Linear elasticity
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Linear elasticity models the macroscopic mechanical properties of solids assuming "small" deformations.
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Linear elastodynamics is based on three tensor equations:
- dynamic equation
- constitutive equation (anisotropic Hooke's law)
- kinematic equation
where:
is the Cauchy stress
is the body force
is the mass density
is the displacement
is the elasticity tensor
is the strain
is the partial derivative
and
is
.
The elastostatic equations are given by setting
to zero in the dynamic equation. The elastostatic equations are shown in their full form on the 3-D Elasticity entry.
From the basic equations one gets the wave equation
where
is the acoustic differential operator, and δkl is Kronecker delta.
A plane wave has the form
with
of unit length. It is a solution of the wave equation with zero forcing, if and only if ω2 and
constitute an eigenvalue/eigenvector pair of the acoustic algebraic operator
This propagation condition may be written as
where
denotes propagation direction and
is phase velocity.
In isotropic media, the elasticity tensor has the form
where κ is incompressibility, and μ is rigidity. These two parameters are also called the Lamé parameters. If the material is homogeneous (i.e. the elasticity tensor is constant throughout the material), the acoustic operator becomes:
and the acoustic algebraic operator becomes
where
are the eigenvalues of
with eigenvectors
parallel and orthogonal to the propagation direction
, respectively. In the seismological literature, the corresponding plane waves are called P-waves and S-waves (see Seismic wave).
For a static situation (
) in isotropic materials, the wave equation becomes the elastostatic equation :
Taking the divergence of both sides of the elastostatic equation and assuming a conservative force, (
) we have
Noting that summed indices need not match, and that the partial derivatives commute, the two differential terms are seen to be the same and we have:
from which we conclude that:
Taking the Laplacian of both sides of the elastostatic equation, a conservative force will give
and we have
From the divergence equation, the first term on the right is zero (Note: again, the summed indices need not match) and we have:
from which we conclude that:
or, in coordinate free notation
which is just the biharmonic equation in
.
- Gurtin M. E., Introduction to Continuum Mechanics, Academic Press 1981
- L. D. Landau & E. M. Lifschitz, Theory of Elasticity, Butterworth 1986
- Elastostatics (Kip Thorne)



![(\delta_{kl} \partial_{tt}-A_{kl}[\nabla]) \, u_l = \frac{1}{\rho} f_k](../../../math/8/8/8/888bbbca42bfb2ccd912c19ee331cbca.png)
![A_{kl}[\nabla]=\frac{1}{\rho} \, \partial_i \, C_{iklj} \, \partial_j](../../../math/2/8/9/289b0c6f9667496b2bcd9f876f5dc769.png)
![\mathbf{u}[\mathbf{x}, \, t] = U[\mathbf{k} \cdot \mathbf{x} - \omega \, t] \, \hat{\mathbf{u}}](../../../math/6/c/e/6cefbe907d062c9c559aa1b587bdbdb7.png)
![A_{kl}[\mathbf{k}]=\frac{1}{\rho} \, k_i \, C_{iklj} \, k_j](../../../math/f/6/5/f651726c70b54b7e14117fda2d87f340.png)
![A[\hat{\mathbf{k}}] \, \hat{\mathbf{u}}=c^2 \, \hat{\mathbf{u}}](../../../math/a/d/d/add5f05b98ab51bb899561f099639b41.png)

![A_{ij}[\nabla]=\alpha^2 \partial_i\partial_j+\beta^2(\partial_m\partial_m\delta_{ij}-\partial_i\partial_j)\,](../../../math/7/c/5/7c52f5a8a88f6fc0122015e07fdf2636.png)
![A_{ij}[\mathbf{k}]=\alpha^2 k_ik_j+\beta^2(k_mk_m\delta_{ij}-k_ik_j)\,](../../../math/c/a/2/ca24bae0363bf3fc876cc64356ae9515.png)







