The Black Hole Radiation in Massive Gravity

Abstract

We apply the Bogoliubov transformations in order to connect two different vacuums, one~located at past infinity and another located at future infinity around a black hole inside the scenario of the nonlinear theory of massive gravity. The presence of the extra degrees of freedom changes the behavior of the logarithmic singularity and, as a consequence, the relation between the two Bogoliubov coefficients. This has an effect on the number of particles, or equivalently, on the black hole temperature perceived by observers defining the time arbitrarily.

Title changed in order to match the published version. Version focused on the particle creation process of black-hole in massive gravity

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Cited by in corpus (11)

• GUP Modified Hawking Radiation in Bumblebee Gravity
• Greybody factor for black string in dRGT massive gravity
• BTZ black holes in massive gravity
• Thermodynamics of Asymptotically de-Sitter Black Hole in dRGT Massive Gravity from Rényi entropy
• Quasinormal modes of a massless Dirac field in de Rham-Gabadadze-Tolley massive gravity
• Analogies between the Black Hole Interior and the Type II Weyl Semimetals
• Rotating black string in dRGT massive gravity
• Thermodynamics of Black String from Rényi entropy in de Rham-Gabadadze-Tolley Massive Gravity Theory
• The dynamical origin of the graviton mass in the non-linear theory of massive gravity
• GEMS embeddings of Hayward regular black holes in massless and massive gravities
• Classical limit for Dirac fermions with modified action in the presence of the black hole