layers are in compression while the lower layers are in
tension. It is common to increase the tension strength of concrete by reinforcing
it with tendons of high tensile-strength material, such as steel rods (Fig. 2.32).
But many a times this is not sufficient. One of the very interesting ways to
overcome this problem is pre-stressing. If we build up within the concrete some
residual compressive stresses when it is being cast, subsequent tension loading of
the structure will first relieve the compressive stresses before generating tensile
stresses. In this way, the structure will be able to support enhanced tensile loads
before the tensile stresses reach the critical level.
Fig. 2.33 explains how the pre-stressing works. Tendons, most often steel wires,
are put under external tension and the concrete cast around them. After the
concrete is set, the external tension is released. The tendons now try to shrink to
their no-stress lengths, but the concrete around them prevents them from
shrinking to their original length. In the process, there is a residual tension in the
tendons, while there is equivalent compression in the concrete. This residual
compression in concrete helps increase the tensile load capacity of the concrete.
Example 2.14 Pre-stressed concrete
Let us consider a simple pre-stressed concrete structure to serve as an illustration
of the calculations involved. Let a concrete beam of cross-sectional area 5 cm×5
cm and length 2 m be cast with a 10 mm dia mild steel rod under a tension of 20
kN. The external tension in steel released after the concrete is set. What is the
residual compressive stress in the concrete?
Solution:
A tension of 200 kN in the steel bar results in a stress of 20 kN/[¼π(0.010 m)2] =
255 MPa. (This is quite close to the yield strength of commercial structural steel.)
The strain under this stress is ε = 255 MPa/ 210 GPa = 1.21×10- 3
, and the total
elongation of the bar will be (1.21×10- 3
)×2 m = 2.42 mm.
After the tension is released, the steel rod shortens, but it does not reach its
unstrained length, and there is a residual tension in the steel tendon and an equal-
magnitude residual compression
in the concrete. This force
cannot be determined by statics
alone. We have to make
recourse to deformations and
apply a geometric compatibility
condition.
If δs represents the final
elongation of the steel bar (from
its unstrained condition, and δc
represents the contraction of the
concrete, it is clear from the
construction of Fig. 2.34 that δs
+ δc = 2.42 mm. This is the
geometric compatibility
condition.
Let F represent the force, tension in steel and compression in concrete. Then, δs
= FLs/AsEs = F(2 m)/[π/4(0.010 m)2]×210 GPa, and δc = FLc/AcEc = F(2 m)/(0.05
m×0.05 m)×20 GPa.
Thus, from the geometric compatibility condition we get,
( ) ( ) ,
2.32 Reinforcement in a concrete beam
(a) Tendon as cast
(b) The no-stress length of the tendon
(c) The final configuration on release of tension
Fig. 2.34
Fig. 2.33 Pre-stressing
33
Which gives F = 15.03 kN. This is the residual force which produces a
compressive residual stress of 15.03 kN/(0.05 m×0.05 m) = 6.01 MPa. This
leads to considerable strengthening of the structure in tension.
2.9 Strain energy in an axially loaded members
When a force F is slowly applied to a
deformable body (that is supported in such a
way that no rigid-body motion is possible)
work is done as the body deforms. The work
done U in deformation is
∫ (2.12)
This is represented by the area under the F-δ curve of Fig. 2.35. For purely
elastic deformations, the force-deformation curve is linear and therefore the work
done in deformation is given by
. This work is stored within the body
as mechanical energy and is termed as the strain energy. It is a conservative
energy and is released when the load is removed and
the body returns to its original configuration.
Let a number of forces F1, F2, F3, … ct on the body
(or the structure) and the resulting displacements at
their points of application be δ1, δ2, δ3, …. The work
done in deformation is independent of the order in
which the forces are applied. We apply the forces
simultaneously such that the total work of
deformation is given by the sum of the work done by
individual forces:
∑ (2.13)
Let us calculate the strain energy of a bar subjected
to an axial load as shown in Fig. 2.36. The deformation δ (elongation, in this
case) is given by FL/AE, and the strain energy U is then
.
2.10 Calculating deflections by energy methods: Castigliano theorem
Consider an elastic body which is fully supported in the sense that its rigid body
translation and rotation are not permitted. Let it deform under the action of n
forces, F1, F2, F3, …, Fn. Let the total strain energy be U, which is a function of
F1, F2, F3, …, Fn: ( ).
Let us first load the body with all the forces F1,
F2, F3, …, Fn, and, then, increase one of the load,
say Fi, by a small amount, say δFi. The additional
strain work done can be written as:
(a)
Let us next reverse the order of loading. We first
apply the small load δFi on the body before any
other load is applied. After this load is applied,
all other loads F1, F2, F3, …, Fn are applied on the body. Under the combined
action of all these loads, the point of application of load Fi moves through an in-
line distance of δi. The work done by this small force δFi is then23
dU = δFiδi (b)
Since the order of loading (in the linear elastic case) should be immaterial, we
can equate the two values of work given by Eqs. (a) and (b), to get:
(2.14)
This is known as Castigliano theorem24
. It states that if the total strain energy of
a structural system is expressed in terms of the external loads applied to it, the
deflection at any one loading point (in-line with the load) is obtained by taking
the partial derivative of the strain energy with respect to the load at that point.
We illustrate the use of this theorem, first to two simple cases in Examples 2.15
and 2.16, and then apply it to a more involved problem of a truss. Example 2.17
introduces a process that can be generalized and can also be used for solving
statically indeterminate cases as illustrated in Example 2.18.
Example 2.15 An elementary truss
Consider again the truss with a roller support (Fig. 2.38) discussed previously as
Example 2.3. Determine using the energy method the displacement of point C
23
The factor of ½ is missing in this expression because the load δFi remains
constant while the displacement δi takes place. 24
There are some simple extensions to Castigliano theorem. One of the simple
extensions is its application to non-linear systems where the strain energy
∫ is replaced with ∫ , which is termed as the complementary
energy.
Fig. 2.35 The area under the
force-displacement curve is the
work done in deformation
Fig. 2.36 A bar under
an axial load P
Fig. 2.37 An elastic body
34
where the load of 20 kN is applied. All members are made of steel (E = 210
GPa) and have a circular cross-section of 20 mm dia.
Solution:
Since the energy method involves taking the derivative with respect to the force applied at the point where the deflection is to be calculated, we replace the load of 200 kN with a variable load P. Also, since the use of Castigliano theorem gives displacement only in line of the force with respect to which the derivative of the energy is taken, we cannot find the horizontal displacement of point C since there is no horizontal force present there. However, we can overcome this deficiency by introducing a dummy force Q in the horizontal direction at C, and then taking the derivative with respect to Q before equating Q to zero.
A simple equilibrium analysis of the joint at C using the FBD given in Fig. 2.39b,
gives:
from the vertical force
balance, and
from the
horizontal force balance.
These give , and
. The force in the element AB
is zero as before. The total strain energy,
then, is:
( )
( )
The vertical displacement of point C
(in line with force P) is obtained by
taking the partial derivative of U
with respect to P:
( )
Replacing P with 100 kN, Q with 0,
LCA with m, LCB with 1 m, E with
210 GPa, and A with π(0.02 m)2 /4,
we get
= 0.0058 m, nearly the
same as was obtained in Example 2.3.
To determine the horizontal displacement at C, we take the partial derivative of U
with respect to Q:
( )
, which on substitutions of values gives ,
the negative sign indicating that it is in a direction opposed to that shown for Q.
The amount of work involved here with the energy method is far less than that in
Example 2.3, and the results here are more accurate.
Example 2.16 Tug of war revisited
Consider once again the tug of war discussed as Example 2.1. We determine here
the total elongation of the rope using the energy method. The cross-section of the
rope was given as 0.0006 m2, and the value of the elastic modulus for the manila
rope was taken as 100 MPa.
Solution:
To find the total elongation by energy method, we need to anchor the rope at one
end (say, at point A) and apply a force P at the other end (see Fig. 2.41). The
total energy will be determined in terms of P and partially differentiated with
respect to P. To find the total strain energy of the system, we need to determine
the load in each section of the rope which can be obtained by simple equilibrium
Fig. 2. 38 An elementary truss
Fig. 2.41 FBD for application of energy method
(a) Truss (b) FBD of pin C
Fig. 2.39 Introducing forces P and Q
Fig 2.40 Tug of war
20kN
1 m
1 m
A
CB
35
analysis. Once we obtain the forces we can calculate strain energies by
evaluating . Table below organizes these calculations:
Table 2.2 Calculation of elongation of the rope of Example 2.16
The total strain energy is given as ∑ , where summation is taken
over all the segments of the rope. The deflection at the free end is obtained by
taking the partial derivative of the total energy with respect to P.
(∑ )
∑
( )
where the value of ∑ ( )
has been substituted from Table 2.2. Plugging in the
value of A = 0.0006 m2 and that of E as 100 MPa, and the value of P as 300 N,
we get m, or 6.67 cm, the same as was obtained in Example 2.1.
Example 2.17 Unit force method
Consider the truss shown in
Fig. 2.42. The truss is
pinned at point A and is
supported on rollers at
point B. This implies that
while at A, there could be
horizontal as well as
vertical reactions, there is
no horizontal reaction at B.
All joints are assumed as
pin joints, and as has been
explained earlier, all
members are two force
members and hence carry
only axial loads, tensile or compressive. We will illustrate the use of energy
method to determine the vertical displacement at joint F and the horizontal
movement at the roller support B. All members are made of steel and have a
cross-sectional are of 6 cm2.
Solution:
As before, we need to introduce dummy forces P and Q, respectively, at points F
and B in-line with the displacement desired. The method of solution is exactly
the same as in the previous examples, but because of the larger numbers of
members involved we devise a scheme that will permit reduction of labour.
The total strain energy of the truss will be the sum of the strain energies of the
individual members:
∑
The deflection in the direction of force P is obtained by taking the partial
derivative of U with respect to P:
∑
∑
∑
(a)
Attention is drawn to the fact that the here are the forces in the members in
the presence of all loads, including P and Q. The values of may be imagined to
be made up of two parts, one due to the actual loads on the structure, and the
other due to the
application of dummy
loads P and Q. After
we evaluate the sum
specified in Eq. (a)
above, we plug in the
value of P and Q as
zero. This implies
that in the final step,
the value of ’s will
be the original values
of ’s without P and
Q.
The term
, which
is the rate of change of with P can be interpreted as the additional force in the
ith
member due to a unit load at P. This interpretation is valid because of the
linear dependence on P of the additional load in the ith
member.
We, therefore, organize our calculations in two distinct parts: We first calculate
the actual values of ’s, i.e., the v lues of ’s without P and Q. These are used
as values for the first part of the terms in Eq. (a). We, then, calculate the values
of ’s th t would result when unit force is pplied in pl ce of P, without any of
Segment Length, L Force, F F2L ( )
EF 2 m P 2P2 4P
DE 1.5 m P + 250 N 1.5P2 + 750P + 93750 3P + 750
CD 1.5 m P + 500 N 1.5P2 + 1500P + 375000 3P + 1500
BC 2 m P + 200 N 2P2 + 800P + 80000 4P + 800
AB 1.5 m P − 50 N 1.5P2 − 150P + 3750 3P − 150
Fig. 2.42 Example 2.17
Fig. 2.43
36
the other external forces being present. These values of ’s will be used in pl ce
of the partial derivatives
.
This procedure is termed as the unit force method.
Determination of ’s in absence of forces P and Q:
We first determine the reactions R1x, R1y, and R2y by considering the structure as a
whole bin the FBD shown in Fig. 2.44a. The equilibrium equations are:
∑ : ,
∑ : , and
∑ : .
The three equations can be solved simultaneously to give , ,
and .
Once the reactions are known, we can go from pin to pin to calculate the axial
forces in all the members. Consider, for example, the FBD of pin B shown as
Fig. 2.44b. By writing the two force balance equations and noting that
( ) , we get
∑ : ( ) ,
∑ : ( ).
Solving the second of these first, we get , and then .
We can similarly move from pin to pin and calculate all the forces.
We next calculate the value of L/AE for each member of the truss. For example,
for member AF which is 2 m long, the value of L/AE is given as (2 m)/(0.0006
m2)×(210 GPa) = 1.588×10
−8 N
−1. Table 2.3 gives the values of F and L/AE for
all the members of the truss.
Calculation of through
calculation of the Fi’s for a unit
load of P
Refer to Fig. 2.45 which shows
the FBD of the truss for a unit
load at the location of P and no
other load. Clearly, the reactions
at A and B are 0.5 N, each. We
again go from pin to pin, draw
the relevant FBD and calculate
the force in each member.
These have been shown in the 4th
column of Table 2.3.
The last column of Table 2.3 shows the product
for each member of
the truss. The sum of these over all the members gives the deflection of point D,
in-line with the dummy force P. Thus,
Δv,E = 1.176×10−3
m, or 1.18 mm.
This is quite a general procedure for trusses.
Horizontal deflection at the roller support at B:
Fig. 2.44 Some FBD’s for determining the forces
Fig. 2.45 FBD for unit load at F
Table 2.3 Calculation of vertical movement of pin C
Member Force
Fi, kN
L/AE
(×10−8
N−1
)
(×10−5
m)
AD −16.7 1.24 −0.67 13.9
AF + 13.3 1.59 0.89 18.8
BE −25.0 1.24 −0.67 20.8
BF + 20.0 1.59 0.89 28.3
CD −16.7 1.24 −0.67 13.9
CE −16.7 1.24 −0.67 13.9
CF +5.0 1.59 1 8.00
DF 0 1.24 0 0.00
EF −8.3 1.24 0 0.00
Total 117.6
37
We next calculate the
horizontal deflection
at the roller support at
B. For this purpose,
we place a dummy
horizontal load at
point B.
Here again, we use
the same procedure
as above. The
calculation of Fi’s is
does not depend on the dummy loads and we get the same values as in column 2
of Table 2.3. The values of L/AE for the various members are also unchanged.
We, however, have to calculate dFi’s under the unit lo d Q. For this purpose we
use an FBD as shown in Fig. 2.46 and calculate the resulting tensions in each of
the members. Clearly, the vertical reactions R1y and R2y are zero, and the
horizontal reaction R1x is – 1 N. It is easy to see that there will be tension only in
the members AF and BF, both +1 N.
Table 2.4 organizes the calculation of the horizontal movement at the roller
support at B. Here the values in the second and the third columns (Fi, and L/AE)
are the same as in Table 2.3, but column 4 shows the values of the axial forces in
the various members when only the load Q (equal to 1 N) is applied at point B.
As was noted above, only two non-zero entries (for members AF and BF) result.
The last column of Table 2.4 shows the product
for each member of
the truss. The sum of these over all the members gives the horizontal deflection
of point B (in-line with the dummy force Q), which is seen as 52.9×10−5
m,
slightly more than half a millimetre.
Example 2.18 Application of energy method to a statically indeterminate problem
Let us once again consider
the same truss as in
Examples 2.16 and 2.17 and
shown in Fig. 2.42 with one
change: The roller support is
replaced by a pinned
support. This is as shown in
Fig. 2.47. This will
introduce a horizontal
reaction at support point B.
There will now be four
reactions and only three
equilibrium equations to
determine them. The
problem, therefore, is
statically indeterminate. We illustrate below the general strategy to solve such
problems using energy method.
Solution:
The problem is quite
easily solved by making
the point B free to move
horizontally but applying
a horizontal force Q ( in
kN) at this point to
control its movement.
The strategy consists of
calculating the
horizontal movement of point B in terms of the load Q, and then determining the
value of Q for which this movement is zero. It should be clear that this value of
Q for which the movement is zero is the value of the horizontal reaction at point
B.
Fig. 2.46 FBD for a unit horizontal load at B
Table 2.4 Calculation of horizontal movement of the roller support B
Member Force
Fi, kN
L/AE
(×10−8
N−1
)
(×10−4
m)
AD −16.7 1.24 0 0
AF + 13.3 1.59 1 21.1
BE −25.0 1.24 0 0.00
BF + 20.0 1.59 1 31.8
CD −16.7 1.24 0 0
CE −16.7 1.24 0 0
CF +5.0 1.59 0 0
DF 0 1.24 0 0
EF −8.3 1.24 0 0
Total 52.9
Fig. 2.48 Replacing reaction with an undetermined force
Fig. 2.47 A statically indeterminate truss
38
The vertical components of the reactions remain unchanged from the
determination in Example 2.16: and . The forces in
the various members can be calculated by considering the FBDs of the various
pins. This is quite straight forward, and the values so obtained are tabulated as
column 2 in Table 2.5 below. The values in column 3 and 4 of this table will be
the same as in the corresponding column of Table 2.5, and then column 5 is
modified as shown. The horizontal displacement of point B under the action of a
force Q at that point is thus (52.9 +3.18Q) ×10−5
m, with Q in kN.
This displacement is zero when Q = − 52.9/3.18 = − 16.6 kN. Since the ctu l pin
B is restrained from moving, the reaction at point B must be 16.6 kN, inwards.
We have, thus, solved the statically indeterminate problem. Once this is known,
we can calculate loads in all the members of the truss.
2.11 Strain energy in an elastic body
We have so far considered the strain energy of axially loaded structures. Let us
extend this to a more general state of stress and strain. Consider an infinitesimal
cubical element of dimensions δx, δy, and δz along the three coordinate axes. Let
this be acted upon by a force which produces a stress ζxx in the x-direction. The
force acting on these faces is . If the strain in the x-direction is εxx, the
elongation is εxxδx. The strain energy of this infinitesimal element, thus, is
( )( )
( )
, where δV is
the volume of the element. For a finite body
then we can find the strain energy by
integration over the whole volume:
∫
`
(2.15)
It stands to reason that the stress ζxx does not
do any work with the strains εyy and εzz, since
these strains result in displacements which are
perpendicular to this stress. Similar work will
be done by the other stress components.
Let us now look at the work done by shear
stress components. Consider a shear element
as shown in Fig. 2.50 where the lower
surface is anchored and the upper surface has
a shear stress of ηyx. Let the element undergo
a shear strain of γyx as shown. This implies
that the upper surface with a force of ηyxδxδz
acting on it undergoes a displacement of
γyxδy. The strain energy of this infinitesimal
element, thus, is
( )( )
( )
For a finite body then we can find the strain energy by integration over the whole
volume:
∫
` (2.16)
Similarly for the other shear components. Combining the strain energies for
normal and shear strains, we can write the equation for the general state of strain
for a body of volume V as
∫ ( )
` (2.17)
Table 2.5 Calculation of horizontal movement of the roller support B
Member Force
Fi, kN
L/AE
(×10−8
N−1
)
(×10−5
m)
AD −16.7 1.24 0 0
AF + 13.3 + Q 1.59 1 21.1 + 1.59Q
BE −25.0 1.24 0 0.00
BF + 20.0 + Q 1.59 1 31.8 + 1.59Q
CD −16.7 1.24 0 0
CE −16.7 1.24 0 0
CF +5.0 1.59 0 0
DF 0 1.24 0 0
EF −8.3 1.24 0 0
Total 52.9 + 3.18Q
Fig.2.49 An infinitesimal
element under tension
Fig. 2.50 A Shear element
39
Summary
The general strategy for solving the problems of the mechanics of
deformable bodies consists of three major steps:
1. Consideration of static equilibrium and determination of loads in
members of the structures. This equilibrium analysis invariably requires
drawing up strategically chosen free body diagrams (FBDs),
2. consideration of relations between loads and deformations, and
3. consideration of the conditions of geometric compatibility.
The second step above requires the considerations of the materials as well as
the geometry of the structures. This step in itself may be divided into three
distinct phases:
a. We convert loads to stresses in the various members (macro to micro),
b. the stresses are then converted to strains using the material properties
(micro to micro transformation), and finally,
c. with the use of the geometry of the structure, we determine
deformations from the strains so calculated (micro to macro).
The strength of this method lies in the fact that the first and the third steps
above require the consideration of the geometry of the structure (and are
independent of the material), while the second step requires considerations
of only the material of the structure. Thus, the stress-strain relation obtained
from the tensile test with its most simple loading conditions can be used to
predict behaviour of very complicated structure, since the second step above
is independent of loading and geometry and depends entirely on the
material.
We may, at time, need to go in the reverse direction. We may be given the
total deformation from which we need to determine the loading: we
calculate strains from deformation, convert strains to stress using material
properties, and then integrate stress to determine the loading. The strategy
here too is macro to micro to micro to macro.
There are many problems in which we cannot take the steps enumerated
above in a linear sequence, because there are not enough equations of
equilibrium to solve for all the unknown loads. In such cases we have to
consider simultaneously all the three steps, even if we were interested in
only one, say, in determining the forces in the system. Such problems are
known as statically indeterminate problems. Examples 2.3 to 2.5 illustrate
the methodology to be adopted for solving such problems.
As we apply an axial load to a member and it develops a strain εxx in the
axial direction, there is also a transverse strain in the y- and z- directions. The
strain in a transverse direction is a fixed (negative) proportion of the strain in
the axial direction.
where ν is termed as the Poisson ratio and is a property of the material. With
this, the net longitudinal strain in any direction is related to all the three
tensile stress components.
Change in temperature of a structural member introduces thermal strains so
that the net strains of an element subject to a general state of stress and to a
change in temperature is given by:
( ) (2.9)
( ) , and
( )
We define the shear strain γxy in the element at a point as the distortion in the
shape of the element as measured by the change in angle between two
mutually perpendicular lines (parallel to x- and y- directions).
The shear stress is related to shear stress by the relation: . Shear
strain in a plane depends only on the shear stress in that plane and no other
stress component. Heating of a material too does not introduce any shear
strain.
The stress-strain properties of a material are determined by a tensile test. In
Sec. 2.6 we introduced the following concepts:
Proportional limit: The stress up to which the stress is linearly proportional
to strain.
Elastic limit: The stress up to which the material upon unloading returns to
its undeformed length. Both proportional and elastic limits are difficult
to determine.
Permanent set: The residual strain in a material after unloading.
Yield strength: The stress level at which the permanent set is 0.2% (or the
residual strain is 0.002). A material is modelled as elastic up till this
level of loading.
