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

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dc.contributor.authorGuerrero Román, Mercedes
dc.contributor.authorMora Pérez, Gerardo
dc.contributor.authorOlmo, Gonzalo J.
dc.contributor.authorOrazi, Emanuele
dc.contributor.authorRubiera García, Diego
dc.date.accessioned2023-06-16T14:18:50Z
dc.date.available2023-06-16T14:18:50Z
dc.date.issued2021-11
dc.descriptionMG is funded by the predoctoral contract 2018-T1/TIC-10431. DRG is funded by the Atraccion de Talento Investigador programme of the Comunidad de Madrid (Spain) No. 2018-T1/TIC-10431, and acknowledges further support from the Ministerio de Ciencia, Innovacion y Universidades (Spain) project No. PID2019-108485GB-I00/AEI/10.13039/501100011033, and the FCT projects No. PTDC/FIS-PAR/31938/2017 and PTDC/FIS-OUT/29048/2017. This work is supported by the Spanish projects FIS2017-84440-C2-1-P and PID2020-116567GB-C21 (MINECO/FEDER, EU) , the project PROMETEO/2020/079 (Generali-tat Valenciana) , and the Edital 006/2018 PRONEX (FAPESQ-PB/CNPQ, Brazil, Grant 0015/2019) . This article is based upon work from COST Action CA18108, supported by COST (European Cooperation in Science and Technology) .
dc.description.abstractWe 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.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Economía y Competitividad (MINECO)/FEDER
dc.description.sponsorshipMinisterio de Ciencia e Innovación (MICINN)
dc.description.sponsorshipComunidad de Madrid
dc.description.sponsorshipGeneralitat Valenciana
dc.description.sponsorshipFundação para a Ciência e a Tecnologia (FCT)
dc.description.sponsorshipFAPESQ-PB/CNPQ
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/69606
dc.identifier.doi10.1088/1475-7516/2021/11/025
dc.identifier.issn1475-7516
dc.identifier.officialurlhttp://dx.doi.org/10.1088/1475-7516/2021/11/025
dc.identifier.relatedurlhttps://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/4640
dc.issue.number11
dc.journal.titleJournal of cosmology and astroparticle physics
dc.language.isoeng
dc.publisherIOP Publishing
dc.relation.projectID(PTDC/FIS-PAR/31938/2017; PTDC/FIS-OUT/29048/2017)
dc.relation.projectIDPID2019-108485GB-I00/AEI/10.13039/501100011033
dc.relation.projectID2018-T1/TIC-10431
dc.relation.projectIDPROMETEO/2020/079
dc.relation.projectID(FIS2017-84440-C2-1-P; PID2020-116567GB-C21)
dc.relation.projectID006/2018 PRONEX; 0015/2019
dc.rights.accessRightsopen access
dc.subject.cdu51-73
dc.subject.keywordTime
dc.subject.ucmFísica-Modelos matemáticos
dc.subject.ucmFísica matemática
dc.titleCharged BTZ-type solutions in Eddington-inspired Born-Infeld gravity
dc.typejournal article
dspace.entity.typePublication
relation.isAuthorOfPublication4b7f9b47-e7ee-4161-8023-3d1940a4d6d3
relation.isAuthorOfPublication3729ced5-9cbe-4f32-9550-6f320f10832a
relation.isAuthorOfPublication.latestForDiscovery3729ced5-9cbe-4f32-9550-6f320f10832a

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