Hawking radiation and Dirac quasinormal modes of 3D EMDΛ black holes

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Abstract

Some properties of the Hawking radiation emitted by the family of black holes of the Einstein-Maxwell-Dilaton with cosmological constant theory in three dimensions found by Chan and Mann are studied using the complex paths method and the Damour-Ruffini method. The exact values of the quasinormal frequencies of the massless Dirac field propagating on a particular black hole of this family are calculated. Taking as a basis the results obtained for the values of the quasinormal frequencies the instability of some modes is discussed. The extension of these results to the black holes of the Einstein-Maxwell-Dilaton theory in four dimensions is studied in the appendix.

Original languageEnglish
Pages (from-to)167-190
Number of pages24
JournalGeneral Relativity and Gravitation
Volume37
Issue number1
DOIs
StatePublished - Jan 2005
Externally publishedYes

Keywords

  • Dirac quasinormal modes
  • Einstein-Maxwell-Dilaton
  • Hawking radiation
  • Three-dimensional black hole

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