Inside an asymptotically flat hairy black hole
Published version
Peer-reviewed
Repository URI
Repository DOI
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Authors
Dias, ÓJC
Horowitz, GT
Pinto Da Silva e Conceicao Santos, Jorge https://orcid.org/0000-0002-4199-4190
Abstract
We study the interior of a recently constructed family of asymptotically flat, charged black holes that develop (charged) scalar hair as one increases their charge at fixed mass. Inside the horizon, these black holes resemble the interior of a holographic superconductor. There are analogs of the Josephson oscillations of the scalar field, and the final Kasner singularity depends very sensitively on the black hole parameters near the onset of the instability. In an Appendix, we give a general argument that Cauchy horizons cannot exist in a large class of stationary black holes with scalar hair.
Description
Keywords
Regular Article - Theoretical Physics, Black Holes, Classical Theories of Gravity
Journal Title
Journal of High Energy Physics
Conference Name
Journal ISSN
1029-8479
1029-8479
1029-8479
Volume Title
2021
Publisher
Springer Science and Business Media LLC