Near-extremal fluid mechanics

Abstract We analyse near-extremal black brane configurations in asymptotically AdS4 spacetime with the temperature T, chemical potential μ, and three-velocity u ν , varying slowly. We consider a low-temperature limit where the rate of variation is much slower than μ, but much bigger than T. This lim...

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Main Authors: Upamanyu Moitra, Sunil Kumar Sake, Sandip P. Trivedi
Format: Article
Language:English
Published: SpringerOpen 2021-02-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP02(2021)021
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spelling doaj-dc63b0c7aa9f41ce84fd7f09f5bf69682021-02-07T12:08:03ZengSpringerOpenJournal of High Energy Physics1029-84792021-02-012021217810.1007/JHEP02(2021)021Near-extremal fluid mechanicsUpamanyu Moitra0Sunil Kumar Sake1Sandip P. Trivedi2Department of Theoretical Physics, Tata Institute of Fundamental ResearchDepartment of Theoretical Physics, Tata Institute of Fundamental ResearchDepartment of Theoretical Physics, Tata Institute of Fundamental ResearchAbstract We analyse near-extremal black brane configurations in asymptotically AdS4 spacetime with the temperature T, chemical potential μ, and three-velocity u ν , varying slowly. We consider a low-temperature limit where the rate of variation is much slower than μ, but much bigger than T. This limit is different from the one considered for conventional fluid-mechanics in which the rate of variation is much smaller than both T, μ. We find that in our limit, as well, the Einstein-Maxwell equations can be solved in a systematic perturbative expansion. At first order, in the rate of variation, the resulting constitutive relations for the stress tensor and charge current are local in the boundary theory and can be easily calculated. At higher orders, we show that these relations become non-local in time but the perturbative expansion is still valid. We find that there are four linearised modes in this limit; these are similar to the hydrodynamic modes found in conventional fluid mechanics with the same dispersion relations. We also study some linearised time independent perturbations exhibiting attractor behaviour at the horizon — these arise in the presence of external driving forces in the boundary theory.https://doi.org/10.1007/JHEP02(2021)021AdS-CFT CorrespondenceBlack HolesClassical Theories of GravityHolography and condensed matter physics (AdS/CMT)
collection DOAJ
language English
format Article
sources DOAJ
author Upamanyu Moitra
Sunil Kumar Sake
Sandip P. Trivedi
spellingShingle Upamanyu Moitra
Sunil Kumar Sake
Sandip P. Trivedi
Near-extremal fluid mechanics
Journal of High Energy Physics
AdS-CFT Correspondence
Black Holes
Classical Theories of Gravity
Holography and condensed matter physics (AdS/CMT)
author_facet Upamanyu Moitra
Sunil Kumar Sake
Sandip P. Trivedi
author_sort Upamanyu Moitra
title Near-extremal fluid mechanics
title_short Near-extremal fluid mechanics
title_full Near-extremal fluid mechanics
title_fullStr Near-extremal fluid mechanics
title_full_unstemmed Near-extremal fluid mechanics
title_sort near-extremal fluid mechanics
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2021-02-01
description Abstract We analyse near-extremal black brane configurations in asymptotically AdS4 spacetime with the temperature T, chemical potential μ, and three-velocity u ν , varying slowly. We consider a low-temperature limit where the rate of variation is much slower than μ, but much bigger than T. This limit is different from the one considered for conventional fluid-mechanics in which the rate of variation is much smaller than both T, μ. We find that in our limit, as well, the Einstein-Maxwell equations can be solved in a systematic perturbative expansion. At first order, in the rate of variation, the resulting constitutive relations for the stress tensor and charge current are local in the boundary theory and can be easily calculated. At higher orders, we show that these relations become non-local in time but the perturbative expansion is still valid. We find that there are four linearised modes in this limit; these are similar to the hydrodynamic modes found in conventional fluid mechanics with the same dispersion relations. We also study some linearised time independent perturbations exhibiting attractor behaviour at the horizon — these arise in the presence of external driving forces in the boundary theory.
topic AdS-CFT Correspondence
Black Holes
Classical Theories of Gravity
Holography and condensed matter physics (AdS/CMT)
url https://doi.org/10.1007/JHEP02(2021)021
work_keys_str_mv AT upamanyumoitra nearextremalfluidmechanics
AT sunilkumarsake nearextremalfluidmechanics
AT sandipptrivedi nearextremalfluidmechanics
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