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Lecture Notes: Introduction to Finite Element Method

Chapter 3. Two-Dimensional Problems

II. Finite Elements for 2-D Problems

A General Formula for the Stiffness Matrix

Displacements (u, v) in a plane element are interpolated from nodal displacements (ui, vi) using shape functions Ni as follows,

 

 

 

 

 

u1

 

 

u

N1 0 N2

 

v

 

 

 

0 L

1

 

or u = Nd (11)

 

=

 

 

 

u2

 

v

 

0 N1

0

N

2 L v

 

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

 

 

 

M

 

 

 

 

 

 

 

 

 

 

 

 

where N is the shape function matrix, u the displacement vector and d the nodal displacement vector. Here we have assumed that u depends on the nodal values of u only, and v on nodal values of v only.

From strain-displacement relation (Eq.(8)), the strain vector

is,

ε = Du = DNd,

or

ε = Bd

(12)

where B = DN is the strain-displacement matrix.

© 1997-2002 Yijun Liu, University of Cincinnati

82

Lecture Notes: Introduction to Finite Element Method

Chapter 3. Two-Dimensional Problems

Consider the strain energy stored in an element,

U = 12 σT ε dV = 12 (σx εx +σy εy +τxyγ xy )dV V V

= 12 (Eε)T ε dV = 12 εT Eε dV

V V

= 12 dT BT EB dVd

V

= 1 dT kd

 

2

 

From this, we obtain the general formula for the element

 

stiffness matrix,

 

k = BT EB dV

(13)

V

 

Note that unlike the 1-D cases, E here is a matrix which is given by the stress-strain relation (e.g., Eq.(5) for plane stress).

The stiffness matrix k defined by (13) is symmetric since E is symmetric. Also note that given the material property, the behavior of k depends on the B matrix only, which in turn on the shape functions. Thus, the quality of finite elements in representing the behavior of a structure is entirely determined by the choice of shape functions.

Most commonly employed 2-D elements are linear or quadratic triangles and quadrilaterals.

© 1997-2002 Yijun Liu, University of Cincinnati

83

Lecture Notes: Introduction to Finite Element Method

Chapter 3. Two-Dimensional Problems

Constant Strain Triangle (CST or T3)

This is the simplest 2-D element, which is also called linear triangular element.

 

v3

 

 

 

 

3

 

u3

 

 

(x3, y3)

 

 

y

v

 

 

 

 

 

v2

 

 

 

 

 

v1

(x, y)

u

2

u2

1

 

(x2, y2)

u1

 

 

(x1, y1)

 

 

 

 

 

 

 

x

Linear Triangular Element

For this element, we have three nodes at the vertices of the triangle, which are numbered around the element in the counterclockwise direction. Each node has two degrees of freedom (can move in the x and y directions). The displacements u and v are assumed to be linear functions within the element, that is,

u = b1 + b2 x + b3 y, v = b4 + b5 x + b6 y

(14)

where bi (i = 1, 2, ..., 6) are constants. From these, the strains are found to be,

εx = b2 , εy = b6 , γ xy = b3 + b5

(15)

which are constant throughout the element. Thus, we have the name “constant strain triangle” (CST).

© 1997-2002 Yijun Liu, University of Cincinnati

84

Lecture Notes: Introduction to Finite Element Method

Chapter 3. Two-Dimensional Problems

Displacements given by (14) should satisfy the following six equations,

u1 = b1 + b2 x1 + b3 y1 u2 = b1 + b2 x2 + b3 y2

M

v3 = b4 + b5 x3 + b6 y3

Solving these equations, we can find the coefficients b1, b2, ..., and b6 in terms of nodal displacements and coordinates. Substituting these coefficients into (14) and rearranging the terms, we obtain,

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

v

 

 

 

 

 

 

u

 

N

 

 

0

 

N

 

 

 

0 N

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0 u

 

 

 

 

 

(16)

 

=

 

 

 

 

1

 

 

 

 

 

2

 

 

 

 

 

3

 

2

 

 

 

 

v

 

 

0 N1

0 N2

 

0

 

N3 v2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

3

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

v3

 

 

 

 

where the shape functions (linear functions in x and y) are

 

N1 =

1

 

 

 

{(x2 y3 x3 y2 ) +( y2 y3 )x +(x3 x2 ) y}

 

2A

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

N

 

=

 

1

 

{(x

y

x y

 

) +( y

 

y

)x +(x

 

 

x

 

 

) y}

(17)

2

 

 

 

3

3

 

 

3

 

 

 

 

2A

 

 

3

 

1

1

 

 

 

 

1

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

N

 

=

 

1

{(x y

 

x

 

 

y

) +( y

y

 

)x +(x

 

 

x

 

) y}

 

3

 

 

2

2

2

2

 

 

 

 

 

2A

 

1

 

 

 

1

 

1

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

and

© 1997-2002 Yijun Liu, University of Cincinnati

85

Lecture Notes: Introduction to Finite Element Method Chapter 3. Two-Dimensional Problems

 

1

 

1

x

y

 

 

A =

det

 

 

1

 

1

 

(18)

2

1

x2

y2

 

 

 

1

x

3

y

 

 

 

 

 

 

 

 

 

3

 

is the area of the triangle (Prove this!).

