Strain Energy

Internal Energy and the First Law of Thermodynamics

When external forces are applied to a deformable body, these forces perform work on the body. According to the first law of thermodynamics, the work done on the system by the external forces, δ W , and the heat that flows into the system, δ Q , is equal to the change in its internal energy, δ U , and kinetic energy, δ K : δ W + δ Q = δ U + δ K .

Under adiabatic conditions ( δ Q = 0 ) and quasi-static equilibrium ( δ K = 0 ), this reduces to: δ W = δ U Hence, the infinitesimal external work done on the body is entirely stored as internal energy.

Virtual Work of External Forces

Let the displacement field in the body be 𝐮 = ( u , v , w ) and let δ 𝐮 = ( δ u , δ v , δ w ) be infinitesimal virtual displacements, which are arbitrary small variations in the displacement field consistent with boundary conditions.

The corresponding infinitesimal virtual strains are obtained from the virtual displacement gradients: δ ϵ x x = ( δ u ) x , δ ϵ y y = ( δ v ) y , δ ϵ z z = ( δ w ) z and the shear strains: δ γ x y = ( δ u ) y + ( δ v ) x , etc.

The external work done by the external forces consists of two parts: 1. The work of surface tractions, δ W S , and
2. The work of body forces, δ W B .

Thus, δ W = δ W S + δ W B

The work of body forces is given by δ W B = V ρ 𝐛 δ 𝐮 d V where 𝐛 = [ b x , b y , b z ] is the body force per unit mass.

The work of surface traction is given by δ W S = s 𝐭 𝐧 ^   d S

For a surface element with outward normal
𝐧 = [ n x n y n z ] , the traction vector is defined as: 𝐭 = 𝐧 𝝈 where 𝝈 is the Cauchy stress matrix: 𝝈 = [ σ x x σ x y σ x z σ y x σ y y σ y z σ z x σ z y σ z z ]

and the virtual displacement is the column vector: δ 𝐮 = [ δ u δ v δ w ] .

Hence, the virtual work on the surface is: δ W S = S 𝐭 δ 𝐮 d S = S ( 𝐧 𝝈 ) δ 𝐮 d S

Expanding this term explicitly as shown in your derivation: \begin{aligned} \mathbf n \cdot \boldsymbol{\sigma} \cdot \delta \mathbf u &= \begin{bmatrix} n_x & n_y & n_z \end{bmatrix}\begin{bmatrix} \sigma_{xx} & \sigma_{xy} & \sigma_{xz} \\ \sigma_{yx} & \sigma_{yy} & \sigma_{yz} \\ \sigma_{zx} & \sigma_{zy} & \sigma_{zz} \end{bmatrix} \begin{bmatrix} \delta u \\ \delta v \\ \delta w \end{bmatrix}\\ &=n_x(\sigma_{xx}\delta u + \sigma_{xy}\delta v + \sigma_{xz}\delta w) + n_y(\sigma_{yx}\delta u + \sigma_{yy}\delta v + \sigma_{yz}\delta w)\\ &\qquad + n_z(\sigma_{zx}\delta u + \sigma_{zy}\delta v + \sigma_{zz}\delta w) \end{aligned}

Define the vector 𝐅 = 𝝈 δ 𝐮 = [ σ x x δ u + σ x y δ v + σ x z δ w σ y x δ u + σ y y δ v + σ y z δ w σ z x δ u + σ z y δ v + σ z z δ w ] , then 𝐭 δ 𝐮 = n x F x + n y F y + n z F z This shows clearly that the expression 𝐭 δ 𝐮 acts as the dot product of the normal vector 𝐧 with the vector 𝐅 = 𝝈 δ 𝐮 .

Using the Divergence Theorem

Apply the divergence theorem to convert the surface integral to a volume integral: S ( F x n x + F y n y + F z n z ) d S = V ( F x x + F y y + F z z ) d V

