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Phys. Rev. D 68, 104025 (2003) [6 pages]

Updated limits on TeV-scale gravity from the absence of neutrino cosmic ray showers mediated by black holes

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Luis A. Anchordoqui1, Jonathan L. Feng2, Haim Goldberg1,3, and Alfred D. Shapere4
1Department of Physics, Northeastern University, Boston, Massachusetts 02115, USA
2Department of Physics and Astronomy, University of California, Irvine, California 92697, USA
3Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
4Department of Physics, University of Kentucky, Lexington, Kentucky 40506, USA

Received 24 July 2003; published 24 November 2003

We revise existing limits on the D-dimensional Planck scale MD from the nonobservation of microscopic black holes produced by high energy cosmic neutrinos in scenarios with D=4+n large extra dimensions. Previous studies have neglected the energy radiated in gravitational waves by the multipole moments of the incoming shock waves. We include the effects of energy loss, as well as form factors for black hole production and recent null results from cosmic ray detectors. For n>~5, we obtain MD>1.0–1.4TeV. These bounds are among the most stringent and conservative to date.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.68.104025
DOI:
10.1103/PhysRevD.68.104025
PACS:
04.70.-s, 04.50.+h, 13.15.+g, 96.40.Tv