Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslation

Abstract One interesting proposal to solve the black hole information loss paradox without modifying either general relativity or quantum field theory, is the soft hair, a diffeomorphism charge that records the anisotropic radiation in the asymptotic region. This proposal, however, has been challeng...

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Main Authors: Hsu-Wen Chiang, Yu-Hsien Kung, Pisin Chen
Format: Article
Language:English
Published: SpringerOpen 2020-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2020)089
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spelling doaj-563b903b6b5f416c8b5ec511e56b23c92020-12-20T12:04:24ZengSpringerOpenJournal of High Energy Physics1029-84792020-12-0120201212510.1007/JHEP12(2020)089Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslationHsu-Wen Chiang0Yu-Hsien Kung1Pisin Chen2Leung Center for Cosmology and Particle Astrophysics, National Taiwan UniversityLeung Center for Cosmology and Particle Astrophysics, National Taiwan UniversityLeung Center for Cosmology and Particle Astrophysics, National Taiwan UniversityAbstract One interesting proposal to solve the black hole information loss paradox without modifying either general relativity or quantum field theory, is the soft hair, a diffeomorphism charge that records the anisotropic radiation in the asymptotic region. This proposal, however, has been challenged, given that away from the source the soft hair behaves as a coordinate transformation that forms an Abelian group, thus unable to store any information. To maintain the spirit of the soft hair but circumvent these obstacles, we consider Hawking radiation as a probe sensitive to the entire history of the black hole evaporation, where the soft hairs on the horizon are induced by the absorption of a null anisotropic flow, generalizing the shock wave considered in [1, 2]. To do so we introduce two different time-dependent extensions of the diffeomorphism associated with the soft hair, where one is the backreaction of the anisotropic null flow, and the other is a coordinate transformation that produces the Unruh effect and a Doppler shift to the Hawking spectrum. Together, they form an exact BMS charge generator on the entire manifold that allows the nonperturbative analysis of the black hole horizon, whose surface gravity, i.e. the Hawking temperature, is found to be modified. The modification depends on an exponential average of the anisotropy of the null flow with a decay rate of 4M, suggesting the emergence of a new 2-D degree of freedom on the horizon, which could be a way out of the information loss paradox.https://doi.org/10.1007/JHEP12(2020)089Black HolesClassical Theories of GravitySpace-Time Symmetries
collection DOAJ
language English
format Article
sources DOAJ
author Hsu-Wen Chiang
Yu-Hsien Kung
Pisin Chen
spellingShingle Hsu-Wen Chiang
Yu-Hsien Kung
Pisin Chen
Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslation
Journal of High Energy Physics
Black Holes
Classical Theories of Gravity
Space-Time Symmetries
author_facet Hsu-Wen Chiang
Yu-Hsien Kung
Pisin Chen
author_sort Hsu-Wen Chiang
title Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslation
title_short Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslation
title_full Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslation
title_fullStr Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslation
title_full_unstemmed Modification to the Hawking temperature of a dynamical black hole by a flow-induced supertranslation
title_sort modification to the hawking temperature of a dynamical black hole by a flow-induced supertranslation
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2020-12-01
description Abstract One interesting proposal to solve the black hole information loss paradox without modifying either general relativity or quantum field theory, is the soft hair, a diffeomorphism charge that records the anisotropic radiation in the asymptotic region. This proposal, however, has been challenged, given that away from the source the soft hair behaves as a coordinate transformation that forms an Abelian group, thus unable to store any information. To maintain the spirit of the soft hair but circumvent these obstacles, we consider Hawking radiation as a probe sensitive to the entire history of the black hole evaporation, where the soft hairs on the horizon are induced by the absorption of a null anisotropic flow, generalizing the shock wave considered in [1, 2]. To do so we introduce two different time-dependent extensions of the diffeomorphism associated with the soft hair, where one is the backreaction of the anisotropic null flow, and the other is a coordinate transformation that produces the Unruh effect and a Doppler shift to the Hawking spectrum. Together, they form an exact BMS charge generator on the entire manifold that allows the nonperturbative analysis of the black hole horizon, whose surface gravity, i.e. the Hawking temperature, is found to be modified. The modification depends on an exponential average of the anisotropy of the null flow with a decay rate of 4M, suggesting the emergence of a new 2-D degree of freedom on the horizon, which could be a way out of the information loss paradox.
topic Black Holes
Classical Theories of Gravity
Space-Time Symmetries
url https://doi.org/10.1007/JHEP12(2020)089
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AT pisinchen modificationtothehawkingtemperatureofadynamicalblackholebyaflowinducedsupertranslation
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