Strain hardening refers to the increase in yield strength of a material due to
its plastic straining. It is exhibited by materials in which the stress-
strain curve slopes upward in some part of the plastic region.
Ultimate strength is the maximum nominal stress in a material before
necking begins.
Necking refers to sudden and localized sharp reduction of cross-sectional
area.
Most of the differences between the behaviour of ductile and brittle material
arises from the fact that there is little plastic deformation in a brittle
40
material. A brittle material undergoes fracture with very little strain,
much less than that for a ductile material. Glass, for example shows no
plastic deformation at all. Another feature to note is that the strength to
fracture is much larger in compression than in tension.
As a structure is loaded the displacements of the points of application of
external loads result in work being done. This work done is stored as the
strain energy of the body given as
∑ . The work done on a simple
bar by an axial load is calculated as
.
Castigliano theorem states that if the total strain energy of a structural
system is expressed in terms of the external loads applied to it, the deflection
at any one loading point (in-line with the load) is obtained by taking the
partial derivative of the strain energy with respect to the load at that point:
.
The procedure consists of applying a load P at the point where the deflection
is to be calculated and in the direction in which the deflection is desired.
This may involve replacing an existing load with P, or inserting a dummy
load. The loads Fi’s in the v rious members re c lcul te in terms of the
unknown load P, and then the total energy U is calculated. After taking the
partial derivative of U with respect to P, the actual value of P is plugged in
(or P is replaced by zero, in case it is a dummy load). This gives the desired
deflection.
In the case of more involved trusses, it was shown that we could simplify the
calculation of the deflection at the location of a load P by rewriting the
partial derivative as:
∑
∑
∑
.
Here we first calculate Fi’s without the lo d P, and then calculate the value
of as the increment in ’s for unit lo d P. This is known as the
unit load method whose calculations can be organized as in Table 2.3 or 2.4
Statically indeterminate problems can also be solved using the energy
method. The strategy consists of relaxing one of the boundary constraints by
letting that boundary point move. A dummy load is introduced at that
location in place of the reaction that would have been there if the constraint
was not relaxed. The deflection of the boundary point is then calculated in
terms of that dummy load. We next obtain the value of the dummy load
required to make the movement of that point as zero. This value is the
desired reaction at that point.
The strain energy per unit volume of the body is given by
( )
The total strain energy can be obtained by integrating it over the entire
volume of the body.
41
3 Torsion of circular shafts
3.1 Introduction
A slender rod which is subjected primarily to twisting or torsional load is termed
as a shaft. One of the more important uses of torsional members is in the
transmission of power or motion through
circular shafts. A shaft is used to transmit
the torque generated by an electric motor
to the load it rotates. The torque produced
by the engine of a car is transmitted to its
wheels by a shaft. When a coil spring
elongates, the wire constituting its coil is
twisted. Torsion bars are also used as
springs in automobile suspension (Fig.
3.1).
In problems involving torsion of shaft we may be interested in determining:
The stresses that result when the shaft carries a specified twisting
moment. We may consequently determine the maximum twisting
moment that the shaft can carry without failure.
The twist in the shaft when carrying a specified twisting moment. In
application to torsional springs, we may like to determine the spring
constant, which is the angular twist per unit twisting moment.
To obtain the relations between twisting moment, angle of twist, and the stresses
and strains we shall follow the strategy that we outlined in the last chapter, but in
a reversed order. The reason for this is that unlike the situations involving axial
loading treated in the last chapter, it is not possible to make the assumption of
uniform stresses in cases of torsional loading. In fact, it will be shown that the
stresses on the cross-section of a shaft vary with the distance from the axis of the
shaft.
For a constant diameter shaft, we shall first assume a total angle of twist θ for an
applied twisting moment T. We then use the geometric considerations to convert
this macro quantity to the strain at various points in the shaft. This is the macro
to micro stage. We next use the material properties to convert strains to stresses.
This is the micro to micro transformation. In the last stage we convert the
stresses into torque, a micro to macro conversion. This completes the solution to
the problem.
3.2 Relating angle of twist to twisting moment
Fig. 3.2 shows a circular shaft25
of radius R and length L
clamped at one end and
subjected to a twisting moment
T. Let the shaft undergo a twist
through an angle θ as shown.
We first determine the strain
components in the shaft. For this
purpose we make some
simplifying assumptions26
:
Circular cross-sections
of the shaft perpendicular to the axis remain plane, i.e., there is no
warping of the shaft,
cross-sections of the shaft do not deform, i.e., there are no strains within
a cross-section of the shaft. Radial lines within the cross-sections remain
straight and radial, and
there is no change in length of the shaft, i.e., there is no axial strain.
25
We assume a circular shaft because many of the assumptions made here are not
valid for non-circular shafts 26
These assumptions can be shown to be true by using some fascinating
symmetry arguments. See Crandall, Dahl and Lardner, An introduction to the
mechanics of solids,2 ed., McGraw-Hill
Fig. 3.1 Torsion bar used as
suspension in automobiles
Fig. 3.2 A circular shaft under torsion
42
The above assumptions imply that there are no linear strains. Therefore, using the
cylindrical polar coordinates as shown,
No distortion of the sections rules out shear strains and γrθ and γzr also vanish.
The only non-zero component of strain is γrθ which we now proceed to
determine.
Calculation of strain from macro distortion
For this purpose we take a
slice of length dz at a distance
z from the clamped end as
shown in Fig. 3.3. The
detailed geometry of
distortion is shown in Fig.
3.4. Let the twist of the face
at z be θ, and that at z + dz be
θ + dθ. To calculate the shear
strain in the shaft, consider a
‘rect ngul r’ element ABCD
on the surface of the cylinder.
After distortion, the shape of
this element changes to
A1B1CD. The angular twist dθ
of this element is the angle that the
movement from A to A1 subtends at the axis
passing through point O on the axis of the
shaft. What, then, is the strain? We see that
which was originally a right angle has
now changed to . Thus, it has reduced
by . Therefore, the strain here is equal
to which is seen as AA1/DA. Thus,
the strain at r = R is
.
It can be seen that the strain γθz is not
constant with r. Consider the deformation at a radius of r. Here, the point E has
shifted to point E1, so that strain at this radius is given by EE1/dz, or,
( )
. (3.1)
Converting strain to stress
Conversion of strain to stress is simple. Since there is no strain other than the
shear strain γθz (and its complementary shear strain γzθ), there is only one
component of strain ηθz (and its complementary
shear stress ηzθ). These stress components on an
element are shown in Fig. 3.5. The shear stress
component can be obtained by multiplying the
strain with the shear modulus G:
( ) ( )
,
(3.2)
where G is the shear modulus of the
material. Please note that neither
the geometry nor the nature of
loading enters this step. The
variation of shear stress with the
radius r is shown in Fig. 3.6.
Converting stress into loading
Consider an elemental area in the
cross-section of the shaft at radius r
and angle θ as shown in Fig. 3.7. The shear stress at this location is ( )
. If the area of the element is dA, the shear force on this element is
. It is easy to see that the force on an element of equal area which is
diametrically opposite to this element is equal in magnitude but has the opposite
direction. This is true of all elements of the cross-
section and, therefore, the net shear force on the
section is zero. But that is not true for the moment
about the origin. Every elemental shear force
contributes a counter-clockwise (hence, positive27
)
moment, so they add up. The sum of moment can be
found by simple integration. The force on the
element shown at a radius of r is stress times its area,
or,
. Therefore, its contribution to the
twisting moment about O is radius times this force,
27
Consistency of results requires that we define our co-ordinate directions and
sign conventions very clearly. It is common to use only right- handed triad for
the direction of axes: Curl the fingers of your right hand from the positive x- to
the positive y-axis. The thumb then points in the positive z-direction. We shall
use only right-handed triads in this book.
Fig. 3.3 The slice whose distortion is studied
Fig. 3.4
Fig. 3.6 The shear stress distribution on
the cross-section of the shaft
Fig.3.7 Shear force on
an elemental area
Fig. 3.5 Shear stresses on
an element
43
or,
. Thus, the total twisting moment T is
∫
∫
The integral ∫
is termed as the second moment of the area about the polar
axis of the section. Many authors term this as the polar moment of area. It is a
geometric property of the area and is denoted by28
Izz. This reduces the
expression for the twisting moment T to
(3.3)
We have completed the solution of the problem of the torsion of a shaft under a
twisting moment. We can recast Eqs. 3.1-3.3 to obtain any quantity of interest.
Replacing dθ/dz from Eq. 3.3 in the expression for the shear stress η,
( )
(3.4)
The total twist θ is obtained by integrating dθ/dz over the entire length of the
shaft:
∫
∫
(3.5)
The product GIzz is termed as the torsional rigidity of a shaft. The more its value,
the less is the twist produced for a given length and twisting moment
3.3 Stresses and strain in a circular shaft
We now evaluate the value of Izz for a circular shaft of radius R. We replace the
elemental area dA of Fig. 3.7 with its value rdθdr, and integrate over θ from 0 to
2π, and over r from 0 to R:
∫
∫ ∫
( ) ∫
, or
for a circular shaft. (3.6)
The torsional rigidity GIzz of a circular shaft varies as the fourth power of its
radius or diameter.
28
Many texts use the symbol J to denote the second moment of area about the
polar (z-) axis. We prefer here the symbol I with two subscripts denoting the
distance from the specified axis.
The maximum shear stress in a shaft occurs where the value of r is maximum,
i.e., at r = R. Using Value of Izz from Eq. 3.6 in Eq. 3.4, we get
(
)
Thus, the maximum shear stress in a shaft for a given twisting moment T
decreases as D3.
We illustrate below the use of these formulae.
Example 3.1 Diesel generating set
The shaft of a 2 MW diesel generating set rotates at 500 RPM. What is the
minimum diameter of the steel shaft connecting the diesel engine to the electric
generator if the shear stress in not to exceed 40 MPa?
Solution:
We first calculate the torque from the power being transmitted: P = T×ω. Here ω
is the angular speed equal to 2π×RPM/60 = 52.36 rad/s. Torque T then is (2×106
W)/(52.36 rad/s) = 3.82×104 N.m. This is the twisting moment in the shaft. The
shear stress varies across the section of the shaft with the maximum stress
occurring at the surface at r = R, where R is the radius of the shaft.
To calculate the stress in the shaft at r = R, we use Eq. 3.4 with the value of Izz
given by Eq. 3.6:
( )
With T =3.82×104 N.m and η(R) = 40 MPa, we get R = [2×3.82×10
4 N.m/(π×40
MPa)]1/3
= 0.085 m, or 8.5 cm. Thus, the diameter of the shaft needs to be at
least 17 cm.
What is the twist per meter run of the pipe?
To obtain the twist angle θ per meter run, use Eq. 3.5 with L = 1 m:
( ) ( )
( ) , ( )
- , or 0.133
o per meter run,
a negligible amount.
Example 3.2 Torsion bar
Fig. 3.8 shows a torsion bar used as suspension in an automobile. The load from
the wheels is applied to a rigid arm as shown. Calculate the spring constant for
the bar.
44
Solution:
The twist in the bar
then is given by Eq.
3.5 as:
. For
an applied force F, the
torque T is F×(0.7 m),
L = 2 m, G for steel is
80 GPa, and Izz =
π(0.04)4/32. Plugging
in the values, we get
for a load F, a twist of 6.96×10−5
F. This twist results in an upward motion of the
load point of 0.7×θ, or 4.87×10−5
F. Thus, the effective spring constant for the
torsion bar spring is k = 20.53 kN/m.
Example 3.3 Power shaft
Fig. 3.9 shows a power shaft of diameter 4 cm transmitting power to two
machines. The shaft is driven by a belt drive that applies a torque of 40 kN.m at
pulley A. The power take-off is again through belts at pulleys B and C. if the
shaft diameter is 8 cm, determine the total twist of the shaft and the maximum
value of shear stress in the shaft.
Solution:
We first draw a diagram depicting the variation of twisting moment along the
axis of the shaft. To determine the twisting moment T at any location in the
shaft, we externalize the moment there by taking a section at that point and draw
an FBD. Fig. 3.10a shows an FBD for determining the value of T for all values
of z between 0 and 1.5 m. The torque acting on pulley A is 40 kN.m, and using
the right-hand thumb29
rule for directions of torques, it is pointed in the positive
z-direction, and hence, positive. We arbitrarily show the twisting moment at z to
be positive T. The moment balance of this FBD shows that T must be −40 kN.m.
This is valid for all vales of z between 0 and 1.5 m.
If, however, the value of z is larger than 1.5 m, the resulting FBD is as shown in
Fig. 3.10b, and the value of T is −20 kN.m. The v ri tions of T with the value of
z have been plotted in Fig. 3.10c. This is known as the Twisting or Torsion
Moment Diagram (TMD)30
The value of shear stress is
given by Eq. 3.4. The maximum
shear stress will occur in the
section AB where the twisting
moment is the maximum. And
it will be at the surface where
the value of r is the maximum
(equal to R):
( )
( )( )
[The diameter of the shaft is 8
cm throughout. The value of Izz
is πD4/32, or π(0.08 m)
4/32 =
4.02×10−6
m4.]
This is a fairly large value, close
to the failure strength of structural steel. We probably need a thicker shaft to
give it a margin of safety.
The twist of the shaft section AB of length L = 1.5 m which carries a uniform T of
−40 kN.m is given by Eq. 3.5 s
29
Right hand thumb rule states that if you curl the fingers of your right hand in
the sense of the torque, the thumb points in the direction of the moment vector. 30
These TMDs are a big help in the analysis of shafts which do not have uniform
twisting moments along them. We can draw the TMDs directly without drawing
FBDs if we follow the following procedure: (1) start from T = 0 at the left most
end; (2) at every location where a concentrated moment To acts, decrease the
value of T by To, if To is positive, or increase by To if it is negative. We will
come across similar procedures for drawing shear force diagrams (SFDs) and
bending moment diagrams (BMDs) in Chapter 4.
Fig. 3.9 Power shaft
Fig. 3.10 Twisting moment diagram
Fig. 3.8 Torsion bar
45
( )( )
( )( )
A reasonable value of G for steel is 80 GPa.
Similarly, the twist of shaft section BC is exactly half of this, since it carries only
h lf the twisting moment (−20 kN.m), i.e., 0.093 r d.
The tot l twist of the sh ft is the lgebr ic sum of the two: −0.279 r d or −16o.
The negative sign indicates that the end at C twists clockwise with respect to the
end A.
Example 3.4 Twist in a tapered shaft
We next consider a tapered shaft in which the polar moment of area, and
therefore, contribution to the twist varies
along the axis of the shaft. Fig. 3.11
shows a 1 m long tapered steel shaft
subjected to a twisting moment of 1
kN.m. If the base diameter is 10 cm and
the tip diameter is 7 cm, determine the
total twist of the shaft.
Solution:
The contribution dθ to the twist
of the shaft by a section of
length dz at z is given by
(T/GIzz)dz. In this problem the
twisting moment T is constant
along the length of the shaft, but
Izz varies with z. It can be
verified that the linear variation
of diameter D is given by
( ) ( ). The value of Izz varies as fourth
power of the diameter, i.e., as
πD4/32. Fig. 3.12 shows the
variations of the twisting
moment, area, the polar moment
of area, and the contribution to
twist along the length of the tapered shaft. The total twist can be obtained by
integrating the contribution of an elemental length. Thus,
∫
∫ ( )
.
We insert here the value of Izz in terms of the diameter D(z), which, in turn, is
expressed in terms of z as above.
∫
( ) , * + -
= 0.024 rad or about 1.4
degrees.
Where and what will be the magnitude of the maximum shear stress in this
tapered shaft? The shear stress is maximum (at a given section) at the outer most
location, i.e., at r = R. Thus,
( )
Since Izz varies as R4, and T is constant along the shaft, the value of maximum η
along the length of the shaft varies like R−3
, i.e., the maximum value of the shear
stress along the length occurs where R has the minimum value. The maximum
shear stress, therefore, occurs at the tip where D is 0.07 m, Izz is π×(0.07 m)4/32 =
2.36×10−6
m4, and T = 1 kN.m.
( ) ( ) ( )
Example 3.5 Cable in a sleeve
Fig. 3.13 shows a 4 mm dia long cable in
a sleeve used to control a setting
remotely. As we turn the knob the
connecting cable twists inside the sleeve.
The sleeve is provided so that the cable
does not flip. The friction between the
sleeve and the cable applies a torque on
the cable which needs to be overcome.
This torque is estimated to be about 0.3
N.m per meter run of the cable. If the
torque needed at the setting point is 0.5
N.m, determine the maximum length of the cable, if the cable material can
withstand a shear stress of 100 MPa. What would be the play? (The play is the
angle through which you need to turn to effect a change in setting when you
reverse the setting.)
Solution:
Fig. 3.14 shows the TMD of a cable of length z. The maximum torque in the
cable is (− 0.5 −0.3z) N.m, and occurs at the knob-end. The maximum shear
Fig. 3.12 Variations of twisting
moment, area, polar moment of
area, and the contribution to twist
along a tapered shaft
Fig. 3.11 Tapered shaft
Fig.3.13 Cable in a sleeve
46
stress would be at the surface of the cable, i.e., at r = 0.002 m. Eq. 3.4 gives
( )
( m) ( )N.m
( m) ( )
Using the condition that
maximum shear stress is
limited to 100 MPa31, we
get the maximum value of z
as [(100×106/79.6×106) –
0.5]/0.3 m, or 2.5 m.
The maximum twisting
moment, then, is (−) 1.25
N.m, and the twist is given
by Eq. 3.5 as
( ) ( )
( ) , ( m) - or 88
o. This is the play in the cable.
Example 3.6 Geared shafts
Fig. 3.15 show two steel shafts geared together. One end of the first shaft is built
in a wall. Find the maximum shear stress in the shafts and the total rotation of
the free end of the second shaft.
Solution:
The first step in
solving this problem
is to determine the
twisting moments
along the two shafts
and to draw the
twisting moment
diagrams. Clearly,
the torque in the
thinner (second) shaft
is 3 kN.m throughout
its length. To determine the torque in the thicker (first) shaft one has to be
careful. The torques in the two shafts are not equal. (Why? Why does a simple
torque balance not give the correct result?32
) The problem can be solved if it is
realized that the contact force F between the two gears must be equal and
opposite. And therefore, the torque in the first shaft is 10/6 of 3 kN.m, or 5
31
We need to use a negative sign with ηmax here. 32
It is because we have not shown the bearings that will be required to hold the
shafts in place. The bearings will apply forces on the shaft which will produce
moments that should also go in the moment balance equation.
kN.m. This torque is negative, i.e.,
clockwise looking from the right end.
Fig. 3.16 shows the twisting moment
diagram for the two shafts.
The maximum torque in a shaft is
given by ( ), where
R is the radius of the shaft. The
maximum value of the shear stress in
the first shaft is ( ) ( ) , ( ) - . This is quite safe. The
maximum value of the shear stress in
the second shaft is ( ) ( ) , ( ) - . Thus, the
maximum (shear) stress in the shafts is 70.8 MPa.
Let us next find the total twist at the free end. The twist in the each of the two
shafts is obtained from the equation .
Twist in the first shaft, ( ) ( ) ( ) , ( ) - , counter-clockwise
looking from right.
Twist in the second shaft (with respect to the geared end
of the shaft,
( ) ( ) ( ) , ( ) - , clockwise looking from right.
To find the total twist of the free end with respect to the
fixed end of the first shaft we cannot just add the two
twists. Consider the motion of the gears as shown in Fig.
3.17. Angle θ1 represents the clockwise movement of the
larger gear (on shaft 1). It is clear that angle θ2 which
represents the counter-clockwise movement of the
smaller gear due to gearing alone is 10/6 of θ1. This is the rotation of the left end
of shaft 2. Since θ1 is 0.0064 rad, angle θ2 is 0.01 rad counter-clockwise. The
twist of shaft 2, which is 0.03 rad counter-clockwise is superimposed on the
motion of the gear, to obtain the total rotation of the free end as 0.01 rad + 0.03
rad = 0.04 rad or 2.3 degree.
3.4 Hollow shaft
We shall see here that hollow shafts provide excellent rigidity for weight of
material. Consider a hollow circular shaft of inner radius Ri and an outer radius
of Ro as shown in Fig. 3.18. The value of Izz can be obtained by replacing dA in
r2dA with rdθdr and integrating over θ from 0 to 2π and over r from Ri to Ro.
Fig. 3.14 TMD of the cable
Fig. 3.15 Geared shafts
Fig. 3.17
Geometry of twist
Fig. 3.16 Twisting moment diagram for
geared shafts
47
∫
∫ ∫
( )
(
) (3.7)
The maximum shear stress in the shaft will be near
the surface, i.e., at r =Ro. Therefore, the maximum
stress in the shaft ( ) ⁄ varies
inversely as Izz. If we define the torque carrying
capacity of the shaft as the maximum torque the
shaft can carry without the stress exceeding a
specified limit, it is clear that this varies directly as
the value of Izz (for a fixed value of Ro). The curve
labelled (a) in Fig. 3.19 which plots the variation of Izz (as the fraction of the Izz of
the solid shaft of radius Ro) also represents the variation of the torque carrying
capacity. The curve (b) plots the variation of the weight (which varies as the area
of cross-section) of
the shaft. The curve
(c) shows the
torque carrying
capacity per unit
weight of the shaft
showing clearly the
cost effectiveness33
of a hollow shaft34
.
3.5 Statically indeterminate shafts
There are many
situations in which
the twisting
moments in shafts
33This, of course, has not taken into account the increased manufacturing
cost of the hollow shaft. 34
This is quite as expected. An element nearer the surface has larger stresses and
contributes more to the torsional moment. Therefore, the material nearer the
surface is used more effectively to bear the torsional load than an equal area near
the axis. Seen in another way, it is an area nearer the outer surface that makes a
larger contribution to Izz, the value of the polar moment of inertia.
cannot be determined by considerations of equilibrium alone. In such shafts the
geometrical constraints on twists need to be invoked to solve the problems.
