Geometry of Black Hole Spacetimes
Kapitel i bok, 2018
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
9781108186612 (ISBN)
Ämneskategorier
Matematik
Fysik
DOI
10.1017/9781108186612.002