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

Abstract

The radiation of vector particles by black holes in (1+2) dimensions is investigated within the WKB approximation. We consider the process of quantum tunnelling of bosons through an event horizon of the black hole. The emission temperature for the Schwarzschild background geometry coincides with the Hawking temperature and for the Rindler spacetime the temperature is the Unruh temperature. We also obtain the radiation temperatures for the de Sitter spacetime.

7 pages, no figures, journal version

References in corpus (5)

• Fermions Tunnelling from Black Holes
• Tunnelling, Temperature and Taub-NUT Black Holes
• Exact Hawking Radiation of Scalars, Fermions, and Bosons Using the Tunneling Method Without Back-Reaction
• Pair Production of Arbitrary Spin Particles by Electromagnetic Fields
• Field theory of massive and massless vector particles in the Duffin - Kemmer - Petiau formalism

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• Hawking radiation of massive bosons via tunneling from black strings
• Modified Hawking temperatures of black holes in Lorentz violation theory
• Studies on Thin-shells and Thin-shell Wormholes