Perturbative calculation of quasinormal modes of AdS Schwarzschild black holes

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DC Field	Value	Language
dc.contributor.author	Musiri S.
dc.contributor.author	Ness S.
dc.contributor.author	Siopsis G.
dc.date.accessioned	2021-04-05T04:32:23Z	-
dc.date.available	2021-04-05T04:32:23Z	-
dc.date.issued	2006
dc.identifier.issn	15507998
dc.identifier.other	2-s2.0-33644629558
dc.identifier.uri	https://ir.swu.ac.th/jspui/handle/123456789/15036	-
dc.identifier.uri	https://www.scopus.com/inward/record.uri?eid=2-s2.0-33644629558&doi=10.1103%2fPhysRevD.73.064001&partnerID=40&md5=e9a2a466ef189cc46cd18a19ff5c3dae
dc.description.abstract	We calculate analytically quasinormal modes of AdS Schwarzschild black holes including first-order corrections. We consider massive scalar, gravitational and electromagnetic perturbations. Our results are in good agreement with numerical calculations. In the case of electromagnetic perturbations, ours is the first calculation to provide an analytic expression for quasinormal frequencies, because the effective potential vanishes at zeroth order. We show that the first-order correction is logarithmic. © 2006 The American Physical Society.
dc.title	Perturbative calculation of quasinormal modes of AdS Schwarzschild black holes
dc.type	Article
dc.rights.holder	Scopus
dc.identifier.bibliograpycitation	Physical Review D - Particles, Fields, Gravitation and Cosmology. Vol 73, No.6 (2006)
dc.identifier.doi	10.1103/PhysRevD.73.064001
Appears in Collections:	Scopus 1983-2021

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