Hence, δ W S = V ( F x x + F y y + F z z ) d V

\begin{aligned} \delta W = \int_S &\mathbf t \cdot \delta \mathbf u \, dS + \int_V \rho \mathbf b \cdot \delta \mathbf u \, dV\\ = \int \Bigg( &\frac{\partial \sigma_{xx}}{\partial x} \, \delta u + \sigma_{xx} \frac{\partial (\delta u)}{\partial x} + \frac{\partial \sigma_{xy}}{\partial x} \, \delta v + \sigma_{xy} \frac{\partial (\delta v)}{\partial x} + \frac{\partial \sigma_{xz}}{\partial x} \, \delta w + \sigma_{xz} \frac{\partial (\delta w)}{\partial x}\\ &+ \frac{\partial \sigma_{yx}}{\partial y} \, \delta u + \sigma_{yx} \frac{\partial (\delta u)}{\partial y} + \frac{\partial \sigma_{yy}}{\partial y} \, \delta v + \sigma_{yy} \frac{\partial (\delta v)}{\partial y} + \frac{\partial \sigma_{yz}}{\partial y} \, \delta w + \sigma_{yz} \frac{\partial (\delta w)}{\partial y}\\ &+ \frac{\partial \sigma_{zx}}{\partial z} \, \delta u + \sigma_{zx} \frac{\partial (\delta u)}{\partial z} + \frac{\partial \sigma_{zy}}{\partial z} \, \delta v + \sigma_{zy} \frac{\partial (\delta v)}{\partial z} + \frac{\partial \sigma_{zz}}{\partial z} \, \delta w + \sigma_{zz} \frac{\partial (\delta w)}{\partial z} \Bigg) dV\\ &+ \int (\rho b_x \delta u + \rho b_y \delta v + \rho b_z \delta w) \, dV\\ = \int &\Bigg\{ \left( \frac{\partial \sigma_{xx}}{\partial x} + \frac{\partial \sigma_{yx}}{\partial y} + \frac{\partial \sigma_{zx}}{\partial z} + \rho b_x \right) \delta u + \left( \frac{\partial \sigma_{xy}}{\partial x} + \frac{\partial \sigma_{yy}}{\partial y} + \frac{\partial \sigma_{zy}}{\partial z} + \rho b_y \right) \delta v\\ &+ \left( \frac{\partial \sigma_{xz}}{\partial x} + \frac{\partial \sigma_{yz}}{\partial y} + \frac{\partial \sigma_{zz}}{\partial z} + \rho b_z \right) \delta w + \sigma_{xx} \frac{\partial (\delta u)}{\partial x} + \sigma_{yy} \frac{\partial (\delta v)}{\partial y} + \sigma_{zz} \frac{\partial (\delta w)}{\partial z}\\ &+ \sigma_{xy} \left( \frac{\partial (\delta v)}{\partial x} + \frac{\partial (\delta u)}{\partial y} \right) + \sigma_{xz} \left( \frac{\partial (\delta w)}{\partial x} + \frac{\partial (\delta u)}{\partial z} \right) + \sigma_{yz} \left( \frac{\partial (\delta v)}{\partial z} + \frac{\partial (\delta w)}{\partial y} \right) \Bigg\} dV\\ \end{aligned} Since σ x i x + σ y i y + σ z i z + ρ b i = 0 , we conclude that δ W = V ( σ x x δ ϵ x x + σ y y δ ϵ y y + σ z z δ ϵ z z + σ x y δ γ x y + σ x z δ γ x z + σ y z δ γ y z ) d V .  

Strain Energy Density

It follows from the first law of thermodynamics under adiabatic and static conditions ( δ W = δ U ) that δ U = V ( σ x x δ ϵ x x + σ y y δ ϵ y y + σ z z δ ϵ z z + σ x y δ γ x y + σ x z δ γ x z + σ y z δ γ y z ) d V .

The change in internal energy (due to mechanical forces) per unit volume is called the strain energy density, denoted by U 0 : δ U = V δ U 0 d V .

By comparing the last two equations, we obtain δ U 0 = σ x x δ ϵ x x + σ y y δ ϵ y y + σ z z δ ϵ z z + σ x y δ γ x y + σ x z δ γ x z + σ y z δ γ y z .

The above equation may be expressed in differential form as d U 0 = σ x x d ϵ x x + σ y y d ϵ y y + σ z z d ϵ z z + σ x y d γ x y + σ x z d γ x z + σ y z d γ y z .

Notice that the terms involving the shear strains can be written as the sum of two components corresponding to tensorial shear strains ϵ i j .
For example: σ x y γ x y = σ x y ϵ x y + σ y x ϵ y x .

Therefore, \bbox[5px,border:1px #f2f2f2;background-color:#f2f2f2]{\begin{aligned} dU_0&=\sigma_{xx}\,d\epsilon_{xx}+\sigma_{xy}\, d\epsilon_{xy}+\sigma_{xz}\,d\epsilon_{xz}+\cdots+\sigma_{zz}d\epsilon_{zz}\\ &=\sum_{i=1}^3\sum_{j=1}^3 \sigma_{ij}\, d\epsilon_{ij} \end{aligned}}

It follows from the above expression that \bbox[5px,border:1px #f2f2f2;background-color:#f2f2f2]{ \frac{\partial U_0}{\partial \epsilon_{ij}} = \sigma_{ij}. }

References

  1. Boresi, A. P., Schmidt, R. J., & Sidebottom, O. M. (1993). Advanced mechanics of materials (6th ed.). John Wiley & Sons.
  2. Malvern, L. E. (1969). Introduction to the mechanics of a continuous medium. Prentice Hall.
  3. Sokolnikoff, I. S. (1956). Mathematical theory of elasticity (2nd ed.). McGraw-Hill.