Neutrino telescopes as a direct probe of supersymmetry breaking
- 1. Department of Astronomy and Space Sciences Laboratory, University of California, Berkeley, California 94720 (United States)
- 2. Department of Physics, University of California, Berkeley, California 94720 (United States)
- 3. Theory Group, Lawrence Berkeley National Laboratory, Berkeley, California 94720 (United States)
Description
We consider models where the scale of supersymmetry breaking lies between 5x106 and 5x108 GeV. In this class of theories, which includes models of mediated supersymmetry breaking, the lightest supersymmetric particle is the gravitino, and the next to lightest is typically a long-lived charged slepton with a lifetime between a microsecond and a second, depending on its mass. We investigate the production of these particles by the diffuse flux of high energy neutrinos colliding with nucleons in the Earth, and the potential for their observation in large ice or water Cerenkov detectors. The small production cross section is partially compensated by the very long range of sleptons. The signal, two well-separated parallel tracks, has very little background. Using the Waxman-Bahcall limit for the neutrino flux results in up to four events a year in km3 experiments
Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.92.221802;
- arXiv
- arXiv:hep-ph/0312197v1;
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 92
- Journal Issue
- 22
- Journal Page Range
- p. 221802-221802.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36019287
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COSMIC NEUTRINOS; CROSS SECTIONS; GRAVITONS; ICE; LIFETIME; MASS; NUCLEONS; PARTICLE TRACKS; PEV RANGE; PROBES; SIGNALS; SPARTICLES; SUPERSYMMETRY; SYMMETRY BREAKING; TELESCOPES; WATER
- Descriptors DEC
- BARYONS; COSMIC RADIATION; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; GRAVITATIONAL RADIATION; HADRONS; HYDROGEN COMPOUNDS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; NEUTRINOS; OXYGEN COMPOUNDS; POSTULATED PARTICLES; RADIATIONS; SYMMETRY
Optional Information
- Notes
- (c) 2004 The American Physical Society