Math 2.0

Mechanics of deformable solids Definition

Green–Lagrange strain tensor

Builds on Deformation gradientCauchy–Green deformation tensorStrain tensor

Definition

Let φ ⁣:B→ℝ3\varphi \colon B \to \R^3 be a deformation of an open set B⊆ℝ3B \subseteq \R^3, with deformation gradient FF and right Cauchy–Green tensor C=FTFC = F^T F. The Green–Lagrange strain tensor is the field E=12(C−I)=12(FTF−I),E = \tfrac12 (C - I) = \tfrac12 (F^T F - I), where II is the 3×33 \times 3 identity matrix.

Remarks

With the displacement u(X)=φ(X)−Xu(X) = \varphi(X) - X, so that F=I+∇uF = I + \nabla u, one has E=12(∇u+(∇u)T+(∇u)T∇u).E = \tfrac12 \left( \nabla u + (\nabla u)^T + (\nabla u)^T \nabla u \right). Dropping the quadratic term gives the infinitesimal strain tensor ε=12(∇u+(∇u)T)\varepsilon = \tfrac12 (\nabla u + (\nabla u)^T). For the simple shear with FF having rows (1,γ,0)(1, \gamma, 0), (0,1,0)(0, 1, 0), (0,0,1)(0, 0, 1), the tensor EE has rows (0,γ/2,0)(0, \gamma/2, 0), (γ/2,γ2/2,0)(\gamma/2, \gamma^2/2, 0), (0,0,0)(0, 0, 0). For a rotation by the angle θ\theta about the third axis, E=0E = 0. But ε\varepsilon has diagonal entries cos⁡θ−1\cos\theta - 1, cos⁡θ−1\cos\theta - 1, 00, which is nonzero for θ∉2πℤ\theta \notin 2\pi\Z. So the small-strain tensor fails to vanish for large rotations. The tensor EE is also called the Green–St. Venant or Lagrangian finite strain tensor.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Finite_strain_theory, Finite strain tensors
About this page
TagEA6CAV8ZSH
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Kinddefinition
WritingW0 stub
MSC74A05
DefinesGreen–Lagrange strain tensor
UsesDeformation gradient, Cauchy–Green deformation tensor, Strain tensor
Changed3 November 2026

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