Integrability conditions between the first and second Cosserat deformation tensor in geometrically nonlinear micropolar models and existence of minimizers

preprint2015arXivOpen access

Abstract

In this note we extend integrability conditions for the symmetric stretch tensor UU in the polar decomposition of the deformation gradient ∇φ=F=R U\nablaφ=F=R\,U to the non-symmetric case. In doing so we recover integrability conditions for the first Cosserat deformation tensor. Let F=Rˉ UˉF=\bar R\,\bar U with Rˉ:Ω⊂R3⟶SO(3)\bar R:Ω\subset\mathbb{R}^3\longrightarrow\mathrm{SO}(3) and Uˉ:Ω⊂R3⟶GL(3)\bar U:Ω\subset\mathbb{R}^3\longrightarrow \mathrm{GL}(3). Then K:=RˉTGrad Rˉ=Anti(1detUˉ[Uˉ(CurlUˉ)T−12tr(Uˉ(CurlUˉ)T)1 ⁣ ⁣1]Uˉ),\mathfrak{K}:={\bar R}^T\mathrm{Grad}\,{\bar R}=\mathrm{Anti}\Big( \frac{1}{\mathrm{det} \bar U}\Big[\bar U(\mathrm{Curl} \bar U)^T-\frac{1}{2} \mathrm{tr}(\bar U(\mathrm{Curl} \bar U)^T) 1\!\!1 \Big]\bar U\Big), giving a connection between the first Cosserat deformation tensor Uˉ\bar U and the second Cosserat tensor K{\mathfrak{K}}. (Here, Anti denotes an isomorphism between R3×3\mathbb{R}^{3\times 3} and So(3):={ A∈R3×3×3 ∣ A.u∈so(3)  ∀u∈R3}\mathfrak{So}(3):=\{\,\mathfrak{A}\in\mathbb{R}^{3\times 3\times 3}\,|\,\mathfrak{A}.u\in\mathfrak{so}(3)\;\forall u\in \mathbb{R}^3\}.) The formula shows that it is not possible to prescribe Uˉ\bar U and K\mathfrak{K} independent from each other. We also propose a new energy formulation of geometrically nonlinear Cosserat models which completely separate the effects of nonsymmetric straining and curvature. For very weak constitutive assumptions (no direct boundary condition on rotations, zero Cosserat couple modulus, quadratic curvature energy) we show existence of minimizers in Sobolev-spaces.

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