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Relic Neutrinos and Z-Resonance Mechanism for Highest Energy Cosmic Rays

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Published 2000 December 29 © 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation James L. Crooks et al 2001 ApJ 546 L1 DOI 10.1086/318056

1538-4357/546/1/L1

Abstract

The origin of the highest energy cosmic rays remains elusive. The decay of a superheavy particle (X) into an ultraenergetic neutrino which scatters from a relic neutrino or antineutrino at the Z-resonance has attractive features. Given the necessary X mass of 1014-1015 GeV, the required lifetime, 1015-1016 yr, renders model building a serious challenge, but three logical possibilities are considered: (1) X is a Higgs scalar in SU(15) belonging to high-rank representation, leading to power-enhanced lifetime; (2) a global X quantum number has exponentially suppressed symmetry breaking by instantons; and (3) with additional space dimension(s), localization of X within the real-world brane leads to Gaussian decay suppression, the most efficient of the suppression mechanisms considered.

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10.1086/318056