Math 2.0

Mechanics of deformable solids Definition

Infinitesimal strain theory

Builds on DeformationStrain tensorGreen–Lagrange strain tensor

Definition

Let u ⁣:B→ℝ3u \colon B \to \R^3 be the displacement of a deformation of an open set B⊆ℝ3B \subseteq \R^3. Infinitesimal strain theory is the approximation valid when ∥∇u(X)∥≪1\norm{\nabla u(X)} \ll 1 for all X∈BX \in B, in which:

  1. terms of order two and higher in ∇u\nabla u are neglected;
  2. the Green–Lagrange tensor is replaced by its linear part, the strain tensor ε=12(∇u+(∇u)T)\varepsilon = \tfrac12 (\nabla u + (\nabla u)^T);
  3. the reference and the deformed configurations are identified, so material and spatial coordinates are not distinguished.

Remarks

A uniform extension u(X)=(10−3X1,0,0)u(X) = (10^{-3} X_1, 0, 0) satisfies the smallness condition. Its strain ε=diag⁡(10−3,0,0)\varepsilon = \operatorname{diag}(10^{-3}, 0, 0) differs from E=diag⁡(10−3+1210−6,0,0)E = \operatorname{diag}(10^{-3} + \tfrac12 10^{-6}, 0, 0) only in the neglected term. A rotation of the body by 9090 degrees does not satisfy the smallness condition, since ∇u=Q−I\nabla u = Q - I has norm of order 11. The linear theory would assign it a spurious strain. The smallness of the strain alone is not enough: rotations must also be small.

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  1. Deformation concept
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  3. Strain tensor concept
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Further reading

  1. Web https://en.wikipedia.org/wiki/Infinitesimal_strain_theory
About this page
TagZCHHTZ1FHS
URIm2://ZCHHTZ1FHS
Kinddefinition
WritingW0 stub
MSC74A05, 74B05
DefinesInfinitesimal strain theory
UsesDeformation, Strain tensor, Green–Lagrange strain tensor
Changed3 November 2026

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