Hawking radiation of rotating BTZ Black hole based on modified dispersion relation and Rarita-Schwinger equation
arXiv:2304.12359 · doi:10.1142/S0217751X23500689
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 modified dispersion relation (MDR) on the tunneling of fermions rises 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 σ. Further, the entropy and the heat capacity of the black hole are also studied.
15 pages, 2 figures and submitted to International Journal of Modern Physics A bearing revised manuscript number IJMPA-D-23-00039R1
References in corpus (10)
- Fermions Tunnelling from Black Holes
- Anomalies, Hawking Radiations and Regularity in Rotating Black Holes
- Hawking radiation of Dirac particles via tunnelling from rotating black holes in de Sitter spaces
- Hawking temperature from tunnelling formalism
- Clouds of strings in third-order Lovelock gravity
- Quantum Gravity and Recovery of Information in Black Hole Evaporation
- Thermodynamics of a black hole based on a generalized uncertainty principle
- Exponential corrections to black hole entropy
- Modified Dirac equation with Lorentz invariance violation and its solutions for particles in an external magnetic field
- Modified Hawking radiation of stationary and nonstationary Kerr-Newman-de Sitter black hole