Please use this identifier to cite or link to this item: http://hdl.handle.net/10773/27049
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dc.contributor.authorFernandes, Pedro G. S.pt_PT
dc.contributor.authorHerdeiro, Carlos A. R.pt_PT
dc.contributor.authorPombo, Alexandre M.pt_PT
dc.contributor.authorRadu, Eugenpt_PT
dc.contributor.authorSanchis-Gual, Nicolaspt_PT
dc.date.accessioned2019-11-27T10:51:45Z-
dc.date.available2019-11-27T10:51:45Z-
dc.date.issued2019-10-21-
dc.identifier.issn2470-0010pt_PT
dc.identifier.urihttp://hdl.handle.net/10773/27049-
dc.description.abstractWe consider an augmented Einstein-Maxwell-scalar model including an axionic-type coupling between the scalar and electromagnetic field. We study dyonic black hole solutions in this model. For the canonical axionic coupling emerging from high energy physics, all charged black holes have axion hair. We present their domain of existence and investigate some physical properties. For other axionic-type couplings, two classes of black hole solutions may coexist in the model: scalar-free Reissner-Nordström black holes and scalarized black holes. We show that in some region of the parameter space the scalar-free solutions are unstable. Then, there is nonuniqueness since new scalarized black hole solutions with the same global charges, which are entropically preferred over the scalar-free solutions and, moreover, emerge dynamically from the instability of the former, also exist.pt_PT
dc.language.isoengpt_PT
dc.publisherAmerican Physical Societypt_PT
dc.relationUID/MAT/04106/2019pt_PT
dc.relationinfo:eu-repo/grantAgreement/FCT/5876/147212/PTpt_PT
dc.relationPTDC/FIS-OUT/28407/2017pt_PT
dc.relationPD/BD/142842/2018pt_PT
dc.relationStronGrHEP-690904pt_PT
dc.relationFunFiCO-777740pt_PT
dc.rightsopenAccesspt_PT
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/pt_PT
dc.subjectBlack holespt_PT
dc.titleCharged black holes with axionic-type couplings: classes of solutions and dynamical scalarizationpt_PT
dc.typearticlept_PT
dc.description.versionpublishedpt_PT
dc.peerreviewedyespt_PT
degois.publication.titlePhysical Review Dpt_PT
degois.publication.volume100pt_PT
dc.relation.publisherversionhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.100.084045pt_PT
dc.identifier.doi10.1103/PhysRevD.100.084045pt_PT
dc.identifier.essn2470-0029pt_PT
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