Quasinormal Modes and Thermodynamics of Linearly Charged BTZ Black Holes in Massive Gravity in (Anti) de Sitter Space-time: Scientific Explanation

Authors

  • P. Prasia Department of Physics, Cochin University of Science and Technology, Kochi 682022, India.
  • V. C. Kuriakose Department of Physics, Cochin University of Science and Technology, Kochi 682022, India.

DOI:

https://doi.org/10.9734/bpi/ntpsr/v5/9493D

Keywords:

Quasinormal modes, black holes, scientific explanation, General Theory of Relativity (GTR)

Abstract

We investigate the Quasi-Normal Modes (QNMs) and the thermodynamics of linearly charged BTZ black holes in huge gravity in the (Anti)de Sitter ((A)dS) space-time in this paper. The behavior of QNMs is observed to fluctuate with the massive parameter of the graviton as well as the charge of the black hole. In the (A)dS space-time, the thermodynamics of such black holes are also studied in depth. The behavior of specific heat with temperature for such black holes indicates a phase transition that is dependent on the graviton's massive parameter as well as the charge of black hole.

Published

2022-06-11

How to Cite

P. Prasia, & V. C. Kuriakose. (2022). Quasinormal Modes and Thermodynamics of Linearly Charged BTZ Black Holes in Massive Gravity in (Anti) de Sitter Space-time: Scientific Explanation . New Trends in Physical Science Research Vol. 5, 90–108. https://doi.org/10.9734/bpi/ntpsr/v5/9493D