Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-Nordstrom

Abstract The direct product of two-dimensional anti-de Sitter spacetime with a two-sphere is an exact solution of four-dimensional Einstein-Maxwell theory without a cosmological constant. In this paper, we analytically solve the coupled gravitational and electromagnetic perturbation equations of AdS...

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Main Author: Achilleas P. Porfyriadis
Format: Article
Language:English
Published: SpringerOpen 2018-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP07(2018)064
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spelling doaj-ab2e9b8a8e3e428da15af3ee18be69df2020-11-25T00:09:55ZengSpringerOpenJournal of High Energy Physics1029-84792018-07-012018711310.1007/JHEP07(2018)064Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-NordstromAchilleas P. Porfyriadis0Department of Physics, UCSBAbstract The direct product of two-dimensional anti-de Sitter spacetime with a two-sphere is an exact solution of four-dimensional Einstein-Maxwell theory without a cosmological constant. In this paper, we analytically solve the coupled gravitational and electromagnetic perturbation equations of AdS 2 × S 2 in Einstein-Maxwell theory. On the other hand, AdS 2 × S 2 also describes the near-horizon region of the extreme Reissner-Nordstrom (ERN) black hole. We therefore also solve the connection problem: we show how the AdS 2 × S 2 perturbation equations arise from an appropriate near-horizon approximation of the corresponding equations for the ERN and then, using matched asymptotic expansions, we analytically extend the AdS 2 × S 2 solutions away from the near-horizon region connecting them with solutions in the far asymptotically flat region. From the point of view of ERN our results may be thought of as computing the classical scattering matrix for gravitational and electromagnetic waves which probe the near-horizon region of the black hole.http://link.springer.com/article/10.1007/JHEP07(2018)0642D GravityAdS-CFT CorrespondenceBlack Holes
collection DOAJ
language English
format Article
sources DOAJ
author Achilleas P. Porfyriadis
spellingShingle Achilleas P. Porfyriadis
Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-Nordstrom
Journal of High Energy Physics
2D Gravity
AdS-CFT Correspondence
Black Holes
author_facet Achilleas P. Porfyriadis
author_sort Achilleas P. Porfyriadis
title Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-Nordstrom
title_short Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-Nordstrom
title_full Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-Nordstrom
title_fullStr Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-Nordstrom
title_full_unstemmed Scattering of gravitational and electromagnetic waves off AdS 2 × S 2 in extreme Reissner-Nordstrom
title_sort scattering of gravitational and electromagnetic waves off ads 2 × s 2 in extreme reissner-nordstrom
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-07-01
description Abstract The direct product of two-dimensional anti-de Sitter spacetime with a two-sphere is an exact solution of four-dimensional Einstein-Maxwell theory without a cosmological constant. In this paper, we analytically solve the coupled gravitational and electromagnetic perturbation equations of AdS 2 × S 2 in Einstein-Maxwell theory. On the other hand, AdS 2 × S 2 also describes the near-horizon region of the extreme Reissner-Nordstrom (ERN) black hole. We therefore also solve the connection problem: we show how the AdS 2 × S 2 perturbation equations arise from an appropriate near-horizon approximation of the corresponding equations for the ERN and then, using matched asymptotic expansions, we analytically extend the AdS 2 × S 2 solutions away from the near-horizon region connecting them with solutions in the far asymptotically flat region. From the point of view of ERN our results may be thought of as computing the classical scattering matrix for gravitational and electromagnetic waves which probe the near-horizon region of the black hole.
topic 2D Gravity
AdS-CFT Correspondence
Black Holes
url http://link.springer.com/article/10.1007/JHEP07(2018)064
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