A geometric framework for black hole perturbations

Details A geometric framework for black hole perturbations A geometric framework for black hole perturbations

2011-02-11

arxiv.org/abs/1102.2451v2

Phys.Rev.D83:127502,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, 1 figure

Scientific paper

10.1103/PhysRevD.83.127502

Black hole perturbation theory is typically studied on time surfaces that extend between the bifurcation sphere and spatial infinity. From a physical point of view, however, it may be favorable to employ time surfaces that extend between the future event horizon and future null infinity. This framework resolves problems regarding the representation of quasinormal mode eigenfunctions and the construction of short-ranged potentials for the perturbation equations in frequency domain.

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