Scalar Hairy Black Holes in Four Dimensions are Unstable
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Peer-reviewed
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Abstract
We present a numerical analysis of the stability properties of the black holes with scalar hair constructed by Herdeiro and Radu. We prove the existence of a novel gauge where the scalar field perturbations decouple from the metric perturbations, and analyze the resulting quasinormal mode spectrum. We find unstable modes with characteristic growth rates which for uniformly small hair are almost identical to those of a massive scalar field on a fixed Kerr background.
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Physical Review Letters
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Journal ISSN
0031-9007
1079-7114
1079-7114
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120
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American Physical Society
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Except where otherwised noted, this item's license is described as All rights reserved
Sponsorship
Science and Technology Facilities Council (ST/P000681/1)
Science and Technology Facilities Council (ST/P000673/1)
Science and Technology Facilities Council (ST/L000636/1)
Science and Technology Facilities Council (ST/P000673/1)
Science and Technology Facilities Council (ST/L000636/1)
B. G. was supported by an STFC studentship. J. E. S. was supported in part by STFC Grants No. PHY-1504541 and No. ST/P000681/1.