Scaling and universality in extremal black hole perturbations

Abstract We show that the emergent near-horizon conformal symmetry of extremal black holes gives rise to universal behavior in perturbing fields, both near and far from the black hole horizon. The scale-invariance of the near-horizon region entails power law time-dependence with three universal feat...

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Published in:Journal of High Energy Physics
Main Authors: Samuel E. Gralla, Peter Zimmerman
Format: Article
Language:English
Published: SpringerOpen 2018-06-01
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP06(2018)061
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author Samuel E. Gralla
Peter Zimmerman
author_facet Samuel E. Gralla
Peter Zimmerman
author_sort Samuel E. Gralla
collection DOAJ
container_title Journal of High Energy Physics
description Abstract We show that the emergent near-horizon conformal symmetry of extremal black holes gives rise to universal behavior in perturbing fields, both near and far from the black hole horizon. The scale-invariance of the near-horizon region entails power law time-dependence with three universal features: (1) the decay off the horizon is always precisely twice as fast as the decay on the horizon; (2) the special rates of 1/t off the horizon and 1/v $$ 1/\sqrt{v} $$ on the horizon commonly occur; and (3) sufficiently high-order transverse derivatives grow on the horizon (Aretakis instability). The results are simply understood in terms of near-horizon (AdS2) holography. We first show how the general features follow from symmetry alone and then go on to present the detailed universal behavior of scalar, electromagnetic, and gravitational perturbations of d-dimensional electrovacuum black holes.
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spelling doaj-art-c92f7da3db484f7a84791c2cd8ce95792025-08-19T20:07:57ZengSpringerOpenJournal of High Energy Physics1029-84792018-06-012018613910.1007/JHEP06(2018)061Scaling and universality in extremal black hole perturbationsSamuel E. Gralla0Peter Zimmerman1Department of Physics, University of ArizonaDepartment of Physics, University of ArizonaAbstract We show that the emergent near-horizon conformal symmetry of extremal black holes gives rise to universal behavior in perturbing fields, both near and far from the black hole horizon. The scale-invariance of the near-horizon region entails power law time-dependence with three universal features: (1) the decay off the horizon is always precisely twice as fast as the decay on the horizon; (2) the special rates of 1/t off the horizon and 1/v $$ 1/\sqrt{v} $$ on the horizon commonly occur; and (3) sufficiently high-order transverse derivatives grow on the horizon (Aretakis instability). The results are simply understood in terms of near-horizon (AdS2) holography. We first show how the general features follow from symmetry alone and then go on to present the detailed universal behavior of scalar, electromagnetic, and gravitational perturbations of d-dimensional electrovacuum black holes.http://link.springer.com/article/10.1007/JHEP06(2018)061Black HolesConformal and W SymmetryAdS-CFT CorrespondenceBlack Holes in String Theory
spellingShingle Samuel E. Gralla
Peter Zimmerman
Scaling and universality in extremal black hole perturbations
Black Holes
Conformal and W Symmetry
AdS-CFT Correspondence
Black Holes in String Theory
title Scaling and universality in extremal black hole perturbations
title_full Scaling and universality in extremal black hole perturbations
title_fullStr Scaling and universality in extremal black hole perturbations
title_full_unstemmed Scaling and universality in extremal black hole perturbations
title_short Scaling and universality in extremal black hole perturbations
title_sort scaling and universality in extremal black hole perturbations
topic Black Holes
Conformal and W Symmetry
AdS-CFT Correspondence
Black Holes in String Theory
url http://link.springer.com/article/10.1007/JHEP06(2018)061
work_keys_str_mv AT samuelegralla scalinganduniversalityinextremalblackholeperturbations
AT peterzimmerman scalinganduniversalityinextremalblackholeperturbations