Quasinormal modes of a Schwarzschild black hole surrounded by free static spherically symmetric quintessence: Electromagnetic perturbations

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dc.creatorZhang, Yu
dc.creatorGui, Yuanxing
dc.creatorYu, Fei
dc.creatorLi, Fenglin
dc.date2006-12-01
dc.date2007-05-29
dc.date.accessioned2026-07-07T10:41:07Z
dc.date.available2026-07-07T10:41:07Z
dc.descriptionIn this paper, we evaluated the quasinormal modes of electromagnetic perturbation in a Schwarzschild black hole surrounded by the static spherically symmetric quintessence by using the third-order WKB approximation when the quintessential state parameter $ w_{q}$ in the range of $-1/3<w_{q}<0$. Due to the presence of quintessence, Maxwell field damps more slowly. And when at $-1<w_{q}<-1/3$, it is similar to the black hole solution in the ds/Ads spacetime. The appropriate boundary conditions need to be modified.
dc.description6 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0612010
dc.identifierhttp://arxiv.org/abs/gr-qc/0612010
dc.identifierGen.Rel.Grav.39:1003-1010,2007
dc.identifierdoi:10.1007/s10714-007-0434-2
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181533
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuasinormal modes of a Schwarzschild black hole surrounded by free static spherically symmetric quintessence: Electromagnetic perturbations
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