Angular momentum-area proportionality of extremal charged black holes in odd dimensions
General Relativity and Quantum Cosmology
2017-09-28 v1 High Energy Physics - Theory
Abstract
Extremal rotating black holes in Einstein-Maxwell theory feature two branches. On the branch emerging from the Myers-Perry solutions their angular momentum is proportional to their horizon area, while on the branch emerging from the Tangherlini solutions their angular momentum is proportional to their horizon angular momentum. The transition between these branches occurs at a critical value of the charge, which depends on the value of the angular momentum. However, when a dilaton is included, the angular momentum is always proportional to the horizon area.
Keywords
Cite
@article{arxiv.1309.2088,
title = {Angular momentum-area proportionality of extremal charged black holes in odd dimensions},
author = {Jose Luis Blazquez-Salcedo and Jutta Kunz and Francisco Navarro-Lerida},
journal= {arXiv preprint arXiv:1309.2088},
year = {2017}
}
Comments
5 pages, 2 figures