Quasinormal modes and thermodynamic phase transitions

dc.creatorBerti, Emanuele
dc.creatorCardoso, Vitor
dc.date2008-02-13
dc.date.accessioned2026-07-07T11:56:02Z
dc.date.available2026-07-07T11:56:02Z
dc.descriptionIt has recently been suggested that scalar, Dirac and Rarita-Schwinger perturbations are related to thermodynamic phase transitions of charged (Reissner-Nordström) black holes. In this note we show that this result is probably a numerical coincidence, and that the conjectured correspondence does not straightforwardly generalize to other metrics, such as Kerr or Schwarzschild (anti-)de Sitter. Our calculations do not rule out a relation between dynamical and thermodynamical properties of black holes, but they suggest that such a relation is non-trivial.
dc.description3 pages, submitted to Phys.Rev.D as a Brief Report
dc.identifierhttps://arxiv.org/abs/0802.1889
dc.identifierhttp://arxiv.org/abs/0802.1889
dc.identifierPhys.Rev.D77:087501,2008
dc.identifierdoi:10.1103/PhysRevD.77.087501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205448
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleQuasinormal modes and thermodynamic phase transitions
dc.typetext

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