Charged rotating black holes in Einstein-Maxwell-Chern-Simons theory with a negative cosmological constant

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dc.contributor.authorBlázquez Salcedo, José Luis
dc.contributor.authorKunz, Jutta
dc.contributor.authorNavarro Lérida, Francisco
dc.contributor.authorRadu, Eugen
dc.date.accessioned2023-06-17T22:00:28Z
dc.date.available2023-06-17T22:00:28Z
dc.date.issued2017-03-13
dc.description© 2017 American Physical Society. J.L.B.S. would like to thank Robert Mann and Carlos Herdeiro for helpful comments and discussions. We gratefully acknowledge support by the DFG Research Training Group 1620 "Models of Gravity." E.R. acknowledges funding from the FCT-IF program. This work was also partially supported by the H2020-MSCA-RISE-2015 Grant No. StronGrHEP-690904 and by CIDMA Project No. UID/MAT/04106/2013. J.L.B.S. and J.K. gratefully acknowledge support by the grant FP7, Marie Curie Actions, People, International Research Staff Exchange Scheme (Grant No. IRSES-606096). F.N.-L. acknowledges funding from Complutense University under Project No. PR26/16-20312.
dc.description.abstractWe consider rotating black hole solutions in five-dimensional Einstein-Maxwell-Chern-Simons theory with a negative cosmological constant and a generic value of the Chern-Simons coupling constant.. Using both analytical and numerical techniques, we focus on cohomogeneity-1 configurations, with two equal-magnitude angular momenta, which approach at infinity a globally anti-de Sitter background. We find that the generic solutions share a number of basic properties with the known Cvetic, Lu, and Pope black holes which have lambda = 1. New features occur as well; for example, when the Chern-Simons coupling constant exceeds a critical value, the solutions are no longer uniquely determined by their global charges. Moreover, the black holes possess radial excitations which can be labelled by the node number of the magnetic gauge potential function. Solutions with small values of. possess other distinct features. For instance, the extremal black holes there form two disconnected branches, while not all near-horizon solutions are associated with global solutions.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. H2020
dc.description.sponsorshipUnión Europea. PF7
dc.description.sponsorshipUniversidad Complutense de Madrid
dc.description.sponsorshipDFG
dc.description.sponsorshipFCT-IF program
dc.description.sponsorshipCIDMA
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/43823
dc.identifier.doi10.1103/PhysRevD.95.064018
dc.identifier.issn2470-0010
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevD.95.064018
dc.identifier.relatedurlhttps://journals.aps.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/17919
dc.issue.number6
dc.journal.titlePhysical review D
dc.language.isoeng
dc.publisherAmer Physical Soc
dc.relation.projectIDStronGrHEP (690904)
dc.relation.projectIDOPTI-VFA (606096)
dc.relation.projectIDPR26/16-20312
dc.relation.projectIDUID/MAT/04106/2013
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordGauged supergravity
dc.subject.keyword5 dimensions
dc.subject.keywordSymmetries
dc.subject.keywordSpace
dc.subject.keywordHair
dc.subject.keywordMass
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleCharged rotating black holes in Einstein-Maxwell-Chern-Simons theory with a negative cosmological constant
dc.typejournal article
dc.volume.number95
dspace.entity.typePublication
relation.isAuthorOfPublication2a6d99a8-5cf7-4359-b1e1-b96adfb2fb3f
relation.isAuthorOfPublication.latestForDiscovery2a6d99a8-5cf7-4359-b1e1-b96adfb2fb3f
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