Perturbative calculation of quasi-normal modes of arbitrary spin in Schwarzschild spacetime

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DC Field	Value	Language
dc.contributor.author	Musiri S.
dc.contributor.author	Siopsis G.
dc.date.accessioned	2021-04-05T04:32:09Z	-
dc.date.available	2021-04-05T04:32:09Z	-
dc.date.issued	2007
dc.identifier.issn	3702693
dc.identifier.other	2-s2.0-34250617054
dc.identifier.uri	https://ir.swu.ac.th/jspui/handle/123456789/14936	-
dc.identifier.uri	https://www.scopus.com/inward/record.uri?eid=2-s2.0-34250617054&doi=10.1016%2fj.physletb.2007.04.068&partnerID=40&md5=e4fe69203f6482fd68edafd339fc1f6e
dc.description.abstract	We calculate analytically the asymptotic form of quasi-normal modes of perturbations of arbitrary spin of a Schwarzschild black hole including first-order corrections. We use the Teukolsky equation which applies to both bosonic and fermionic modes. Remarkably, we arrive at explicit expressions which coincide with those derived using the Regge-Wheeler equation for integer spin. Our zeroth-order expressions agree with the results of WKB analysis. In the case of Dirac fermions, our results are in good agreement with numerical data. © 2007 Elsevier B.V. All rights reserved.
dc.title	Perturbative calculation of quasi-normal modes of arbitrary spin in Schwarzschild spacetime
dc.type	Article
dc.rights.holder	Scopus
dc.identifier.bibliograpycitation	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. Vol 650, No.4 (2007), p.279-285
dc.identifier.doi	10.1016/j.physletb.2007.04.068
Appears in Collections:	Scopus 1983-2021

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