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

Details Hawking radiation and Dirac quasinormal modes of 3D EMDλ black holes Hawking radiation and Dirac quasinormal modes of 3D EMDλ black holes

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005gregr..37..167l&link_type=abstract

General Relativity and Gravitation, Volume 37, Issue 1, pp.167-190

Mathematics

Logic

16

Three-Dimensional Black Hole, Einstein–Maxwell–Dilaton, Hawking Radiation, Dirac Quasinormal Modes

Scientific paper

Some properties of the Hawking radiation emitted by the family of black holes of the Einstein Maxwell Dilaton with cosmologicalconstant theory in three dimensions found by Chan and Mann are studiedusing the complex paths method and the Damour Ruffini method. Theexact values of the quasinormal frequencies of the massless Diracfield propagating on a particular black hole of this family arecalculated. Taking as a basis the results obtained for the values ofthe quasinormal frequencies the instability of some modes isdiscussed. The extension of these results to the black holes of theEinstein Maxwell Dilaton theory in four dimensions is studied in theappendix.

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