PreprintCC BY 4.0arXiv
Charged Black Hole Solution in Hoyle Narlikar Gravity and its Thermodynamic Properties
Abstract
In this paper, we derive a new class of analytic black hole solutions within the framework of Hoyle--Narlikar gravity, where the black hole is surrounded by an electric charge acting as the source. After obtaining the corresponding metric, we investigate the thermodynamic properties of the resulting black hole solutions, including the Hawking temperature and entropy. Subsequently, we compute the specific heat and Gibbs free energy in order to analyse the thermodynamic stability of the black hole in Hoyle--Narlikar gravity. An interesting result of our analysis is that the black hole becomes thermodynamically stable for large values of the horizon radius within this framework.
Related
- Thermodynamic stability of the new black hole solution in f(R,G,T) gravity
- Molecular-Level Evaluation of the Thermodynamic Properties of Charged Solutions from Submolar to Molar Ion Concentrations
- Exploring thermodynamic and photonic properties of new black hole solutions in F(R) gravity theory
- Thermodynamic Supercritical Scaling Law for the charged Gauss-Bonnet AdS Black Hole
- General solution of the Dirac equation for electrons bound by a charged atomic chain
BibTeX
@misc{ghosh2026charged,
title = {{Charged Black Hole Solution in Hoyle Narlikar Gravity and its Thermodynamic Properties}},
author = {Aniruddha Ghosh and Ujjal Debnath},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.15176},
eprint = {2609.15176},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.15176},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Charged Black Hole Solution in Hoyle Narlikar Gravity and its Thermodynamic Properties
AU - Aniruddha Ghosh
AU - Ujjal Debnath
PY - 2026
DA - 2026/09/14
PB - arXiv
DO - 10.48550/arxiv.2609.15176
UR - https://arxiv.org/abs/2609.15176
AB - In this paper, we derive a new class of analytic black hole solutions within the framework of Hoyle--Narlikar gravity, where the black hole is surrounded by an electric charge acting as the source. After obtaining the corresponding metric, we investigate the thermodynamic properties of the resulting black hole solutions, including the Hawking temperature and entropy. Subsequently, we compute the specific heat and Gibbs free energy in order to analyse the thermodynamic stability of the black hole in Hoyle--Narlikar gravity. An interesting result of our analysis is that the black hole becomes thermodynamically stable for large values of the horizon radius within this framework.
ER -