Intermediate scalings for solv, nil, and SL2 (R) black branes
- Autores
- Arias, Raúl Eduardo; Landea, Ignacio Salazar
- Año de publicación
- 2019
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In this work, we will study black brane solutions that are not translationally invariant in the spatial directions along which it extends. Instead, we require homogeneity, which still allows points along the spatial directions to be related to each other by symmetries. We find Einstein-Maxwell-anti-de Sitter black hole solutions of which the near-horizon geometry corresponds to solv (Bianchi V1-1), nil (Bianchi II), or SL2(R) (Bianchi VIII). Interestingly, we observe that at intermediate temperatures our solutions have an scaling regime where different spacetime directions scale differently. We also compute the dc conductivities for these charged solutions and study how they scale in this intermediate regime.
Fil: Arias, Raúl Eduardo. Scuola Internazionale Superiore Di Studi Avanzati; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Landea, Ignacio Salazar. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina - Materia
-
General Relativity
Classical solutions
Black brane - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/130075
Ver los metadatos del registro completo
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Intermediate scalings for solv, nil, and SL2 (R) black branesArias, Raúl EduardoLandea, Ignacio SalazarGeneral RelativityClassical solutionsBlack branehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this work, we will study black brane solutions that are not translationally invariant in the spatial directions along which it extends. Instead, we require homogeneity, which still allows points along the spatial directions to be related to each other by symmetries. We find Einstein-Maxwell-anti-de Sitter black hole solutions of which the near-horizon geometry corresponds to solv (Bianchi V1-1), nil (Bianchi II), or SL2(R) (Bianchi VIII). Interestingly, we observe that at intermediate temperatures our solutions have an scaling regime where different spacetime directions scale differently. We also compute the dc conductivities for these charged solutions and study how they scale in this intermediate regime.Fil: Arias, Raúl Eduardo. Scuola Internazionale Superiore Di Studi Avanzati; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Landea, Ignacio Salazar. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaAmerican Physical Society2019-05-31info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/130075Arias, Raúl Eduardo; Landea, Ignacio Salazar; Intermediate scalings for solv, nil, and SL2 (R) black branes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 99; 10; 31-5-2019; 1-142470-00102470-0029CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.99.106015info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.106015info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:37:13Zoai:ri.conicet.gov.ar:11336/130075instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:37:13.869CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Intermediate scalings for solv, nil, and SL2 (R) black branes |
title |
Intermediate scalings for solv, nil, and SL2 (R) black branes |
spellingShingle |
Intermediate scalings for solv, nil, and SL2 (R) black branes Arias, Raúl Eduardo General Relativity Classical solutions Black brane |
title_short |
Intermediate scalings for solv, nil, and SL2 (R) black branes |
title_full |
Intermediate scalings for solv, nil, and SL2 (R) black branes |
title_fullStr |
Intermediate scalings for solv, nil, and SL2 (R) black branes |
title_full_unstemmed |
Intermediate scalings for solv, nil, and SL2 (R) black branes |
title_sort |
Intermediate scalings for solv, nil, and SL2 (R) black branes |
dc.creator.none.fl_str_mv |
Arias, Raúl Eduardo Landea, Ignacio Salazar |
author |
Arias, Raúl Eduardo |
author_facet |
Arias, Raúl Eduardo Landea, Ignacio Salazar |
author_role |
author |
author2 |
Landea, Ignacio Salazar |
author2_role |
author |
dc.subject.none.fl_str_mv |
General Relativity Classical solutions Black brane |
topic |
General Relativity Classical solutions Black brane |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
In this work, we will study black brane solutions that are not translationally invariant in the spatial directions along which it extends. Instead, we require homogeneity, which still allows points along the spatial directions to be related to each other by symmetries. We find Einstein-Maxwell-anti-de Sitter black hole solutions of which the near-horizon geometry corresponds to solv (Bianchi V1-1), nil (Bianchi II), or SL2(R) (Bianchi VIII). Interestingly, we observe that at intermediate temperatures our solutions have an scaling regime where different spacetime directions scale differently. We also compute the dc conductivities for these charged solutions and study how they scale in this intermediate regime. Fil: Arias, Raúl Eduardo. Scuola Internazionale Superiore Di Studi Avanzati; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Landea, Ignacio Salazar. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina |
description |
In this work, we will study black brane solutions that are not translationally invariant in the spatial directions along which it extends. Instead, we require homogeneity, which still allows points along the spatial directions to be related to each other by symmetries. We find Einstein-Maxwell-anti-de Sitter black hole solutions of which the near-horizon geometry corresponds to solv (Bianchi V1-1), nil (Bianchi II), or SL2(R) (Bianchi VIII). Interestingly, we observe that at intermediate temperatures our solutions have an scaling regime where different spacetime directions scale differently. We also compute the dc conductivities for these charged solutions and study how they scale in this intermediate regime. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-05-31 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://hdl.handle.net/11336/130075 Arias, Raúl Eduardo; Landea, Ignacio Salazar; Intermediate scalings for solv, nil, and SL2 (R) black branes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 99; 10; 31-5-2019; 1-14 2470-0010 2470-0029 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/130075 |
identifier_str_mv |
Arias, Raúl Eduardo; Landea, Ignacio Salazar; Intermediate scalings for solv, nil, and SL2 (R) black branes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 99; 10; 31-5-2019; 1-14 2470-0010 2470-0029 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.99.106015 info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.106015 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
American Physical Society |
publisher.none.fl_str_mv |
American Physical Society |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844614392117723136 |
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13.070432 |