Possibility of catastrophic black hole growth in the warped brane-world scenario at the LHC

Roberto Casadio, Sergio Fabi, and Benjamin Harms
Phys. Rev. D 80, 084036 – Published 26 October 2009

Abstract

In this paper, we present the results of our analysis of the growth and decay of black holes possibly produced at the Large Hadron Collider, based on our previous study of black holes in the context of the warped brane-world scenario. The black hole mass accretion and decay is obtained as a function of time, and the maximum black hole mass are obtained as a function of a critical mass parameter. The latter occurs in our expression for the luminosity and is related to the size of extra-dimensional corrections to Newton’s law. Based on this analysis, we argue against the possibility of catastrophic black hole growth at the LHC.

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  • Received 24 February 2009

DOI:https://doi.org/10.1103/PhysRevD.80.084036

©2009 American Physical Society

Authors & Affiliations

Roberto Casadio1,*, Sergio Fabi2,†, and Benjamin Harms2,‡

  • 1Dipartimento di Fisica, Università di Bologna and INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, Italy
  • 2Department of Physics and Astronomy, The University of Alabama, Box 870324, Tuscaloosa, Alabama 35487-0324, USA

  • *casadio@bo.infn.it
  • fabi001@bama.ua.edu
  • bharms@bama.ua.edu

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Issue

Vol. 80, Iss. 8 — 15 October 2009

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