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