Abstract
We uncover two mechanisms that can render Kerr black holes unstable in scalar-tensor gravity, both associated with the presence of matter in the vicinity of the black hole and the fact that this introduces an effective mass for the scalar. Our results highlight the importance of understanding the structure of spacetime in realistic, astrophysical black holes in scalar-tensor theories.
Originalsprog | Engelsk |
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Artikelnummer | 111101 |
Tidsskrift | Physical Review Letters |
Vol/bind | 111 |
Udgave nummer | 11 |
ISSN | 0031-9007 |
DOI | |
Status | Udgivet - 10 sep. 2013 |