We follow the same three-step process that was invoked in the last chapter:
Use equilibrium analysis to write equations for the twisting moments in
the various parts of the shaft. There may not be enough equations to
determine the moments explicitly.
Convert twisting moments to twists in each part.
Write geometrical compatibility conditions to complete the analysis.
We illustrate the procedure with a few examples.
Example 3.7 A shaft built in at both ends
Consider a composite steel
shaft ABC built up of two 1 m
long steel sections, AB of 10
cm dia and BC of 15 cm dia
(Fig. 3.20). A torque of 100
kN.m is applied to the collar
in the middle. The two ends
of the shaft are built into
walls so that there is no
rotation of the ends. What is
the twist produced in the
shaft?
Solution:
Equilibrium analysis
Let the reactions at the two
ends be T1 and T2 as shown.
From the condition of the
equilibrium of moments we
get T1 + T2 + 100 kN.m = 0. It
should be clear that either T1
or T2 or both should have a
negative sign. This is the only
equation we get from the
statics for the two unknown
reactions T1 and T2. Clearly
this is a statically
indeterminate problem. We need to consider deformations as well.
Fig. 3.18 Hollow
cylindrical shaft
(a) Variation of the value of Izz of hollow shaft
(b) Variation of the weight of hollow shaft
(c) Variation of the ratio of strength to weight
Fig. 3.19 Comparison of hollow shaft with solid shaft for
various ratios of the internal and external radii
(a) The composite built in shaft
(b) FBD for determining torques in part AB
(c) FBD for determining torques in part BC
(d) Torsion or twisting moment diagram
Fig. 3.20
48
We need to determine the twisting moments in the two halves to calculate the
twists therein. For this purpose, we take a section first in the part AB and draw an
FBD for the left part as shown in Fig. 3.20b. Here T is the twisting moment in
the shaft. The equilibrium of this FBD gives T1 + T = 0, or T = − T1. Fig. 3.20c
shows the FBD for determining the twisting moment in the second part of the
shaft. From this we get T1 + T + 100 kN.m = 0, or T = − T1 – 100 kN.m. Fig.
3.20d shows the complete twisting or torsion moment diagram (TMD) of the
shaft35
. If we have chosen the sign of T1 correctly, then both halves of the shaft
have negative twisting moments36
.
Relating torques and twists
Now that we know the twisting moments, we can calculate the twist using Eq.
3.5: ⁄ .
The values of Izz are:
for shaft AB: πD4/32 = π(0.1 m)
4/32 = 9.81×10
−6 m
4
for shaft BC: πD4/32 = π(0.15 m)
4/32 = 49.7×10
−6 m
4
( )( )
( )( ) , and
( )( )
( )( )
Geometric compatibility
Since both ends of the shaft are
built in, the net twist in the shaft
must be zero: θAB +θBC =0. This
gives:
−1.92×10−6
T1 –
0.38×10−6
T1 – 0.038 = 0, which
gives
T1 = −16.6 kN
With this value of T1, we can
calculate the twist at point B as
35
The reader can verify that we could have drawn this TMD directly without
drawing FBDs if we had followed the procedure outlined in footnote 5. 36
It is clear that the sign of T1 that we have chosen here cannot be correct
because with this we have negative twisting moments in both halves of the shaft.
This, of course, is not possible since if one part twists clockwise, the other must
twist counter-clockwise. But it does not matter for our analysis here.
θAB = −1.92×10−6
T1 =
(−1.92×10−6) × (−16.6 kN) = 0.032
rad
Example 3.8 Meshed gears
Fig. 3.21 shows two shafts, one of dia
6 cm and the other of 4 cm, carrying
identical meshed gears in the middle.
The length of each shaft is 1 m. The
two shafts are disengaged, the top
shaft A rotated by 10o
in the direction
shown, and then the two gears are
meshed again. Shaft A will untwist a
bit twisting shaft B till the
equilibrium is reached. Determine the
locked in torque at equilibrium.
Solution:
Equilibrium requires that the contact
force between the gears be equal and
opposite. Since the two gears are identical, the torques in the two shafts are
equal but opposite. Let this residual torque be To, positive To in (the left part of)
shaft A and negative To in (the left part of) shaft B.
Let us assume that wall at left applies on shaft A a reaction torque T1, and on
shaft B a reaction torque T2. The TMDs of the two shafts can be calculated and
are as shown in Fig. 3.22. These have been drawn under the assumption that T1
and T2 are both positive.
Now let us look at the deformation of
shaft A. It is clear that the twist in the
left half must be the same but opposite
of that in the right half, for the total
twist from end to end to be zero. Since
the two halves have identical
geometries, it stands to reason that the
torque in the two halves must be equal
and opposite. There is, thus, only one
solution: the twisting moment in the
left half is + To/2, and that in the right
h lf is − To/2. Similarly, we can argue
that the twisting moment in the left
half of shaft B be − To/2, and that in the
Fig. 3.21 Two meshed shafts
(a) TMD for top shaft
(b) TMD for bottom shaft
Fig. 3.23 Actual TMDs of the two shafts
(a) TMD for top shaft
(b) TMD for bottom shaft
Fig. 3.22 TMDs of the two shafts under
the assumptions that the reactions on the
left wall are T1 and T2, respectively.
49
right half be + To/2. These are shown in Fig. 3.23.
Geometric compatibility
Refer to Fig. 3.24. Shaft A was rotated by 10o when
the two gears were engaged. After engagement and
letting go, the shaft A unwinds by an angle θ2
which is the same as winding up of shaft B (since
the gear ratio is one). The residual twist in shaft A
is now θ1. It should be clear that the geometric
compatibility condition is:
θ1 + θ2 = 100 = 0.175 rad
We can calculate the twists θ1 and θ2 using Eq. 3.5:
θ = TL/GIzz. Thus,
( ) ( m)
( G ) , ( m) - , and
( ) ( m)
( G ) , ( m) - .
Using these in the geometric compatibility condition, we get
2.46×10−6
To + 12.45×10−6
To = 0.175
This gives To, the locked-in twisting moment as 11.7 kN.m.
3.6 Composite shaft
Let us next consider twisting of a composite shaft that is made up of inner core of
one material clad with an outer sleeve of another material as shown in Fig. 3.25.
To solve this problem, let us look carefully through the derivation of the torsion
formulae in Section 3.2 and figure out the changes we would need to make on
account of two different materials in the cross-section.
We had assumed a twist angle θ and showed
using geometry that there is only one shear
strain component γzθ which is given by Eq. 3.1
as ( )
. This does not change with
the material. Thus, here too, stain γzθ varies
linearly with the distance r from the longitudinal
axis, independent of material.
We had next converted the shear strain to shear
stress by multiplying it with G, the shear
modulus. Here the material dependence arises.
In the inner core up to r = r1, we multiply the
strain with the value of G = G1 for the core material, and in the outer sleeve for r
between r1 and r2, we multiply with the value of G = G2 for the sleeve material,
which is higher. Thus, the graph for shear stress is kinky with two different
slopes, one for the core and the other for the sleeve. This is shown in Fig. 3.26.
The next step in Section 3.2 was considering the shear force on a small element,
calculating its contribution to the twisting moment about the axis, and integrating
over the entire cross-section:
∫
∫
Here, unlike what we did in Section 3.2,
we cannot take G outside the integral
since it is not constant over the section.
But we can do it part-wise: we divide
the area in to two parts, one, with r
between 0 and r1, which covers the core
with modulus G1, and the other with r
between r1 and r2, which covers the
sleeve with modulus G2.
∫
∫
∫
2∫
∫
3
2 ∫
∫
3
or
( ) (3.8)
where I1 is the polar moment of the core area and I2 is the polar moment of the
sleeve area. Compare this with Eq. 3.3. The term GIzz for a uniform shaft is
replaced with (G1I1 + G2I2). Similarly,
( ) (3.9)
The torsional rigidity of the composite shaft is, thus,
( ) ( ).
Here , and (
) .
Fig. 3.24 Geometric
compatibility condition
Fig. 3.26 Shear strain and shear
stress distribution across a
composite shaft
Fig. 3. 25 A composite shaft
50
3.7 Torsion of thin-walled tubes
We have so far found exact solution to the problem of torsion in circular (and
hollow circular) shafts. It is not possible to find such solutions for shafts of
arbitrary cross-sections. However, we can find quite easily the approximate
solution for a thin-walled shaft of arbitrary section. Consider such a shaft as
shown in Fig. 3.27. We use the n, s, z
co-ordinate system as shown, with
the coordinate axis s along the central
line of the tube wall. The dominant
stress component in this case is ηzs
(along with the complementary stress
component ηsz). We shall assume,
without proof, that the other stress
components are either absent or are
negligibly small.
We show in Fig. 3.27b a small
element of length dz of the shaft.
The shear stress ηzs is distributed over
the top and bottom surface of the
element while the complementary
shear stress ηsz is distributed over the surfaces marked 1 and 2 in the figure. We
introduce here the concept of shear flow q defined as the shear force per unit
length of the tubular surface:
∫ (3.10)
In Fig. 3.27b we have shown the net shear forces on the vertical surfaces as shear
flow q times the length dz of the surface. The first thing to notice is that shear
force per unit length on the vertical surface 1 is the same as on the horizontal
surface. The next thing to notice is that the two forces shown are the only
significant vertical forces on the element, and therefore, q1 = q2, that is, the shear
flow is the same at two arbitrary positions, and hence everywhere, along a cross-
section of the tubular shaft37
.
We can now relate the shear flow q to the twisting moment T. Consider an
element of length δs in the cross-section of the shaft as shown in Fig. 3.28a. The
37
This of course implies that if the wall thickness is constant, the shear stress is
constant too. And also that as the wall thickness increases the shear stress
decreases, and vice-versa. The nomenclature shear stress originates perhaps from
the fact that there is a definite analogy between shear flow in the thin wall of a
shaft and the flow of an incompressible fluid in a channel.
shear force on this element is qδs whose moment about an arbitrary point O is
hqδs, which is 2qδA, where δA is the grey area in Fig. 3.28a. The total twisting
moment, then, is simply the shear flow q times twice the area A of the cross-
section of the tube: , from which we can extract the value of the shear
flow38
as:
(3.11)
Example 3.9: A hollow circular shaft
Let us evaluate the stresses in a hollow circular shaft by the approximate method
outlined in Sec.3.7 and compare the results with those obtained by the exact
method. Consider the hollow circular steel shaft of length 1 m shown in Fig.
3.29. It is subjected to a twisting moment T = 100 N.m. Compare the stresses
obtained by the exact and the approximate methods.
Solution:
Eq. 3.4 gives the stresses in a circular
shaft: ( )
, where Izz for a hollow
shaft is given by Eq. 3.7 as
(
).
For the given values,
,( ) ( ) -
.
38
One interesting fact about this derivation is that this relation has been obtained
without any reference to the material properties, and therefore, is applicable both
to elastic and plastic deformations.
(a) (b)
Fig. 3.27 A thin-walled torsion tube
(a) (b)
Fig. 3.28 Relating shear flow to the twisting moment
Fig. 3.29 Hollow circular shaft
51
The shear stress at r = 20 mm, then, is ( ) ( )
13.5 MPa, and at r = 16 mm is ( ) ( )
10.8 MPa. The shear stress varies linearly between these two values across
the thickness of the shaft.
The shear flow q by approximate procedure is given by Eq. 3.11 as , where A
is the area enclosed by the mean line of the section (here a circle of radius 18
mm). Thus, A = π(0.018 m)2 = 1.02×10
−3 m
2, and ( ) (
) = 49 N/m. The average shear stress can be obtained by dividing the
shear flow q by the wall thickness t to get ( ) ( ) The maximum stress is underestimated by a mere 9%.
Example 3.10 A thin rectangular tubular shaft
Consider a tubular shaft of rectangular
section as shown in Fig. 3.30.It is subjected
to a twisting moment of 100 N.m. What are
the stresses in the various sides of the
rectangle?
Solution:
The shear flow q by approximate procedure is given by Eq. 3.11 as , where A
is the area enclosed by the mean line of the section. The value of A for the given
section is (22 cm – 2 cm)×(12 cm – 2.5 cm) or 0.19 m2. The shear flow is
( ) ( 0.19 m2) = 263.2 N/m. The shear flow is constant
throughout the tube. The shear stress in the shorter (thinner) sides is q/t, or
(263.2 N/m)/(0.02 m) = 13.2 kPa, and the shear stress in the longer (thicker) sides
is (263.2 N/m)/(0.025 m) = 10.5 kPa.
3.8 Plastic deformation in torsion
Let us next look at what happens when a shaft is loaded beyond its plastic limit.
This discussion will serve as a simple model of how problems in elastic-plastic
deformations can be handled. Consider a shaft made up of an elastic-plastic
material whose stress-strain behaviour can be modelled as shown in Fig. 3.31.
The material is linearly elastic till the yield shear stress level39
ηY is reached, after
which the material deforms perfectly plastically with the stress remaining
constant at the yield stress value. If we unload such a material after it has been
39
Fig. 3.30 is similar to Fig. 2.29c, except that linear stress and strain have been
replaced with shear stress and strain. It will be shown later in Sec. 6.10 that the
yield shear stress ηY is related quite simply to the yield stress ζY: ηY = ½ ζY.
deformed up to point A in Fig. 3.32, it follows
a straight line AB with slope G, the shear
modulus.
As a shaft is twisted, and the assumptions
about its behaviour that plane sections remain
plane and do not distort hold, the shear strain
will vary linearly with the radius ( ( ) ⁄ ) as shown in Sec. 3.2. The strains
are then converted to stresses using the stress-
strain relation. Fig. 3.32a-d show the shear
stresses for various levels of straining. When the maximum shear strain is less
than γY, the shear stress distribution is linear as shown in Fig. 3.32a. The
maximum shear stress is less than ηY. As the twisting increases, the value of the
maximum strain increases, the stresses increase till the stress and strain reach the
yield values as shown in Fig. 3.32b. The slope of the stress-radius line increases
as shown. Thereafter, the plastic behaviour kicks in. The yield value of shear
stress is obtained at a radius r = ro < R. The shear stress for r between 0 and ro
increases linearly from 0 to ηY, and thereafter remains constant at ηY for r > ro.
This is shown by the stress distribution of Fig. 3.32c.
For Fig. 3.32c, the shear stress distribution is given as40
:
( ) ( )
, for (a)
As the twisting moment increases further, the value of ro, the radius at which the
yield value is reached decreases and more of the shaft is under plastic
40
Since the value of dθ/dz is not known, γzθ is not determined, and, therefore, ro
is undetermined thus far.
Fig. 3.30 A rectangular tubular
shaft
Fig. 3.31 Elastic-plastic behaviour
(a) (b) (c) (d)
Fig. 3.32 Shear stress distribution in an elastic-plastic shaft
52
deformation. Fig. 3.32d shows the condition when the entire shaft has undergone
plastic deformation.
The shear stress distribution is related to twisting moment by using the same
procedure we followed in Sec. 3.2: We take a small area element rdθdr at radius
r and determine the shear force on it as ηrdθdr. The contribution to the twisting
moment of this elemental force is obtained by taking its moment about origin (by
multiplying the force with radius r) and integrating over the entire area:
∫ ∫ ( )
(b)
If we plug in Eq. (b) the value of η as given by Eq. (a), we can obtain the value of
ro. Once ro is obtained, we can determine the value of dθ/dz and complete the
solution of the problem.
Example 3.11 Twist in a shaft with plastic deformation
A shaft of 4 cm dia is subjected to a twisting moment of 2 kN.m. Determine the
twist per meter length of the shaft. The yield shear stress for steel is 125 MPa.
Solution:
Let us first assume that only elastic deformation takes place. Eq. 3.4 gives the
maximum shear stress as ( ) ( ) , ( ) - , well above the yield value. Following the
derivation and notation of the last section, let ro represent the radius at which
plastic deformation is reached41
. Then,
∫ ∫ ( )
∫ ( )
∫ ( ) ∫
0
∫ ∫
1
0
(
)
(
)1 (a)
Plugging in the values of ηY = 125 MPa, T = 2.0 kN.m, and R = 0.02 m, we get ro
= 0.0112 m, or 1.12 cm. The stress at this radius is the yield shear stress 125
MPa. For the value of shear modulus of 80 GPa, this gives a shear strain of 125
MPa/ 80 GPa = 1.56×10−3
at r = 0.0112 m.
41
We cannot find the value of ro by using Eq. 3.2 because it has been derived
under the assumption that the deformation is linear elastic everywhere.
Using these values and the fact that the shear strain is given by ( ) ⁄ for all r, we get ⁄ ( ) 1.56×10
−3/11.2×10
−3 m = 0.14
m−1
. Therefore, the twist per meter ⁄ is 0.14 rad/m.
3.9 Limit Torque
In the preceding section we have seen the difficulties that arise when we
undertake the analysis of both elastic and plastic deformations. The analysis was
possible at all because we were taking a very simple case of pure torsion on a
uniform circular bar.
We can however work with a simpler model
in much of engineering work with
complicated structures. In this model which
is termed as limit analysis, we take a fully-
plastic stress distribution and omit the earlier
elastic-plastic considerations. The load for
which the structure first becomes fully-plastic
is termed as the limit load.
Limit analysis is based on the idea that any
structure made up of materials with fairly
well-defined yield point will not undergo very
large deformations till all of it is in the plastic
region. And, therefore, deformations will be small as long as the load is less than
the limit load for that structure. Limits load, in general, are much easier to
calculate. Let us consider a shaft in the plastic limit when the whole cross-
section is in the plastic state. The stress distribution is then very simple, as
shown in Fig. 3.33. The calculation of the limit torque42
for such a distribution is
quite simple:
∫ ∫ ( )
∫
As long as the applied torque is below this value, some part of the structure will
be in the elastic range and the twist will not be excessive. Limit analysis is quite
extensively used, at least as a first approximation, in the design of structures.
42
The limit load for this case can be obtained quite easily from Eq. (a) in the
solution of Example 3.10. The limit load corresponds to ro vanishing.
Replacing ro by 0, gives the same result as here.
Fig. 3.33 Fully-plastic stress
distribution
53
3.10 Strain energy in torsion
We had introduced in Sec. 2.9 the concept of strain energy. The energy method
based on Castigliano theorem was introduced in Sec. 2.10 where a number of
examples involving axially-loaded members were solved. The method was also
applied to a statically indeterminate problem. We introduced in Sec 2.11 the
calculation of strain energy for an arbitrarily loaded structure. We now extend
the energy methods to cases involving torsion.
Let us consider a shaft of radius R and of length L subjected to a pure torsional
moment T. The strain energy is obtained from Eq. 2.16 using the stress
distribution given by Eq. 3.4.
∫
∫
∫
.
/
∫
∫
∫
∫
(3.12)
where A is the cross-sectional area and the integral of r2 over A has been replaced
by the polar moment of area Izz.
Castigliano theorem can be quite easily extended for the case of a torque load T
to give the twist θ as:
(3.13)
We now illustrate the application of Castigliano theorem.
Example 3.12 Stepped shaft
Consider the stepped steel shaft shown in Fig. 3.34. It consists of three parts:
part A (dia 20 mm, length
1 m), part B (dia 16 mm,
length 1.5 m), and part C
(dia 10 mm, length 2.0
m). It is subjected to three
twisting torques of 300
N.m, 200 N.m and 100
N.m as shown.
Determine the total twist
of the free end of the
shaft.
Solution:
Since Castigliano theorem requires that the total energy be differentiated with
respect to torque applied at the point where the twist angle is to be determined,
we replace the torque of 100 N.m by T. The TMD of the composite shaft, then,
is as shown in Fig. 3.35. The total strain energy is given by:
( )6( ) ( )
( )
( ) ( )
( )
( )
( )
7,
and
( )0( ) ( )
( ) ( )
( )
1
Using 100 N.m as the value of T, we get θ = 3.9 rad, or 223o, a fairly large twist.
Let us, as a check, calculate the maximum shear stress in the shaft. The
maximum shear stress in a circular shaft is given by . This has
been obtained by substituting the value of Izz in terms of R, and determining the
stress η at r = R. This gives the values 47.7 MPa for the part A of the shaft, 46.6
MPa for the part B, and 63.3 MPa for the part C. These appear to be safe even as
the twist appears to be excessive.
Example 3.13 Coil spring
Fig. 3.36a shows a
closely-wound coil spring
consisting of n turns of a
wire of radius of r wound
into a coil of radius R.
Determine the elongation
of the spring under the
action of an axial force P,
and, thereby, obtain the
spring constant.
Solution:
This example
provides a
dramatic
illustration of the
power of energy
method and of
Castigliano
Fig. 3.34 Stepped shaft
Fig. 3.35 TMD of the stepped shaft
(a) (b)
Fig. 3.36 Coiled spring
(a) (b)
Fig. 3.37 Statically indeterminate shaft
54
theorem. Fig. 3.36b shows the FBD of the spring with the wire cut at an arbitrary
location. We can, by equilibrium of moments conclude that the twisting moment
T on the wire is clearly equal to PR, the product of the load P and the radius R of
the coil, independent of the location of the cut. Thus, the twisting moment
everywhere in the wire is PR. Therefore, the strain energy due to the twisting
moment in the wire constituting the spring is obtained by writing the strain
energy dU of an elemental length and integrating it over the entire length of the
wire, i.e., for n coils of radius R. The total energy of the spring is given by
∫( )
( )
∫
( )
( ), since the total length of
the wire is 2πnR.
We can evaluate the shear force acting on the wire as V = P. These shear forces
also contribute to the strain energy, but it can be shown that their contribution is
of order (r/R)2 of the contribution of twisting moments, and hence can be
neglected.
Use of Castigliano theorem then gives the deflection of the spring in the direction
of application of force P as:
( )
( )( )
The spring constant
Example 3.14 Statically-indeterminate torsion problem
Consider a composite shaft consisting of a solid steel shaft and an aluminium
tube as shown in Fig. 3.37. If a torque of 5 kN.m is applied to the rigid disc
attached to the left end, determine the twist of the composite shaft.
