Evolution of Randall-Sundrum Black Holes in Dense Media

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.

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