Different phases of hairy black holes in AdS5 space
We investigate the thermodynamics of hairy black holes in asymptotically anti-de Sitter (AdS) space, including backreaction. Resorting to the Euclidean path integral approach, we show that matter conformally coupled to Einstein gravity in five dimensions may exhibit a phase transition whose endpoint...
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todo:paper_15507998_v91_n4_p_Giribet2023-10-03T16:25:09Z Different phases of hairy black holes in AdS5 space Giribet, G. Goya, A. Oliva, J. We investigate the thermodynamics of hairy black holes in asymptotically anti-de Sitter (AdS) space, including backreaction. Resorting to the Euclidean path integral approach, we show that matter conformally coupled to Einstein gravity in five dimensions may exhibit a phase transition whose endpoint turns out to be a hairy black hole in AdS5 space. The scalar field configuration happens to be regular everywhere outside and on the horizon and behaves asymptotically in such a way that respects the AdS boundary conditions that are relevant for AdS/CFT. The theory presents other peculiar features in the ultraviolet, like the existence of black holes with arbitrarily low temperature in AdS5. This provides a simple setup in which the fully backreacting problem of a hair forming in AdS at a certain critical temperature can be solved analytically. © 2015 American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_15507998_v91_n4_p_Giribet |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
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R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| description |
We investigate the thermodynamics of hairy black holes in asymptotically anti-de Sitter (AdS) space, including backreaction. Resorting to the Euclidean path integral approach, we show that matter conformally coupled to Einstein gravity in five dimensions may exhibit a phase transition whose endpoint turns out to be a hairy black hole in AdS5 space. The scalar field configuration happens to be regular everywhere outside and on the horizon and behaves asymptotically in such a way that respects the AdS boundary conditions that are relevant for AdS/CFT. The theory presents other peculiar features in the ultraviolet, like the existence of black holes with arbitrarily low temperature in AdS5. This provides a simple setup in which the fully backreacting problem of a hair forming in AdS at a certain critical temperature can be solved analytically. © 2015 American Physical Society. |
| format |
JOUR |
| author |
Giribet, G. Goya, A. Oliva, J. |
| spellingShingle |
Giribet, G. Goya, A. Oliva, J. Different phases of hairy black holes in AdS5 space |
| author_facet |
Giribet, G. Goya, A. Oliva, J. |
| author_sort |
Giribet, G. |
| title |
Different phases of hairy black holes in AdS5 space |
| title_short |
Different phases of hairy black holes in AdS5 space |
| title_full |
Different phases of hairy black holes in AdS5 space |
| title_fullStr |
Different phases of hairy black holes in AdS5 space |
| title_full_unstemmed |
Different phases of hairy black holes in AdS5 space |
| title_sort |
different phases of hairy black holes in ads5 space |
| url |
http://hdl.handle.net/20.500.12110/paper_15507998_v91_n4_p_Giribet |
| work_keys_str_mv |
AT giribetg differentphasesofhairyblackholesinads5space AT goyaa differentphasesofhairyblackholesinads5space AT olivaj differentphasesofhairyblackholesinads5space |
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1782030149560041472 |