Evolution of Randall-Sundrum Black Holes in Dense Media
High Energy Physics - Phenomenology
2007-05-23 v1
Abstract
In the framework of Randall-Sundrum model, we discuss the evolution of microscopic black holes created by cosmic particles hitting a neutron or a strange star. We set up the general equations of evolution for the black hole mass and momentum in a dense medium, and discuss the possibility of collapse due to the black hole's growth inside the star.
Keywords
Cite
@article{arxiv.hep-ph/0305147,
title = {Evolution of Randall-Sundrum Black Holes in Dense Media},
author = {Veronique Van Elewyck},
journal= {arXiv preprint arXiv:hep-ph/0305147},
year = {2007}
}
Comments
2 pages, Latex. Talk presented at the XXXVIIIth Rencontres de Moriond (Electroweak Interactions and Unified Theories), Les Arcs, France, March 15-22, 2003. To appear in the Proceedings