Quasinormal modes and thermodynamic phase transitions
arXiv:0802.1889 · doi:10.1103/PhysRevD.77.087501
Abstract
It 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.
3 pages, submitted to Phys.Rev.D as a Brief Report
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