Quasinormal modes of gravitational perturbation around a Schwarzschild black hole surrounded by quintessence

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dc.creatorZhang, Yu
dc.creatorGui, Y X
dc.date2006-12-01
dc.date.accessioned2026-07-07T10:57:53Z
dc.date.available2026-07-07T10:57:53Z
dc.descriptionIn this paper, the quasinormal modes of gravitational perturbation around a Schwarzschild black hole surrounded by quintessence were evaluated by using the third-order WKB approximation. Due to the presence of quintessence, the gravitational wave damps more slowly.
dc.identifierhttps://arxiv.org/abs/gr-qc/0612009
dc.identifierhttp://arxiv.org/abs/gr-qc/0612009
dc.identifierClass.Quant.Grav.23:6141-6147,2006
dc.identifierdoi:10.1088/0264-9381/23/22/004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186908
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleQuasinormal modes of gravitational perturbation around a Schwarzschild black hole surrounded by quintessence
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