Solution:
Let the torque carried by the steel rod and the aluminium tube be T1 and T2,
respectively. Fig. 3.37b shows the FBD of the rigid end disc. From the
equilibrium of this disc:
T1 + T2 = 5 kN.m (a)
Since there is no other equilibrium equation, this problem is statically
indeterminate. All we have besides Eq. a is the geometric compatibility
condition that the twists θ1 and θ2 of the two shafts are equal. Let us determine
θ1 and θ2 by energy method. The total strain energy is given by:
The twists of the two shafts are obtained by partially differentiating U with
respect to T1 and T2, respectively. Equating the two twists, we get
Here, the value of Izz,1, the polar moment of inertia of the steel rod is πD4/32 =
π(0.050 m)4/32 = 0.61×10
−6 m
4, and that of Izz,2, the polar moment of inertia of
the luminium tube is π(Do4 – Di
4) /32 = π(0.080
4 – 0.60
4) m
4/32 = 2.75×10
−6 m
4.
The values of G1 and G2 are about 80 GPa and 26 GPa, respectively. Using the
value of L as 0.5 m, the equivalence of twists gives:
3.90×10−6
T1 = 6.99×10−6
T2, or T1 = 1.79T2 (b)
Solving Eqs. a and b simultaneously, we obtain the values of T1 and T2 as 3.2
kN.m and 1.8 kN.m, respectively. The (equal) twists in the two shafts are then
obtained as 0.0125 rad or 7.17o.
Summary
When a circular shaft is subjected to a pure torsional load, there is no
warping or distortion of cross-sectional planes, and consequently there
is only one component of strain, namely γzθ (and its complementary
strain γθz).
o We first assume a twist angle θ and determine the value of the
strain γzθ as rdθ/dz using purely geometrical considerations.
o We next convert the shear strains to shear stresses using the shear
modulus G: ηzθ = Gγzθ = Grdθ/dz.
o We next take a small element within the cross-section of the shaft,
write an expression for shear force acting on it in terms of the shear
stresses, take its moment about the axis of the shaft and integrate
over the entire cross-sectional area to obtain the twisting moment T
as GIzzdθ/dz. Here Izz is the second moment of area (polar) of cross-
section, defined as integral of r2dA over the cross-section. The
value of Izz for a solid cylinder was found to be πD4/32, and for a
hollow shaft as (
) .
o The twist θ is given by TL/GIzz.
The quantity GIzz is seen as the torsional stiffness which is defined as
the torque required to produce a unit twist per meter length of a shaft.
Since an area nearer the surface has a larger values of stresses that
contributes more to the twisting moment than an equal area nearer the
axis, hollow shafts are much more effective in resisting torsional loads.
There are many situations in which the twisting moments in shafts
cannot be determined by considerations of equilibrium alone. In such
shafts the geometrical constraints on twists need to be invoked to solve
55
the problems. Such problems are termed as statically indeterminate
ones. We follow the same three-step process that was invoked in the last
chapter:
o Use equilibrium analysis to write equations for the twisting
moments in the various parts of the shaft. There may not be enough
equations to determine the moments explicitly.
o Convert twisting moments to twists in each part.
o Write geometrical compatibility conditions to complete the
analysis.
For composite shafts made up of a core of one material overlaid with a
sleeve of another material, the torsional stiffness is given by ( ).
The concept of shear flow q defined as the shear force per unit length of
the wall was introduced for the approximate analysis of thin tubular
shafts. It was shown that , where A is the area enclosed by the
mean line of the wall of the shaft.
Limit load refers to the load under the assumption that the whole of the
structure has yielded and the shear stress everywhere is ηY. If the
applied torque is well below the limit torque so obtained, we can
presume that the twist of the shaft is not excessive.
The strain energy in torsion of a shaft is given by
.
56
4 Forces and moments in beams
4.1 Introduction
We have so far considered two types of structural elements: axially loaded truss
elements that resisted axial forces, tension or compression, and shaft-like
elements that resisted twisting moments. Beams that resist transverse loads by
bending are other common structural elements. We define a beam as a slender
element (i.e., an element whose cross-sectional dimensions are much smaller
than its length dimension) that essentially resists loads acting transverse to its
length. Roof beams that support the roofs of buildings are beams. The horizontal
deck of a road flyover supported on columns is a beam structure. The leaf
springs of an automobile suspension transfer the weight of the car to the axle
(and further to wheels) through beam action. A wing of an airplane is a beam. So
is the cantilever beam shown in Fig. 4.1.
For the beam to be in equilibrium, the net force or moment on the beam or on
ny p rt of it must be zero. Let us ‘cut’ the c ntilever be m shown in Fig. 4.1a
near the wall and draw the free-body diagrams (FBDs) of the two parts as shown
in Figs. 4.1b and c. Clearly, we need a force V and a moment M to balance the
applied load P on the part shown in Fig. 4.1c. These are the forces and moments
of internal reaction and these arise because of the deformations that are caused
by the applied load. There are, of course, equal and opposite reactions on the
stump of the beam built in the wall as shown in Fig. 4.1b.
We can, in general, resolve the internal resistance forces and moments in to their
components. Fig. 4.2 shows that resolution. The following are the nomenclature
and the actions of the various components:
Fx: the axial force that results in elongation (or compression, if
it is negative) of the member.
Fy and Fz: shear forces that result in shearing at the section. The shear
forces are conventionally assigned the symbol V.
Mz: the axial moment that is the torsion moment that causes
twisting of the member. This was the subject matter of the
last chapter.
Mx and My: transverse moments that are termed as the bending moments
and cause the member to bend. Moment Mx results in
bending the beam in the y-z plane while the moment Mz
results in bending the beam in the x-y plane.
We had in Chapter 2 laid out the general strategy for solving the problems of the
mechanics of deformable bodies as consisting of three major steps:
(a) (b) (c)
Fig. 4.1 A cantilever beam
Fig.4.2 Forces and moments in a beam
57
Consideration of static equilibrium and determination of loads in various
members,
Consideration of relations between loads and deformations, (first converting
loads to stresses, then transforming stresses to strain using the properties
of the material, and then converting strains to deformations), and
Considerations of the conditions of geometric compatibility.
In that chapter we had also studied the structures bearing axial loads. In Chapter
3 we considered slender members bearing twisting moments. These were termed
as shafts. We learnt to determine the variations of torsion moments (Mz in the
notation introduced above) as torsion moment diagrams (TMDs), and then to
calculate the resultant shear stresses and twisting angles of the shafts
In view of the importance of the role of beam members in engineering and other
structures, we devote this chapter to beams, and that too, to only the first step of
the 3-step process outlined above. The loads which are of immediate relevance
to a beam are the shear forces Fy and Fz and the bending moments Mx and My
which are caused by the transverse loads as shown in Fig. 4.3. It can be verified
easily that the shear force component Fz
and the bending moment component My
are caused only by the vertical load Pz,
whereas the shear force component Fy and
the bending moment component Mz are
caused only by the transverse load Py..
This leads us to a very simple stratagem:
we calculate the bending moments and
shear forces for the vertical and horizontal
loads separately (assuming that the other
loads are absent), and then patch up the
results. We shall, in the discussion that
follows, consider only the vertical load
system, which can easily be replicated for the horizontal loads.
4.2 Sign convention
It is imperative from the point of view of consistency that we define the sign
convention for shear force and bending moment at a section. Fig. 4.4 shows a
beam which has been sectioned and the two resulting parts separated. The shear
forces and the bending moments at the two sections are equal and opposite, as
shown. We adopt the convention given in Table 4.1to ensure that shear force (or
the bending moment) at either of the two sections have the same sign:
Table 4.1 Sign convention43
Sign of the
outward normal
to the section
Actual direction
of the force or
moment
Assigned sign to the
shear force or bending
moment
Along the + ve
coordinate
direction
Along the +ve
coordinate
direction
+ ve
Along the − ve
coordinate
direction
Along the − ve
coordinate
direction
+ ve
Along the + ve
coordinate
direction
Along the − ve
coordinate
direction
− ve
Along the − ve
coordinate
direction
Along the +ve
coordinate
direction
− ve
It can be verified that the shear forces and bending moments shown in Fig. 4.4
are all positive according to this convention. This convention44
can be
43
It is interesting to note that this sign convention results in a beam bending
concave upwards with a positive bending moment and convex upwards for a
negative bending moment.
Fig. 4.3 Loads on a beam
Fig. 4.4 Positive shear stress and bending moment
58
summarized graphically as Fig. 4.5. Either
of these two can be used as an icon for the
sign convention employed.
4.3 Loads and supports
One common classification of beams is
based on the kind of supports on which a
beam rest. There are three idealized
support systems for beams as shown in Fig. 4.6. Support A is a termed as a
pinned support. Here the beam is attached to the support in such a manner that it
is not restrained from rotating about this point. Consequently, the reaction from
the support is just a force which can be resolved in to two force components RA,x
and RA,y. The support here cannot apply a moment on the beam. The support
shown at point B is termed as a roller support. Here the reaction from the support
can only be a vertical force RB,y. The roller does not restrain the beam from
moving horizontally, and hence there is no horizontal force applied by the
support. As in the case of pinned support, there is no reaction moment at a roller
support as well. Beams with only pinned or roller supports are termed as simply-
supported.
The support shown at C is called a built-in support. Here the beam is built into
the wall so that it is restrained from rotating about point C. The beam will have a
zero slope at such a point. This is a consequence of the restraining moment My
that the support applies to the beam at that point. Considerations of equilibrium
will require that the reaction RC,y be equal to P, and the moment My applied on the
beam by the support will be PL, where L is the length of the beam. A beam can
have a built-in support at either one end or both ends. The beam shown at right
in Fig. 4.6 with only one end built-in (and no support at the other end) is termed
as a cantilever beam.
The lower two diagrams in Fig. 4.6 show the conventional representations of the
three types of idealized supports. Please note that these are idealizations. Most
practical supports are more complicated, but many can be analysed quite
satisfactorily by replacing them with one or the other of these idealizations. The
dashed lines in these represent the (exaggerated) deflected shapes of the beams.
Note that the cantilevered beam has zero slope at the built-in end. Table 4.2
summarizes these idealized supports.
44
Please note that many current books use a sign convention entirely different
from this. It is, therefore, advisable that the sign convention used be noted in
each problem that you solve. The sign convention can be denoted easily by a
graphical symbol similar to the ones shown in Fig. 4.5
We, in a similar fashion, idealize the loads that the beams carry. The left top
diagram in Fig. 4.7 show a simply-supported beam with a concentrated or a point
load, while the on the right shows one with a distributed load. A point load is
specified as a force P with appropriate force units like N.
Table 4.2 Idealized beam supports
Support type Freedom of motion Reactions present
Built-in support
No degree of freedom A moment as well as
horizontal and vertical
reaction forces
Pinned support
Single degree of freedom
- rotation.
Horizontal and vertical
reaction forces
Roller support
Two degrees of freedom –
rotation and horizontal
movement
Only vertical reaction
force
Fig. 4.5 Graphically representation
of sign convention
Fig. 4.6 Three type of beam supports and their conventional representations
59
A distributed load, on the other hand, is specified by a load density w as force per
unit length with appropriate units like N/m. What is shown on the beam on right
is idealized as a uniformly distributed load, wherein the load density w per unit
length does not change along the length of the beam.
However, in some situations, the load density could vary, as is shown in Fig.
4.8a. Here the load is distributed, but the loading density varies along the length
of the beam. It is modelled as a linearly varying distributed load. If the load
density is w N/m at the end of the beam of length L, the load density at any x
from the left end is given simply by wx/L N/m.
A beam could also be subject to an externally-applied bending moment as shown
in Fig. 4.8b. Here too, the dashed line represents the (exaggerated) deflected
shapes of the beam.
4.4 Determining shear forces and bending moments
Determination of shear forces and bending moments at any point in a beam is
rather a straight forward procedure. The procedure consists of taking a section of
the beam at that point to expose the shear force V and the bending moment M at
that point and drawing a free body diagram (FBD) of one portion of the beam.
We will first solve a couple of simple examples to illustrate the procedure and
then draw up a generalized scheme of doing things in more complicated
situations.
Example 4.1 A cantilever beam with a load at the free end
Consider a cantilever beam as shown in Fig. 4.9. It is loaded at the free end.
Draw the shear
force diagram
(SFD) and the
bending moment
diagram (BMD).
Solution:
We first calculate
the reactions at the
support. A simple
equilibrium analysis
shows that the end
reaction is a force P
upwards and a
clockwise moment
PL as shown. We
next calculate the
shear force V and
the bending moment
M at an arbitrary
location x from the
support. For this
purpose we take a
section at that
location and draw
the FBD of the
(a) (b)
Fig. 4.8
(a) A simply-supported beam with non-uniformly distributed loading
(b) A simply-supported beam with a concentrated applied bending moment
Fig. 4.7 Two idealized loadings of beam
Fig. 4.9 SFD and BMD for a cantilever beam with end load
(a) A cantilever beam with support reactions
(b) FBD of the section beyond x
(c) Shear force diagram (SFD)
(d) Bending moment diagram (BMD)
60
right-hand portion45
of the beam as Fig. 4.9b. The shear force and the bending
moment on this section are the external loads acting on this part of the beam and
will be shown on the FBD. We do not know their directions. In such a case we
show them assuming they are positive. Since the exposed face on which they are
acting has an outward normal in the negative x-direction, the positive shear force
must be downward and the positive bending moment must be clockwise (as
shown).
A simple equilibrium analysis46
of this FBD gives:
∑ : or (a)
∑ : ( ) , or ( ) (b)
Since the location of the section x is arbitrary, and changing the value of x does
not change either the FBD or Eqs. (a) and (b), these equations give the shear
force and the bending moment at all values of x between 0 and L. The resulting
values have been plotted as shear force and bending moment diagrams in Figs.
4.9c and 4.9d, respectively. These show the variations of the respective
quantities with x.
Example 4.2 A simply-supported beam with a concentrated load in the middle
Consider a simply-supported beam with a concentrated load at the mid-point as
shown in Fig. 4.10a. Draw SFD and BMD for this beam.
Solution:
The first step in the solution of this problem is determining the reactions at the
support. Drawing an FBD of the entire beam (or using symmetry) we can easily
find the two vertical reactions to be P/2 each. To determine the shear force (SF)
and the bending moment (BM) at any location x (measured from the left support)
of the beam, we need to externalize the SF and BM by taking a section of the
45
We could have chosen either pat of the beam but have chosen to draw the FBD
for the right-hand portion of the beam because this results in an FBD with fewer
unknown forces simplifying the equations. 46
M,x in Eq. (b) denotes that moments have been taken about a point at x. This is
convenient because the moment contribution of the unknown force V about this
point is zero.
It may further be noted that in the equilibrium equation, the sign to be used with
the bending moment is the standard sign convention for moments: positive for
clockwise and negative for counter-clockwise. Even though the bending moment
shown is positive (negative on a face with negative outward normal), it is taken
as positive in the equilibrium equation.
beam there and drawing the FBD. It should be obvious that there are two kinds
of FBDs depending on whether the value of x is less than L/2 or greater than L/2.
Fig. 4.10b shows the FBD for x < L/2. We shall show the SF and BM as external
loads on this FBD. We do not know their directions. As before, we show them
assuming they are positive. Since the exposed face on which they are acting has
an outward normal in the positive x-direction, the positive shear force must be
upward and the positive bending moment must be counter-clockwise (as shown).
A simple equilibrium analysis of this FBD gives, for x < L/2:
∑ : or (a)
∑ : , or (b)
Thus, for x < L/2, SF has a constant value of – P/2 while the value of the BM
increases linearly from 0 at x = 0 to a value of PL/4 at x = L/2.
Fig. 4.10 SFD and BMD for a simply-supported beam with a concentrated load
in the middle
(a) Loading diagram
(b) FBD when the section is taken in left half of the beam
(c) FBD when the section is taken in right half of the beam
(d) Shear force diagram
(e) Bending moment diagram
61
This formulation is valid only for x < L/2. For x > L/2, the generic FBD changes
and is as shown in Fig. 4.10c. Here the applied load P too figures in the FBD.
An equilibrium analysis of this FBD gives, for x > L/2:
∑ : or (c)
∑ : ( ) , or
( ) (d)
Thus, for x > L/2, SF has a constant value of + P/2 while the value of the BM
decreases linearly from PL/4 at x = L/2 to a value of zero at x = 0. The resulting
SFD and BMD47
are plotted in Figs. 4.10d and 4.10e, respectively.
4.5 General procedure for drawing shear force and bending moment diagrams by method of sections
On the basis of the method adopted in the last two examples, the following
generalized procedure may be formulated:
Draw an idealized loading diagram of the beam.
Determine the reactions at all supports. If the reactions cannot be
determined, the beam is statically indeterminate and further progress
cannot be made without considering the deflections of the beam. These
will be introduced in Chapter 7.
Determine the number of segments with distinct loading pattern to
cover the entire beam. In Example 4.2, we needed two different types
of FBD: one without the concentrated load P, and the other with it. In
practice, this means that we segment the beam such that the end of a
segment is at the location of a discontinuity in loading pattern. These
could be the concentrated loads or moments, or where the type of
distributed loads changes.
For each of the segments identified above, introduce a cutting plane (at a
location x from the left end) and draw an FBD of either part of the beam
(as convenient). In example 4.1 we had drawn the FBD of the right
portion (since it carried fewer loads), while in Example 4.2, we drew the
FBD of the left portions (since these permitted simpler expressions for
force moments).
47
Since the BM is positive, the beam bends concave upwards, as is physically
apparent from the loading
Introduce the unknown shear force V and the bending moment M at the
cutting plane. These should be shown assuming they are positive
according to the sign convention introduced in Table 4.1 above. Thus,
in Example 4.1 where we had drawn the FBD of the right-hand part of
the beam, the cut face has the outward normal in the negative x-direction
and, therefore, the positive SF is downwards and the positive BM is
clockwise. This is exactly opposite of the case of Example 4.2 where the
outward normal is in the positive x-direction and, therefore, the positive
SF is upwards and the positive BM is counter-clockwise.
Fig. 4.11 SFD and BMD for a simply-supported beam loaded
symmetrically with two concentrated loads
(a) Loading diagram
(b) FBD when the section is taken in the left third of the beam
(c) FBD when the section is taken in the middle third of the beam
(d) FBD when the section is taken in the right third of the beam
(e) Shear force diagram
(f) Bending moment diagram
62
Determine the expressions for SF and BM by equilibrium
considerations, equating the sum of vertical forces and the moment
(about a convenient point) to zero.
Plot the resulting expression to obtain the shear-force and bending
moment diagrams (SFD and BMD). These diagrams are conventionally
drawn exactly beneath the loading diagram of the beam as in Figs. 4.9
and 4.10.
We give below a few more examples to illustrate the general procedure.
Example 4.3 A simply-supported beam with two concentrated loads
Consider a simply-supported beam of length L with two loads acting at L/3 and
2L/3 from the end as shown in Fig. 4.11. Draw the SFD and BMD of this beam.
Solution:
As usual, we begin with determining the reactions at the supports. Through a
simple equilibrium analysis (or by using the symmetry of the problem) the
reaction at either support is a force P upwards..
It is easy to see that we need to segment the beam in this case in three different
ways. One kind of FBD results when the section is taken for with no
loads acting on it (as in Fig. 4.11b). Another kind results when the section is
taken for a value of x between L/3 and 2L/3. In such an FBD one external load P
acts at x = L/3 (as in Fig. 4.11b). And the third kind results when the section is
taken for a value of x between 2L/3 and L. In such an FBD two external loads
act, one at x = L/3 and the other at x = 2L/3 (as in Fig. 4.11c).
We next show the unknown shear force V and the bending moment M at the
newly exposed sections assuming they are positive and using the sign convention
of Table 4.1. In each of the three FBDs, the positive SF is upwards and the
positive BM is counter-clockwise, since all outward normals are along the
positive x-axis.
From the equilibrium analysis of the FBD of Fig. 4.11b, we get for x < L/3:
∑ : or (a)
∑ : , or (b)
Similarly, from the equilibrium analysis of the FBD of Fig. 4.11b, we get for L/3
>x > 2L/3:
∑ : or (c)
∑ : ( ) ,
or , a constant (d)
And from the equilibrium analysis of the FBD of Fig. 4.11c, we get for x > 2L/3:
∑ : or (e)
∑ : ( ) ( ) ,
or ( ) (f)
Fig. 4.12 SFD and BMD for a simply-supported beam with
uniformly distributed load
(a) Loading diagram
(b) Typical FBD for a segment of the beam
(c) Distributed load replaced by a statically equivalent load
(d) Shear force diagram
(e) Bending moment diagram
63
The resulting SFD and BMD48
have been plotted as Figs 4.11e and f.
Example 4.4 A simply-supported beam with uniformly distributed loading
Consider a simply-supported beam with a uniformly distributed load of w N/m as
shown in Fig. 4.12. Draw the SFD and BMD for this beam.
48
Here too, the BM is positive and the beam bends concave upwards, as is
physically apparent from the loading.
Solution:
The total load on this beam is wL. The symmetry of the beam suggests49
that the
reaction at each support is wL/2. Since there is no discontinuity in the loading
with no concentrated load or moment, only one kind of FBD as drawn in Fig.
4.12b suffices for this problem. The presence of distributed load poses a problem
in determining the moment contribution of the loading. To this, we replace the
distributed load with its statically equivalent load50
as shown in Fig. 4.12c. It
consists of the total load wx acting at the centroid of the distributed load, which is
at the mid-point of the beam, i.e., at a distance of x/2 from the left end.
From the equilibrium analysis of the FBD of Fig. 4.12c, we get for all values of
x:
∑ :
or (a)
Thus, the shear force varies linearly, with a value of at x = 0, and a value
of at x = L. It is zero at x = L/2. The variations of shear force are
plotted as SFD in Fig. 4.12d.
∑ : ( ) ( )( ) ,
or (b)
This represents a parabola with M = 0 at x = 0 and L, and a maximum value of
at the mid-point x = L/2. These variations of bending moment along the
length of the beam are plotted as BMD in Fig. 4.12e.
