Geometry of Black Hole Spacetimes
Kapitel i bok, 2018

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 a 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 to 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.

Författare

Thomas Bäckdahl

Chalmers, Matematiska vetenskaper, Analys och sannolikhetsteori

Lars Andersson

Max Planck Institute for Gravitational Physics (Albert Einstein Institute)

Pieter Blue

University of Edinburgh

Asymptotic Analysis in General Relativity

9-85

Ämneskategorier

Matematik

Fysik

DOI

10.1017/9781108186612.002

Mer information

Senast uppdaterat

2020-12-11