Cosmic neutrinos of ultra-high energies and detection possibility

Details Cosmic neutrinos of ultra-high energies and detection possibility Cosmic neutrinos of ultra-high energies and detection possibility

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..32..461b&link_type=abstract

Astrophysics and Space Science, vol. 32, Feb. 1975, p. 461-482.

Astronomy and Astrophysics

Astrophysics

90

Cosmic Rays, Neutrinos, Particle Flux Density, Proton Scattering, Astronomical Models, Cosmic Ray Showers, Diffuse Radiation, Galaxies, Proton-Proton Reactions, Radiation Counters, Radiation Spectra, Universe

Scientific paper

A rigorous upper bound for high energy neutrino flux is obtained on the basis of the observed intensity of diffuse X and gamma rays. The general formulas are derived for the neutrino fluxes produced in proton collisions with microwave photons in the metagalaxy and in p-p collisions in both the metagalaxy and within the galaxies. The neutrino flux due to normal galaxies is calculated, taking into account the distribution in the cosmic ray spectrum.

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