Example 4.5 A simply-supported beam loading with a concentrated moment at the middle
Consider a simply-supported beam of length L loaded in the middle with a
concentrated moment M0 as shown in Fig. 4.13a.Draw the shear force and
bending moment diagrams for this beam.
49
This can also be obtained by drawing the FBD of the whole beam and
replacing the distributed load by the statically equivalent load system consisting
of the total load wL acting at the mid-point of the beam. A statically equivalent
load is the alternate load which produces the same net force and moment at any
point. 50
It can easily be verified that the loading shown in Figs. 4.12b and 4.12c are
statically equivalent as defined above.
Fig. 4.13 SFD and BMD for a simply-supported beam with a concentrated
moment
(a) Loading diagram
(b) Typical FBD for a section in first half of the beam
(c) Typical FBD for a section in second half of the beam
(d) Shear force diagram
(e) Bending moment diagram
64
Solution:
We begin with determining the reactions at the supports. Through a simple
equilibrium analysis the reaction at the left support is determined as a force equal
to M0/L, while t the right support it is − M0/L. The negative sign indicated that
the reaction at the right support is directed downwards, as shown in the figure51
.
We need to segment the beam in two different ways: one, when the section is
taken at (without including the concentrated moment M0 in it) acting on
it (as in Fig. 4.13b), and the other when which included the concentrated
moment M0 in the resulting FBD shown as Fig. 4.13c.
We next show the unknown shear force V and the bending moment M at the
newly exposed sections assuming they are positive and using the sign
convention. In either FBD, the positive SF is upwards and the positive BM is
counter-clockwise since the outward normal in either case is along the positive x-
axis.
From the equilibrium analysis of the FBD of Fig. 4.13c, we get for x < L/2:
∑ : or (a)
∑ : ( ) , or ( ) (b)
Thus, the shear force V is constant in this part, while the bending moment M
increases linearly from 0 to at the mid-point of the beam.
Similarly, from the equilibrium analysis of the FBD of Fig. 4.13c, we get for L/2
>x > L:
∑ : or (c)
∑ : ( ) ,
or ( ) (d)
The shear force V is constant in this part too, with the same value as in the first
part. The bending moment M shows an interesting behaviour: it jumps down
from to at x = L/2 nd then incre ses, g in line rly, from −
at the mid-point to 0 at the end-point of the beam52
. The resulting SFD and
BMD are plotted as Figs. 4.13d and e.
51
It has been assumed here, for simplification, that at least one support is not
restraining the beam horizontally, so that there is no horizontal reaction force.
Anyway, the presence of a horizontal force will not affect the SFD and BMD. 52
Attention is drawn to and interesting feature of SFDs and BMDs as is apparent
to the five examples given so far: the line depicting shear force has a
discontinuity wherever there is a concentrated force as a load, and the BMD is
The deflected (but exaggerated) shape of the beam is shown as the broken line in
Fig. 4.13a. As noted earlier, the beam deflects concave upwards where the BM is
positive and convex upwards where it is negative.
4.6 The area method of drawing the SFDs and BMDs
The method of sections outlined in the last section is a simple method of
determining shear forces and bending moments, but it can get quite tedious in all
but very simple cases. We give here an alternate method known as the area
method.
now seen to be discontinuous at the location of the concentrated moment. We
will elaborate on this later.
Fig. 4.14 Elemental FBDs for three different kinds of loads
65
Consider the beam shown in Fig. 4.14, which carries a concentrated load P at
location B and a concentrated moment M0 at location C as shown. A part of the
beam (segment DE) is subject to a distributed load. The density q(x) of this load
measured in N/m may vary along the length.
Let us determine how the SF and BM change with x along the beam. Let us first
take a small element of length dx at a location x within the segment AB where no
load acts on the beam. We draw an FBD of this element of the beam as shown in
Fig. 4.14b. Here we have shown shear force V and bending moment M at location
x, and shear force V + dV and bending moment M + dM at location x + dx. It can
be verified that all directions have been shown such that SF and BM at either
location are positive. The application of equilibrium to this FBD gives:
∑ : , or (a)
∑ : , or (b)
This implies that the SF as well as BM does not change along a beam segments
which does not carry any load.
We next consider an elemental section of the beam which includes point B, the
location of the concentrated load. Fig. 4.14d shows the FBD of this element.
The application of equilibrium to this FBD gives:
∑ : , or (c)
∑ : ( ) , or for
infinitesimal dx, (d)
These indicate that at the location of a concentrated load, the shear force jumps
up by a value equal to the load (acting downwards), but there is no change in the
value of the bending moment. It can be deduced quite easily that had the load P
been acting in the upwards direction, the SF would have jumped down by the
same value.
Fig. 4.14d shows the FBD of an element of the beam which includes point C, the
location of the concentrated moment M0. The application of equilibrium to this
FBD gives:
∑ : , or (e)
∑ : , or for infinitesimal dx,
(f)
Thus, at the location of a concentrated moment, the bending moment jumps down
by a value equal to the applied moment, but there is no change in the value of the
shear force across such an element.
We last consider an elemental section at a point within the segment DE which
carries a distributed load. The FBD of such a section is shown as Fig. 4.14e.
For x within the beam segment DE, the equations of equilibrium53
give:
∑ : or , or
(g)
∑ : ( ) , or
(h)
This suggests that for a distributed load, the rate of change of shear force at a
location is equal to the (downward) load density at that point. And, similarly, the
rate of change of bending moment is equal to the (negative of) shear force at that
point. We can recast the equations (g) and (h) as:
∫
(4.1)
∫
(4.2)
The area method gets its nomenclature from these two equations which say state
that the change in SF across a beam segment is equal to the area under the
loading curve of that segment, and the change in BM across a beam segment is
equal to the area under the shear force curve of that segment54
.
The eight equations (a) – (h) above (along with Eqs. 4.1 and 4.2) provide a
framework for an very convenient method for drawing the FBDs and BMDs of
the beams directly without drawing FBDs of different segments..
Let us first consider Eqs. (a), (c), (e), (g) and 4.1, all pertaining to changes in
shear force V. Eq. (a) states that V does not change across any element which
does not carry any load. Eq. (c) suggests that at the location of a concentrated
load, the shear force jumps up by a value equal to the load (acting downwards).
Eq. (e) states that V does not change across any element carrying a concentrated
53
Two things should be noted here. First, the contribution of the distributed load
to the moment equation has been obtained by replacing the distributed load by its
statically equivalent concentrated load qdx at the midpoint of the element, i.e., at
location dx/2. Second, this contribution is negligible since this moment is of
second infinitesimal order, while the other terms are of first order only. 54
The difference in signs in Eqs. 4.1 and 4.2 is due to the fact that the load
density q has been defined as positive downwards. If we had taken the usual sign
convention that upward forces are positive, we would have got a negative sign
before integral in both the equations.
66
moment, and Eq. (g) says that the rate of change in shear force is equal to the
density of loading.
In fact, Eq. 4.1 summarizes all this information quite succinctly if we assume a
concentrated load as the integral of the load density at that point. The change in
shear force across a segment of the beam is equal to area under the loading
density curve.
From these we can deduce the following procedure to draw the SFD:
1.1. First draw the loading diagram of the beam.
1.2. Calculate the reaction at the supports.
1.3. Start drawing the SFD at a point slightly left of the left support where
the shear force is taken as zero.
1.4. Travel along the beam to the right, modifying the SF using the rules
given below.
1.5. Shear force does not change over the segment of the beam with no
external load.
1.6. The presence of a concentrated moment does not change the value of
shear force.
1.7. A concentrated force causes a jump in SFD at the location of the force:
go up for every load downwards, down for every load upwards.
1.8. The slope of the SFD at any location is equal to the distributed load
density (load per unit length). Positive slopes for loads downward, and
negative slopes for loads acting upwards.
1.9. Change in SF between any two locations is equal to the area under the
distributed load curve. Positive changes for negative areas and negative
changes for positive areas.
1.10. Proceed till you are slightly right of the right support where the SF
should be zero again. This last is a check on calculations.
This is known as the area method of drawing the shear force diagram. It can be
verified quite easily that the SFDs Figs. 4.9c, 4.10d, 4.11e, 4.12d, and 4.13d
follow from the respective loading diagrams using the above rules.
We, in a similar fashion, can deduce the rules for drawing the BMDs from Eqs.
(b), (d), (f), (h) and 4.2, all pertaining to changes in bending moment M. Eq. (b)
states that M does not change across any element which does not carry any load
or moment. Eq. (d) implies that at the location of a concentrated load too, there is
no change in the value of the bending moment. Eq. (f) states that at the location
of a concentrated moment the bending moment jumps down by a value equal to
the (positive) applied moment. Eq. (h) states that the rate of change in bending
moment is equal to the (negative of) shear force at that point.
Eq. 4.2 contains all of the above points. The change in bending moment while
traversing a segment of the beam is equal to the area under the shear force curve
(but with a reversed sign) over that segment.
The following procedure may be adopted for drawing the BMDs:
2.1. First complete the shear force diagram of the beam.
2.2. Start at a point slightly left of the left support where the bending
moment is taken as zero.
2.3. Travel along the beam to the right, modifying the BM using the rules
given below.
2.4. The slope of the BMD at any location is equal to (negative of) the SF
value at that location
2.5. Change in BM between any two locations is equal to the (negative of)
the area under the SF curve.
2.6. Concentrated moments cause a jump in BMD at the location of the
moment.
2.7. Go up for every negative concentrated moment, down for every positive
concentrated moment.
2.8. Proceed till you are slightly right of the right support where the BM
should again be zero again. This last is a check on calculations.
This is known as the area method of drawing the BMDs. It can be verified quite
easily that the BMDs Figs. 4.9d, 4.10e, 4.11f, 4.12e, and 4.13e follow from the
respective shear force diagrams using the above rules.
The following example illustrates the simplicity of the method of area.
Example 4.6 Beam with an overhang
Consider a 4 m long simply-supported beam with an overhang as shown in Fig.
4.15. The overhang portion AB carries a distributed load of density 20 kN.m.
There are two concentrated loads at locations C and E as shown. It also carries a
concentrated counter-clockwise moment of magnitude 20 kN.m at location D.
Draw the SFD and BMD for this beam.
Solution:
We first determine the reactions R1 and R2 at the supports. With reference to the
loading diagram of Fig. 4.15, we can write the equilibrium equations. Equating
the vertical forces to zero, we get:
67
.
/ ( ) ,
or (a)
We next take the moment of all the forces about the left support and equate it to
zero to get55
:
( ) ( ) ( ) ( ) ( ) ( ) ( ) , (b)
From Eq. (b) we get
Using this value in Eq. (a) we get
We are now ready to draw the shear force diagram.
55
Here again we take the moment of the distributed load by replacing it with the
statically equivalent load, which is the total force (20 kN)·(1 m) acting at the
centroid (of this load) which is located at 0.5 m from the left end of the beam.
We start at zero at the left end. We first encounter the uniformly distributed load.
Using rules 1.8 and 1.9 above, the shear force would increase at a constant the
rate of 20 kN/m, and after one meter it would have increased from 0 at A to 20
kN at B, as shown. A concentrated load (acting upwards) occurs at the location
B. Therefore, following rule 1.7, the value of shear force jumps down by 70 kN
(the value of R1) from 20 kN to − 50 kN. Since there is no lo d on segment BC,
the value of SF through this segment remains constant (rule 1.5). At location C,
the she r force jumps up from − 50 kN to − 10 kN (rule 1.7), and thereafter
remains constant at this value across segment CE, since the this segment does not
have any load except a concentrated moment at D, and rule 1.6 says that SF does
not change due to the presence of a concentrated moment. The downward load at
E makes the SF jump up through 40 kN from – 10 kN to + 30 kN (rule 1.7
again). The shear force remains constant at this value through segment EF, and
then jumps down to 0 at F because of the presence of the concentrated load R2 =
30 kN. The final value of 0 completes the check (rule 1.10).
It should be obvious that this method of area is so much simpler than the method
of sections where we would have needed to draw five different kinds of FBDs
and, then, write ten equilibrium conditions for those five FBDs.
After completing the SFD, we can draw the BMD too. We start at zero for a
point slightly left of point A. The SF increases linearly from 0 at A to 20 kN at B.
By rule 2.4, then, the slope of the B D ch nges line rly from zero to − 20
kN·m/m. The linear change in slope implies that the curve is of second order in
x, that is, it is parabolic, as shown. The change in the value of the bending
moment in going from A to B is the area under the SFD in this segment (rule 2.5),
which is ( ) ( ) ( ) . This area is positive and,
therefore, the change in BM is – 10 kN.m, giving a value of BM at point B as –
10 kN.m. The shear force across segment BC is constant at – 50 kN, so the slope
of the BM curve there is constant at + 50 kN.m/m, and the value of the BM
through this section of length 1 m changes (linearly) through 50 kN.m, the area
under the SF curve in this segment (rule 2.5). The value of BM at point C is 40
kN.m.
From point C to D, the SF is – 10 kN, and therefore the BM curve slopes up at
this rate and the value of BM changes from 40 kN.m to 45 kN.m in 0.5 m. The
presence of a positive external concentrated moment of 20 kN.m at point D
makes the BM jump down to 25 kN.m at this point (rule 2.6), after which the
curve continues its upward march at a rate of + 10 kN.m/m to acquire a value of
30 kN.m at point E. The SF in the last segment EF is constant at +30 kN.
Therefore, the BM there decreases linearly from a value of 30 kN.m to 0 in a
length of 1 m. The end value of 0 indicates that the calculations are in order.
Fig. 4.15 Drawing SFD and BMD using area method
68
Example 4.7 A built-in frame
Consider the frame ABCD shown in Fig. 4.16a which is built in at A. Draw the
SFDs and BMDs of the various segments of the frame.
Solution:
To begin the analysis, we need to consider the FBDs of the various sections of
the frame.
Fig. 4.16b shows the upper segment DC of the frame. There will be a force and
moment acting at the point C due to the restraining action of the segment CB.
Using the requirements of equilibrium we evaluate the vertical force as P
upwards and the moment as PL/2 clockwise.
Using the area method outlined above, we can easily obtain the SFD and BMD of
this segment as shown in Fig. 4.16b.
The FBD of the segment CB is shown in Fig. 4.16c. The load at point C of this
segment is equal and opposite to that at point C of the segment DC. Using
equilibrium of this segment we obtain the force at point B as P upwards, and the
moment there to be PL/2 clockwise. The force in this segment is axial and,
therefore, there is no shear force anywhere. The BMD has been obtained using
the rules 2.1, 2.6 and 2.8. The positive sign of the bending moment indicates that
this segment will bend concave upwards (viewing from right), which agrees with
what is expected intuitively.
We then move on to the cantilevered section AB, which carries a force P
downwards and a counter-clockwise moment PL/2 at point B as shown in Fig.
4.16c. We can obtain the reaction force and moment at end A by equilibrium
considerations. Due to the upward force P, the SFD jumps down to –P at the left
end A and remains so up till the other end where it jumps down to 0. The BMD
jumps down to − PL/2 at point A due to the presence of a concentrated moment
PL/2, and thereafter increases at a constant rate of P because of the presence of
the shear force –P throughout this length reaching a value of + PL/2 at the end B.
It jumps back to zero there because of the presence of a counter-clockwise
moment PL/2.
Example 4.8: An optimization problem
Consider a simply-supported beam of length L carrying a load 2P at the middle
as shown in Fig. 4.17a. It also carries a load P at each of the two ends. The two
supports are located a distance a inwards from the ends. Determine the value of
the distance a required to minimize the maximum bending moment in the beam.
Fig. 4.16 Drawing FBDs and BMDs of the various segments of a frame
69
Solution:
From the symmetry of the beam (or from the two equilibrium equations for the
whole beam) we determine the reaction force at either support to be 2P.
We first draw the SFD using the area method. We start the SFD slightly left of
the left end of the beam with a zero value. A downward force P is encountered at
the left end which causes the SFD to jump up to a value of P (Fig. 4.17b). Since
there is no other loading till the left support, the SF remains constant at P till
then. The reaction at the left support is 2P upwards which causes the SFD to
jump down by 2P to a value of –P at the left support. We continue in a similar
manner and complete the SFD as shown.
The BMD is also drawn in the same fashion (Fig. 4.17c). We start at zero. In the
first segment of length a, the SF is constant at a value of +P, and therefore, the
BM in this section decreases at the rate of P per unit length. The change in value
till the left support is the areas under the SFD of this segment, which is Pa.
Thus, the v lue of B t the left support is −Pa. In the second segment (of
length L/2 – a) the v lue of SF is −P and, therefore, the slope of bending moment
curve here is +P. The change in value of BM is P(L/2 − a) from −Pa. Thus, the
value of bending moment at the mid-point is [−Pa + P(L/2 − a)], or +P(L/2 −
2a). We can continue in the same fashion56
and complete the BMD.
The magnitude of the maximum negative bending moment is Pa, and the
magnitude of the maximum positive moment is P(L/2 − 2a). As the value of a
increases, the first value increases while the second decreases. A little reflection
should convince the reader that the minimum of the maximum value will occur
when these two magnitudes are equal:
( ), or , or .
Thus, we minimize the maximum value of the bending moment by locating the
supports at L/6 from either end of the beam.
Summary
Study of the behaviour of beams is very important because the beams are central
to the design of most structures. We, in this chapter have concentrated on
determining the variations in shear forces and bending moments along the length
of the beam.
We first introduced the types of supports and the loads that the beams carry.
Three idealized supports were identified:
The built-in support which allows no degree of freedom to the beam and
admits both components of the reaction force as well as a reaction
moment.
The pin support which allows one degree of freedom, the freedom to
rotate about that point. This support admits both components of the
reaction force but does not admit a reaction moment
A roller support which restraints the beam only from the vertical motion
and, therefore, admits only the vertical reaction force component.
We next introduced the sign convention for the shear force and bending moment.
The sign is based on two parameters: the direction of the outward normal at the
section, and the direction of the force or the moment itself. If both of these are in
the positive coordinate directions, or both in the negative coordinate directions,
the sign of SF or BM is taken as positive. And if one of them is positive and the
other negative, the sign is taken as negative. This is summarized in Table 4.1 and
as icons of Fig. 4.5.
The method of sections for drawing the SFDs and BMDs uses the following
procedure:
56
Or use the symmetry of the beam.
Fig. 4.17
70
Draw an idealized loading diagram of the beam.
Determine the reactions at all supports.
Determine the number of segments with distinct loading patterns to
cover the entire beam.
For each of the segments identified above, introduce a cutting plane (at a
location x from the left end) and draw an FBD of either part of the beam
(as convenient).
Introduce the unknown shear force V and the bending moment M at the
cutting plane.
Determine the expressions for SF and BM by equilibrium
considerations, equating the sum of vertical forces and the moment
(about a convenient point) to zero.
The other method of determining SFDs and BMDs is the method of areas is
based on the two equations:
, and
.
From the integration of these we concluded that the change in SF across a beam
segment is equal to the area under the loading curve of that segment, and the
change in BM across a beam segment is equal to the area under the shear force
curve of that segment.
The following process for drawing SFD was concluded:
First draw the loading diagram of the beam.
Calculate the reaction at the supports.
Start drawing the SFD at a point slightly left of the left support where
the shear force is taken as zero.
Shear force does not change over the segment of the beam with no
external load.
A concentrated force causes a jump in SFD at the location of the force:
go up for every load downwards, down for every load upwards.
The slope of the SFD at any location is equal to the distributed load
density (per unit length). Positive slope for loads downwards and
negative slope for loads acting upwards.
Change in SF between any two locations is equal to the area under the
distributed load curve. Positive changes for negative areas and negative
changes for positive areas.
The following process for drawing BMD was concluded:
First complete the shear force diagram of the beam.
Start at a point slightly left of the left support where the bending
moment is taken as zero.
The slope of the BMD at any location is equal to (negative of) the SF
value at that location
Change in BM between any two locations is equal to the (negative of)
the area under the SF curve.
Concentrated moments cause a jump in BMD at the location of the
moment. Go up for every negative concentrated moment, down for
every positive concentrated moment.
71
5 Stresses in beams
5.1 Introduction
In problems involving bending of beams we may be interested in
determining:
The stresses that result when a beam carries the specified loads.
We may consequently determine the maximum load that a shaft
can carry without failure.
The deflection of a beam when carrying the specified loads.
We have seen in the last chapter that almost all loads in beam result in
variation of the resulting bending
moment and shear stress along its
length. This inevitably introduces
complications in the determination of
the behaviour of the beam. To obtain a
foothold on the problem we first
consider a very simple case of a beam subject to pure bending57
as shown
in Fig. 5.1.
To obtain the relations between the bending moment Mb and the stresses
and strains we shall follow the strategy that we outlined in Chapter 3
while dealing with the case of torsion of a shaft. This was the reverse of
the generalized strategy outlined in Chapter 2. The reason for this again
is the same as in the case of torsion: unlike the situations involving axial
loading treated in Chapter 2, it is not possible to make the assumption of
uniform stresses in the case of bending of beams.
Before going
further, let us
determine the
nature of
deformations in
beams under
pure bending and
the nature of
stresses that
result from such
deformations.
Fig. 5.2 shows a
beam with a grid
drawn on it. This
beam is
subjected to a
positive bending
moment, and
bends as shown.
It is clear from
the enlarged
portion shown in
Fig. 5.2c that the
beam elements
57
The bending moment can be constant along the length of a beam only if the
shear force V is zero everywhere. This is possible only if there is no other load on
the beam except concentrated moments at the two ends.
Fig. 5.1 Beam in pure bending
Fig. 5.2 Bending stresses in beams
(a) Undeformed beam
(b) Beam after bending
(c) Enlarged portion showing that there is contraction
near the top and extension near the bottom
72
near the top surface of the beam are under compression, while those near
the bottom are in elongation. As a consequence, there are compressive
stresses near the top and tensile stresses near the bottom. It should be
clear that since there in no net tension (or compression) in the beam, the
forces due these stresses must total out to zero. The bending moment at
the section is the integrated moment of the elemental forces due to these
stresses.
The strategy for this problem then consists of:
First using symmetry considerations to establish the nature of
deformation in the beam under pure bending.
