Dynamics of Charged and Rotating NUT Black Holes in Rastall Gravity
General Relativity and Quantum Cosmology
2020-02-27 v2 High Energy Physics - Theory
Abstract
In this work, we generalized the Kerr-Newman-NUT black hole solution in Rastall gravity from Ref. 1. Here we are more focused on the black hole dynamics such as the event horizons, ergosurface, ZAMO, thermodynamic properties, and the equatorial circular orbit around the black hole such as static radius limit, null equatorial circular orbit, and innermost stable circular orbit. We present how the NUT and Rastall parameter affects the dynamic of the black hole.
Keywords
Cite
@article{arxiv.1908.09629,
title = {Dynamics of Charged and Rotating NUT Black Holes in Rastall Gravity},
author = {Hadyan L. Prihadi and Muhammad F. A. R. Sakti and Getbogi Hikmawan and Freddy P. Zen},
journal= {arXiv preprint arXiv:1908.09629},
year = {2020}
}
Comments
24 pages, 30 figures, Prepared for submission to IJMPD