Fermionic halos at finite temperature in AdS/CFT
- Autores
- Argüelles, Carlos Raúl; Grandi, Nicolás Esteban
- Año de publicación
- 2018
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We explore the gravitational backreaction of a system consisting in a very large number of elementary fermions at finite temperature, in asymptotically AdS space. We work in the hydrodynamic approximation, and solve the Tolman-Oppenheimer-Volkoff equations with a perfect fluid whose equation of state takes into account both the relativistic effects of the fermionic constituents, as well as its finite temperature effects. We find a novel dense core-diluted halo structure for the density profiles in the AdS bulk, similarly as recently reported in flat space, for the case of astrophysical dark matter halos in galaxies. We further study the critical equilibrium configurations above which the core undergoes gravitational collapse towards a massive black hole, and calculate the corresponding critical central temperatures, for two qualitatively different central regimes of the fermions: the diluted-Fermi case, and the degenerate case. As a probe for the dual CFT, we construct the holographic two-point correlator of a scalar operator with large conformal dimension in the worldline limit, and briefly discuss on the boundary CFT effects at the critical points.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Física La Plata - Materia
-
Ciencias Astronómicas
Física
AdS-CFT correspondence
holography and condensed matter physics (AdS/CMT) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/104652
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Fermionic halos at finite temperature in AdS/CFTArgüelles, Carlos RaúlGrandi, Nicolás EstebanCiencias AstronómicasFísicaAdS-CFT correspondenceholography and condensed matter physics (AdS/CMT)We explore the gravitational backreaction of a system consisting in a very large number of elementary fermions at finite temperature, in asymptotically AdS space. We work in the hydrodynamic approximation, and solve the Tolman-Oppenheimer-Volkoff equations with a perfect fluid whose equation of state takes into account both the relativistic effects of the fermionic constituents, as well as its finite temperature effects. We find a novel dense core-diluted halo structure for the density profiles in the AdS bulk, similarly as recently reported in flat space, for the case of astrophysical dark matter halos in galaxies. We further study the critical equilibrium configurations above which the core undergoes gravitational collapse towards a massive black hole, and calculate the corresponding critical central temperatures, for two qualitatively different central regimes of the fermions: the diluted-Fermi case, and the degenerate case. As a probe for the dual CFT, we construct the holographic two-point correlator of a scalar operator with large conformal dimension in the worldline limit, and briefly discuss on the boundary CFT effects at the critical points.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Física La Plata2018info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/104652enginfo:eu-repo/semantics/altIdentifier/url/http://hdl.handle.net/11336/95751info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/JHEP05(2018)118info:eu-repo/semantics/altIdentifier/issn/1029-8479info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP05(2018)118info:eu-repo/semantics/altIdentifier/hdl/11336/95751info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:54:57Zoai:sedici.unlp.edu.ar:10915/104652Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:54:57.375SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Fermionic halos at finite temperature in AdS/CFT |
title |
Fermionic halos at finite temperature in AdS/CFT |
spellingShingle |
Fermionic halos at finite temperature in AdS/CFT Argüelles, Carlos Raúl Ciencias Astronómicas Física AdS-CFT correspondence holography and condensed matter physics (AdS/CMT) |
title_short |
Fermionic halos at finite temperature in AdS/CFT |
title_full |
Fermionic halos at finite temperature in AdS/CFT |
title_fullStr |
Fermionic halos at finite temperature in AdS/CFT |
title_full_unstemmed |
Fermionic halos at finite temperature in AdS/CFT |
title_sort |
Fermionic halos at finite temperature in AdS/CFT |
dc.creator.none.fl_str_mv |
Argüelles, Carlos Raúl Grandi, Nicolás Esteban |
author |
Argüelles, Carlos Raúl |
author_facet |
Argüelles, Carlos Raúl Grandi, Nicolás Esteban |
author_role |
author |
author2 |
Grandi, Nicolás Esteban |
author2_role |
author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Física AdS-CFT correspondence holography and condensed matter physics (AdS/CMT) |
topic |
Ciencias Astronómicas Física AdS-CFT correspondence holography and condensed matter physics (AdS/CMT) |
dc.description.none.fl_txt_mv |
We explore the gravitational backreaction of a system consisting in a very large number of elementary fermions at finite temperature, in asymptotically AdS space. We work in the hydrodynamic approximation, and solve the Tolman-Oppenheimer-Volkoff equations with a perfect fluid whose equation of state takes into account both the relativistic effects of the fermionic constituents, as well as its finite temperature effects. We find a novel dense core-diluted halo structure for the density profiles in the AdS bulk, similarly as recently reported in flat space, for the case of astrophysical dark matter halos in galaxies. We further study the critical equilibrium configurations above which the core undergoes gravitational collapse towards a massive black hole, and calculate the corresponding critical central temperatures, for two qualitatively different central regimes of the fermions: the diluted-Fermi case, and the degenerate case. As a probe for the dual CFT, we construct the holographic two-point correlator of a scalar operator with large conformal dimension in the worldline limit, and briefly discuss on the boundary CFT effects at the critical points. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Física La Plata |
description |
We explore the gravitational backreaction of a system consisting in a very large number of elementary fermions at finite temperature, in asymptotically AdS space. We work in the hydrodynamic approximation, and solve the Tolman-Oppenheimer-Volkoff equations with a perfect fluid whose equation of state takes into account both the relativistic effects of the fermionic constituents, as well as its finite temperature effects. We find a novel dense core-diluted halo structure for the density profiles in the AdS bulk, similarly as recently reported in flat space, for the case of astrophysical dark matter halos in galaxies. We further study the critical equilibrium configurations above which the core undergoes gravitational collapse towards a massive black hole, and calculate the corresponding critical central temperatures, for two qualitatively different central regimes of the fermions: the diluted-Fermi case, and the degenerate case. As a probe for the dual CFT, we construct the holographic two-point correlator of a scalar operator with large conformal dimension in the worldline limit, and briefly discuss on the boundary CFT effects at the critical points. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/104652 |
url |
http://sedici.unlp.edu.ar/handle/10915/104652 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://hdl.handle.net/11336/95751 info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/JHEP05(2018)118 info:eu-repo/semantics/altIdentifier/issn/1029-8479 info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP05(2018)118 info:eu-repo/semantics/altIdentifier/hdl/11336/95751 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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application/pdf |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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