期刊
ASTROPARTICLE PHYSICS
卷 23, 期 1, 页码 11-17出版社
ELSEVIER
DOI: 10.1016/j.astropartphys.2004.11.002
关键词
ultra-high energy cosmic rays; ultra-high energy neutrinos
As ultra-high energy cosmic ray protons propagate through the universe, they undergo photo-meson interactions with the cosmic microwave background, generating the 'cosmogenic' neutrino flux. If, however, a substantial fraction of the cosmic ray primaries are heavy nuclei rather than protons, they would preferentially lose energy through photo-disintegaration so the corresponding neutrino flux may be substantially depleted. We investigate this issue using a Monte Carlo simulation of cosmic ray propagation through intragalactic radiation fields and assess the impact of the altered neutrino fluxes on next-generation neutrino telescopes. (C) 2004 Elsevier B.V. All rights reserved.
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