Hawking radiation of rotating BTZ black hole based on modified dispersion relation and Rarita–Schwinger equation

Author:

Gayatri Devi Sapam1,Ablu Meitei I.1,Ibungochouba Singh T.2,Keshwarjit Singh Aheibam3,Yugindro Singh K.1

Affiliation:

1. Department of Physics, Manipur University, Canchipur 795003, Imphal, Manipur, India

2. Department of Mathematics, Manipur University, Canchipur 795003, Imphal, Manipur, India

3. Department of Physics, DM College of Science, Imphal 795001, Imphal, Manipur, India

Abstract

In this paper, tunneling of fermions from rotating BTZ black hole is investigated using modified dispersion relation (MDR) and Rarita–Schwinger equation. The effect of MDR on the tunneling of fermions raises the Hawking temperature of rotating BTZ black hole. It is observed that the modified Hawking temperature of the black hole depends not only on the radial parameters of the black hole but also on the angular parameters of the black hole and the coupling constant [Formula: see text]. Further, the entropy and the heat capacity of the black hole are also studied.

Publisher

World Scientific Pub Co Pte Ltd

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

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