03 One Dimensional Problems
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Transcript of 03 One Dimensional Problems
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One Dimensional Problems
Lecture Notes
Dr Mohd Afendi
Universiti Malaysia Perlis
ENT467 Finite Element Analysis
Chapter 3
2
Introduction
Total potential energy, stress-strain and strain-displacement relationships are used in developing
FEM for one dimensional problems. Same basic procedure for two- and three-
dimensional problems.
For one-dimensional problems, the vector is afunction ofx.
u=u(x), =(x), = (x), T=T(x), f=f(x)
Stress-strain and strain-displacement relations are:
=du
Edx
3
Introduction
Three types of loading:
Body force, f (self weight due to gravity)
Traction, T (frictional resistance, viscous drag)
Point load, Pi.
Figure 1
4
Finite Element Modelling
In one dimensional problems, every node ispermitted to displace only in the xdirection.
Each node has only one degree of freedom (dof).
Element division, numbering scheme.
Figure 2
5
Finite Element Modelling
Displacement along each dof is denoted by Q=[Q1,
Q2,,Qn]T
and global node vector, F=[F1,,Fn]T
.
Figure 3
6
Finite Element Modelling
Global numbering.
Element connectivity.
Figure 4
Figure 5
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Coordinates andShape Functions
Natural or intrinsic coordinate system, :
Figure 6
12 1
2( ) 1x x
x x
8
Coordinates andShape Functions
The unknown displacement field within an elementwill be interpolated by a linear distribution.
Approximation becomes more accurate if moreelements are considered.
Figure 7
9
Coordinates andShape Functions
Linear shape function:
Linear displacement:
where q1 and q2 are nodal displacement
In matrix notation: u= Nq N = [N1, N2]T and q = [q1, q2]T
1 2
1 1( ) , ( )
2 2N N
1 1 2 2u N q N q
10
Coordinates andShape Functions
Stress derivation.
Strain-displacement relation.
Also, since:
We have:
chain rule
du du d
dx d dx
differentiate1
2 1 2 1
2 2( ) 1
dx x
x x dx x x
1 1 2 2 1 2
1 1
2 2u N q N q q q
1 2
2
du q q
d
11
Coordinates andShape Functions
Then, substitute into previous equation:
This equation can be written as:
= Bq
matrix B is the element strain-displacement matrix.
The stress, from Hookes law, is:
=EBq
1 22 1
1( )q qx x
2 1
1= [ 1 1]
x x
B
12
Example 3.1
Referring to the following figure:
(a) Evaluate , N1and N2at point P.
(b) Ifq1= 0.003 in and q2= -0.005 in,determine the value of the displacement qatpoint P
x2 = 36 inx = 24 inx1 = 20 in
21 P
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Example 3.1
Answer:
Using Eq. 3.4 the coordinate of P is given by:
Using Eq. 3.7a we get:
1 2
x1 = 20 in
P
x2 = 36 in
x = 24 in
5.01)2024(16
2p 25.075.0 21 NandN
inup 001.0)005.0(25.0)003.0(75.0 14
Problem 3.1
Consider the bar in Fig. 3.1. Cross-section Ae= 1.2 in2, and
Young modulus E = 30x106 psi. If q1= 0.02 and q2 = 0.025
in determine the following: The displacement at point P
The strain and stress
The element stiffness matrix
The strain energy in the element
1 2
x1 = 15 in
P
x2 = 23 in
x = 20 in
Figure 3.1
15
Problem 3.1
Answer
(a) q=0.023125 in
(b) = 0.000625 and = 18750 psi
16
Potential-Energy Approach
General expression for potential-energy approach:
Since the continuum has been discretized into finiteelements, the expression for becomes:
T T T1 u f u T u P2
Ti iV V S
i
dV dV dS
T T1
2
Ti i
e e ee e e i
Adx u fAdx u Tdx Q P
17
Potential-Energy Approach
Then, the equation can be written as:
where Ueis the element strain energy.
T Te i i
e ee e e i
U u fAdx u Tdx Q P
1
2
Te e
U Adx
18
Potential-Energy Approach
Element Stiffness Matrix
Consider the strain energy term.
Substitute for = EBqand =Bqinto above equation.
From previous equation:
1
2
Te e
U Adx
T T T T1 1or [ ]2 2
e ee eU E Adx U E Adx q B Bq q B B q
2 1 or2 2
elx xdx d dx d
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Potential-Energy Approach
The element strain energy Ueis now written as:
where Eeis Youngs modulus. Note that , then:
which result in:
1T T
1
1
2 2
ee e e
lU A E d
q B B q
1
12d
T 21 1 1 [ 1 1]12e e e ee
U A l E l
q q
T1 1 11 12
e ee
e
A EU
l
q q
20
Potential-Energy Approach
This equation can be written as:
where the element stiffness matrix ke is given by:
T1
2
eeU q k q
1 11 1
e e e
e
E A
l
21
Potential-Energy Approach
Force terms
Element body force term:
This equation can be written as:
Integrals of the shape functions:
T1 1 2 2( )ee e
u fAdx A f N q N q dx
1T T
2
e e
ee e
A f N dxu fAdx
A f N dx
q
11 1
1
21
12 2 2
1
2 2 2
e ee
e e
e
l lN dx d
l lN dx d
22
Potential-Energy Approach
The body force term can be written as:
or
where the element body force vector fe is:
T T 112e
ee
Au fAdx l f q
T T e
eu fAdx q f
112e e
e
Al ff
23
Potential-Energy Approach
The element traction force term:T
1 1 2 2( )e eu Tdx N q N q Tdx
1T T
2
e
ee
T N dxu Tdx
T N dx
q
T T e
eu Tdx q T
112e eTlT
24
Potential-Energy Approach
At this stage, element matrices ke, feand Tehave
been obtained. Then, the total potential energy canbe written as:
where Kis the global stiffness matrix, F is the global loadvectorand Q is the global displacement vector.
