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Stability Of Structures: Continuous Models
Transcript of Stability Of Structures: Continuous Models
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18Stability OfStructures:
Continuous Models
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Lecture 18: STABILITY OF STRUCTURES: CONTINUOUS MODELS 182
TABLE OF CONTENTS
Page
18.1. Example 1: The Euler Column 18318.1.1. Critical Load Analysis . . . . . . . . . . . . . . 184
18.1.2. Linearization Limitations . . . . . . . . . . . . . 185
18.1.3. Reformulation as Eigenproblem . . . . . . . . . . . 186
18.2. The Fixed-Pinned Column 186
18.2.1. Critical Load Analysis . . . . . . . . . . . . . . 186
18.3. Elastically Restrained Column 188
18.3.1. Problem Description . . . . . . . . . . . . . . . 188
18.3.2. Critical Load Analysis . . . . . . . . . . . . . . 188
18.3.3. Equivalent Spring Constant . . . . . . . . . . . . . 1810
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183 18.1 EXAMPLE 1: THE EULER COLUMN
This Lecture focuses on buckling analysis ofcontinuous modelsof elastic systems. This process
leads to ordinary or partial differential equations. Those can be solved in closed form only for simple
1D structures, such as prismatic columns treated by linearized prebuckling (LPB).
Despite limitations in terms of obtaining analytical solutions, such problems are important for dis-
playing key intrisic features of continuous models. For example, the associated eigenproblem has
an infinite (but denumerable) set of eigenvalues, meaning an infinite number of critical loads. (Thisshould not be surprising, since continuous models have an infinite number of degrees of freedom.)
Of these, the lowest buckling load is of primary interest to designers.
We illustrate the treatmentof continuous modelsusing viaseveralexamples involving elastic columns
with simple boundary conditions. All of the examples have closed form solutions.
18.1. Example 1: The Euler Column
xx
y yy
v(x)
P P
P
B
M(x) =P v(+ as drawn)
P
X X'
v(x)
X'x
X
constantEI
P
B
X
(a) (b) (c)
elastic
AA A
Lassumed
buckled shape
Figure18.1. The Euler column: (a) problem definition; (b) FBD of whole column assuming a
buckled shapev(x)with its amplitude exaggerated for visibility; (c) FBD at distancexfrom top.
The Euler column is shown in Figure 18.1(a). It is a homogeneous, prismatric, elastic column pinned
(hinged, simply supported) at both ends A and B, and subjected to axial loadP . The elastic modulus
isE. Reference axes are chosen as follows:x is longitudinal, with origin at end A;zis normal to the
plane of thefigure and selected so thatI= Izzis theminimumsecond order of inertia of the columncross section aboutz; finallyy lies in the plane of the figure. For example, if the cross section is a
solid rectangle of widthband thicknesst
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185 18.1 EXAMPLE 1: THE EULER COLUMN
are L = n , in which n= 1, 2, . . .is a positive integer. Square both sides for convenience:2L2 = n2 2, replace2 by P/(E I), solve for Pand tag those loads as critical:
Pcr,n=n2 2E I
L2 , n= 1, 2, . . . (18.7)
As can be observed, there is an infinite number of critical loads. These are the nontrivial solutions
of the characteristic equation (18.5). The lowest one is associated with n= 1:
Pcr,1= Pcr= 2E I
L2 . (18.8)
This is called theEuler critical load.
Mode shape 1(n=1)
P = P =
Mode shape 2(n=2)
Mode shape 3(n=3)
cr cr1 L
E I2
2 P =cr2 L
4 E I2
2 P =cr3 L
9 E I2
2
L
L/2
L/2
L/3
L/3
L/3
Figure18.2. First three buckling mode shapes for the Euler column.
The buckling mode shapes associated with the set of critical loads (18.7) are
vcr,n(x) = Bsinnx
L. (18.9)
Ifn= 1 the mode shape is a half sine wave, similar to that drawn in Figure 18.1(c). Ifn= 2 we geta complete sine wave, ifn= 3, one-and-a-half sine wave, etc. These buckling shapes are drawn forn= 1, 2, 3 in Figure 18.2.
18.1.2. Linearization Limitations
TheLPBassumption does yields thecritical loads,but also bringsabout thefollowing inconsistencies,
some of which have an air of paradox.
The foregoing solution says nothingabout the amplitudeof the buckling modes (18.8) in termsof the data. This is a consequence of the LPB assumptions, which led to a simple linear ODE but
filters thaat information. Determination of thispostbucklingbehavior is quite involved, since it
requires solving a nonlinear ODE in terms of elliptic functions. Such analysis shows that the
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Lecture 18: STABILITY OF STRUCTURES: CONTINUOUS MODELS 186
buckled columncontiinues to take up on increasing load, albeit very slowly, as long as it remains
elastic.
