Squashed, magnetized black holes in D=5 minimal gauged supergravity

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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.accessioned2023-06-17T12:26:30Z
dc.date.available2023-06-17T12:26:30Z
dc.date.issued2018-02-09
dc.description© 2018 Springer. We gratefully acknowledge support by the DFG Research Training Group 1620 "Models of Gravity". E. R. acknowledges funding from the FCT-IF programme. This work was also partially supported by the H2020-MSCA-RISE-2015 Grant No. StronGrHEP-690904, and by the CIDMA project UID/MAT/04106/2013. F. N.-L. acknowledges funding from Complutense University - Santander under project PR26/16-20312. J. L. B.-S. and J. K. acknowledge support from FP7, Marie Curie Actions, People, International Research Staff Exchange Scheme (IRSES-606096).
dc.description.abstractWe construct a new class of black hole solutions in five-dimensional Einstein-Maxwell-Chern-Simons theory with a negative cosmological constant. These configurations are cohomogeneity-1, with two equal-magnitude angular momenta. In the generic case, they possess a non-vanishing magnetic potential at infinity with a boundary metric which is the product of time and a squashed three-dimensional sphere. Both extremal and non-extremal black holes are studied. The non-extremal black holes satisfying a certain relation between electric charge, angular momenta and magnitude of the magnetic potential at infinity do not trivialize in the limit of vanishing event horizon size, becoming particle-like (non-topological) solitonic configurations. Among the extremal black holes, we show the existence of a new one-parameter family of supersymmetric solutions, which bifurcate from a critical Gutowski-Reall configuration.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. H2020
dc.description.sponsorshipUnión Europea. FP7
dc.description.sponsorshipDFG Research Training Group
dc.description.sponsorshipFCT-IF programme
dc.description.sponsorshipCIDMA
dc.description.sponsorshipUniversidad Complutense de Madrid/Banco de Santander
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/47044
dc.identifier.doi10.1007/JHEP02(2018)061
dc.identifier.issn1029-8479
dc.identifier.officialurlhttp://dx.doi.org/10.1007/JHEP02(2018)061
dc.identifier.relatedurlhttps://link.springer.com/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/12014
dc.issue.number2
dc.journal.titleJournal of high energy physics
dc.language.isoeng
dc.publisherSpringer
dc.relation.projectIDStronGrHEP (690904)
dc.relation.projectIDIRSES (606096)
dc.relation.projectID1620
dc.relation.projectIDUID/MAT/04106/2013
dc.relation.projectIDPR26/16-20312
dc.rightsAtribución 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es/
dc.subject.cdu53
dc.subject.keywordCosmological constant
dc.subject.keyword5 dimensions
dc.subject.keywordSpacetimes
dc.subject.keywordHolography
dc.subject.keywordRotation
dc.subject.keywordStrings
dc.subject.keywordTensor.
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleSquashed, magnetized black holes in D=5 minimal gauged supergravity
dc.typejournal article
dspace.entity.typePublication
relation.isAuthorOfPublication2a6d99a8-5cf7-4359-b1e1-b96adfb2fb3f
relation.isAuthorOfPublication.latestForDiscovery2a6d99a8-5cf7-4359-b1e1-b96adfb2fb3f
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