Using the geometric considerations to determining the tensile
strain across the beam section as a function of the vertical
coordinate. This is the macro to micro conversion discussed in
Section 2.1.
We next use the material properties to convert these strains to
stresses. This is a micro to micro transformation.
In the last stage we convert the stresses into bending moment, a
micro to macro conversion. We use the fact that the total
bending moment is the given Mb, and the total tensile force at the
section is zero. This completes the solution to the problem.
5.2 Relating curvature of the beam to the bending moment
Consider a beam with a cross-
section that is laterally symmetric
(i.e., it has symmetry about a
vertical axis) subjected to a pure
bending moment Mb as shown in
Fig. 5.3. Under the action of this
positive bending moment, the
beam bends and acquires a
curvature. The coordinate axes
used here are shown in the figure.
By using symmetry arguments we
can show that the following
assumptions are valid in this case of pure bending of a beam of uniform
and symmetrical (about a vertical axis) section:
The beam bends in the shape of a circular arc. This follows from
the argument that a uniform bending moment acting along the
length of the beam must result in a uniform curvature.
Plane cross-sections of the beam remain plane after the bending.
Thus, plane sections 1-2 and 3-4 of the undeformed beam of Fig.
5.4 remain plane in the deformed shape as well.
Initially parallel sections (sections 1-2 and 3-4 of the undeformed
beam of Fig. 5.4) must deform so that they have a common point
of intersection as shown. This common point of intersection is
the centre of curvature of the deformed beam.
Calculation of strain from the geometry of deformation
We now consider the geometry of deformation further to obtain an
expression for strain.
It was argued above that the beam elements near the top are under
compression while those near the bottom are under tension. It stands to
logic, then, that there must be a plane in the beam (near the middle) which
is neither under tension nor
compression. Let AB
represent such a plane for
the beam segment 1-2-3-4 of
Fig. 5.4. This plane with its
extension to the rest of the
beam is termed as the
neutral plane of the beam.
It should be understood that
we do not, as yet, know
where this is located, except
for the fact it must be
somewhere between the top
and the bottom surfaces of
the beam.
Let us consider a plane CD a
distance y up from the
neutral plane AB. The
undeformed lengths of
Fig. 5.3 A symmetrical beam
Fig. 5.4 Geometry of deformation of a beam
73
planes (along the x-axis) AB and CD are equal to begin with. Since the
length of the plane AB is unchanged (this being the neutral plane), the
undeformed length of the plane AB or CD is seen as from Fig. 5.4b,
where ρ is the radius of curvature58
of the neutral plane of the beam. The
deformed length of the plane CD is ( ) . Thus, the contraction in
the length of this plane located a distance y up from the neutral plane is
ydθ. The strain at this location is, thus, given by
(5.1)
It can be seen that in this simple case of pure bending (i.e., with no
loading other than the bending moment which is constant along the length
of the beam) there are no shear strain components. However, there will
be longitudinal strains εyy and εzz due to the presence of ζxx through
Poisson ratio.
Converting strain to stress
Conversion of strain to stress is simple. The tensile stress component can
be obtained by multiplying the strain with the elastic modulus E:
( ) ( )
(5.2)
Note that we know neither
the value of y (because the
location of the neutral plane
has not yet been established)
nor the value of ρ, the radius
of curvature59
. But we have
two conditions that we shall
shortly use.
The distribution of the
stresses across the section is
58
The radius of curvature ρ is ∞ for a flat beam. As the beam bends, the value of
ρ decreases. We introduce the term curvature for 1/ρ. Curvature is usually
denoted by κ (read kappa). The value of κ increases as the beam bends. It is 0 for
a flat beam (corresponding to ρ = ∞). 59
But we have two conditions that we have not used so far. The total axial force
on the section is zero, and the total moment acting on the section is Mb.
like that shown in Fig. 5.5. The trace zz of the neutral plane is termed as
the neutral axis. Note here we have shown the neutral axis to be nearer
the bottom plane of the beam. This results in the top plane of the beam to
be farther away from the neutral axis (NA) than the bottom plane is.
Consequently, the maximum compressive stress is larger than the
maximum tensile stress in the beam.
Since there are no shear strain components, there will be no shear
stresses. Further, there are no other longitudinal stresses, ζyy or ζzz, in this
case of pure bending60
.
Converting stress into
loading
Consider an elemental area
dA in the right face of the
beam as shown in Fig. 5.6.
The force acting on this
elemental area due to the
bending stress is ζdA acting
along the normal to the
section as shown. Note that
we have shown this force outwards from the area, assuming ζ to be
tensile (i.e., positive). The algebra below will automatically take care of
the sign if the stress is compressive. The neutral plane of the beam is
shown as grey61
. The z-axis is the neutral axis of the section under
consideration.
The total axial force on the beam can be found by integration as
∫
. Substituting the value of ζ using Eq. 5.2, we get
∫
∫
∫
where y is the vertical distance measured from the neutral axis.
But there is no axial force Fx in this case of pure bending. Therefore,
60
We can now determine the lateral shear strains εyy and εzz as
.
61 Note again that we do not as yet know the location of the neutral plane.
Fig. 5.5 Stress distribution on a section of the
beam
Fig. 5.6 Calculating loading at a section
74
∫
(5.3)
What does this imply? It simply defines the location of the neutral axis
from which the distance y is measured. Thus, the neutral axis of a beam is
located such that the first moment of area about that axis is zero.
Recall that the centroid of an area is defined as the point about which the
first moment of area is zero. Therefore, the neutral axis of a beam passes
through the centroid of the cross-section62
.
We next calculate the moment (about the z-axis) of these elastic forces
and equate it to Mb, the bending moment on the beam:
∫ ∫ (
)
∫
The integral ∫
is recognized as the second moment of area Izz
about the z-axis, which, in this case, is the centroidal axis. This is a
geometric quantity. Once the shape of a cross-section is known, the value
of Izz can be calculated. See Appendix A to learn some important
properties of the second moment of area and the procedure for its
calculation.
We can, therefore, write an expression for 1/ρ, the reciprocal of the radius
of curvature (which is termed as the curvature κ = 1/ρ) of the beam as
(5.4)
The product is termed as the bending rigidity of the beam. The more
the value of the bending rigidity, the less is the curvature κ of the beam
(for a given value of the bending moment), and more is the radius of
curvature ρ.
We can combine Eqs. 5.2 and 5.4 to obtain
(5.5)
These stresses are termed as the bending stresses.
62
We had chosen the location of the neutral plane in Fig. 5.6 closer to the bottom
of the beam anticipating this result.
The bending formulae (Eqs. 5.4 and 5.5) are sometimes summarized63
as:
(5.6)
It may be noted that the equation above have been obtained for the case of
pure bending, i.e., for the case of constant bending moment in the absence
of any other load. The results for the more general case are very difficult
to obtain. But wherever these have been obtained, it is seen that for
slender members, the resulting stress distribution is quite close to those
obtained above. It is for this reason that we use the results obtained here
in the general case as well.
Since the values of and are zero, the lateral strains and
are given by
(5.7)
Thus, the normal strains in the plane of the cross-section are proportional
to the axial strains, but of opposite sign. Further, since εxx varies with y,
the vertical distance measured from the neutral axis, the strains εyy and εzz
change across the cross-section. This leads to the deformation64
of the
section as shown in Fig. 5.7.
Notice from Eq. 5.6 that the curvature of the beam 1/ρ is given by
63
Notice the similarity of this with a similar equation that we can obtain for the
case of torsion of a shaft from Eqs. 3.2 and 3.3:
.
Note that in this equation for shafts, the z-axis is the longitudinal axis, unlike in
the present case where the z-axis is a transverse axis while the longitudinal axis is
represented as the x-axis.
64
Note, in particular, that the neutral axis (which is the trace of the neutral
surface in the section) is now curved. This transverse curvature of the cross-
section of the beam is termed as anticlastic curvature. The neutral plane now has
double curvature, one in the x-y plane, and the other in the y-z plane.
75
The quantity EIzz can be interpreted as the stiffness of the beam. The
more its value, the less is the curvature of the beam, i.e., less is the
bending.
We give below a few examples of calculation of bending stresses.
Example 5.1 Maximum stresses in a cantilever beam
Consider a 2 m long cantilever MS beam of section 10 mm × 20 mm
loaded as shown in Fig. 5.8. Determine the location and magnitude of the
maximum bending
stress.
Solution:
We need to obtain the
bending moment
distribution first. For
this, we follow the
procedure introduced in
the last chapter, and
first calculate the
reactions at support.
From the balance of
vertical forces we can
see straight away that there will be an upward reaction of 200 kN at the
support. From the moment balance we obtain the moment at support to
be 300 N.m, counter-clockwise as shown.
We draw the SFD by the method of areas. We start at 0, jump down 200
N at the left support (load being upwards), continue at ‒200 N till the first
load is encountered. The downwards load makes the SF jump up to ‒100
N at 1 m. The SF jumps up again at the second load.
The BMD is drawn in the same fashion. We start at 0, jump down to ‒300
N.m at the support because of the presence of the positive reaction
moment. Through the first one meter of the beam, the BM line has a
positive slope of 200 N.m/m (equal to the negative of the constant shear
force). The value of BM at 1 m, the midpoint of the beam, is ‒100 N.m.
The change in value of BM between x = 0 m to x = 1 m is equal to the
area under the SFD over this length. From x = 1 m to x = 2 m, the slope
of the B D is +100 N.m/m, the SF being const nt t ‒100 N over this
length.
We, thus, see that the maximum bending moment occurs at the root of the
c ntilever where its v lue is ‒300 N.m. This, then, would be the loc tion
of the maximum stresses. Since the BM is negative, the beam would
bend convex up. The curvature 1/ρ given by Eq. 5.4 will be negative.
The value of Iyy needed in this equation has been obtained in Appendix B
(Eq. B.6) as bh3/12, where b is the width of the section (10 mm in this
case), and h is the height of the section (30 mm). Thus, the value of Iyy is
(10×10‒3
m) × (30×10‒3
m)3/12, which is 2.25×10
‒8 m
4.
The maximum tensile stress occurs at the top of the beam (y = 0.010 m)
at the root (x = 0), and is given by Eq. 5.5 as
( ) ( )
= 200 MPa
The value of the maximum compressive stress will be the same, except
that it will be at the bottom of the root of the beam. The beam is loaded
almost to its ultimate strength.
Note that given a bending moment, the stresses are independent of the
material of the beam. A beam with lesser elastic modulus will bend more
(giving larger values of curvature 1/ρ and strains) but will produce same
stresses.
Fig. 5.7 Deformation of the shape of a rectangular beam
(a) The undeformed rectangular section (b) variation of longitudinal stress
ζxx with distance y from the neutral axis (c) variation of longitudinal strain
εxx across y (d) variation of lateral strains εyy and εzz with y (e) the deformed
shape of the cross-section (deformation exaggerated). Note that the neutral
axis which is the trace of the neutral surface in the section) is curved.
Fig. 5.8 A cantilever beam
76
It is interesting to compare these results with the case when the beam
section has the longer side horizontal. Notice that the length of the
horizontal side now is a factor of 3 larger, the vertical side a factor of 3
smaller, the value on Izz as now two factors in 3 smaller. The maximum
bending stress that varies like y/Izz is 3 times larger, and the radius of
curvature that varies like Izz is two factors in 3 smaller, i.e., the curvature
(1/ρ) is 1/9th of when the beam section is vertical. These results are
summarized in Table 5.1.
It is clear that when more material of the beam is away from the
centroidal axes (on either side of it), more is the value of the second
moment of area, and the stiffer is the beam.
Example 5.2 Bending stresses in an angle-section beam
Consider a simply supported angle-section steel beam loaded as shown in
Fig. 5.9. Its section is the same as was used in Example B.5. Determine
the maximum tensile and compressive stresses in the beam.
Solution:
To draw the SFD and BMD, we calculate the reactions at the supports.
We determine the reaction at the right support by writing the balance of
moments about the left support. This reaction is found to be 50 N. Then,
by vertical force balance, the reaction at left support is found to be 250 N
as shown.
The SFD of the beam can be drawn easily by the method of areas. The
SFD jumps up through 100 N at the left-end because of the presence of a
downward force, then jumps down through 250 N to ‒150 N due to the
concentrated reaction at 1 m, jumps up through 200 N to +50 N because
of the downward load at 2 m length, and then jumps down to zero because
of the 50 N upward reaction at the right support.
The BMD of the beam starts at zero and has a slope of 100 N.m/m
through the first 1 m length. The value at 1 m is equal to the (negative of)
area under the SFD over this length, which is 100 N.m. We complete the
BMD in the same fashion following the rules given in Sec. 4.6.
There are two extrema in the BMD: a negative 100 N.m value at x = 1 m,
and a positive 50 N.m value at x = 1 m.
The centroid of the cross-section of the beam can be determined by taking
the first moment of the area about an axis passing through the bottom of
the section as was done in Example A.5 in Appendix A where the vertical
value of it was found to be 16.1 mm.
The second moment of the area about the centroidal axis was also
determined there. The strategy was to divide the area into two rectangles,
and then for each rectangle first determining the value of I about its own
centroidal axis, and then using the parallel-axes theorem to transfer it to
the neutral axis, i.e., the centroidal axis of the full section. The value was
determined as Izz = 2.99×10‒7
m4.
We can next determine the stresses. At location x = 1 m where the
m ximum neg tive bending moment of ‒100 N.m acts, the beam bends
convex up so that the maximum tensile stress acts at the top plane which
Fig. 5.9 A simply supported angle-section beam
Table 5.1 Comparison of two different orientations of beam sections
Section orientation
Factor
b 10 mm 30 mm 3
h 30 mm 10 mm 1/3
Izz 2.25×10‒8 m4 0.25×10‒8 m4 1/32
ζxx 200 MPa 600 MPa 3
Radius of curvature ρ (at the
point of maximum bending
moment)
15 m 1.67 m 1/32
77
has a value of y = +33.9 mm measured from the neutral axis. Similarly,
the maximum compressive stress act at the bottom plane which has a
value of y = +16.1 mm measured from the neutral axis.
We use Eq. 5.5 to determine the stresses. These are arranged in the Table
5.2 given below.
At location x = 1 m where the bending moment is ‒100 N.m, the
maximum tensile stress (at y =0.0339 m) is given by:
( )( )
The maximum compressive stress occurs at the bottom plane at y =
‒0.0161 m:
( )( )
We can similarly determine the stresses at the location x = 2 m where the
bending moment is +50 N.m. These are shown in the table above.
Example 5.3 Comparison of rectangular, T-section and I-section beams
Consider three cross-
sections of beams shown
in Fig. 5.10. The three
sections have equal
areas and, hence equal
weights per unit length
of the beams. Compare
the maximum tensile
and compressive
stresses in the three
beams for a bending
moment Mb.
Solution:
The calculations have been organized in Table 5.3. We first calculate the
location of the neutral axes by calculating the y-coordinates of the
centroids of the three sections. This is determined by dividing the areas
into the requisite number of rectangles and then using the formula:
∑ ∑ .
Next, we calculate the second moment of inertia. For this, again, we
divide the cross-section in a number of rectangles, calculating the value of
I for each rectangle about its own centroidal axis, and the transferring it to
the neutral axis using the parallel-axes theorem. Thus,
∑.
( )
/ .
Table 5.2 Stresses at the locations of maximum positive and negative bending
moments
x-location 1 m 2 m
Bending moment, Mb ‒100 N.m +50 N.m
Stress distribution
Maximum tensile stress At top plane (y = 0.0339
m)
11.3 MPa
At bottom plane (y =
‒0.0161 m)
2.7 MPa
Maximum compressive
stress
At bottom plane (y =
‒0.0161 m)
‒5.4 MPa
At top plane (y = 0.0339
m)
‒5.6 MPa
(a) (b) (c)
Fig. 5.10 Three beam sections of equal areas
78
The stresses are then evaluated from Eq. 5.5. These stresses vary linearly
from zero at the neutral axis. The stresses are compressive above the
neutral axis and tensile below it. In each case, the maximum compressive
stress occurs in the top plane, while the maximum tensile stress occurs at
the bottom most plane.
It should be noted that in the case of a T-beam, the maximum
compressive stress is much smaller than the maximum tensile stress since
the neutral axis is closer to the compressive side65
.
Another thing to note is the reduction in the maximum stress in the I-
section. This is a result of a larger value of Izz, which in turn results from
more of the section area (compared to the rectangular section) being away
from the central axis. Since an are ’s contribution in Izz is weighted by y2,
the areas far away from the centroidal axis contribute more, making the
beam stiffer.
65
But the total compressive force is exactly equal to the total tensile force on the
section, there being no net axial force. There is more area of the section on the
compressive side than on the tensile side. It is for this reason that the neutral axis
has shifted upwards causing a reduction of tensile stresses.
5.3 Composite beams
Consider the case of pure bending of a composite beam made up by
bonding two materials of different elastic properties, in particular, of
different elastic moduli. Let us consider a section with symmetry about y-
axis as shown in Fig. 5.11. Let this beam be subjected to pure bending
with a positive bending moment Mb. Let us determine the moment
curvature relations for this beam following the procedure used in Sec. 5.2.
Using the symmetry of the situation, we can again argue that plain
sections will remain plain and that the beam will bend in a circular arc.
The geometry of deformation will be the same as depicted in Fig. 5.4, and
we would get an expression for the linear strain similar to Eq. 5.1
(5.8)
where ρ is the curvature of the neutral plane, i.e., a plane that does not
have any strain, and y is the distance measured from the neutral plane.
Note that, as before, for a given curvature of the beam, the strain varies
linearly the distance from the neutral plane and does not depend on the
material of the beam.
However, when we continue to the next step of converting to stress, the
material properties come in and the stress is given by
( ) ( )
(5.9)
where Ei stands for the elastic modulus of the specific material at that
location. Note, in particular, that while the strain at the junction of two
materials is continuous, the stress shows a discontinuity (see Fig. 5.12).
Note that the strain, as well as the stress, is zero at the neutral plane. The
strain increases linearly on either side of the neutral axis, compressive
above it and tensile below it66
. The stress distribution is discontinuous.
The stress jumps at the location where the material changes,. The strain,
being a purely geometrical quantity in a beam, shows no such jump.
Consider two points close together on either side of the interface of the
66
The bending moment, being positive, introduces positive curvature (concave
upwards) resulting in the strains as shown.
Table 5.3 Comparative stresses in beams of equal weight
Section
Location of NA from the
base
30 mm 38 mm 30 mm
Izz 5.40×10‒7 m4 5.21×10‒7 m4 6.77×10‒7 m4
Stress distribution
y for max tensile stress ‒30 mm ‒38 mm ‒30 mm
y for max comp. stress +30 mm +22 mm +30 mm
max tensile stress 5.56×104Mb Pa 7.29×104Mb Pa 4.43×104Mb Pa
Max comp. stress 5.56×104Mb Pa 4.22×104Mb Pa 4.43×104Mb Pa
Fig. 5.11 Beam with composite section
79
two materials. Since the strains are the same, the changed value of E will
result in different values of
stress on the two sides.
Hence the jump67
.
The location of neutral
plane and the value of ρ are
as yet undetermined. To
evaluate these we, as
before, use the
considerations of
equilibrium. The total
force on the section is evaluated as by integration as ∫
.
Substituting the value of ζ using Eq. 5.9, we get
∫
∫
,
where Ei is the elastic modulus of the
material specific to the area element dA
(and y is the distance of the area element
measured from the neutral plane).
This axial force should vanish, and
therefore, the neutral plane should be
located such that ∫
.
To interpret this equation, consider Fig.
5.13. The distance y is measured from the
neutral axis. Let distance y’ be measured from an arbitrary axis from
which the neutral axis is located at a distance of . Then , and
the equation of equilibrium becomes
∫( )
,
67
Two things may be noted in Fig. 5.12. First, near the interface the value of
stress in the upper material is less than that in the lower material. This indicates
that the value of E for the upper material is less than that for the lower material.
Second, note that all the straight lines depicting the stresses in the various
materials originate from zero value at the neutral axis. Why?
or, ∫ ∫
,
or, ∫ ∫
.
We now consider the integral over the whole area as a sum of a number of
integrals, each over an area of uniform material.
Thus, ∫ ∑ ∫
∑ .
Similarly, ∫ ∑ ∫ ∑
, where
represents the location of the centroid of the ith area in coordinate
system. From these we get
∑
∑
(5.10)
This gives the location of the neutral axis within the section68
.
To obtain the moment curvature relation, we write the equilibrium
condition for the moments:
∫ ∫ (
)
∫
The last integral is again interpreted as the sum of integrals over areas of
different (homogeneous) materials to obtain ∑ . Then,
the curvature κ = 1/ρ can be seen as
∑ (5.11)
where Izz,i is the second moment of the area Ai about the neutral axis of
the section.
Once the curvature is known, we can calculate the strain as
68
It may be noted that in Eq. 5.10 the areas of different materials are weighted by
the elastic moduli of the materials. These happens because this relation is
obtained from the balance of force equation where forces are determined from
the stresses which are E times the strain. The strains, by themselves, are
geometric quantities.
A consequence of this is that the neutral plane shifts towards the area with the
larger modulus of elasticity.
Fig. 5.13
(a) (b) (c)
Fig. 5.12 (a) beam section (b) strain distribution
(c) stress distribution
80
∑ (5.12)
and
∑ (5.13)
where E is the elastic modulus of the
relevant material.
Example 5.4 Stresses in a sandwich beam
Consider a beam of sandwich construction
in which two steel plates are separated by
a block of lightweight rigid foam material
with a negligibly small elastic modulus
compared to that of steel (Fig. 5.14). Find
the stress distribution for a bending moment of 100 N.m.
Solution:
It is easy to see from the symmetry of the section that the neutral plane is
situated at the middle. We can also use Eq. 5.10 to obtain the location of
the centroid.
∑
∑
, where A1 refers to the
area of the lower steel plate with E1 = 200 GPa and = 10 mm, A2
refers to the area of foamy material with a negligibly small vale of E, and
A3 to the area of the upper plate with E3 = 200 GPa and .
