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    A nonlinear elliptic problem with terms concentrating in the boundary

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    In this paper we investigate the behavior of a family of steady state solutions of a nonlinear reaction diffusion equation when some reaction and potential terms are concentrated in a ϵ\epsilon-neighborhood of a portion Γ\Gamma of the boundary. We assume that this ϵ\epsilon-neighborhood shrinks to Γ\Gamma as the small parameter ϵ\epsilon goes to zero. Also, we suppose the upper boundary of this ϵ\epsilon-strip presents a highly oscillatory behavior. Our main goal here is to show that this family of solutions converges to the solutions of a limit problem, a nonlinear elliptic equation that captures the oscillatory behavior. Indeed, the reaction term and concentrating potential are transformed into a flux condition and a potential on Γ\Gamma, which depends on the oscillating neighborhood

    Isotropization of the universe during inflation

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    A primordial inflationary phase allows one to erase any possible anisotropic expansion thanks to the cosmic no-hair theorem. If there is no global anisotropic stress, then the anisotropic expansion rate tends to decrease. What are the observational consequences of a possible early anisotropic phase? We first review the dynamics of anisotropic universes and report analytic approximations. We then discuss the structure of dynamical equations for perturbations and the statistical properties of observables, as well as the implication of a primordial anisotropy on the quantization of these perturbations during inflation. Finally we briefly review models based on primordial vector field which evade the cosmic no-hair theorem.Comment: 9 pages, 3 figures. Invited review article for the French Academy of Scienc
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