Differentiating (18.7) three times gives a nonzero transverse shear load Vy (x)= E I Bv cr1=E I( 3/L3)Bcos(x/L). Evaluation at x=0 or x= Lgives a nonzero transverse shearforce whereas Figure 18.1(b) shows zero horizontal reactions there. A similar inconsistency
arises if one differentiates four times. This gives a nonzero lateral load p(x)but no such loadexists. Thisparadoxindicates that the sine-wave result must be corrected once the buckling
mode amplitude becomesfinite.
The analysis does not take into account imperfections such an initially crooked column, or axialload eccentricity. Such an analysis is beyond the level of this course, but one basic result is used
in the justification of theSouthwell plotexperimental procedure described in Lecture 19.
18.1.3. Reformulation as Eigenproblem
Lecture 17 emphasized that a discrete stability problem handled through the LPB assumptions may
be presented as a matrix eigenproblem. This is also the case for the linearized continuous problem,
but it requires a reformulation. For the Euler column, the two end boundary conditionsv(0) = 0 andv(L) = 0 may be written conjointly as
1 0
cos L sin L
A
B
=
0
0
. (18.10)
This is a matrix eigenproblem in = P/(E I), but note that (unlike the discrete case) this variabledoes not appear linearly. For a nontrivial solution, meaning that Aand B are not both zero, the
determinant of the matrix on the left side must vanish. This leads to the condition
sin L= 0 (18.11)which agrees with that previously found from the characteristic equation (18.5). This reformulation
becomes useful in more complicated cases.
18.2. The Fixed-Pinned Column
As second example we consider the configuration shown in Figure 18.3(a). The buckled column is
drawn in Figure 18.3(b) in a deflected position. The most notable difference with respect tp the Euler
column of Figure 18.1(a) is the presence of additional reaction forces: the lateral reactions RAand
RB , and thefixed end momentMB . These are positive as shown in Figure 18.3(b).
18.2.1. Critical Load Analysis
Equilibrium ofyforces in Figure 18.3(b) gives RA= RB . Equilibrium of moments taken withrespect to either A or B yields MB= RA/L. Next consider the FBD of the portion AX shown inFigure 18.3(c). Equilibrium with respect to Xgives the non-homogeneous ODE
E Iv (x) + Pv(x) = RAx=MBx
L. (18.12)
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187 18.2 THE FIXED-PINNED COLUMN
xx
y yy
v(x)
P P
PB
B
M(x)(+ as drawn)
P
X X'
v(x)
X'
X
constantEI
P
B
X
(a) (b) (c)
elastic
A
A A
Lassumed
buckled shape
RA
AR = RB
M
x
RA
RA
Figure18.3. Columnfixed at one end and simply supported (hinged, pinned) at the other.
The LHS is the same as in (18.1), but the RHS is no longer zero. Dividing through byE Iand setting
2 = P/(E I)gives after some manipulations
v(x) + 2 v(x) = 2MBx
P L. (18.13)
The general solution is the sum of the homogeneous solutionvH(x) = Asin x +Bcos xand theparticular solutionv P (x) = MBx/(P L):
v(x)
=Asin x
+Bcos x
+
MBx
P L
. (18.14)
The three kinemtic BCs arevA= v(0) = 0,vB (0) = v(L) = 0 andv B= v(L) = 0. These providethree equations:
B + MBL
= 0, A sin L +Bcos L + 0, A l MBP L
= 0. (18.15)
Solving these equations simultaneously one obtains the characteristic equation
tan L= L . (18.16)
The samllest roots of this transcendental equation, to 4 places, is L=
4.493. The corresponding
critical load is
Pcr=20.19E I
L2 . (18.17)
Since 20.19 2.05 2 this critical load is approximately twice that of the Euler column. Thusfixingone end has substantially increased the critical load.
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Lecture 18: STABILITY OF STRUCTURES: CONTINUOUS MODELS 188
x
x
y,vy
v(x)
PP P
P
L
RA
RA
RA
M = kB
B
B
AM(x)=P v+R xx
P
P
RA
(a) (b) (c) (d)
k
AA
CB
Belastic beam
beam-columnX
Figure18.4. Column with elastic restraint: a torsional spring, at end B.
18.3. Elastically Restrained Column
The title configuration is of interest because it covers the three boundary condition cases tested in the
Column Buckling Lab.as special cases.
