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Radially excited rotating black holes in Einstein-Maxwell-Chern-Simons theory

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dc.contributor.authorBlázquez Salcedo, José Luis
dc.contributor.authorKunz, Jutta
dc.contributor.authorNavarro Lerida, Francisco
dc.contributor.authorRadu, Eugen
dc.date.accessioned2023-06-18T06:48:04Z
dc.date.available2023-06-18T06:48:04Z
dc.date.issued2015-08-17
dc.description© 2015 American Physical Society. We gratefully acknowledge support by the DFG Research Training Group 1620 "Models of Gravity" and by the Spanish Ministerio de Ciencia e Innovacion, research Project No. FIS2011-28013. The work of E. R. is supported by the FCT-IF programme and the CIDMA strategic Project No. UID/MAT/04106/2013.
dc.description.abstractRotating black holes in Einstein-Maxwell-Chern-Simons theory possess remarkable features when the Chern-Simons coupling constant reaches a critical value. Representing single asymptotically flat black holes with horizons of spherical topology, they exhibit nonuniqueness. In particular, there even exist extremal and nonextremal black holes with the same sets of global charges. Both extremal and nonextremal black holes form sequences of radially excited solutions that can be labeled by the node number of the magnetic gauge potential function. The extremal Reissner-Nordstrm solution is no longer always located on the boundary of the domain of existence of these black holes, nor does it remain the single extremal solution with vanishing angular momentum. Instead a whole sequence of rotating extremal J = 0 solutions is present, whose mass converges towards the mass of the Reissner-Nordstrm solution. These radially excited extremal solutions are all associated with the same near horizon solution. Moreover, there are near horizon solutions that are not realized as 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.sponsorshipMinisterio de Ciencia e Innovacion (MICINN)
dc.description.sponsorshipDFG Research Training Group "Models of Gravity
dc.description.sponsorshipFCT-IF programme
dc.description.sponsorshipCIDMA strategic Project
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/33864
dc.identifier.doi10.1103/PhysRevD.92.044025
dc.identifier.issn1550-7998
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevD.92.044025
dc.identifier.relatedurlhttp://journals.aps.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/24230
dc.issue.number4
dc.journal.titlePhysicall Review D
dc.language.isoeng
dc.publisherAmer Physical Soc
dc.relation.projectIDFIS2011-28013
dc.relation.projectID1620
dc.relation.projectIDUID/MAT/04106/2013
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordOdd dimensions
dc.subject.keywordUniqueness
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleRadially excited rotating black holes in Einstein-Maxwell-Chern-Simons theory
dc.typejournal article
dc.volume.number92
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