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- W2767171641 abstract "We proof 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 create the effect of extra-particles creation due to the distortions on the notions of time defined by the different observers at large scales. This however does not mean extra-particle creation at the horizon level." @default.
- W2767171641 created "2017-11-10" @default.
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- W2767171641 date "2017-10-14" @default.
- W2767171641 modified "2023-09-27" @default.
- W2767171641 title "The Hawking radiation in massive gravity: Path integral and the Bogoliubov method" @default.
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- W2767171641 hasPublicationYear "2017" @default.
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