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arXiv · 1610.03540

Geometry of black hole spacetimes

Lars Andersson·Thomas Bäckdahl·Pieter Blue
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Abstract

These notes, based on lectures given at the summer school on Asymptotic Analysis in General Relativity, collect material on the Einstein equations, the geometry of black hole spacetimes, and the analysis of fields on black hole backgrounds. The Kerr model of a rotating black hole in vacuum is expected to be unique and stable. The problem of proving these fundamental facts provides the background for the material presented in these notes. Among the many topics which are relevant for the uniqueness and stability problems are the theory of fields on black hole spacetimes, in particular for gravitational perturbations of the Kerr black hole, and more generally, the study of nonlinear field equations in the presence of trapping. The study of these questions requires tools from several different fields, including Lorentzian geometry, hyperbolic differential equations and spin geometry, which are all relevant to the black hole stability problem.

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Lars Andersson, Thomas Bäckdahl, Pieter Blue. 2016-10-11. Geometry of black hole spacetimes. https://arxiv.org/abs/1610.03540

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