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Linear Elasticity Equations

Summary of the Equations of Linear Elasticity

The stiffness matrix of linear elastic isotropic material contains two parameters:

  • E, Young's modulus (elastic modulus)

  • ν, Poisson’s ratio

Define the following quantities.

σ=stressf=body forceε=strainu=displacement

The equilibrium equation is

·σ=f

The linearized, small-displacement strain-displacement relationship is

ε=12(u+uT)

The balance of angular momentum states that stress is symmetric:

σij=σji

The Voigt notation for the constitutive equation of the linear isotropic model is

[σ11σ22σ33σ23σ13σ12]=E(1+ν)(12ν)[1ννν000ν1νν000νν1ν00000012ν00000012ν00000012ν][ε11ε22ε33ε23ε13ε12]

The expanded form uses all the entries in σ and ε takes symmetry into account.

[σ11σ12σ13σ21σ22σ23σ31σ32σ33]=E(1+ν)(12ν)[1ν000ν000ν12ν000000012ν00000012ν000001ν000ν12ν00012ν0012ν01ν][ε11ε12ε13ε21ε22ε23ε31ε32ε33](1)

In the preceding diagram, • means the entry is symmetric.

3D Linear Elasticity Problem

The toolbox form for the equation is

·(cu)=f

But the equations in the summary do not have ∇u alone, it appears together with its transpose:

ε=12(u+uT)

It is a straightforward exercise to convert this equation for strain ε to ∇u. In column vector form,

u=[ux/xux/yux/zuy/xuy/yuy/zuz/xuz/yuz/z]

Therefore, you can write the strain-displacement equation as

ε=[100000000012012000000012000120001201200000000010000000001201200012000120000000120120000000001]uAu

where A stands for the displayed matrix. So rewriting Equation 1, and recalling that • means an entry is symmetric, you can write the stiffness tensor as

σ=E(1+ν)(12ν)[1ν000ν000ν12ν000000012ν00000012ν000001ν000ν12ν00012ν0012ν01ν]Au=E(1+ν)(12ν)[1ν000ν000ν01/2ν01/2ν00000001/2ν0001/2ν0001/2ν01/2ν00000ν0001ν000ν000001/2ν01/2ν0001/2ν0001/2ν00000001/2ν01/2ν0ν000ν0001ν]u

Make the definitions

μ=E2(1+ν)λ=Eν(1+ν)(12ν)E(1ν)(1+ν)(12ν)=2μ+λ

and the equation becomes

σ=[2μ+λ000λ000λ0μ0μ0000000μ000μ000μ0μ00000λ0002μ+λ000λ00000μ0μ000μ000μ0000000μ0μ0λ000λ0002μ+λ]ucu

If you are solving a 3-D linear elasticity problem by using PDEModel instead of femodel, use the elasticityC3D(E,nu) function (included in your software) to obtain the c coefficient. This function uses the linearized, small-displacement assumption for an isotropic material. For examples that use this function, see StationaryResults.

By default, the toolbox uses the zero Neumann boundary condition and assumes that the boundary is stress-free.

Plane Stress

Plane stress is a condition that prevails in a flat plate in the x-y plane, loaded only in its own plane and without z-direction restraint. For plane stress, σ13 = σ23 = σ31 = σ32 = σ33 = 0. Assuming isotropic conditions, the Hooke's law for plane stress gives the following strain-stress relation:

[ε11ε222ε12]=1E[1ν0ν10002+2ν][σ11σ22σ12]

Inverting this equation, obtain the stress-strain relation:

(σ11σ22σ12)=E1ν2(1ν0ν10001ν2)(ε11ε222ε12)

Convert the equation for strain ε to ∇u.

ε=[10000121200121200001]uAu

Now you can rewrite the stiffness matrix as

[σ11σ12σ21σ22]=[E1ν200Eν1ν20E2(1+ν)E2(1+ν)00E2(1+ν)E2(1+ν)0Eν1ν200E1ν2]u=[2μ(μ+λ)2μ+λ002λμ2μ+λ0μμ00μμ02λμ2μ+λ002μ(μ+λ)2μ+λ]u

Plane Strain

Plane strain is a deformation state where there are no displacements in the z-direction, and the displacements in the x- and y-directions are functions of x and y but not z. The stress-strain relation is only slightly different from the plane stress case, and the same set of material parameters is used.

For plane strain, ε13 = ε23 = ε31 = ε32 = ε33 = 0. Assuming isotropic conditions, the stress-strain relation can be written as follows:

(σ11σ22σ12)=E(1+ν)(12ν)(1νν0ν1ν00012ν2)(ε11ε222ε12)

Convert the equation for strain ε to ∇u.

ε=[10000121200121200001]uAu

Now you can rewrite the stiffness matrix as

[σ11σ12σ21σ22]=[E(1ν)(1+ν)(12ν)00Eν(1+ν)(12ν)0E2(1+ν)E2(1+ν)00E2(1+ν)E2(1+ν)0Eν(1+ν)(12ν)00E(1ν)(1+ν)(12ν)]u=[2μ+λ00λ0μμ00μμ0λ002μ+λ]u

Axisymmetric Analysis

Axisymmetric analysis speeds up simulations by simplifying 3-D solids using their symmetry around the axis of rotation and analyzing only the 2-D axisymmetric section. Use polar coordinates r,θ,z for radial, circumferential, and axial directions. If z is the axis of rotation, the symmetry around the z-axis means that the stress components are independent of the θ coordinate. The stress equilibrium equations for an axisymmetric structural mechanics are as follows:

σrrr+σrzz+1r(σrrσθθ)+fr=0τrzr+σzzz+τrzr+fz=0

τ is the shear stress, and γ is the shear strain. Assuming isotropic conditions, the stress-strain relation can be written as follows:

(σrσzσθτrz)=E(1+ν)(12ν)(1νν00ν1ν00001ν000012ν2)(εrεzεθγrz)

See Also

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