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

2006/12/31 by Yu Zhang, Yuanxing Gui, Fei Yu +2 · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Boundary value problem #Differential geometry #Noncommutative and Quantum Gravity Theories #Perturbation (astronomy) #Photon sphere #Quasinormal mode #Quintessence #Schwarzschild metric #Schwarzschild radius #WKB approximation #gr-qc

paper · pdf · doi:10.1007/s10714-007-0434-2

published as Gen.Rel.Grav.39:1003-1010,2007 · 6 pages, 3 figures

openalex publication_date 2007/04/24 · arxiv created 2007/05/29 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

In 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.

Citations

• Quintessence and black holes
• Stability and quasinormal modes of the massive scalar field around Kerr black holes
• The quasi-normal modes of the Schwarzschild black hole
• Quasinormal modes: the characteristic `sound' of black holes and neutron stars
• The highly damped quasinormal modes of d -dimensional Reissner–Nordström black holes in the small charge limit
• Absorption and quasinormal modes of classical fields propagating on 3D and 4D de Sitter spacetime

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