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Nearly BPS black holes and the spectrum of N=4 Yang Mills
<!--HTML--><p>We will discuss quantum corrections in the gravitational path integral around nearly 1/16-BPS black holes in asymptotically AdS5 x S5 space, dual to heavy operators in N=4 SYM. These quantum corrections come from a version of the N=2 super-Schwarzian theory which captures t...
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| Lenguaje: | eng |
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2022
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| Acceso en línea: | http://cds.cern.ch/record/2806616 |
| _version_ | 1780973004654641152 |
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| author | Turiaci, Gustavo Joaquin |
| author_facet | Turiaci, Gustavo Joaquin |
| author_sort | Turiaci, Gustavo Joaquin |
| collection | CERN |
| description | <!--HTML--><p>We will discuss quantum corrections in the gravitational path integral around nearly 1/16-BPS black holes in asymptotically AdS5 x S5 space, dual to heavy operators in N=4 SYM. These quantum corrections come from a version of the N=2 super-Schwarzian theory which captures the breaking of the SU(1,1|1) near horizon symmetry at finite temperature and chemical potential. Using this approach, holography predicts the presence of a gap between the BPS black holes and the lightest near-BPS black holes, and the spectrum of near-BPS states that lie above this gap. We will also discuss stringy and non-perturbative corrections that can affect the black hole spectrum.</p> |
| id | cern-2806616 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2022 |
| record_format | invenio |
| spelling | cern-28066162022-11-02T22:05:13Zhttp://cds.cern.ch/record/2806616engTuriaci, Gustavo Joaquin Nearly BPS black holes and the spectrum of N=4 Yang MillsNearly BPS black holes and the spectrum of N=4 Yang MillsTH String Theory Seminar<!--HTML--><p>We will discuss quantum corrections in the gravitational path integral around nearly 1/16-BPS black holes in asymptotically AdS5 x S5 space, dual to heavy operators in N=4 SYM. These quantum corrections come from a version of the N=2 super-Schwarzian theory which captures the breaking of the SU(1,1|1) near horizon symmetry at finite temperature and chemical potential. Using this approach, holography predicts the presence of a gap between the BPS black holes and the lightest near-BPS black holes, and the spectrum of near-BPS states that lie above this gap. We will also discuss stringy and non-perturbative corrections that can affect the black hole spectrum.</p>oai:cds.cern.ch:28066162022 |
| spellingShingle | TH String Theory Seminar Turiaci, Gustavo Joaquin Nearly BPS black holes and the spectrum of N=4 Yang Mills |
| title | Nearly BPS black holes and the spectrum of N=4 Yang Mills |
| title_full | Nearly BPS black holes and the spectrum of N=4 Yang Mills |
| title_fullStr | Nearly BPS black holes and the spectrum of N=4 Yang Mills |
| title_full_unstemmed | Nearly BPS black holes and the spectrum of N=4 Yang Mills |
| title_short | Nearly BPS black holes and the spectrum of N=4 Yang Mills |
| title_sort | nearly bps black holes and the spectrum of n=4 yang mills |
| topic | TH String Theory Seminar |
| url | http://cds.cern.ch/record/2806616 |
| work_keys_str_mv | AT turiacigustavojoaquin nearlybpsblackholesandthespectrumofn4yangmills |