Asymptotically-flat supergravity solutions deep inside the black-hole regime
Asymptotically-flat supergravity solutions deep inside the black-hole regime
We construct an infinite family of smooth asymptotically-flat supergravity solutions that have the same charges and angular momenta as general supersymmetric D1-D5-P black holes, but have no horizon. These solutions resemble the corresponding black hole to arbitrary accuracy outside of the horizon: they have asymptotically flat regions, AdS 3× S3 throats and very-near-horizon AdS2 throats, which however end in a smooth cap rather than an event horizon. The angular momenta of the solutions are general, and in particular can take arbitrarily small values. Upon taking the AdS 3× S3 decoupling limit, we identify the holographically-dual CFT states.
AdS-CFT Correspondence, Black Holes in String Theory
Bena, Iosif
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Giusto, Stefano
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Martinec, Emil J.
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Russo, Rodolfo
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Shigemori, Masaki
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Turton, David
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Warner, Nicholas P.
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February 2018
Bena, Iosif
216ba0a8-1a3a-4f4b-b43d-f964e41953d6
Giusto, Stefano
8242c759-c708-479e-bc7d-fb50682fc415
Martinec, Emil J.
650e0325-0c1c-4177-9475-4eaaf978cca8
Russo, Rodolfo
20c23f07-6009-40d2-89a4-d821ffac5655
Shigemori, Masaki
c9a1f8e8-3e89-4235-a66a-d0c66e855ff6
Turton, David
6ce84b30-3cc0-42aa-ace5-f298d4260e9b
Warner, Nicholas P.
ec710058-e4e8-4edc-b521-7205b70e09ff
Bena, Iosif, Giusto, Stefano, Martinec, Emil J., Russo, Rodolfo, Shigemori, Masaki, Turton, David and Warner, Nicholas P.
(2018)
Asymptotically-flat supergravity solutions deep inside the black-hole regime.
Journal of High Energy Physics, 2018 (2), [14].
(doi:10.1007/JHEP02(2018)014).
Abstract
We construct an infinite family of smooth asymptotically-flat supergravity solutions that have the same charges and angular momenta as general supersymmetric D1-D5-P black holes, but have no horizon. These solutions resemble the corresponding black hole to arbitrary accuracy outside of the horizon: they have asymptotically flat regions, AdS 3× S3 throats and very-near-horizon AdS2 throats, which however end in a smooth cap rather than an event horizon. The angular momenta of the solutions are general, and in particular can take arbitrarily small values. Upon taking the AdS 3× S3 decoupling limit, we identify the holographically-dual CFT states.
Text
10.1007%2FJHEP02(2018)014
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Accepted/In Press date: 23 January 2018
e-pub ahead of print date: 2 February 2018
Published date: February 2018
Keywords:
AdS-CFT Correspondence, Black Holes in String Theory
Identifiers
Local EPrints ID: 417947
URI: http://eprints.soton.ac.uk/id/eprint/417947
ISSN: 1126-6708
PURE UUID: 5135b492-f8a5-40e1-a8fe-b8cc467efbc7
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Date deposited: 19 Feb 2018 17:30
Last modified: 18 Mar 2024 03:43
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Contributors
Author:
Iosif Bena
Author:
Stefano Giusto
Author:
Emil J. Martinec
Author:
Rodolfo Russo
Author:
Masaki Shigemori
Author:
Nicholas P. Warner
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