Advanced elasticity/Nonlinear elasticity
There are two types models of nonlinear elastic behavior that are in common use. These are :
- Hyperelasticity
- Hypoelasticity
Contents |
Hyperelasticity[edit]
Hyperelastic materials are truly elastic in the sense that if a load is applied to such a material and then removed, the material returns to its original shape without any dissipation of energy in the process. In other word, a hyperelastic material stores energy during loading and releases exactly the same amount of energy during unloading. There is no path dependence.
If
is the Helmholtz free energy, then the stress-strain behavior for such a material is given by
where
is the Cauchy stress,
is the current mass density,
is the deformation gradient,
is the Lagrangian Green strain tensor, and
is the left Cauchy-Green deformation tensor.
We can use the relationship between the Cauchy stress and the 2nd Piola-Kirchhoff stress to obtain an alternative relation between stress and strain.
where
is the 2nd Piola-Kirchhoff stress and
is the mass density in the reference configuration.
Isotropic hyperelasticity[edit]
For isotropic materials, the free energy must be an isotropic function of
. This also mean that the free energy must depend only on the principal invariants of
which are
In other words,
Therefore, from the chain rule,
From the Cayley-Hamilton theorem we can show that
Hence we can also write
The stress-strain relation can then be written as
A similar relation can be obtained for the Cauchy stress which has the form
where
is the right Cauchy-Green deformation tensor.
Cauchy stress in terms of invariants[edit]
For w:isotropic hyperelastic materials, the Cauchy stress can be expressed in terms of the invariants of the left Cauchy-Green deformation tensor (or right Cauchy-Green deformation tensor). If the w:strain energy density function is
, then
(See the page on the left Cauchy-Green deformation tensor for the definitions of these symbols).
-
Proof 1: The second Piola-Kirchhoff stress tensor for a hyperelastic material is given by where
is the right Cauchy-Green deformation tensor and
is the deformation gradient. The Cauchy stress is given bywhere
. Let
be the three principal invariants of
. ThenThe derivatives of the invariants of the symmetric tensor
areTherefore we can write
Plugging into the expression for the Cauchy stress gives
Using the left Cauchy-Green deformation tensor
and noting that
, we can write
-
Proof 2: To express the Cauchy stress in terms of the invariants
recall that
The chain rule of differentiation gives us
Recall that the Cauchy stress is given by
In terms of the invariants
we havePlugging in the expressions for the derivatives of
in terms of
, we haveor,
-
Proof 3: To express the Cauchy stress in terms of the stretches
recall that
The chain rule gives
The Cauchy stress is given by
Plugging in the expression for the derivative of
leads toUsing the spectral decomposition of
we haveAlso note that
Therefore the expression for the Cauchy stress can be written as
Saint-Venant–Kirchhoff material[edit]
The simplest constitutive relationship that satisfies the requirements of hyperelasticity is the Saint-Venant–Kirchhoff material, which has a response function of the form
where
and
are material constants that have to be determined by experiments. Such a linear relation is physically possible only for small strains.


![\begin{align}
I_{\boldsymbol{C}} = I_1 & = \text{tr}(\mathbf{C}) = C_{ii} = \lambda_1^2 + \lambda_2^2 + \lambda_3^2 \\
II_{\boldsymbol{C}} = I_2 & = \tfrac{1}{2}\left[\text{tr}(\mathbf{C}^2) - (\text{tr}~\mathbf{C})^2 \right]
= \tfrac{1}{2}\left[C_{ik}C_{ki} - C_{jj}^2\right] = \lambda_1^2\lambda_2^2 + \lambda_2^2\lambda_3^2 + \lambda_3^2\lambda_1^2 \\
III_{\boldsymbol{C}} = I_3 & = \det(\mathbf{C}) = \lambda_1^2\lambda_2^2\lambda_3^2
\end{align}](http://upload.wikimedia.org/math/9/c/4/9c485f28608801c922f15878e3c8f077.png)