Using the strain-displacement relation (8), results (16) and (17), we have,

 

εx

 

 

 

=

 

εy

 

 

 

γ xy

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

u1

 

 

 

 

y

 

0

y

 

0

y

0

v

 

 

 

 

23

31

 

1

 

 

 

1

 

 

 

 

 

 

 

 

12

 

 

u2

 

 

Bd =

0

x

 

0

x

 

0

x

 

(19)

 

 

 

 

 

 

2A

 

 

 

32

x

 

13

x

 

 

21

v

 

 

 

 

x

32

y

23

 

y

31

21

y

 

2

 

 

 

 

 

 

 

13

 

 

 

12

u

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

3

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

v3

 

 

where xij = xi - xj and yij = yi - yj (i, j = 1, 2, 3). Again, we see constant strains within the element. From stress-strain relation

(Eq.(5), for example), we see that stresses obtained using the CST element are also constant.

Applying formula (13), we obtain the element stiffness matrix for the CST element,

k = BT EB dV = tA(BT EB)

(20)

V

 

in which t is the thickness of the element. Notice that k for CST is a 6 by 6 symmetric matrix. The matrix multiplication in (20) can be carried out by a computer program.

© 1997-2002 Yijun Liu, University of Cincinnati

86

Lecture Notes: Introduction to Finite Element Method

Chapter 3. Two-Dimensional Problems

Both the expressions of the shape functions in (17) and their derivations are lengthy and offer little insight into the behavior of the element.

 

ξ=0

 

η=0

 

3

η=b

 

 

ξ=a

 

η=1

 

 

ξ=1

 

 

(a, b)

2

1

The Natural Coordinates

We introduce the natural coordinates (ξ,η) on the triangle, then the shape functions can be represented simply by,

N1

= ξ, N2

= η, N3 =1ξ η

(21)

Notice that,

 

 

N1

+ N2 + N3

=1

(22)

which ensures that the rigid body translation is represented by the chosen shape functions. Also, as in the 1-D case,

Ni

1,

at node i;

(23)

=

at the other nodes

 

0,

 

and varies linearly within the element. The plot for shape function N1 is shown in the following figure. N2 and N3 have similar features.

© 1997-2002 Yijun Liu, University of Cincinnati

87

Lecture Notes: Introduction to Finite Element Method

Chapter 3. Two-Dimensional Problems

ξ=0

3

N1

ξ=1

1

2

1

Shape Function N1 for CST

We have two coordinate systems for the element: the global coordinates (x, y) and the natural coordinates (ξ,η). The

relation between the two is given by

x = N1x1 + N2 x2

+ N3x3

(24)

y = N1 y1 + N2 y2 + N

3 y3

 

or,

x = x13ξ + x23η + x3

(25)

y = y13ξ + y

23η + y3

 

where xij = xi - xj and yij = yi - yj (i, j = 1, 2, 3) as defined earlier.

Displacement u or v on the element can be viewed as functions of (x, y) or (ξ,η). Using the chain rule for derivatives,

we have,

u

x

y u

u

 

 

∂ ξ

 

 

∂ ξ

∂ ξ

 

 

x

 

 

x

 

(26)

 

u

 

=

x

y

 

u

 

= J

u

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

∂η

 

∂η

∂η

 

 

y

 

 

y

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

where J is called the Jacobian matrix of the transformation.

© 1997-2002 Yijun Liu, University of Cincinnati

88

Lecture Notes: Introduction to Finite Element Method Chapter 3. Two-Dimensional Problems

From (25), we calculate,

x13

y13

 

 

1

 

1

y23

y13

 

 

J = x

 

y

 

,

J

 

=

 

x

 

x

 

(27)

23

23

 

2A

23

 

 

 

 

 

 

 

 

 

13

 

 

where det J = x13 y23 x23 y13 = 2A has been used (A is the area of the triangular element. Prove this!).

From (26), (27), (16) and (21) we have,

u

x =uy

1 y23

2A x23

u

y13 ∂ ξ x13 u∂η

=

1 y23

y13

u1 u3

 

 

x

 

x

u

u

 

2A

23

 

 

 

13

2

3

 

Similarly,

v

x =vy

1 y23

y13

v1 v3

 

 

x

 

x

v

 

v

 

 

2A

23

2

3

 

 

13

 

 

 

(28)

(29)

Using the results in (28) and (29), and the relations

ε = Du = DNd = Bd, we obtain the strain-displacement matrix,

 

1

 

y23

0

y31

0 y12

0

 

B =

 

 

0

x

32

0

x

 

0

x

21

 

(30)

 

 

 

2A

 

 

 

 

 

13

 

 

 

 

 

 

x

32

y

23

x

y

31

x

21

y

 

 

 

 

 

 

 

 

 

13

 

 

12

 

 

which is the same as we derived earlier in (19).

© 1997-2002 Yijun Liu, University of Cincinnati

89

Lecture Notes: Introduction to Finite Element Method

Chapter 3. Two-Dimensional Problems

Applications of the CST Element:

Use in areas where the strain gradient is small.

Use in mesh transition areas (fine mesh to coarse mesh).

Avoid using CST in stress concentration or other crucial areas in the structure, such as edges of holes and corners.

Recommended for quick and preliminary FE analysis of 2-D problems.

Analysis of composite materials (for which the CST is NOT appropriate!)

© 1997-2002 Yijun Liu, University of Cincinnati

90

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