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Evolution of Randall-Sundrum Black Holes in Dense Media

Veronique Van Elewyck
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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.

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BibTeXRIS

Veronique Van Elewyck. 2003-05-14. Evolution of Randall-Sundrum Black Holes in Dense Media. https://arxiv.org/abs/hep-ph/0305147

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