18.3.1. Problem Description
Consider the modification of the classical Euler column pictured in Figure 18.4(a). The column is
simply supported (pinned) at both ends A and B, and axially loaded by P . The rotation atBis further
restrained by a torsional spring with stiffness k.
ColumnABhas lengthLand constant flexural rigidityE I, in whichI Izzis the minimum momentof inertia of the cross section that controls buckling. (For a rectangular cross section of width bandthickness t < b,I= Izz= b t3/12.) The column is simply supported (pinned) at both endsAandB,and axially loaded by P . The rotation atBis further restrained by a torsional spring with stiffness k.
Selectxas shown and consider the buckling shape v(x)sketched in Figure A.1(b). The end rotation
at Bis B= v(L), positive CCW. The spring at Bapplies a restoring end moment MB= kB .For convenience in obtaining dimensionless equations we define
k= E IL
(18.18)
where is a numerical coefficient. If= 0 the problem reduces to that of the classical Euler column,whereas if we obtain the case of a column simply supported at Aandfixed (clamped) atB.
18.3.2. Critical Load Analysis
The FBD of the complete column is shown in Figure 18.4(b). Taking moments with respect toBone
finds that
RA= MB /L= kB /L= E IB /L2. (18.19)
Prior to Fall 2010, this used to be Experimental Lab 3. It is now aLab-Homework, meaning that the results are presented
as part of an assigned Homework rather than a formal Lab Report.
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189 18.3 ELASTICALLY RESTRAINED COLUMN
Now cut the column at section Xat distancexas sketched in Figure 18.4(c). Moment equilibrium
with respect toXyields the second order differential equation
E Iv + Pv= RAx= kBx
L= E IBx
L2 , (18.20)
which results from equating the bending moment M(x) = E Iv to Pv +RAx . Dividing throughbyE Iand calling2 = P/E Iproduces the canonical form
v + 2 v= BxL2
. (18.21)
The general solution of (18.21) is the sum of the homogeneous and particular solutions:
v(x) = C1sin x + C2cos x Bx
2L2. (18.22)
Sincev(0)= 0, C2= 0. The rotation is (x)= v(x)= C1 cos x B /(2L2). Evaluatingthis atx= LyieldsB= (L) = C1 cos L B /(
2
L
2
), from which we can solve for the endrotation:
B= C13L2
+ 2L2cos L . (18.23)
Inserting this into the solution (18.22) with C2=0 gives v(x)= C1sin x C1xcos L/(+2L2). Applying now the second boundary condition: v(L) = 0, furnishes the stability equation
v(L) = C1
sin L L + 2L2cos L
= 0. (18.24)
For buckling to occur, C1=0, and the expression in parentheses in (18.24) must vanish. Calling=
L, which is also a dimensionless variable, we obtain the trascendental equation
tan = 2 + (18.25)
For a given 0 we seek the solutioncr >0 of (18.25) closest to zero. If= 0 there is no closedform solution and it is better to proceed numerically, using for example a Newton solver. It is easily
shown that for= [0, ], cr
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Lecture 18: STABILITY OF STRUCTURES: CONTINUOUS MODELS 1810
The critical load Pcrand the effective lengthLe(tabulated above) are
Pcr=2crE I
L2 =
2E I
L2e, Le=
crL (18.26)
This solution also applies to the buckling of a column AB rigidly connected at B to an elastic
beam BC, as illustrated in Figure 1(d). This is actually one of the configurations to be tested in
Lab 3. All that is needed is to work out the appropriate value of k= MBCB /BCB obtained from amoment-deflection analysis of beamBCsubjected to an applied end momentMBCB = MB .
18.3.3. Equivalent Spring Constant
Suppose the restraining elastic beamBCinFigureA.1has lengthLr= LBC, modulusErandmomentof inertia Iraboutz. Assume a simply support condition at C. Under an end moment MBapplied
as pictured in Figure 18.4(d), the restraining beam deflects by vr= MBxr(L2rx2r)/(6ErIrLr),in which xris the distance from C. The end rotation isB
= (dvr/dx)
|xr
Lr
=MBLr/(3ErIr),
whence the equivalent torsional spring stiffness is k= MB /B is 3ErIr/Lr. Comparing with (1)shows that= 3(L/Lr)(ErIr)/(E I). If the restraining beam is fabricated of the same material andhas the same cross section dimensions of the beam-column, as is the case in Lab 3, Er= E,Ir= I,and= 3L/Lr.
E. M. Popov,Engineering Mechanics of Solids, Prentice Hall, NJ, 1999, case 5 of Table 10, p. 853.
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