Black hole entropy sourced by string winding condensate

Abstract We calculate the entropy of an asymptotically Schwarzschild black hole, using an effective field theory of winding modes in type II string theory. In Euclidean signature, the geometry of the black hole contains a thermal cycle which shrinks towards the horizon. The light excitations thus in...

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Main Authors: Ram Brustein, Yoav Zigdon
Format: Article
Language:English
Published: SpringerOpen 2021-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP10(2021)219
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author Ram Brustein
Yoav Zigdon
author_facet Ram Brustein
Yoav Zigdon
author_sort Ram Brustein
collection DOAJ
description Abstract We calculate the entropy of an asymptotically Schwarzschild black hole, using an effective field theory of winding modes in type II string theory. In Euclidean signature, the geometry of the black hole contains a thermal cycle which shrinks towards the horizon. The light excitations thus include, in addition to the metric and the dilaton, also the winding modes around this cycle. The winding modes condense in the near-horizon region and source the geometry of the thermal cycle. Using the effective field theory action and standard thermodynamic relations, we show that the entropy, which is also sourced by the winding modes condensate, is exactly equal to the Bekenstein-Hawking entropy of the black hole. We then discuss some properties of the winding mode condensate and end with an application of our method to an asymptotically linear-dilaton black hole.
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spelling doaj.art-5078d3771b344657a96c42979f18abbf2022-12-21T21:49:50ZengSpringerOpenJournal of High Energy Physics1029-84792021-10-0120211011410.1007/JHEP10(2021)219Black hole entropy sourced by string winding condensateRam Brustein0Yoav Zigdon1Department of Physics, Ben-Gurion UniversityDepartment of Physics, Ben-Gurion UniversityAbstract We calculate the entropy of an asymptotically Schwarzschild black hole, using an effective field theory of winding modes in type II string theory. In Euclidean signature, the geometry of the black hole contains a thermal cycle which shrinks towards the horizon. The light excitations thus include, in addition to the metric and the dilaton, also the winding modes around this cycle. The winding modes condense in the near-horizon region and source the geometry of the thermal cycle. Using the effective field theory action and standard thermodynamic relations, we show that the entropy, which is also sourced by the winding modes condensate, is exactly equal to the Bekenstein-Hawking entropy of the black hole. We then discuss some properties of the winding mode condensate and end with an application of our method to an asymptotically linear-dilaton black hole.https://doi.org/10.1007/JHEP10(2021)219Black HolesBlack Holes in String TheoryTachyon Condensation
spellingShingle Ram Brustein
Yoav Zigdon
Black hole entropy sourced by string winding condensate
Journal of High Energy Physics
Black Holes
Black Holes in String Theory
Tachyon Condensation
title Black hole entropy sourced by string winding condensate
title_full Black hole entropy sourced by string winding condensate
title_fullStr Black hole entropy sourced by string winding condensate
title_full_unstemmed Black hole entropy sourced by string winding condensate
title_short Black hole entropy sourced by string winding condensate
title_sort black hole entropy sourced by string winding condensate
topic Black Holes
Black Holes in String Theory
Tachyon Condensation
url https://doi.org/10.1007/JHEP10(2021)219
work_keys_str_mv AT rambrustein blackholeentropysourcedbystringwindingcondensate
AT yoavzigdon blackholeentropysourcedbystringwindingcondensate