Nearly Static Magnetized Kerr Black-hole in Non-linear Electrodynamics
General Relativity and Quantum Cosmology
2023-03-15 v1
Abstract
We have analyzed the thermodynamics of slowly rotating magnetized Kerr black-hole, with typical spin parameter (nearly static) in the background of non-linear electrodynamics. In particular we have studied the Bekenstein-Hawking entropy, Hawking temperature, angular momentum, specific heats and identified regions of parameters for possible phase-transitions. It turns out that once the stability lost the black-hole never come back to its original stable position.
Cite
@article{arxiv.2303.07736,
title = {Nearly Static Magnetized Kerr Black-hole in Non-linear Electrodynamics},
author = {K. G. Managave and H. A. Redekar and R. B. Kumbhar and S. P. Das and K. Y. Rajpure},
journal= {arXiv preprint arXiv:2303.07736},
year = {2023}
}
Comments
9pages, 12 figures