The Black Hole Radiation in Massive Gravity
General Relativity and Quantum Cosmology
2018-02-08 v3 High Energy Physics - Theory
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.
Cite
@article{arxiv.1407.7796,
title = {The Black Hole Radiation in Massive Gravity},
author = {Ivan Arraut},
journal= {arXiv preprint arXiv:1407.7796},
year = {2018}
}
Comments
Title changed in order to match the published version. Version focused on the particle creation process of black-hole in massive gravity