Black hole radiation of massive spin-2 particles in (3+1) dimensions

Abstract

This paper is devoted to the study of radiation of massive spin-2 boson (graviton with a nonzero mass) through the event horizon of a generic static and spherically symmetric black hole in (3+1) dimensions. To this end, we consider the problem in the framework of quantum tunneling phenomenon. We evaluate the tunneling rate of the massive gravitons by applying the semiclassical WKB approximation to the Fierz-Pauli equation. The temperature of the radiation is obtained with the aid of the Boltzmann expression. Our findings are in good agreement with the existing Hawking radiation studies in the current literature.

Accepted for publication in The European Physical Journal Plus {http://www.springer.com/13360}. A typo in Ref.29 has been fixed

References in corpus (9)

• Fermions Tunnelling from Black Holes
• Tunnelling, Temperature and Taub-NUT Black Holes
• Temporal contribution to gravitational WKB-like calculations
• Born-Infeld extension of new massive gravity
• Tunneling of Vector Particles from Lorentzian Wormholes in 3+1 Dimensions
• Black hole radiation of spin-1 particles in (1+2) dimensions
• Uninformed Hawking Radiation
• Black hole emission of vector particles in (1+1) dimensions
• Problems of Massive Gravities

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