Using these values, we get
( ) ( ) ( ) ( ) ( ) ( )
( ) ( ) ( ) ( )
0.40 m
The curvature is given by Eq. 5.11
∑
, E2 being negligibly small.
Here refer to the second moment of the three areas about the neutral
axis (passing through the middle of the section as shown above).
moment of the lower area about its own axis + area×
(distance between the neutral axis and the centroid of
area 1)2
= (0.08 m)×(0.02 m)3/12 + (0.08 m)×(0.02 m)×(0.04 m –
0.01 m)2
= 1.49×10‒6
m4.
Similarly, moment of the upper area about its own axis + area×
(distance between neutral axis and the centroid of area 3)2
= (0.08 m)×(0.02 m)3/12 + (0.08 m)×(0.02 m)×(0.04 m –
0.07 m)2
= 1.49×10‒6
m4.
Then,
( ) ( ) ( ) ( )
= 1.68×10‒4
m‒1
The value of the maximum compressive stress is then determined from
Eq. 5.9 with E = 200 GPa, and y = 0.04 m,
( )
( ) ( )
(1.68×10‒4
m‒1
)
= ‒1.34 ,
The minus sign indicating that it is a compressive stress. We can
similarly determine the maximum
tensile stress (at y = ‒ 0.04 m) s
+1.34 MPa.
The rigid foam serves the purpose of
shifting the two steel areas away from
the centroid increasing the
contribution of each area to Izz,
thereby increasing the stiffness of the
beam. If the foam was not separating the two steel plates, the total height
of the section would have been 40 mm and the value of Izz would have
been (0.04 m)×(0.04 m)3/12 = 0.213×10
‒6 m
4, much less than that of the
composite beam with the resulting decrease in beam stiffness, increase in
curvature and increase in the maximum value of stresses. It is always
Fig. 5.14 A sandwich beam
Fig. 5.15 The stress distribution in
sandwich beam
81
beneficial to keep the section areas far
away from the axis. It was for the same
reason that I-beam of Example 5.3 was
better than the rectangular section.
Example 5.5 Reinforced concrete beam
Reinforced concrete construction is a very
ingenious use of two materials with
complementary properties. Common concrete is a brittle material which
has good strength in compression (about
20 MPa). Structural steel on the other hand
has good strength a tension (about 200
MPa). All beams have compression on
one side and tension on the other. This
suggests that we combine the two
materials to produce beams in which steel
is loaded in tension while concrete is
loaded in compression.
Fig. 5.16 shows the section of such a
reinforced concrete beam. What is the maximum bending moment this
beam can transmit?
Solution:
Let us take the value of Ec, the elastic modulus of concrete as 20 GPa,
while that for steel, Es as 200 GPa.
We will use the following strategy to solve this problem:
1. Locate the neutral axis using Eq. 5.10.
2. Determine the stiffness of the beam using Eq. 5.11.
3. Assuming a bending moment Mb, calculate using Eq. 5.13 the
maximum compressive stress in concrete and maximum tensile
stress in steel.
4. Equate these stresses to the specified limiting stresses. The
minimum of the two maximum moments will be the answer to the
problem.
We first determine the location of the neutral axis for the section using
Eq. 5.10. Here, for steel: Es = 200 GPa, m, and As =
5×π×(0.020 m)2/4, and for concrete: Ec = 20 GPa, m, and Ac
= (0.450 m)×(0.200 m). Using these values in Eq. 5.10, we get
∑
∑
m.
Note that as expected, the stiffer material in the lower half of the section
brings the neutral axis down (from 225 mm for the concrete alone).
The stiffness of the composite beam is obtained from ∑ (refer Eq.
5.11). The values of Izz’s re obt ined by first ev lu ting the I’s bout the
centroidal axis of the concerned area and, then, transferring it to the
neutral axis using the parallel-axes theorem.
( )( )
( )( )(
)
m4
( ) 64
5 7
4 ( )
( )
( ) 5
m4
Therefore, the stiffness of the beam is ∑ =
( )( ) ( )( ) =
3.86×107 N.m
2,
And the curvature is
The maximum compressive load will occur in the top plane of the beam
which is (450 ‒ 205) mm w y from the neutr l pl ne. From Eq. 5.13,
( )( )
Pa, and
Fig. 5.16 Reinforced
concrete beam section
Fig. 5.17 Stress distribution
in a reinforced concrete beam
82
( )( )
Pa
For a maximum permissible compressive stress of 20 MPa in concrete,
the maximum permissible moment is given by , or
Mb = 157.6 kN.m. For a maximum tensile stress of 200 MPa in steel, the
maximum permissible moment is given by , or Mb
= 249 kN.m. The minimum of these two, then, is the permissible
maximum moment that this reinforced concrete beam can sustain.
Example 5.6 Force required to bend a strip
Consider a strip of length l, width
b and height h clamped to a block
with a circular arc surface of
radius R as shown in Fig. 5.18.
On application of a force P to the
free end, a length c of the strip
(AB) comes in contact with the
block. Find the force P.
Solution:
We are given that the length AB of
the strip has a constant radius of curvature. This implies that the bending
moment over this length is constant, which, in turn, implies that the shear
stress on this part of the strip vanishes and that there is no other loading
on this part. Let us consider the shape of the SFD of this strip. The SF
over the length AB is constant at zero. There is no load over the portion
BC. This implies that SF over this segment too is constant. This constant
SF will jump up through P at the end C because of the presence of a
concentrated load P (downwards) at that point.. But the shear force must
be zero after end C. This is possible only if the SF is constant at +P over
the segment BC. Since there no SF over AB, and the SF over BC must be
+P, there must be a concentrated reaction at point B where the strip loses
contact with the radius block. The resultant SFD must be as shown in
Fig. 5.19.
The BM at the free end C must be zero. The presence of a negative SF
over the length BC implies that the BM is increasing over this segment,
and therefore, it must be ‒Pd
at point B. The BM over
portion AB has, thus, a
constant value of ‒Pd. This
would require a clamping
moment of +Pd. The resultant
BMD must be as shown in
Fig. 5.19. It can be verified
from the loading diagram that
this indeed is in agreement
with the other loads on the
strip.
Now we are ready to evaluate the load P in terms of the given parameters.
We know the radius of curvature of the strip over the length AB s ‒R.
The negative sign arises from the fact that the beam is bending convex
upwards. Using Eq. 5.4, we get
( ), or
.
5.4 Stresses in beams carrying shear forces
We have so far considered the
case of a beam in pure bending
only. The only stresses that
exist in such a beam are tensile
stresses, termed as the bending
stresses because they arise from
bending of the beam. In a more
general case, there are other
stresses as well, notably shear stresses. To demonstrate the plausibility of
the presence of shear stresses, consider the simply-supported stack of
planks69
shown in Fig. 5.20. The planks will exhibit relative sliding as
shown. If these planks were glued together, they would tend to slide and
the glue will be in shear trying to hold the planks back from sliding. If it
were a solid beam, this would cause shear stresses to be present which
tend to hold the different layers together.
69
This stack of five planks will have five times the moment carrying capacity of
a single plank. But if we had used a beam of the combined thickness, the
moment carrying capacity would have been 25 times! Can you show this?
Fig. 5.20 Relative sliding in a stack of
planks acting as a beam
Fig. 5.18
Fig. 5.19
83
Consider next the simply-
supported beam loaded in
the middle as shown in
Fig. 5.21. The SFD and
BMD of the beam have
also been shown in the
figure. It is clear that the
beam will have shear
forces acting over its
entire length. The
presence of the shear
forces will cause the
bending moment to vary
along the length as
shown. In fact, this follows from the fact that the slope of the bending
moment line is equal to (negative of) the shear force value.
The presence of a positive bending moment will cause the beam to bend
with a positive curvature resulting in compressive stresses in the upper
part and tensile stresses in the lower part of the beam. But since the
moment varies along the length of the beam, the bending stresses (at the
same value of y) also varies with x. Thus, if
we take a slice of the beam (like the shaded
portion in Fig. 5.21), the bending stress
distributions on its two ends are entirely
different resulting in a mismatch of
horizontal forces.
This fact is illustrated by drawing a free
body diagram of this shaded portion as
shown in Fig. 5.22. The (compressive) bending stresses on the right end
vary linearly in the vertical direction. These would be given by equation
,
where y is measured from the neutral axis of the section. There are no
stresses on the left end since the bending moment there is zero. The
bending stresses alone then give rise to a net horizontal force to the left.
This force tends to slide this slice to the left which results in the
development of shear stresses on the bottom
surface of the slice acting towards right as
shown.
This shear is ηyx with a negative sign (using
the sign convention of stresses introduced in
Chapter 2) . We had seen earlier (Sec. 1.7)
that shear stresses occur in complementary
pairs: . Therefore, a stress component acts on the exposed
x-face of the element (Fig. 5.23). The forces due to these shear stresses
acting on this face give the resultant shear force V at the section.
5.5 Relating shear stresses to the shear force in a beam
The discussion above leads us to the strategy that we adopt to relate shear
stresses to the shear force in a beam. We take a slice of the beam of
length dx extending from a distance y (from the neutral axis) to the top
surface of the beam (see Fig. 5.24a). Let the bending moment on the left
face of this element be M, while that on the right face be M + dM (Fig.
5.24c).
The bending stresses due to these bending moments at the two locations, x
and x +dx (and vertical location y’ from the neutral axis) are then given
by:
( )
, and ( )
( )
The net axial
forces on the two
sections are:
∫
, and
∫( )
where the
integration is to
Fig. 5.21
Fig. 5.22 FBD of a slice of
the beam of Fig. 5.21
Fig. 5.23 Complementary
shear stress on the left face
Fig. 5.24 Bending stresses on an elemental slice of a beam
84
be carried out on area A’, which is the area of the elemental section from
y upwards. Note that at x, the positive ζ is directed in the negative x-
direction (the outward normal there being in the negative x-direction) and,
therefore, F,x (the force, by convention, being positive in positive
coordinate direction) is obtained as the negative of the integral of stresses.
However at x + dx, the positive stresses are in the positive coordinate
direction and, hence, F,x+dx is the integral of the stresses on that face.
The presence of a shear force on this element causes the bending
moments on the two sides of the element to be different, resulting in
different values of the axial forces on either side. The net axial force is
given by
.∫
/
where y’ is the distance measured from the neutral axis and, thus, can be
replaced with y. The integral above is the first moment of area A’ about
the neutral axis, where the area A’ is the area of the section above the
location where we need to determine the shear stress (see Fig. 5.23). This
is given the symbol Q.
(5.14)
This difference in axial forces is balanced by the shear stresses acting on
the bottom surface of the element (Fig. 5.24d). If we assume the average
stress on this surface to be ηyx (= ηxy), the net shear force on this face is
ηyx×(b×dx), where b is the width of the section at y. Since ηyx is positive in
the negative x-direction, this force is in the negative direction. Writing the
axial force equilibrium of the FBD of Fig. 5.24d, we get
( ) ,
or ( )
We replace dM by ‒Vdx (realizing from Eq. 4.2 that
) to obtain
( )
Thus, the average shear stress is given by
( ) ( )
(5.15)
Here V is the shear stress, Q is the first moment (about the neutral axis) of
the section area above y, b is the width of the section at location y, and Izz
is the second moment of the whole area. It can
be shown easily that we can write the following
expression for Q in terms of the distance of the
centroid of area A’ from the neutral axis (Fig.
5.25):
( ) ∫
(5.16)
The following examples illustrate the procedure
for calculating the shear stress distribution across beam sections.
Example 5.7 Shear stress distribution across a uniformly loaded cantilever beam
Consider a cantilever beam loaded uniformly with a load intensity of 100
N/m as shown in Fig. 5.26. The beam has a rectangular section of width
10 mm and depth 30 mm. Find the distribution of shear stresses at the root
section.
Solution:
We first determine the reaction at the built in support. By vertical force
balance the vertical reaction is determined to be 200 N upwards. To
determine the reaction moment at root, we replace the distributed load by
its statically-equivalent
concentrated load of 200 N
at the centroid of the
distributed load, which is
at 1 m point. The moment
balance equation then
gives the reaction moment
as 200 N.m counter-
clockwise.
To draw the FBD, we start
at zero. The shear force
jumps down 200 N due to
Fig. 5.25
Fig. 5.26 A uniformly loaded cantilever beam
and the corresponding SFD and BMD
85
the concentrated force at x = 0. Thereafter, the SFD increases at a
constant rate of 100 N/m due to the uniformly distributed load of the same
density, till it reaches the value of 0 at the free end of the beam.
To calculate the shear stress, we do not need to calculate the bending
moments. However, we do so here just to illustrate again the area method
of drawing the BMDs. After starting at 0, the BMD jumps down to 200
N.m because of the positive reaction moment of the same magnitude.
Then, due to a negative shear force which is constantly decreasing in
magnitude, the bending moment
increases with a linearly decreasing
rate, i.e., the BMD has a parabolic
shape as shown in Fig. 5.26. Total
change in BM (as per Eq. 4.2) over
the length of the beam is equal to the
area under the SF curve over the
same length. This is 200 N.m, and
therefore, the BM at the free end
turns out to be 0, as it should be.
The maximum shear force is V =
‒200 N nd occurs t the root of the be m. The she r stress t dist nce
y from the NA is given by Eq. 5.16 as ( )
. Because the section of
the beam is rectangular (b =10 mm, h = 30 mm), its Izz is given by bh3/12
or 2.25×10‒8
m4, and the NA is located at 0.015 m from the top. The
value of b, the width of the section at a distance y from NA is constant at
0.010 m. The value of Q is obtained from Eq. 5.16: ∫
.
Here A’ represents the area above the location y (shaded area in Fig.
5.26). Here ( ) , and therefore,
( )( ) .
/ (
) . The shear stress, then, is
( )
( ) ( )
( ) ( ) (
) .
It is a parabolic distribution with
the maximum at y = 0, i.e., at the
neutral axis, and going to zero at
the top and the bottom surfaces.
Fig. 5.27 shows graphically the shear stress distribution70
across the beam
section.
This shear distribution results in a similar shear strain distribution across
height of the beam. Fig. 5.28 shows an exaggerated view of the
deformation of the beam under the action of shear forces.
Example 5.8 Shear stress distribution on wide-flanged I-beam
Consider a simply-supported overhang beam with uniformly distributed
load as shown in Fig. 5.29. The beam section is a wide-flanged I-
section71
. Obtain the variation of shear stresses in the beam section.
Solution:
As with all statically-determinate beams, we start with the loading
diagram of the
beam, calculate
the reactions at
the support and
draw the SFD of
the beam using
the method of
areas. Because
of a uniformly
distributed load
of 500 N/m, the
SFD has a line
sloping up at the
same rate. But
70 Let us compare the magnitudes of the shear stresses with those of the bending
stresses in this simple case. The maximum bending stresses are of order ( ) , while the maximum shear stresses are of order . Therefore,
. The maximum value of Q in this case is (b.h/2).h/4, and so
. It is reasonable to suppose that M is of order V.L, where L is
the length of the beam, and therefore, . This ratio is small for
slender beams. 71
The horizontal portions away from the central axis are termed as flanges while
the central vertical portion of a beam is termed as web. A wide-flanged I-beam is
also termed as a W-beam
Fig. 5.27 Shear stress distribution on
a rectangular section
Fig. 5.29 A simply-supported overhang beam with uniformly
distributed load
Fig. 5.28 Distortion of a rectangular
beam due to a shear force
86
the presence of the two reactions (750 N each) makes the SF line jump
down by 750 N at the two supports. The resulting SFD is as shown.
The BMD has also been drawn in Fig. 5.29 even though we do not require
it for the purposes of this example.
The maximum positive shear force of 375 N magnitude occurs just before
the two supports, while the maximum negative magnitude occurs just
after the supports. The maximum shear stresses will also occur at these
same locations. We calculate the shear stresses using Eq. 5.15. We
require for this purpose the value of Izz. This is obtained by dividing the
section area into three rectangles A, B, and C, as shown in Fig. 5.30. The
symmetry of the section ensures that the centroid of the section is in the
middle.
We use the parallel axes theorem to calculate
Izz.
, ( ) - ( ) ,
or Izz =2.93×10‒7
m4.
To calculate the value of Q across the section,
first consider the shaded area at a distance y
from the NA as shown in Fig. 5.31a. The value
of Q for this is given by ( ) ( )( ), ( ) - or ( ) valid for y between
0.010 m to 0.020 m. Thus, the value of Q across the flange varies
parabolically from 6×10‒6
m3 at y = 0.01 m to 0 at y = 0.2 m.
For y between 0 and 0.010 m, the shaded area (Fig. 5.31b) is divided in
two parts. The contribution of the top part is clearly the value of Q for y =
0.01 m, and the contribution for the second part is (0.01 m –y)(0.010
m)×[y + (0.01 m –y)/2], or (0.5×10‒6
‒ 0.005y2) m
3. Thus, the value of Q
in the web is ( ) , which is again parabolic, with
a value of 8.5×10-6
m3 at y = 0 and 6×10
‒6 m
3 at y = 0.01 m. Fig. 5.32b
shows the variation of Q.
The shear stress ηxy can now be
determined from Eq. 5.15. At the
location of the maximum shear force
(= 375 N), the maximum shear occurs
at y = 0, and is given by ( ) ( )( ) )( ) .
The value at y =0.01 m is obtained
by using 6×10‒6
m3 for the value of
Q, and is obtained as 0.77 MPa.
In calculating this last value, we have used
0.01 as the value of b, the width of the section.
A value of 0.77 MPa is actually the value of
shear stress at a point slightly below y = 0.01
m where we can take the value of b to be 10
mm. At a point slightly above this point, the
width of the section suddenly increases by a
factor of 4 to 0.040 m and, therefore, there is a
discontinuity in the value of shear stress which
decreases by a factor of 4 to 0.19 MPa. This has been shown in Fig.
5.32c.
Fig. 5.33 shows the distribution of shear stress ηxy across the section. It
may be noted that the web of the section is the primary shear-bearing
element in a wide- flanged beam. The value of the stress ηxy in the flanges
is quite low.
5.6 Shear flow in beams
It was shown above that the shear stress ηxy in the flanges of the wide-flanged I-
beam of the previous
example is quite low. But
it can be shown that the
flanges carry ηxz as well.
To evaluate ηxz, consider
an area at one corner (at a
distance z from the
vertical axis of
symmetry) as shown in
Fig. 5.34. The FBD of
this area is also shown.
Take a small area element
dA in the back face of the section. Let this area be
located at a distance y from the NA. The tensile
stress acting on this area where the bending moment
Fig. 5.30 I-section divided up
in three rectangles
(a) (b)
Fig. 5.31
(a) (b) (c)
Fig. 5.32 (a) The I-section, (b) the
variation of Q, and (c) the
variation of the shear stresses η
across the section.
Fig. 5.33 Shear stress ηxy
distribution in an I-beam
Fig. 5.34 An element and its FBD to determine the
shear stress ηxz
Fig. 5.35 Shear flow in
an I-beam
87
is M c n be t ken to be ‒My/Izz, where Izz is the second moment of the section
re . The tot l force on this element is ‒(My/Izz).dA. The total force on the back
face is then the integral of this over the area of the face. We can , in a similar
fashion, calculate the force acting on the front face of the area. It will be exactly
the same, except that M will be replaced by M + dM, and that this force is
backwards. The net force due to bending stresses on the two faces is the
difference of the two, i.e., the integral over the area of (dM/Izz)ydA. The integral
of ydA is the first moment of area which has been given the symbol Q. Thus, the
net force due to bending stresses is QdM/Izz. The change in moment, as before,
can be replaced by ‒Vdx, where V is the shear force at the section.
This backward force is balanced by the shear force acting on the front
face (of area t.dx) of this element. If ηxz is the average shear stress on this
area
.
From this we obtain
(5.16)
This is same as Eq. 5.15 with section width b replaced with t, the
thickness of the flange.
It is convenient to use the concept of shear flow q first introduced in Sec.
3.7 as ∫
. Thus, both for flange as well as web, we can
write
(5.17)
Fig. 5.35 shows the shear
flow distribution for an I-
beam subject to a negative
shear force V. If the shear
force was positive, all the
arrows would have been
reversed. The shear flow in
the flanges starts at zero at the
tips and is maximum at the junctions with the web72
.
It is pertinent to point out here that the shear flow in bending has been
obtained from purely equilibrium considerations. We have not used any
other tool for these derivations.
Example 5.9 A built-up beam
Consider the built up beam shown in Fig. 5.36. It is held together with 10
mm bolts as shown. If the maximum shear force acting on the beam is 50
kN and the maximum shear stress a bolt can resist is 80 MPa, determine
the maximum spacing s between the bolts.
Solution:
To externalize the shear forces in the bolts, we consider the FBD of an
element of length dx as shown in Fig. 5.37. Because of the presence of
the shear force, the bending moments, and therefore, the bending stresses
on the two opposite faces of this
element are different. The
difference in the axial forces
because of this difference results
in a net force on the element due
to the bending stresses. This
force is resisted by the shear
action Fs,b in the bolts. But there
are two sides to this element.
The unbalanced force is, therefore, resisted by 2Fs,b.
The unbalanced force is determined by Eq. 5.14 as
Each bolt resists this unbalanced load for a length s of the beam, where s
is the distance between the bolts (i.e., the pitch).
.
72
The stress distributions at the junctions are quite complicated. It is for this
reason that the commercially available rolled-sections are provided with
generous fillets to avoid stress concentration.
Fig. 5.36 A built-up beam
Fig. 5.37
88
The value of Izz is evaluated by breaking up the beam section into a
difference of two areas: a rectangle 140 mm wide, 160 mm deep, from
which is subtracted a rectangle 120 mm wide, 140 mm deep. The value
of Izz is
( )( ) ( )( )
The first moment of the area of the face of the FBD about the NA is
obtained by multiplying the area (10 mm × 50 mm) by the distance of its
centroid from the neutr l xis (80 mm ‒ 5 mm). Thus, Q = 3.75×10‒5
m3.
