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

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.

Published version. 24 pages. Significant changes in order to match the published version

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• Spherical photon orbits in the field of Kerr naked singularities
• Photon motion in Kerr-de Sitter spacetimes
• Accretion disks around a static black hole in $f(R)$ gravity
• On a model of magnetically charged black hole with nonlinear electrodynamics
• The Black Hole Radiation in Massive Gravity
• Gauge symmetries and the Higgs mechanism in Quantum Finance
• Revisiting black hole thermodynamics in massive gravity: charged particle absorption and shell of dust falling
• Entropy of higher-dimensional topological dS black holes with nonlinear source
• Vacuum degeneracy in Massive gravity=Multiplicity of fundamental scales
• The dynamical origin of the graviton mass in the non-linear theory of massive gravity
• The $\Lambda$ to zero limit of spacetimes and its physical interpretation