Entropy bound for a rotating system from Anti de Sitter black holes
General Relativity and Quantum Cosmology
2009-10-31 v1
Abstract
General geodesic equations of the motion of spinning systems around the (3+1)-dimensional and (2+1)-dimensional rotating anti-de Sitter black holes have been obtained. Based upon these equations, we derived the entropy bound for a rotating system from Kerr-Anti de Sitter black holes and BTZ black holes, respectively. Our result coincides with that of Hod's derived from Kerr black hole, which shows that the entropy bound of the rotating system is neither dependent on the black hole parameters, nor on spacetime dimensions. It is a universal entropy bound.
Keywords
Cite
@article{arxiv.gr-qc/0003091,
title = {Entropy bound for a rotating system from Anti de Sitter black holes},
author = {Bin Wang and Elcio Abdalla},
journal= {arXiv preprint arXiv:gr-qc/0003091},
year = {2009}
}
Comments
10 pages, Latex file