Phenomenology of Randall-Sundrum Black Holes

Details Phenomenology of Randall-Sundrum Black Holes Phenomenology of Randall-Sundrum Black Holes

2002-04-19

arxiv.org/abs/hep-ph/0204228v3

Phys.Rev. D66 (2002) 024033

Physics

High Energy Physics

High Energy Physics - Phenomenology

Version to appear in Physical Review D; contains additional analysis on sensitivity of OWL

Scientific paper

10.1103/PhysRevD.66.024033

We explore the phenomenology of microscopic black holes in the $S^1/Z_2$ Randall-Sundrum (RS) model. We consider the canonical framework in which both gauge and matter fields are confined to the brane and only gravity spills into the extra dimension. The model is characterized by two parameters, the mass of the first massive graviton $(m_1)$, and the curvature $1/\ell$ of the RS anti-de Sitter space. We compute the sensitivity of present and future cosmic ray experiments to various regions of $\ell$ and $m_1,$ and compare with that of Runs I and II at the Tevatron. As part of our phenomenological analysis, we examine constraints placed on $\ell$ by AdS/CFT considerations.

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