Energy spectrum of cosmic-ray neutrinos in the atmosphere

Details Energy spectrum of cosmic-ray neutrinos in the atmosphere Energy spectrum of cosmic-ray neutrinos in the atmosphere

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ncimc...9..995m&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 9, Sept.-Oct. 1986, p. 995-1020.

Computer Science

50

Atmospheric Radiation, Cosmic Ray Showers, Energy Spectra, Neutrinos, Particle Intensity, Elementary Particle Interactions, High Energy Interactions, Muons, Radioactive Decay

Scientific paper

The differential energy spectrum of cosmic-ray neutrinos in the atmosphere (composed of muon-neutrinos and electron-neutrinos) is calculated on the basis of a recently-proposed realistic collision model as well as experimental results on the primary spectrum in which the contribution of a prompt neutrino is taken into account. For the horizontal direction, the prompt muon-neutrino intensity exceeds that of muon-neutrinos from conventional processes at a neutrino energy of 1 million GeV; moreover, the prompt electron-neutrino intensity exceeds that of electron-neutrinos from conventional processes at an energy of 100,000 GeV. The corresponding values for the vertical direction are 100,000 GeV and 10,000 GeV, respectively.

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