Micromechanics of composites/Infinitesimal deformations

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Infinitesimal Deformations

Let us first consider only infinitesimal strains and linear elasticity. If we assume that the RVE is small enough, we can neglect inertial and body forces. In addition, if the RVE is in equilibrium, conservation of mass automatically holds. Then the equations that govern the motion of the RVE can be written as:

ε=12(𝐮+𝐮T)Strain-Displacement Relationsσ=𝖢:εStress-Strain Relationsσ=0Balance of Linear Momentumσ=σTBalance of Angular Momentumρe˙=σ:(𝐯)𝐪+ρsBalance of Energy.

In the above equations, ε(𝐱) is the strain tensor (small strain), 𝐮(𝐱) is the displacement vector, and 𝖢(𝐱) is the fourth-order tensor of elastic moduli at the point 𝐱Ω.

To get a unique solution of the governing equations, we need boundary conditions on Ω. These boundary conditions may be in the form of applied tractions:

σ𝐧=𝐭¯;σijnj=ti¯

where 𝐧(𝐱) is the outward normal vector to the surface Ω and 𝐭¯(𝐱) is the applied traction.

Alternatively, the boundary conditions may be in the form of applied displacements:

𝐮=𝐮¯;ui=ui¯

where 𝐮¯(𝐱) is the applied displacement.

We usually assume that the portions of the boundary on which tractions and displacements are applied are nonoverlapping, i.e., Ω=ΩtΩu and ΩtΩu=.

If we need to solve the energy equation, we also have to specify heat flux or specified temperature boundary conditions on the RVE.


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