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Spherically Symmetric Scalar Hair for Charged Black Holes

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Title
Spherically Symmetric Scalar Hair for Charged Black Holes
Author(s)
Jeong-Pyong Hong; Motoo Suzuki; Masaki Yamada
Publication Date
2020-09
Journal
PHYSICAL REVIEW LETTERS, v.125, no.11, pp.111104
Publisher
AMER PHYSICAL SOC
Abstract
© 2020 American Physical Society. The no-hair theorem by Mayo and Bekenstein states that there exists no nonextremal static and spherical charged black hole endowed with hair in the form of a charged scalar field with a self-interaction potential. In our recent work [Phys. Lett. B 803,135324 (2020)], we showed that the effect of a scalar mass term is important at an asymptotic infinity, which was omitted to prove the no-hair theorem. In this Letter, we demonstrate that there actually exists static and spherical charged scalar hair, dubbed as Q hair, around charged black holes, by taking into account the backreaction to the metric and gauge field. We also discuss that Q cloud, which is constructed without the backreaction around a Reissner-Nordstrom black hole, is a good approximation to Q hair under a certain limit
URI
https://pr.ibs.re.kr/handle/8788114/7643
DOI
10.1103/PhysRevLett.125.111104
ISSN
0031-9007
Appears in Collections:
Center for Fundamental Theory(순수물리이론 연구단) > 1. Journal Papers (저널논문)
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