Wilson surface central charge from holographic entanglement entropy
Abstract We use entanglement entropy to define a central charge associated to a twodimensional defect or boundary in a conformal field theory (CFT). We present holographic calculations of this central charge for several maximally supersymmetric CFTs dual to eleven-dimensional supergravity in Anti-de...
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doaj-76962f6b301e4097a9f0908bf41577c92020-11-25T02:55:17ZengSpringerOpenJournal of High Energy Physics1029-84792019-05-012019515310.1007/JHEP05(2019)032Wilson surface central charge from holographic entanglement entropyJohn Estes0Darya Krym1Andy O’Bannon2Brandon Robinson3Ronnie Rodgers4New York City College of Technology, City University of New YorkNew York City College of Technology, City University of New YorkSTAG Research Centre, Physics and Astronomy, University of SouthamptonSTAG Research Centre, Physics and Astronomy, University of SouthamptonSTAG Research Centre, Physics and Astronomy, University of SouthamptonAbstract We use entanglement entropy to define a central charge associated to a twodimensional defect or boundary in a conformal field theory (CFT). We present holographic calculations of this central charge for several maximally supersymmetric CFTs dual to eleven-dimensional supergravity in Anti-de Sitter space, namely the M5-brane theory with a Wilson surface defect and three-dimensional CFTs related to the M2-brane theory with a boundary. Our results for the central charge depend on a partition of N M2-branes ending on M M5-branes. For the Wilson surface, the partition specifies a representation of the gauge algebra, and we write our result for the central charge in a compact form in terms of the algebra’s Weyl vector and the representation’s highest weight vector. We explore how the central charge scales with N and M for some examples of partitions. In general the central charge does not scale as M 3 or N 3/2, the number of degrees of freedom of the M5- or M2-brane theory at large M or N , respectively.http://link.springer.com/article/10.1007/JHEP05(2019)032AdS-CFT CorrespondenceGauge-gravity correspondenceM-Theoryp-branes |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
John Estes Darya Krym Andy O’Bannon Brandon Robinson Ronnie Rodgers |
spellingShingle |
John Estes Darya Krym Andy O’Bannon Brandon Robinson Ronnie Rodgers Wilson surface central charge from holographic entanglement entropy Journal of High Energy Physics AdS-CFT Correspondence Gauge-gravity correspondence M-Theory p-branes |
author_facet |
John Estes Darya Krym Andy O’Bannon Brandon Robinson Ronnie Rodgers |
author_sort |
John Estes |
title |
Wilson surface central charge from holographic entanglement entropy |
title_short |
Wilson surface central charge from holographic entanglement entropy |
title_full |
Wilson surface central charge from holographic entanglement entropy |
title_fullStr |
Wilson surface central charge from holographic entanglement entropy |
title_full_unstemmed |
Wilson surface central charge from holographic entanglement entropy |
title_sort |
wilson surface central charge from holographic entanglement entropy |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2019-05-01 |
description |
Abstract We use entanglement entropy to define a central charge associated to a twodimensional defect or boundary in a conformal field theory (CFT). We present holographic calculations of this central charge for several maximally supersymmetric CFTs dual to eleven-dimensional supergravity in Anti-de Sitter space, namely the M5-brane theory with a Wilson surface defect and three-dimensional CFTs related to the M2-brane theory with a boundary. Our results for the central charge depend on a partition of N M2-branes ending on M M5-branes. For the Wilson surface, the partition specifies a representation of the gauge algebra, and we write our result for the central charge in a compact form in terms of the algebra’s Weyl vector and the representation’s highest weight vector. We explore how the central charge scales with N and M for some examples of partitions. In general the central charge does not scale as M 3 or N 3/2, the number of degrees of freedom of the M5- or M2-brane theory at large M or N , respectively. |
topic |
AdS-CFT Correspondence Gauge-gravity correspondence M-Theory p-branes |
url |
http://link.springer.com/article/10.1007/JHEP05(2019)032 |
work_keys_str_mv |
AT johnestes wilsonsurfacecentralchargefromholographicentanglemententropy AT daryakrym wilsonsurfacecentralchargefromholographicentanglemententropy AT andyobannon wilsonsurfacecentralchargefromholographicentanglemententropy AT brandonrobinson wilsonsurfacecentralchargefromholographicentanglemententropy AT ronnierodgers wilsonsurfacecentralchargefromholographicentanglemententropy |
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1724716899648929792 |