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Universe 2017, 3(2), 45; doi:10.3390/universe3020045

The Astrophysical Scales Set by the Cosmological Constant, Black-Hole Thermodynamics and Non-Linear Massive Gravity

1
Department of Physics, Faculty of Science, Tokyo University of Science, 1-3, Kagurazaka, Shinjuku-ku, Tokyo 162-8601, Japan
2
Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
3
Theory Center, Institute of Particle and Nuclear Studies, KEK Tsukuba, Ibaraki 305-0801, Japan
Academic Editor: Lorenzo Iorio
Received: 8 February 2017 / Revised: 5 May 2017 / Accepted: 5 May 2017 / Published: 10 May 2017
View Full-Text   |   Download PDF [313 KB, uploaded 10 May 2017]   |  

Abstract

We calculate explicitly the black-hole temperature for the Schwarzschild de-Sitter solution inside massive gravity by defining the Killing-vector in the direction of the Stückelberg function. We then consider the conditions which an observer in massive gravity has to obey in order to agree with the standard results of General Relativity. View Full-Text
Keywords: cosmological constant; Black-hole temperature; static observers; graviton mass; Stückelberg function cosmological constant; Black-hole temperature; static observers; graviton mass; Stückelberg function
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This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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Arraut, I. The Astrophysical Scales Set by the Cosmological Constant, Black-Hole Thermodynamics and Non-Linear Massive Gravity. Universe 2017, 3, 45.

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