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

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Resumen

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.

Idioma originalInglés
Páginas (desde-hasta)167-190
Número de páginas24
PublicaciónGeneral Relativity and Gravitation
Volumen37
N.º1
DOI
EstadoPublicada - ene. 2005
Publicado de forma externa

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