Quasinormal modes in the background of charged Kaluza-Klein black hole with squashed horizons

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dc.creatorHe, Xi
dc.creatorSongbai-Chen
dc.creatorWang, Bin
dc.creatorCai, Rong-Gen
dc.creatorLin, Chi-Yong
dc.date2008-02-18
dc.date2008-06-17
dc.date.accessioned2026-07-07T11:40:20Z
dc.date.available2026-07-07T11:40:20Z
dc.descriptionWe study the scalar perturbation in the background of the charged Kaluza-Klein black holes with squashed horizons. We find that the position of infinite discontinuities of the heat capacities can be reflected in quasinormal spectrum. This shows the possible non-trivial relation between the thermodynamical and dynamical properties of black holes.
dc.descriptionrevised version, accepted for publication in Phys.Lett.B
dc.identifierhttps://arxiv.org/abs/0802.2449
dc.identifierhttp://arxiv.org/abs/0802.2449
dc.identifierPhys.Lett.B665:392-400,2008
dc.identifierdoi:10.1016/j.physletb.2008.06.038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200224
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuasinormal modes in the background of charged Kaluza-Klein black hole with squashed horizons
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