Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYM
Abstract We numerically construct static localized black holes in ten spacetime dimensions with one compact periodic dimension. In particular, we investigate the critical regime in which the poles of the localized black hole are about to merge. When approaching the critical region, the behavior of p...
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Online Access: | http://link.springer.com/article/10.1007/JHEP11(2018)090 |
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doaj-9181b056020e424e8f5db7e119de29962020-11-25T02:07:40ZengSpringerOpenJournal of High Energy Physics1029-84792018-11-0120181112010.1007/JHEP11(2018)090Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYMMartin Ammon0Michael Kalisch1Sebastian Moeckel2Theoretisch-Physikalisches Institutss, Friedrich-Schiller-Universität JenaTheoretisch-Physikalisches Institutss, Friedrich-Schiller-Universität JenaTheoretisch-Physikalisches Institutss, Friedrich-Schiller-Universität JenaAbstract We numerically construct static localized black holes in ten spacetime dimensions with one compact periodic dimension. In particular, we investigate the critical regime in which the poles of the localized black hole are about to merge. When approaching the critical region, the behavior of physical quantities is described by a single real valued exponent giving rise to a logarithmic scaling of the thermodynamic quantities, in agreement with the theoretical prediction derived from the double-cone metric. As a peculiarity, the localized black hole solution in ten dimensions can be related to the spatially deconfined phase of two dimensional N = 8 8 $$ \mathcal{N}=\left(8,8\right) $$ super Yang-Mills theory (SYM) on a spatial circle. We use the localized black hole solutions to determine the SYM phase diagram. In particular, we compute the location of the first order phase confinement/deconfinement transition and the related latent heat to unprecedented accuracy.http://link.springer.com/article/10.1007/JHEP11(2018)090Black HolesClassical Theories of GravityGauge-gravity correspondence |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Martin Ammon Michael Kalisch Sebastian Moeckel |
spellingShingle |
Martin Ammon Michael Kalisch Sebastian Moeckel Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYM Journal of High Energy Physics Black Holes Classical Theories of Gravity Gauge-gravity correspondence |
author_facet |
Martin Ammon Michael Kalisch Sebastian Moeckel |
author_sort |
Martin Ammon |
title |
Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYM |
title_short |
Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYM |
title_full |
Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYM |
title_fullStr |
Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYM |
title_full_unstemmed |
Notes on ten-dimensional localized black holes and deconfined states in two-dimensional SYM |
title_sort |
notes on ten-dimensional localized black holes and deconfined states in two-dimensional sym |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2018-11-01 |
description |
Abstract We numerically construct static localized black holes in ten spacetime dimensions with one compact periodic dimension. In particular, we investigate the critical regime in which the poles of the localized black hole are about to merge. When approaching the critical region, the behavior of physical quantities is described by a single real valued exponent giving rise to a logarithmic scaling of the thermodynamic quantities, in agreement with the theoretical prediction derived from the double-cone metric. As a peculiarity, the localized black hole solution in ten dimensions can be related to the spatially deconfined phase of two dimensional N = 8 8 $$ \mathcal{N}=\left(8,8\right) $$ super Yang-Mills theory (SYM) on a spatial circle. We use the localized black hole solutions to determine the SYM phase diagram. In particular, we compute the location of the first order phase confinement/deconfinement transition and the related latent heat to unprecedented accuracy. |
topic |
Black Holes Classical Theories of Gravity Gauge-gravity correspondence |
url |
http://link.springer.com/article/10.1007/JHEP11(2018)090 |
work_keys_str_mv |
AT martinammon notesontendimensionallocalizedblackholesanddeconfinedstatesintwodimensionalsym AT michaelkalisch notesontendimensionallocalizedblackholesanddeconfinedstatesintwodimensionalsym AT sebastianmoeckel notesontendimensionallocalizedblackholesanddeconfinedstatesintwodimensionalsym |
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1724930411806588928 |