English

Relative Bending Energy for Weakly Prestrained Shells

Analysis of PDEs 2019-10-02 v1

Abstract

In this paper, we derive a dimensionally reduced model for a thin film prestrained with a given incompatible Riemannian metric: Gh(x,x3)=I3+2hγS(x)+2hγ/2x3B(x)+h.o.t,γ>2,G^h(x',x_3)=I_3+2h^{\gamma}\,S(x')+2h^{\gamma/2}\,x_3B(x')+h.o.t, \,\,\,\gamma>2, where 0<h10<h\ll 1 is the thickness of the film. The problem is studied rigorously by using a variational approach and establishing the Γ\Gamma-convergence of the non-Euclidean version of the nonlinear elasticity functional. It is shown that the residual nonlinear elastic energy scales as O(hγ+2)O(h^{\gamma+2}) as h0h\to 0.

Keywords

Cite

@article{arxiv.1910.00404,
  title  = {Relative Bending Energy for Weakly Prestrained Shells},
  author = {Silvia Jimenez Bolanos and Anna Zemlaynova},
  journal= {arXiv preprint arXiv:1910.00404},
  year   = {2019}
}

Comments

arXiv admin note: text overlap with arXiv:1404.3298, arXiv:1002.2252 by other authors

R2 v1 2026-06-23T11:31:37.108Z