English

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 a0.1a\le 0.1 (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.

Keywords

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

R2 v1 2026-06-28T09:15:52.692Z