Stability of Circular Orbits around a Tidal Charged Black Hole
- Authors: Sharif M.1, Kousar L.1
-
Affiliations:
- Department of Mathematics
- Issue: Vol 126, No 1 (2018)
- Pages: 44-49
- Section: Nuclei, Particles, Fields, Gravitation, and Astrophysics
- URL: https://journals.rcsi.science/1063-7761/article/view/192701
- DOI: https://doi.org/10.1134/S1063776118010090
- ID: 192701
Cite item
Abstract
We study the effects of the tidal charge on the equatorial circular motion of neutral test particles near a tidal charged black hole. This analysis investigates stable as well as unstable circular orbits in all possible configurations of nonextremal and extremal cases. It is found that a negative tidal charge will increase the energy and angular momentum of a neutral test particle moving around a black hole. We obtain a continuous region of stability for both extremal and nonextremal cases. We conclude that the region of stability as well as radius of last stable circular orbit shows increasing behavior for Q < 0.
About the authors
M. Sharif
Department of Mathematics
Author for correspondence.
Email: msharif.math@pu.edu.pk
Pakistan, Lahore, 54590
L. Kousar
Department of Mathematics
Email: msharif.math@pu.edu.pk
Pakistan, Lahore, 54590
Supplementary files