![\boldsymbol{S} = 2~\rho_0~\left[b_0~\boldsymbol{\mathit{1}} + b_1~\boldsymbol{C} + b_2~\boldsymbol{C}^2\right]](http://upload.wikimedia.org/math/9/c/9/9c9d97220df7cf84a4af3071bfd5e4eb.png)
![\boldsymbol{\sigma} = 2~\rho~\left[a_2~\boldsymbol{\mathit{1}} + a_0~\boldsymbol{B} + a_1~\boldsymbol{B}^2\right]](http://upload.wikimedia.org/math/b/8/1/b81f4e067f6c6b2de748a0433e34780d.png)
![\begin{align}
\boldsymbol{\sigma} & =
\cfrac{2}{\sqrt{I_3}}\left[\left(\cfrac{\partial\hat{W}}{\partial I_1} + I_1~\cfrac{\partial\hat{W}}{\partial I_2}\right)\boldsymbol{B} - \cfrac{\partial\hat{W}}{\partial I_2}~\boldsymbol{B} \cdot\boldsymbol{B} \right] + 2\sqrt{I_3}~\cfrac{\partial\hat{W}}{\partial I_3}~\boldsymbol{\mathit{1}} \\
& = \cfrac{2}{J}\left[\cfrac{1}{J^{2/3}}\left(\cfrac{\partial\bar{W}}{\partial \bar{I}_1} + \bar{I}_1~\cfrac{\partial\bar{W}}{\partial \bar{I}_2}\right)\boldsymbol{B} -
\cfrac{1}{3}\left(\bar{I}_1~\cfrac{\partial\bar{W}}{\partial \bar{I}_1} + 2~\bar{I}_2~\cfrac{\partial\bar{W}}{\partial \bar{I}_2}\right)\boldsymbol{\mathit{1}} - \right.\\
& \qquad \qquad \qquad \left. \cfrac{1}{J^{4/3}}~\cfrac{\partial\bar{W}}{\partial \bar{I}_2}~\boldsymbol{B} \cdot\boldsymbol{B} \right] + \cfrac{\partial\bar{W}}{\partial J}~\boldsymbol{\mathit{1}} \\
& = \cfrac{\lambda_1}{\lambda_1\lambda_2\lambda_3}~\cfrac{\partial\tilde{W}}{\partial \lambda_1}~\mathbf{n}_1\otimes\mathbf{n}_1 + \cfrac{\lambda_2}{\lambda_1\lambda_2\lambda_3}~\cfrac{\partial\tilde{W}}{\partial \lambda_2}~\mathbf{n}_2\otimes\mathbf{n}_2 + \cfrac{\lambda_3}{\lambda_1\lambda_2\lambda_3}~\cfrac{\partial\tilde{W}}{\partial \lambda_3}~\mathbf{n}_3\otimes\mathbf{n}_3
\end{align}](http://upload.wikimedia.org/math/6/7/a/67a20501d39e70137edf2eb8a24e28de.png)

is the 
. Let
be the three principal invariants of 


![\boldsymbol{\sigma}
= \cfrac{2}{J}~\left[\cfrac{\partial W}{\partial I_1}~\boldsymbol{F}\cdot\boldsymbol{F}^T+
\cfrac{\partial W}{\partial I_2}~(I_1~\boldsymbol{F}\cdot\boldsymbol{F}^T - \boldsymbol{F}\cdot\boldsymbol{F}^T\cdot\boldsymbol{F}\cdot\boldsymbol{F}^T) +
\cfrac{\partial W}{\partial I_3}~I_3~\boldsymbol{\mathit{1}}\right]](http://upload.wikimedia.org/math/d/9/1/d91ec0d967022cfc301c91b9bcd58c7b.png)
and noting that
, we can write![\boldsymbol{\sigma}
= \cfrac{2}{\sqrt{I_3}}~\left[\left(\cfrac{\partial W}{\partial I_1} +
I_1~\cfrac{\partial W}{\partial I_2}\right)~\boldsymbol{B} -
\cfrac{\partial W}{\partial I_2}~\boldsymbol{B}\cdot\boldsymbol{B}\right] +
2~\sqrt{I_3}~\cfrac{\partial W}{\partial I_3}~\boldsymbol{\mathit{1}}~.](http://upload.wikimedia.org/math/b/d/d/bdd414d8607559f38a725e128ad07a42.png)
recall that


