Hawking radiation from z = 3 and z = 1-Lifshitz black holes

Samuel Lepe, Bruno Merello

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

Resumen

The Hawking radiation considered as a tunneling process, by using a Hamilton-Jacobi prescription, is discussed for both z = 3 and z = 1-Lifshitz black holes. We have found that the tunneling rate (which is not thermal but related to the change of entropy) for the z = 3-Lifshitz black hole (which does not satisfy the Area/4-law) does not yield (give us) the expected tunneling rate: λ ∼ exp(ΔS), where ΔS is the change of black hole entropy, if we compare with the z = 1-Lifshitz black hole (BTZ black hole, which satisfies the Area/4-law).

Idioma originalInglés
Número de artículo1450187
PublicaciónModern Physics Letters A
Volumen29
N.º34
DOI
EstadoPublicada - 10 nov. 2014

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