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
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/104652

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network_name_str SEDICI (UNLP)
spelling 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
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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)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
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instname_str Universidad Nacional de La Plata
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institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
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