Assembly of the global stiffness matrix and loadvector:
T T1
2 Q KQ Q F
( )
e
eee
e
K k
F f + T P
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Galerkin Approach
Galerkins variational form for one dimensionalproblem:
On the discretized region:
T T( ) 0T i iL L Li
Adx fAdx Tdx P
T T( ) 0T i ie e ee e e i
E Adx fAdx Tdx P
26
Galerkin Approach
Summary.
The variational form can be written as:
Or
where
T T T 0e e e i ie e e i
P k q f T
T ( ) 0 KQ F
1 11 1
112
112
e e e
e
e e e
e e
E A
lA l f
Tl
k
f
T
Element bodyforce vector
Element stiffnessmatrix
Element tractionforce
27
Penalty Approach
Penalty approach is used to handle the boundaryconditions.
In this approach, global stiffness K is modified byadding a large number Cto the first diagonalelement which has specified boundary condition.
Similarly, global load vector is also modified byadding Cand boundary condition number.
Consider a displacement boundary condition:
Q1= a1
28
Penalty Approach
The modified stiffness matrix and modified loadvector are given by:
It is that the value ofCis:
Reaction force: R= -CQ
11 12 1 1 1 1
21 22 2 2 2
1 2
( ) NN
N NN N NN
K C K K Q F CaK K K Q F
Q FK K K
4max 10ijC K 11
i Nj N
29
Example 3.4
Consider the bar shown in fig. E3.4. An axial
load P = 200x103
N is applied as shown. Usingthe penalty approach for handling boundaryconditions do the following:
(a) Determine the nodal displacements
(b) Determine the stress in each material
(c) Determine the reaction forces
Ex 3.4
30
300 mm 400 mm
P
1 2
12
3
Aluminum
A1 = 2400 mm2
E1 = 70 x 109 N/m2
Steel
A2 = 600 mm2
E2 = 200 x 109 N/m2
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3131
Ex. 3.4
(a) Determine the nodal displacements
11
11
300
24001070 31k
11
11
400
60010200 32k
1 21
2
Global dof
2 3
2
3
11
11
e
eee
l
AEk
3232
Ex. 3.4
Structural stiffness matrix K is assembled from k1and k2
Global load vector
11
11
300
24001070 31k
11
11
400
60010200 32k
30.330.30
30.386.056.5
056.556.5
106K
TF 010200,0 3
3333
Ex. 3.4
Global load vector is
dofs 1 and 3 are fixed
Using penalty approach, a large number of C isadded to the first and third diagonal element of K
30.330.30
30.386.056.5
056.556.5
106K
TF 010200,0 3
410max ijKC
46 101086.0 C
max
30.860030.30
30.386.056.5
056.556.8600
106K
3434
Ex. 3.4
Finite element equation are given by
46 101086.0 C
0
10200
0
30.860030.30
30.386.056.5
056.556.8600
3
3
2
1
Q
Q
Q
NNNNNN
N
N
F
F
CaF
Q
Q
Q
KKK
KKK
KKCK
2
11
3
2
21
22221
11211
3535
Ex. 3.4
The solution of displacement
0
10200
0
30.860030.30
30.386.056.5
056.556.86003
3
2
1
Q
Q
Q
mmQ T66 101127.823257.0101432.15
3636
EBQ
Ex. 3.4
(b) the stresses in each element
Using Eq. 3.15 and Eq. 3.16
MPa27.5423257.0
101432.1511
300
11070
66
1
111
12
xx
B
MPa29.116101127.8
23257.011
400
110200
6
3
2
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Ex. 3.4
(c) Determine the reaction force at the support
Using Eq. 3.78
3610
11 1023.130101432.151086.0 CQR
riaQCR iPP ,...,2,1)( 11
3610
33 1077.69101127.81086.0 CQR
38
Quadratic Shape Functions
In some problems, use of quadratic interpolationleads to more accurate results.
Consider a typical three-node quadratic element.
Transformation of the coordinate system:
Figure 8
3
2 1
2( )x x
x x
39
Quadratic Shape Functions
In -coordinate, quadratic shape function N1, N2and N3 will be introduced as:
Figure 9
11 2
12 2
3
( ) (1 )
( ) (1 )
( ) (1 )(1 )
N
N
N
40
Quadratic Shape Functions
The displacement field within the element:
Figure 10
1 1 2 2 3 3
oru N q N q N q
u
Nq
41
Quadratic Shape Functions
The strain is given by:
Then,
The stress is given by:
du du d dx d dx
2 1
2 1 2 1 2, , 2 or =
2 2x x
q Bq
E Bq
42
Quadratic Shape Functions
The element stiffness matrix:
The element body force vector:
The element traction-force vector:
7 1 81 7 83 8 8 16
e e e
e
E Al
k
1/ 61/ 62 / 3
ee eA l f
f
1/ 61/ 62 / 3
eel T
T
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Temperature Effects
For thermal stress problems.
Initial strain: 0 = T
The element load vector:
This equation can be simplified as:
1 T0 1
2
e ee e
lE A d
B
2 1
1
1e e e eE A l T
x x
2 1
[ 1 1]
x x
B
44
Temperature Effects
The global load vector:
The desired element load vector:
The stress in each element:
Or
( )e e e
e
F f T P
( )E T Bq
2 1
[ 1 1]E
E Tx x
q
2 1
11
e e e eE A l T
x x