Elliptic Equations with Critical Growth and a Large Set of Boundary Singularities

Nassif Ghoussoub, Frederic Robert

Published 2005-08-18Version 1

We solve variationally certain equations of stellar dynamics of the form $-\sum_i\partial_{ii} u(x) =\frac{|u|^{p-2}u(x)}{{\rm dist} (x,{\mathcal A} )^s}$ in a domain $\Omega$ of $\rn$, where ${\mathcal A} $ is a proper linear subspace of $\rn$. Existence problems are related to the question of attainability of the best constant in the following recent inequality of Badiale-Tarantello [1]: $$0<\mu_{s,\P}(\Omega)=\inf{\int_{\Omega}|\nabla u|^2 dx; u\in \huno \hbox{and}\int_{\Omega}\frac{|u(x)|^{\crit(s)}}{|\pi(x)|^s} dx=1}$$ where $0<s<2$, $\crit(s)=\frac{2(n-s)}{n-2}$ and where $\pi$ is the orthogonal projection on a linear space $\P$, where $\hbox{dim}_{\rr}\P \geq 2$. We investigate this question and how it depends on the relative position of the subspace $\Porth$, the orthogonal of $\P$, with respect to the domain $\Omega$ as well as on the curvature of the boundary $\partial\Omega$ at its points of intersection with $\Porth $.