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The Supersymmetric Index and its Holographic Interpretation

<!--HTML--><p>The supersymmetric index of N=4 SU(N) Super Yang-Mills&nbsp;is a well studied quantity. In <a href="https://arxiv.org/abs/2104.13932">2104.13932</a> we analyzed it using the Bethe Ansatz approach, expressed it as a sum and concentrated on some fami...

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Autor principal: Mamroud, Ohad
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:http://cds.cern.ch/record/2838635
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author Mamroud, Ohad
author_facet Mamroud, Ohad
author_sort Mamroud, Ohad
collection CERN
description <!--HTML--><p>The supersymmetric index of N=4 SU(N) Super Yang-Mills&nbsp;is a well studied quantity. In <a href="https://arxiv.org/abs/2104.13932">2104.13932</a> we analyzed it using the Bethe Ansatz approach, expressed it as a sum and concentrated on some family of contributions to it. In the large N limit each term in this family corresponds to the contribution of a different euclidean black hole to the partition function of the dual gravitational theory. By taking into account non-perturbative contributions (wrapped D3-branes), we further showed a one to one match between the contributions of the gravitational saddles and this family of contributions to the index, both at the perturbative and non-perturbative levels. I'll end with some newer results, concerning the form of these terms at finite N, and new solutions to the Bethe Ansatz equations (i.e. additional contributions to the index beyond the ones described in that paper).</p>
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institution Organización Europea para la Investigación Nuclear
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spelling cern-28386352022-11-02T22:03:08Zhttp://cds.cern.ch/record/2838635engMamroud, OhadThe Supersymmetric Index and its Holographic InterpretationThe Supersymmetric Index and its Holographic InterpretationTH String Theory Seminar<!--HTML--><p>The supersymmetric index of N=4 SU(N) Super Yang-Mills&nbsp;is a well studied quantity. In <a href="https://arxiv.org/abs/2104.13932">2104.13932</a> we analyzed it using the Bethe Ansatz approach, expressed it as a sum and concentrated on some family of contributions to it. In the large N limit each term in this family corresponds to the contribution of a different euclidean black hole to the partition function of the dual gravitational theory. By taking into account non-perturbative contributions (wrapped D3-branes), we further showed a one to one match between the contributions of the gravitational saddles and this family of contributions to the index, both at the perturbative and non-perturbative levels. I'll end with some newer results, concerning the form of these terms at finite N, and new solutions to the Bethe Ansatz equations (i.e. additional contributions to the index beyond the ones described in that paper).</p>oai:cds.cern.ch:28386352022
spellingShingle TH String Theory Seminar
Mamroud, Ohad
The Supersymmetric Index and its Holographic Interpretation
title The Supersymmetric Index and its Holographic Interpretation
title_full The Supersymmetric Index and its Holographic Interpretation
title_fullStr The Supersymmetric Index and its Holographic Interpretation
title_full_unstemmed The Supersymmetric Index and its Holographic Interpretation
title_short The Supersymmetric Index and its Holographic Interpretation
title_sort supersymmetric index and its holographic interpretation
topic TH String Theory Seminar
url http://cds.cern.ch/record/2838635
work_keys_str_mv AT mamroudohad thesupersymmetricindexanditsholographicinterpretation
AT mamroudohad supersymmetricindexanditsholographicinterpretation