Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity

We construct an axially symmetric solution of Eddington-inspired Born-Infeld gravity coupled to an electromagnetic field in 2 + 1 dimensions including a (negative) cosmological constant term. This is achieved by using a recently developed mapping procedure that allows to generate solutions in certai...

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Detalles Bibliográficos
Autores: Guerrero Román, Mercedes, Mora Pérez, Gerardo, Olmo, Gonzalo J., Orazi, Emanuele, Rubiera García, Diego
Tipo de recurso: artículo
Fecha de publicación:2021
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/4640
Acceso en línea:https://hdl.handle.net/20.500.14352/4640
Access Level:acceso abierto
Palabra clave:51-73
Time
Física-Modelos matemáticos
Física matemática
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spelling Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravityGuerrero Román, MercedesMora Pérez, GerardoOlmo, Gonzalo J.Orazi, EmanueleRubiera García, Diego51-73TimeFísica-Modelos matemáticosFísica matemáticaWe construct an axially symmetric solution of Eddington-inspired Born-Infeld gravity coupled to an electromagnetic field in 2 + 1 dimensions including a (negative) cosmological constant term. This is achieved by using a recently developed mapping procedure that allows to generate solutions in certain families of metric-affine gravity theories starting from a known seed solution of General Relativity, which in the present case corresponds to the electrically charged Banados-Teitelboim-Zanelli (BTZ) solution. We discuss the main features of the new configurations, including the modifications to the ergospheres and horizons, the emergence of wormhole structures, and the consequences for the regularity (or not) of these space-times via geodesic completeness.IOP PublishingUniversidad Complutense de Madrid20212021-11-0120212021-11-01journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/4640reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/46402026-06-02T12:44:21Z
dc.title.none.fl_str_mv Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
title Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
spellingShingle Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
Guerrero Román, Mercedes
51-73
Time
Física-Modelos matemáticos
Física matemática
title_short Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
title_full Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
title_fullStr Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
title_full_unstemmed Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
title_sort Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
dc.creator.none.fl_str_mv Guerrero Román, Mercedes
Mora Pérez, Gerardo
Olmo, Gonzalo J.
Orazi, Emanuele
Rubiera García, Diego
author Guerrero Román, Mercedes
author_facet Guerrero Román, Mercedes
Mora Pérez, Gerardo
Olmo, Gonzalo J.
Orazi, Emanuele
Rubiera García, Diego
author_role author
author2 Mora Pérez, Gerardo
Olmo, Gonzalo J.
Orazi, Emanuele
Rubiera García, Diego
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 51-73
Time
Física-Modelos matemáticos
Física matemática
topic 51-73
Time
Física-Modelos matemáticos
Física matemática
description We construct an axially symmetric solution of Eddington-inspired Born-Infeld gravity coupled to an electromagnetic field in 2 + 1 dimensions including a (negative) cosmological constant term. This is achieved by using a recently developed mapping procedure that allows to generate solutions in certain families of metric-affine gravity theories starting from a known seed solution of General Relativity, which in the present case corresponds to the electrically charged Banados-Teitelboim-Zanelli (BTZ) solution. We discuss the main features of the new configurations, including the modifications to the ergospheres and horizons, the emergence of wormhole structures, and the consequences for the regularity (or not) of these space-times via geodesic completeness.
publishDate 2021
dc.date.none.fl_str_mv 2021
2021-11-01
2021
2021-11-01
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/4640
url https://hdl.handle.net/20.500.14352/4640
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,300724

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