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The Hawking Radiation in Massive Gravity: Path Integral and the Bogoliubov Method

Resource type
Authors/contributors
Title
The Hawking Radiation in Massive Gravity: Path Integral and the Bogoliubov Method
Abstract
We prove the consistency of the different approaches for deriving the black hole radiation for the spherically symmetric case inside the theory of Massive Gravity. By comparing the results obtained by using the Bogoliubov transformations with those obtained by using the Path Integral formulation, we find that in both cases, the presence of the extra-degrees of freedom creates the effect of extra-particles creation due to the distortions on the definitions of time defined by the different observers at large scales. This, however, does not mean extra-particle creation at the horizon level. Instead, the apparent additional particles perceived at large scales emerge from how distant observers define their time coordinate, which is distorted due to the existence of extra-degrees of freedom.
Publication
Universe
Volume
9
Issue
5
Pages
228
Date
2023/5
Language
en
ISSN
2218-1997
Short Title
The Hawking Radiation in Massive Gravity
Accessed
6/2/23, 4:19 AM
Library Catalog
Extra
Number: 5 Publisher: Multidisciplinary Digital Publishing Institute
Citation
Arraut, I., Segovia, C., & Rosado, W. (2023). The Hawking Radiation in Massive Gravity: Path Integral and the Bogoliubov Method. Universe, 9(5), 228. https://doi.org/10.3390/universe9050228