Gravitational wave echoes from black holes in massive gravity
arXiv:2011.04032 · doi:10.1103/PhysRevD.103.024058
Abstract
Gravitational waves are rapidly becoming a very reliable tool for testing alternative theories of gravity. In particular, features in the gravitational wave emission during black hole ringdown phase provide a direct probe of the spacetime outside the black hole. In this article, we consider black holes in ghost-free massive gravity. These black holes generically have scalar hair. We found that a simple coupling between gravitational perturbations and this scalar hair can change the quasinormal ringing of the black hole, and in particular, produce echoes in the emitted gravitational waves. This finding provides a clear-cut way to test massive gravity theory using gravitational wave observations.
arXiv comment8 pages, 3 figures. Accepted for publication in Phys. Rev. D
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