The maximum shear stress in a bolt is prescribed as 80 MPa. Therefore,
maximum value of Fs,b is . ( )
/ ( ) . Using this
value in the equation above along with V = 50 kN, we get
( )( )
This gives a value of s as 0.136 m. Thus, the spacing between the bolts
should be less than 13.6 cm.
5.7 Shear centre
Let us next consider
beams with sections that
have symmetry only
about one axis, like a
channel section shown in
Fig. 5.38. Let the shear
force on the section be V.
We can easily find the
shear flow distribution
along the three legs of the section.
These are shown in Fig. 5.38a. The
shear flow in the flanges increases
from 0 at the tips to the maximum
at the junction with the web.
The maximum value of the shear flow can be determined from Eq. 5.17 as
VQ/Izz. The Q here is the first moment about neutral axis of the area of
the upper flange, which is (bt)h/2. The value of Izz is found by breaking
up the area into three parts, determining the I of each about its own
centroidal axis, and then transferring it to the neutral axis using the
parallel-axes theorem:
, ( ) - ( ) .
The maximum value of q is then Vbht/2Izz. The total horizontal shear
force F1 in the flange is the area under the shear flow triangle, which is
½qmax.b, or F1 = Vhb2t/4Izz, pointing to left. The lower flange has the
same value of shear force, except that it is pointed to the right. The shear
force in the web F2 is equal the sectional shear force V.
The resultant force on the section is now V, but the pair of forces F1
produces a couple. Fig. 5.38(c) shows a statically equivalent force system
in which the force V is displaced to a point O, a distance e to the left, with
, or . The point O is termed as the shear
centre of the section. As is shown in Fig. 5.39 the channel bends without
twisting only when the applied load passes through the shear centre.
5.8 Plastic deformations in beams
Consider a beam in pure bending
which is loaded beyond the onset of
yielding. Let the beam be made of a
perfectly elastic-perfectly plastic
material whose behaviour is as
depicted in Fig. 5.40. The yield stress
of the material is ζY, and the
corresponding strain is εY. As the
bending moment applied to the beam
increases the magnitude of the strain
at any point increases linearly with the bending moment. The strain for
any applied moment varies linearly with y according to Eq. 5.1:
(5.1)
(a) (b) (c)
Fig. 5.38 (a) shear flow distribution; (b) resultant
forces in the three legs of the section; (c) point of
action of the statically-equivalent shear force
(a) (b)
Fig. 5.39 (a) The channel twists while
bending when the load does not pass
through the shear centre b) The
channel bends without twisting when
the load acts through the shear centre.
Fig. 5.40
89
And as long as the strain
is less than the yield
strength value of εY, the
bending stress variation is
given by Eεxx, where E is
the elastic modulus of the
material. Under these
conditions, the stress
distribution is as shown
in Fig. 5.41a. The value of ρ is found by considerations of equilibrium, so
that the stresses are given by Eq. 5.5 as
.
This is valid as long as εmax < εY, and consequently, ζmax < ζY. The Value
of bending moment MY for which the maximum stress reaches the yield
strength value is obtained from Eq. 5.6 as ( )
, where h is the
height of the section.
For a rectangular b×h beam, this gives
(5.18)
For values of bending moment larger than MY, the material starts
deforming plastically at the either end. Though the strain distribution is
still linear, the bending stress in no longer linear with y. The value of the
stress acquires the value ζY at a value of y less than h/2 as shown in Fig.
5.41b and remains constant thereafter. If the radius of curvature is ρ for
this case, then ( ) , and ( ) till its value is ζY,
after which it remains constant at ζY. The value of y at which ζ first
becomes ζY is
. We denote
by yY. Thus, the beam is elastic
within the r nge ‒yY to +yY, and plastic outside this range. The value of ρ
is as yet undetermined. We evaluate the bending moment by integrating
ζdA over the whole area.
∫ ∫
∫ .
/
∫ ( )
or,
[
.
/ ]
[
.
/ ]
(5.19)
The value of yY is 0 when the plastic
region spans the whole depth of the beam.
The beam in this condition is resisting the
maximum possible moment it can resist.
Thus, the maximum bending moment
Mmax that the beam can support is obtained
by setting yY = 0 in Eq.5.19:
(5.20)
The value of ρ is easily determined in
terms of yY by noting that the strain at yY
is ‒ Y, so that
, or
.
Combining this with the fact that the
radius of curvature ρY at the point where the plastic deformation just starts
is given by
, we get
. Using this in Eq. 5.19, we get
[
.
/ ], for ρ < ρY. (5.21)
Fig. 5.41 shows the variation of bending moment with the radius of
curvature of the beam for a rectangular-section beam. The maximum
bending moment approaches a value 1.5 times MY asymptotically. The
ratio of the maximum bending moment to the yield bending moment
changes with the section shape. For circular sections, this ratio is 1.7, and
for thin-walled circular tubes it is about 1.3. For typical commercially
available I-beams, this ratio varies between 1.1 and 1.2.
5.9 Strain energy in bending
The expression for strain energy in a structure subject to arbitrary stresses
is given by Eq. 2.17 as
∫ ( )
(2.17)
where the integration is carried over the entire volume of the beam. For
the case of a beam in pure bending (no shear force and bending moment
constant over the entire length), there is only one stress, ζxx given by Eq.
5.5 as
. The strain energy for such a beam is, therefore
(a) (b) (c)
Fig. 5.41
Fig. 5.42 Variation of bending
moment with curvature in elastic-
plastic deformation of a
rectangular-section beam
90
∫
∫ .
/
.∬
/ ∫ .
/
(5.22)
For a uniform beam subject to a constant bending moment, this equation
reduces to
.
In a more general case when a beam is also subjected to transverse shear,
Eq. 2.17 gives the value of strain energy as:
∫ ( )
, or
∫ .
/
(5.23)
It was shown in Example 5.7 that the ratio of the maximum shear stress to
the maximum tensile stress in the case of a uniformly loaded cantilever
beam was . It can be shown that the same holds true to
almost all beams and loadings. This ratio is small for typical slender
beams. Since the stresses are squared in Eq. 5.23, the contribution of
shear stresses to the strain energy is quite small compared to that of the
bending (tensile) stresses and can, therefore, be safely neglected.
Example 5.10 Strain energy of a simply-supported beam
Consider the simply-supported
beam of length L loaded at the mid-
point as shown in Fig. 5.43. Find
the strain energy of the beam if the
section of the beam is rectangular
with depth h and width b.
Solution:
The reader can verify that the SFD
and the BMD of the beam are as
drawn in the figure. Since we need
to integrate the squares of shear stresses and bending stresses over the
length of the beam, let us express SF and BM as functions of the
longitudinal variable x.
It can be seen that we can write:
( )
for 0 < x < L/2,
for L/2 < x < L (a)
And ( )
for 0 < x < L/2,
(
) for L/2 < x < L
(b)
The contribution of bending stresses to the total energy is given by
∫
, where A is the cross-sectional area of the beam.
Expressing ζxx in terms of M(x), and replacing the value of M(x) using Eq.
b above, we get
∫ ( )
∫
∫
( )
,
And expressing Izz in terms of b and h, we get
It can be verified that this has the dimensions of energy. Please note that
we have not included the energy due to shear which is an order of
magnitude smaller for slender beams.
Summary
A beam is a slender member which carries transverse loads or
moments which tend to bend it.
o A beam resists bending moments by developing axial
stresses. These stresses arise because curving of a beam
necessarily implies contraction of material on one side
and elongation on the other side.
o There exists a plane within the beam which undergoes
neither contraction nor extension. This is termed as the
neutral plane. The trace of the neutral plane within a
section of the beam is termed as the neutral axis.
To obtain a relation between the curvature of the beam, the
bending stresses and the moment causing the bending we adopt
the following strategy:
Fig. 5.43
91
o We first use the geometry of bending in the case of pure
bending to relate strains to the distance from the neutral
plane.
o We convert the strains to stresses using the elastic
modulus.
o We next use the equilibrium conditions. The balance of
axial forces gives us the location of the neutral axis as
passing through the centroid of the section area. The
balance of moments then relates the curvature in the
beam to the bending moment acting on it. Eq. 5.6 gives
the relation between the moment Mb, the radius of
curvature ρ, the strain εxx, and the bending stress ζxx.
The bending stresses vary linearly with distance from the neutral
axis, zero on the axis and increasing as we move away. There is
compression on one side and tension on the other side of the
neutral axis.
We introduce the concept of bending rigidity as the curvature
produced per unit bending moment. The bending rigidity for a
uniform beam in pure bending is seen to be the product of the
elastic modulus E and the second moment Izz of the cross-
sectional area about a transverse neutral (centroidal) axis. The
rigidity of a beam increases as the third power of the depth of a
beam.
It was shown through some solved examples that for the beam
sections of the same areas the beam with more material away
from the centroid is more rigid.
The method for handling of composite beams was developed
following the same process as for simple beams. It was shown
that strains in composite beams are determined by geometric
considerations alone as in the case of simple beams, and are
continuous across different materials. The stresses, however, are
not continuous. It was shown that the location of the neutral axis
is obtained by a relation that weights the areas of different
materials with their elastic moduli (Eq. 5.10). The flexural
relation is the same as that for a simple beam except that the
bending rigidity is now replaced by the sum of the bending
rigidity of the constituent areas. The process was explained using
the example of a steel-reinforced concrete beam which exploits
beautifully the differing capabilities of the two materials.
The presence of shear forces causes the variation of bending
moments along the length of a beam resulting in an unbalance of
axial forces. This gives rise to shear stresses ηzx or ηxz. The shear
stresses are given by Eq. 5.15 as ( ) ( ) ,
where Q is the first moment of the area of the section above the
location y, and b is the width of the section at y. The shear stress
is the maximum at the neutral axis and decreases towards either
end of the section.
The shear stresses in slender beams are an order of magnitude
smaller than the bending stresses.
It is convenient to use the concept of shear flow q as
∫
. Thus, both for flange as well as web, we can write
.
The concept of shear centre was introduced as a point within the
beam section through which the external load must pass for the
beam to bend without twisting. It is the point where the single
shear force which is statically equivalent to the sectional shear
distribution must be applied.
The strain energy in slender beams is dominated by the energy
due to bending stresses and is given by ∫ .
/
.
92
93
Appendix B Properties of Areas
B.1 First moments of area and centroid
Consider an area as shown in Fig. B.1. Two first moments of areas are
defined: one about the x- axis, and the other about the y- axis.
∫
, and ∫
(B.1)
The values of Qx and Qy depend on the location of the origin O.
The centroid of the area is defined as the
location of the origin such that Qx and Qy
vanish. We can use this property to determine
the location of the centroid.
Let the coordinate of the origin in the given
coordinate system be xc and yc. We calculate the
first moment of area about this point. The
distances y and x in Eq. B.1 are the replaced by
(y – yc) and (x – xc), respectively:
∫ ( ) , or
∫ ∫
, or
∫
(B.2)
And similarly, ∫
(B.3)
Example B.1 Centroid of a T-section
Consider the T-section shown in Fig. B.2.
Find the location of the centroid.
Solution:
The x location of the centroid is
immediately obtained by using symmetry.
Thus, xc = 2.5 units. The y-coordinate of
the centroid can be obtained by using Eq.
B.3.
We introduce here a very convenient
method for determining the centroid of areas that are made up of simple
areas. Thus, we divide the T-section in to two rectangular areas, a 1×4
unit area labelled A, and a 4×1area labelled B. We know that centroid of
area A is located at its mid-point, i.e., at y = 4.5 units. The centroid of
area B is located at its mid-point, i.e., at y = 2.0 units. The location of the
centroid of the composite area is given by
(∑ ) ∑ (B.4)
Using this formula, we get
( )
units
The location of the centroid is shown in the figure. The centroid is
located nearer the top since the area is top heavy.
B.2 Second moments of area
A second moment of area is a moment in which two lengths are used. We
define three second moments73
:
73
The nomenclature of the second moments has two indices, each indicating the
axis from which the distance is taken. Thus, Izz uses the distance y from the z
axis twice, Iyy uses the distance z from the y axis twice, and Iyz uses the distance y
from the z axis as well as the distance z from the y axis. This last is also called a
cross moment of area.
The polar moment of area used in Chapter 3 is also a second moment where the
distance of the area is measured from the polar axis, i.e., the axis normal to the
area. It will be labeled Ixx in the convention used here:
Fig. A.1
Fig. A.2 T-section
94
∫
; ∫
, and ∫
(B.5)
The dimensions of these second moments are L4, and its SI units are m
4.
Example B.2 Second moment of a rectangular section
Determine the second moment of area of the rectangular section shown in
Fig. B.3 about its centroidal axis.
Solution:
The centroid of this symmetric section obviously
lies at the middle of the area. We take the
coordinate axes with the centroid as the origin.
Let us take a rectangular elemental area of
dimensions δy and δz. Then, by Eq. B.5:
∫
∫ ∫
Carrying out the indicated integrations, we get:
(B.6)
Similarly, .
We next calculate these moments about the y-axis
that coincides with the bottom plane of the
section.
∫
∫ ∫
four times the value when the x-axis passes through the centroid. Clearly,
the value depends on the location of the x-axis. We shall show below that
that the value with the x-axis passing
through the centroid is the minimum of all
possible values.
Example B.3 Second moment of a hollow square section
Determine the second moment of area of
the hollow square section shown in Fig. B.5
about its centroidal axis.
Solution:
We can, using symmetry, see that the centroid will be at the centre of the
section.
∫
∫
∫
Recognizing that the first integral is the Ixx of the outer square (=
a.a3/12), and the second integral is the Ixx of the inner square (= b.b
3/12),
we get the Ixx of the section as ( ) .
This is a general method of determining the moments of composite
sections.
B.3 Parallel axes theorem
We now introduce a very important property of the second moments of
area which is very handy in calculations of
the moments. Refer to Fig. B.6. Consider
First a coordinate system x-y with the
origin O and x-axis passing through the
centroid. The moment in this coordinate
system is given by
∫
Next consider an arbitrary coordinate
system x’-y’ with the x’-axis located a distance d away from the
centroidal axis. The second moment in this new system is
∫
∫ ( ) ∫ ( )
or, ∫
∫ ∫
Since y is measured from the centroidal axes, ∫
is immediately
seen as Ixx, ∫
is the first moment of area about a centroidal axis and
hence zero, and ∫
is nothing but the total area A. This gives:
(B.7)
Fig. A.3 A
rectangular section
Fig. A.4
Fig. A.6
Fig. A.5 Hollow square section
95
This is known as the parallel axes theorem. The second moment about an
axis a distance d away from the centroid is equal to the moment about the
centroidal axes plus area times the square of d.
One can immediately see from this theorem that the second moment about
the centroidal axis is the minimum. This theorem provides a very
convenient tool to obtain moment of inertia of a composite area as is
illustrated below.
Example B.4 Second moment of a T-section about the centroidal axis
Consider the T-section of Example B.1. Determine its second moment
about the centroidal axis.
Solution:
The centroid of the section was determined in Example B.1 to be located
on the centre line a distance 3.25 units up
from the bottom of the T. The origin of
the axes is now taken at this location as
shown.
We split up the area of the section into two
rectangles A and B as before (Fig. B.7).
We can calculate the second moment of
area of A about its own centroidal axes (at
a distance of 4.5 units from the bottom) using Eq. B.6 as (5×13)/12 =
0.417. We then use the parallel axis theorem (Eq. B.7) to shift the axis to
3.25 units above the bottom (from 4.5 units above the bottom. Thus, the
shift distance d is 4.5 – 3.25 = 1.25, and the value of becomes
0.417 + (Area = 5×1)×(1.25)2 = 8.23 units. Similarly, the second
moment of area B about its own centroid (which is 2 units from the
bottom) is 1×43/12 = 5.33 units. When we transfer it to the centroid of the
whole section which is a distance d (= 3.25-2.0 = 1.25 units) away, it
becomes (Area = 5×1)×(1.25)2 = 13.14 units. Thus, the
net moment is units.
Example B.5 Second moment of an angle section about the centroidal axis
Consider the angle section shown in Fig.
B.8. Determine its second moment about
the centroidal axis.
Solution:
We first determine the location of the
centroid of the section. We work with the
division of the section in two rectangles A
and B as shown. The area of A is 400 mm2
and its centroid is at (5 mm, 30 mm) and
the area of B is 500 mm2 and its centroid is
at (25 mm, 5 mm). The coordinates of the
centroid are:
∑
∑
mm,
and ∑
∑
mm.
The location of the centroid has been marked on the figure.
Here, too, we calculate the second moment using the parallel axis
theorem. We first calculate the moments of the two areas about their own
centroidal axis, and the transfer them to the centroidal axis of the
composite section:
,( ) ( ) -
0
( ) 1
0
( ) 1 mm
4.
Fig. A.7
Fig. A.8 An angle section
96
Thus, the second moment of this angle section about the centroidal axis
has been determined as 2.99×10÷7
m4.
B.4 Perpendicular axes theorem
Consider an area as shown in Fig. B.8. Let us consider a right-handed
triad of coordinate axes with x- and y- axes within the plane of the section
and the z-axis pointing outwards from the paper. Using the definitions of
the polar moment of area ∫
. But . Therefore,
∫
∫
∫
. Thus,
(B.8)
This is the perpendicular axes theorem which states that the polar moment
of inertia of a section is the sum of the second moment of the area about
two perpendicular axes within the plane of the area.
Example B.6 Second moment of a circular section
Determine the second moment of a circular
section.
Solution:
Consider the circular section of Fig. B.9. We
need to determine ∫
. Direct
determination of this integral is not easy.
Therefore, we use the perpendicular axes
theorem (Eq. B.8):
The symmetry of the circular section gives us ensures that the moments
and are equal. Thus, . The polar moment had been
evaluated in Sec. 3.3 as
(Eq. 3.6). Therefore,
Fig. A.8
Fig. A.9 A circular section
Table A.1 Properties of some areas
Geometry Area Vertical
location
of
centroid
Second moment of
area about
centroidal axis
Rectangle
bh h/2 bh3/12
Isosceles triangle
bh/2 h/3 bh3/36
Circle
πD2/4 D/2 πD
4/64
I-beam
[2k1+(1‒2k1)] bh h/2
,(
) (
)-
97
Index area method, 64
area, cross moment of, 93
area, first moment, 84, 93
area, polar moment, 43
area, second moment, 43, 93
axis, neutral, 73, 91
beam, 56
beam supports, idealized, 58
beam, built-up, 87
beam, composite, 78
beam, plastic deformations in,
89
beam, sandwich, 80
beam, shear stresses, 82
beam, simply-supported, 58
beams, shear flow, 87
bearing stress, 5
bending moment, 7, 56
bending rigidity, 74, 91
bending strain, 73
bending stress, 73
bending, pure, 71
bending, strain energy, 90
built-in support, 58
built-up beam, 87
cable in a sleeve, 45
Castigliano theorem, 33, 40
centroid, 74, 93
coefficient of thermal expansion,
27
coil spring, 53
complementary planes, 12
composite beam, 78
composite shaft, 49
concrete, pre-stressed, 32
concrete, reinforced, 81
cross moment of area, 93
deformation, plastic, 29
distributed load, 59
elastic limit, 29
elastic modulus, 5, 17
electroplating, residual stresses
in, 27
energy methods, 33
energy, strain, 33
first moment of area, 84, 93
gauge length, 29
generalized Hooke law, 24
Hooke law, generalized, 24
Hooke, Robert, 5
idealized beam supports, 58
idealized stress-strain curves, 30
key, 10
keyway, 10
limit analysis, 52
limit load, 52
linear elastic range, 29
load, distributed, 59
load, point, 58
loading density, 59
method of sections, 61
moment, bending, 7, 56
moment, twisting, 6
necking, 30
neutral axis, 73, 91
neutral plane, 72, 91
normal stress, 11
parallel axes theorem, 95
Pascal, 7
permanent set, 29
perpendicular axes theorem, 96
pinned support, 58
plane, neutral, 72, 91
planes, complementary, 12
plastic deformation, 29
plastic deformation in torsion,
51
plastic deformations in beams,
89
point load, 58
Poisson ratio, 23
polar moment of area, 43
pre-stressing, 32
proportional limit, 29
radius of curvature, 73
rectangular section, second
moment of, 94
reinforced concrete beam, 81
right-hand thumb rule, 44
rigidity, bending, 74, 91
rigidity, torsional, 43
roller support, 58
sandwich beam, 80
second moment of area, 43, 93
second moment of rectangular
section, 94
shaft, composite, 49
shaft, statically indeterminate,
47, 54
shaft, tapered, 45
shear centre, 88
shear flow, 50
shear flow, beams, 87
shear force, 56
shear modulus, 26
shear strain, 25
shear strain in torsion, 42
shear stress, 6
shear stress in torsion, 42
shear stresses in beams, 82
shrink fit, 28
sign convention for shear force
and bending moment, 57
simply-supported beam, 58
spring, kinky, 22
St. Venant principle, 8
statically equivalent loads, 8
statically indeterminate
problems, 20, 37
statically indeterminate shaft,
47, 54
strain, 5
strain energy, 33
strain energy, bending, 90
strain energy, elastic body, 38
strain energy, torsion, 53
strain hardening, 30
strain, bending, 73
strain, shear, 25
strength, yield, 29
stress, 5
stress at a point, 7
stress on oblique planes, 11
stress, bearing, 5
stress, bending, 73
stress, double-index notation, 12
stress, shear, 6
stress, sign convention, 13
stresses, pressure vessel, 14
support, built-in, 58
support, hinged, 9
support, pinned, 58
support, roller, 9
symmetry arguments, 15
tensile test, 28
thermal expansion, coefficient
of, 27
thermal strains, 27
thermal stresses, 27
torsion, 41
torsion bar, 41
98
torsion moment diagram, 44
torsion, plastic deformation, 51
torsion, strain energy, 53
torsional rigidity, 43
torsional strain, 42
torsional stress, 42
twisting moment, 6
twisting moment diagram, 44
two-force member, 9, 10
ultimate stress, 30
unit force method, 35
vibration isolator, 26
yield point, 29
yield strength, 29