Circular geodesics stability in a static black hole in new massive gravity
- Autores
- Aceña, Andrés Esteban; López, Ericson; Aldás, Franklin
- Año de publicación
- 2020
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We study the existence and stability of circular geodesics in a family of asymptotically AdS static black holes in New Massive Gravity theory. We show that the mathematical sign of the hair parameter determines the existence of such geodesics. For a positive hair parameter, the stability regions follow the usual pattern, with the innermost geodesic being null, unstable, and separated from the horizon, followed by a region of unstable timelike geodesics and then a region of stable timelike geodesics, which extends in the asymptotic region.
Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Fil: López, Ericson. Escuela Politécnica Nacional; Ecuador
Fil: Aldás, Franklin. Escuela Politécnica Nacional; Ecuador - Materia
-
BLACK HOLES
CIRCULAR GEODESICS
NEW MASSIVE GRAVITY - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/139815
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Circular geodesics stability in a static black hole in new massive gravityAceña, Andrés EstebanLópez, EricsonAldás, FranklinBLACK HOLESCIRCULAR GEODESICSNEW MASSIVE GRAVITYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study the existence and stability of circular geodesics in a family of asymptotically AdS static black holes in New Massive Gravity theory. We show that the mathematical sign of the hair parameter determines the existence of such geodesics. For a positive hair parameter, the stability regions follow the usual pattern, with the innermost geodesic being null, unstable, and separated from the horizon, followed by a region of unstable timelike geodesics and then a region of stable timelike geodesics, which extends in the asymptotic region.Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; ArgentinaFil: López, Ericson. Escuela Politécnica Nacional; EcuadorFil: Aldás, Franklin. Escuela Politécnica Nacional; EcuadorMolecular Diversity Preservation International2020-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/139815Aceña, Andrés Esteban; López, Ericson; Aldás, Franklin; Circular geodesics stability in a static black hole in new massive gravity; Molecular Diversity Preservation International; Galaxies; 8; 1; 2-2020; 1-82075-4434CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.mdpi.com/2075-4434/8/1/14info:eu-repo/semantics/altIdentifier/doi/10.3390/galaxies8010014info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:09:00Zoai:ri.conicet.gov.ar:11336/139815instacron: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:34982025-09-10 13:09:01.232CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Circular geodesics stability in a static black hole in new massive gravity |
title |
Circular geodesics stability in a static black hole in new massive gravity |
spellingShingle |
Circular geodesics stability in a static black hole in new massive gravity Aceña, Andrés Esteban BLACK HOLES CIRCULAR GEODESICS NEW MASSIVE GRAVITY |
title_short |
Circular geodesics stability in a static black hole in new massive gravity |
title_full |
Circular geodesics stability in a static black hole in new massive gravity |
title_fullStr |
Circular geodesics stability in a static black hole in new massive gravity |
title_full_unstemmed |
Circular geodesics stability in a static black hole in new massive gravity |
title_sort |
Circular geodesics stability in a static black hole in new massive gravity |
dc.creator.none.fl_str_mv |
Aceña, Andrés Esteban López, Ericson Aldás, Franklin |
author |
Aceña, Andrés Esteban |
author_facet |
Aceña, Andrés Esteban López, Ericson Aldás, Franklin |
author_role |
author |
author2 |
López, Ericson Aldás, Franklin |
author2_role |
author author |
dc.subject.none.fl_str_mv |
BLACK HOLES CIRCULAR GEODESICS NEW MASSIVE GRAVITY |
topic |
BLACK HOLES CIRCULAR GEODESICS NEW MASSIVE GRAVITY |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We study the existence and stability of circular geodesics in a family of asymptotically AdS static black holes in New Massive Gravity theory. We show that the mathematical sign of the hair parameter determines the existence of such geodesics. For a positive hair parameter, the stability regions follow the usual pattern, with the innermost geodesic being null, unstable, and separated from the horizon, followed by a region of unstable timelike geodesics and then a region of stable timelike geodesics, which extends in the asymptotic region. Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina Fil: López, Ericson. Escuela Politécnica Nacional; Ecuador Fil: Aldás, Franklin. Escuela Politécnica Nacional; Ecuador |
description |
We study the existence and stability of circular geodesics in a family of asymptotically AdS static black holes in New Massive Gravity theory. We show that the mathematical sign of the hair parameter determines the existence of such geodesics. For a positive hair parameter, the stability regions follow the usual pattern, with the innermost geodesic being null, unstable, and separated from the horizon, followed by a region of unstable timelike geodesics and then a region of stable timelike geodesics, which extends in the asymptotic region. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-02 |
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/11336/139815 Aceña, Andrés Esteban; López, Ericson; Aldás, Franklin; Circular geodesics stability in a static black hole in new massive gravity; Molecular Diversity Preservation International; Galaxies; 8; 1; 2-2020; 1-8 2075-4434 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/139815 |
identifier_str_mv |
Aceña, Andrés Esteban; López, Ericson; Aldás, Franklin; Circular geodesics stability in a static black hole in new massive gravity; Molecular Diversity Preservation International; Galaxies; 8; 1; 2-2020; 1-8 2075-4434 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://www.mdpi.com/2075-4434/8/1/14 info:eu-repo/semantics/altIdentifier/doi/10.3390/galaxies8010014 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Molecular Diversity Preservation International |
publisher.none.fl_str_mv |
Molecular Diversity Preservation International |
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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1842980436884586496 |
score |
12.993085 |