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

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DC Field	Value	Language
dc.contributor.author	Koutsoumbas G.
dc.contributor.author	Musiri S.
dc.contributor.author	Papantonopoulos E.
dc.contributor.author	Siopsis G.
dc.date.accessioned	2021-04-05T04:32:19Z	-
dc.date.available	2021-04-05T04:32:19Z	-
dc.date.issued	2006
dc.identifier.issn	10298479
dc.identifier.other	2-s2.0-33846168776
dc.identifier.uri	https://ir.swu.ac.th/jspui/handle/123456789/15003	-
dc.identifier.uri	https://www.scopus.com/inward/record.uri?eid=2-s2.0-33846168776&doi=10.1088%2f1126-6708%2f2006%2f10%2f006&partnerID=40&md5=2873f9cb8f4f04b09e5af99e96cddc8e
dc.description.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.
dc.title	Quasi-normal modes of electromagnetic perturbations of four-dimensional topological black holes with scalar hair
dc.type	Review
dc.rights.holder	Scopus
dc.identifier.bibliograpycitation	Journal of High Energy Physics. Vol 2006, No.10 (2006), p.-
dc.identifier.doi	10.1088/1126-6708/2006/10/006
Appears in Collections:	Scopus 1983-2021

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