![\boldsymbol{\sigma}
= \cfrac{2}{J}~\left[\left(\cfrac{\partial W}{\partial I_1}+
J^{2/3}~\bar{I}_1~\cfrac{\partial W}{\partial I_2}\right)~\boldsymbol{B} -
\cfrac{\partial W}{\partial I_2}~\boldsymbol{B}\cdot\boldsymbol{B}\right] +
2~J~\cfrac{\partial W}{\partial I_3}~\boldsymbol{\mathit{1}}~.](http://upload.wikimedia.org/math/0/0/f/00f40ca07d5b1ccece93577174a4151e.png)
in terms of ![\begin{align}
\boldsymbol{\sigma}
& = \cfrac{2}{J}~\left[\left(J^{-2/3}~\cfrac{\partial W}{\partial \bar{I}_1} +
J^{-2/3}~\bar{I}_1~\cfrac{\partial W}{\partial \bar{I}_2}\right)~\boldsymbol{B} -
J^{-4/3}~\cfrac{\partial W}{\partial \bar{I}_2}~\boldsymbol{B}\cdot\boldsymbol{B}\right]
+ \\
& \qquad
2~J~\left[-\cfrac{1}{3}~J^{-2}~\left(\bar{I}_1~\cfrac{\partial W}{\partial \bar{I}_1}+
2~\bar{I}_2~\cfrac{\partial W}{\partial \bar{I}_2}\right) +
\cfrac{1}{2}~J^{-1}~\cfrac{\partial W}{\partial J}\right]~\boldsymbol{\mathit{1}}
\end{align}](http://upload.wikimedia.org/math/7/9/c/79c6b49b7d97914ba64863996d9a7221.png)
![\begin{align}
\boldsymbol{\sigma}
& = \cfrac{2}{J}~\left[\cfrac{1}{J^{2/3}}~\left(\cfrac{\partial W}{\partial \bar{I}_1} +
\bar{I}_1~\cfrac{\partial W}{\partial \bar{I}_2}\right)~\boldsymbol{B} -
\cfrac{1}{3}\left(\bar{I}_1~\cfrac{\partial W}{\partial \bar{I}_1}+
2~\bar{I}_2~\cfrac{\partial W}{\partial \bar{I}_2}\right)\boldsymbol{\mathit{1}} - \right. \\
& \qquad \left. \cfrac{1}{J^{4/3}}~
\cfrac{\partial W}{\partial \bar{I}_2}~\boldsymbol{B}\cdot\boldsymbol{B}\right]
+ \cfrac{\partial W}{\partial J}~\boldsymbol{\mathit{1}}
\end{align}](http://upload.wikimedia.org/math/f/4/3/f43da6a703b195491f296e9a1abf4e97.png)
recall that

![\begin{align}
\cfrac{\partial W}{\partial\boldsymbol{C}} & =
\cfrac{\partial W}{\partial \lambda_1}~\cfrac{\partial \lambda_1}{\partial\boldsymbol{C}} +
\cfrac{\partial W}{\partial \lambda_2}~\cfrac{\partial \lambda_2}{\partial\boldsymbol{C}} +
\cfrac{\partial W}{\partial \lambda_3}~\cfrac{\partial \lambda_3}{\partial\boldsymbol{C}} \\
& = \boldsymbol{R}^T\cdot\left[\cfrac{1}{2\lambda_1}~\cfrac{\partial W}{\partial \lambda_1}~\mathbf{n}_1\otimes\mathbf{n}_1 +
\cfrac{1}{2\lambda_2}~\cfrac{\partial W}{\partial \lambda_2}~\mathbf{n}_2\otimes\mathbf{n}_2 +
\cfrac{1}{2\lambda_3}~\cfrac{\partial W}{\partial \lambda_3}~\mathbf{n}_3\otimes\mathbf{n}_3\right]\cdot\boldsymbol{R}
\end{align}](http://upload.wikimedia.org/math/0/6/9/0690cc4f1466f2a40621280ac1f83ce6.png)

![\boldsymbol{\sigma} =
\cfrac{2}{J}~\boldsymbol{V}\cdot
\left[\cfrac{1}{2\lambda_1}~
\cfrac{\partial W}{\partial \lambda_1}~\mathbf{n}_1\otimes\mathbf{n}_1 +
\cfrac{1}{2\lambda_2}~
\cfrac{\partial W}{\partial \lambda_2}~\mathbf{n}_2\otimes\mathbf{n}_2 +
\cfrac{1}{2\lambda_3}~
\cfrac{\partial W}{\partial \lambda_3}~\mathbf{n}_3\otimes\mathbf{n}_3\right]
\cdot\boldsymbol{V}](http://upload.wikimedia.org/math/e/1/6/e16c3b5ec1b5bf612e7f244b105bed9e.png)
we have

![\boldsymbol{\sigma} =
\cfrac{1}{\lambda_1\lambda_2\lambda_3}~
\left[\lambda_1~\cfrac{\partial W}{\partial \lambda_1}~\mathbf{n}_1\otimes\mathbf{n}_1 +
\lambda_2~\cfrac{\partial W}{\partial \lambda_2}~\mathbf{n}_2\otimes\mathbf{n}_2 +
\lambda_3~\cfrac{\partial W}{\partial \lambda_3}~\mathbf{n}_3\otimes\mathbf{n}_3
\right]](http://upload.wikimedia.org/math/8/4/4/8446943129c7cccf8ff25621e4ffdeac.png)
