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Quasi-normal modes of electromagnetic perturbations of four-dimensional topological black holes with scalar hair

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dc.contributor.author Koutsoumbas, G en
dc.contributor.author Musiri, S en
dc.contributor.author Papantonopoulos, E en
dc.contributor.author Siopsis, G en
dc.date.accessioned 2014-03-01T11:44:43Z
dc.date.available 2014-03-01T11:44:43Z
dc.date.issued 2006 en
dc.identifier.issn 1126-6708 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/37111
dc.subject Black Holes en
dc.subject Classical Theories of Gravity en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other DE-SITTER SPACE en
dc.subject.other FIELD HAIR en
dc.subject.other STABILITY en
dc.subject.other SUPERGRAVITY en
dc.subject.other HORIZONS en
dc.title Quasi-normal modes of electromagnetic perturbations of four-dimensional topological black holes with scalar hair en
heal.type other en
heal.identifier.primary 10.1088/1126-6708/2006/10/006 en
heal.identifier.secondary http://dx.doi.org/10.1088/1126-6708/2006/10/006 en
heal.identifier.secondary 006 en
heal.language English en
heal.publicationDate 2006 en
heal.abstract We study the perturbative behaviour of topological black holes with scalar hair. We calculate both analytically and numerically the quasi-normal modes of the electromagnetic perturbations. In the case of small black holes we find evidence of a second-order phase transition of a topological black hole to a hairy configuration. © SISSA 2006. en
heal.publisher INT SCHOOL ADVANCED STUDIES en
heal.journalName Journal of High Energy Physics en
dc.identifier.doi 10.1088/1126-6708/2006/10/006 en
dc.identifier.isi ISI:000242714400084 en
dc.identifier.volume 2006 en
dc.identifier.issue 10 en


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