The black hole stability problem

András Vasy
Stanford University

I will discuss analytic and geometric tools that lead to the understanding of black hole stability with a positive cosmological constant (Kerr-de Sitter spacetimes) and their extensions for making progress on the vanishing cosmological constant case (Kerr). This is based on joint work with Dietrich Haefner and Peter Hintz.

Presentation (PDF File)

Back to Workshop II: Mathematical and Numerical Aspects of Gravitation