Trapping of waves and null geodesics for rotating black holes

S. Dyatlov and M. Zworski
Phys. Rev. D 88, 084037 – Published 24 October 2013

Abstract

We present dynamical properties of linear waves and null geodesics valid for Kerr and Kerr–de Sitter black holes and their stationary perturbations. The two are intimately linked by the geometric optics approximation. For the null geodesic flow the key property is the r-normal hyperbolicity of the trapped set and for linear waves it is the distribution of quasinormal modes: the exact quantization conditions do not hold for perturbations but the bounds on decay rates and the statistics of frequencies are still valid.

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  • Received 24 May 2013

DOI:https://doi.org/10.1103/PhysRevD.88.084037

© 2013 American Physical Society

Authors & Affiliations

S. Dyatlov1 and M. Zworski2

  • 1Department of Mathematics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
  • 2Department of Mathematics, University of California, Berkeley, California 94720, USA

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Issue

Vol. 88, Iss. 8 — 15 October 2013

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