For a differentiable velocity field, the rate-of-strain tensor is the symmetric matrix

D(u)=12(∇u+(∇u)T),D(u)ij=12(∂jui+∂iuj).D(u)=\frac12\bigl(\nabla u+(\nabla u)^{\mathsf T}\bigr), \qquad D(u)_{ij}=\frac12(\partial_j u_i+\partial_i u_j).

Here ∇u\nabla u denotes the , with (∇u)ij=∂jui(\nabla u)_{ij}=\partial_j u_i.

Infinitesimal deformation

If two nearby particles have infinitesimal separation ξ\xi, then ξ˙=(∇u)ξ\dot\xi=(\nabla u)\xi and

ddt∣ξ∣2=2ξTD(u)ξ.\frac{d}{dt}|\xi|^2=2\xi^{\mathsf T}D(u)\xi.

The skew-symmetric part of the gradient contributes local rotation but not this change in squared length. Incompressibility implies tr⁡D(u)=0\operatorname{tr}D(u)=0.

References