Please use this identifier to cite or link to this item: http://hdl.handle.net/10773/21145
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dc.contributor.authorFerreira, H. R. C.pt
dc.contributor.authorHerdeiro, C. A. R.pt
dc.date.accessioned2017-12-13T12:31:38Z-
dc.date.available2017-12-13T12:31:38Z-
dc.date.issued2017-
dc.identifier.issn0370-2693pt
dc.identifier.urihttp://hdl.handle.net/10773/21145-
dc.description.abstractWe establish the existence of stationary clouds of massive test scalar fields around BTZ black holes. These clouds are zero-modes of the superradiant instability and are possible when Robin boundary conditions (RBCs) are considered at the AdS boundary. These boundary conditions are the most general ones that ensure the AdS space is an isolated system, and include, as a particular case, the commonly considered Dirichlet or Neumann-type boundary conditions (DBCs or NBCs). We obtain an explicit, closed form, resonance condition, relating the RBCs that allow the existence of normalizable (and regular on and outside the horizon) clouds to the system's parameters. Such RBCs never include pure DBCs or NBCs. We illustrate the spatial distribution of these clouds, their energy and angular momentum density for some cases. Our results show that BTZ black holes with scalar hair can be constructed, as the non-linear realization of these clouds. (C) 2017 The Author(s). Published by Elsevier B.V.pt
dc.language.isoengpt
dc.publisherElsevierpt
dc.relationinfo:eu-repo/grantAgreement/EC/H2020/690904/EUpt
dc.relationinfo:eu-repo/grantAgreement/FCT/5876/147206/PTpt
dc.rightsopenAccesspor
dc.titleStationary scalar clouds around a BTZ black holept
dc.typearticlept
dc.peerreviewedyespt
ua.distributioninternationalpt
degois.publication.firstPage129pt
degois.publication.lastPage134pt
degois.publication.titlePhysics Letters Bpt
degois.publication.volume773pt
dc.identifier.doi10.1016/j.physletb.2017.08.017pt
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DFis - Artigos
GGDG - Artigos

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