Hairy black holes and solitons in global AdS_5
Hairy black holes and solitons in global AdS_5
We use a mix of analytic and numerical methods to exhaustively study a class of asymptotically global AdS solitons and hairy black hole solutions in negative cosmological constant Einstein Maxwell gravity coupled to a charged massless scalar field. Our results depend sensitively on the charge e of the scalar field. The solitonic branch of solutions we study hits the Chandrashekhar limit at finite mass at small e, but extends to arbitrarily large mass at larger e. At low values of e no hairy black holes exist. At intermediate values of e hairy black holes exist above a critical charge. At large e hairy black holes exist at all values of the charge. The lowest mass hairy black hole is a smooth zero entropy soliton at small charge, but a (probably) singular nonzero entropy hairy black hole at larger charge. In a phase diagram of solutions, the hairy black holes merge with the familiar Reissner-Nordström−AdS black holes along a curve that is determined by the onset of the superradiant instability in the latter family.
Dias, Oscar J.C.
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Figueras, Pau
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Minwalla, Shiraz
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Mitra, Prahar
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Monteiro, Ricardo
1dfb2954-9861-425f-82c5-75185a088b60
Santos, Jorge E.
88cca86d-9e1e-40a7-acba-f7986bd7f84b
Dias, Oscar J.C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Figueras, Pau
92a9d40b-4ed0-45c6-b7c4-e8f9b4addcdb
Minwalla, Shiraz
825e7013-930c-4807-b77e-637bad662e49
Mitra, Prahar
3bc62279-2b31-44c1-8b66-76062e702dd9
Monteiro, Ricardo
1dfb2954-9861-425f-82c5-75185a088b60
Santos, Jorge E.
88cca86d-9e1e-40a7-acba-f7986bd7f84b
Dias, Oscar J.C., Figueras, Pau, Minwalla, Shiraz, Mitra, Prahar, Monteiro, Ricardo and Santos, Jorge E.
(2012)
Hairy black holes and solitons in global AdS_5.
JHEP, 8, [117].
(doi:10.1007/JHEP08(2012)117).
Abstract
We use a mix of analytic and numerical methods to exhaustively study a class of asymptotically global AdS solitons and hairy black hole solutions in negative cosmological constant Einstein Maxwell gravity coupled to a charged massless scalar field. Our results depend sensitively on the charge e of the scalar field. The solitonic branch of solutions we study hits the Chandrashekhar limit at finite mass at small e, but extends to arbitrarily large mass at larger e. At low values of e no hairy black holes exist. At intermediate values of e hairy black holes exist above a critical charge. At large e hairy black holes exist at all values of the charge. The lowest mass hairy black hole is a smooth zero entropy soliton at small charge, but a (probably) singular nonzero entropy hairy black hole at larger charge. In a phase diagram of solutions, the hairy black holes merge with the familiar Reissner-Nordström−AdS black holes along a curve that is determined by the onset of the superradiant instability in the latter family.
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Accepted/In Press date: 6 August 2012
e-pub ahead of print date: 23 August 2012
Additional Information:
Copyright © 2012, SISSA
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Local EPrints ID: 467709
URI: http://eprints.soton.ac.uk/id/eprint/467709
PURE UUID: e9333638-7af0-4502-a24d-23d378e4b74c
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Date deposited: 19 Jul 2022 16:57
Last modified: 17 Mar 2024 03:35
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Contributors
Author:
Pau Figueras
Author:
Shiraz Minwalla
Author:
Prahar Mitra
Author:
Ricardo Monteiro
Author:
Jorge E. Santos
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