56 research outputs found

    Characterization of balls through optimal concavity for potential functions

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    Let p∈(1,n)p\in(1,n). If Ω\Omega is a convex domain in \rn whose pp-capacitary potential function uu is (1−p)/(n−p)(1-p)/(n-p)-concave (i.e. u(1−p)/(n−p)u^{(1-p)/(n-p)} is convex), then Ω\Omega is a ball

    An overdetermined problem for the anisotropic capacity

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    We consider an overdetermined problem for the Finsler Laplacian in the exterior of a convex domain in RN\mathbb{R}^N, establishing a symmetry result for the anisotropic capacitary potential. Our result extends the one of W. Reichel [Arch. Rational Mech. Anal. 137 (1997)], where the usual Newtonian capacity is considered, giving rise to an overdetermined problem for the standard Laplace equation. Here, we replace the usual Euclidean norm of the gradient with an arbitrary norm HH. The resulting symmetry of the solution is that of the so-called Wulff shape (a ball in the dual norm H0H_0)

    Parabolic Minkowski convolutions of viscosity solutions to fully nonlinear equations

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    This paper is concerned with the Minkowski convolution of viscosity solutions of fully nonlinear parabolic equations. We adopt this convolution to compare viscosity solutions of initial-boundary value problems in different domains. As a consequence, we can for instance obtain parabolic power concavity of solutions to a general class of parabolic equations. Our results apply to the Pucci operator, the normalized qq-Laplacians with 1<q≤∞1<q\leq\infty, the Finsler Laplacian and more general quasilinear operators

    Starshapedeness for fully-nonlinear equations in Carnot groups

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    In this paper we establish the starshapedness of the level sets of the capacitary potential of a large class of fully-nonlinear equations for condensers in Carnot groups, once a natural notion of starshapedness has been introduced. Our main result is Theorem 1.2 below.Comment: Accepted for publication in the Journal of the London Mathematical Societ

    On space-time quasiconcave solutions of the heat equation

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    In this paper we first obtain a constant rank theorem for the second fundamental form of the space-time level sets of a space-time quasiconcave solution of the heat equation. Utilizing this constant rank theorem, we can obtain some strictly convexity results of the spatial and space-time level sets of the space-time quasiconcave solution of the heat equation in a convex ring. To explain our ideas and for completeness, we also review the constant rank theorem technique for the space-time Hessian of space-time convex solution of heat equation and for the second fundamental form of the convex level sets for harmonic function

    To logconcavity and beyond

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    In 1976 Brascamp and Lieb proved that the heat flow preserves logconcavity. In this paper, introducing a variation of concavity, we show that it preserves in fact a stronger property than logconcavity and we identify the strongest concavity preserved by the heat flow.Comment: We removed one result, Theorem 3.2 of the old version, due to a gap in the proo
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