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Diffuse fluxes of cosmic high-energy neutrinos

Stecker, F. W.·1979·The Astrophysical Journal

Abstract

Production spectra of high-energy neutrinos from galactic cosmic-ray interactions with interstellar gas and extragalactic ultrahigh-energy cosmic-ray interactions with microwave blackbody photons are presented and discussed. These production processes involve the decay of charged pions and are thus related to the production of cosmic gamma rays from the decay of neutral pions. Estimates of the neutrino fluxes from various diffuse cosmic sources are then made, and the reasons for significant differences with previous estimates are discussed. Small predicted event rates for a DUMAND (deep underwater muon and neutrino detector) type detection system, combined with a possible significant flux of prompt neutrinos from the atmosphere above 50 TeV, may make the study of diffuse extraterrestrial neutrinos more difficult than previously thought.

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Metadata

Authors
Stecker, F. W.
Venue
The Astrophysical Journal
Published
1979-03
Volume
228
Pages
919
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2077722377
Cited by
286
References
0
FWCI
1.73
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Diffuse fluxes of cosmic high-energy neutrinos. https://app.cochat.ai/papers/10.1086/156919
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Stecker, F. W. (1979). Diffuse fluxes of cosmic high-energy neutrinos. The Astrophysical Journal. https://doi.org/10.1086/156919

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