Super-high-energy neutrino spectra in the atmosphere derived from the latest JACEE, MSU, SOKOL and CRN primary spectrum using Z-factors for p-air collisions estimated from Fermi national accelerator data.

Details Super-high-energy neutrino spectra in the atmosphere derived from the latest JACEE, MSU, SOKOL and CRN primary spectrum using Z-factors for p-air collisions estimated from Fermi national accelerator data. Super-high-energy neutrino spectra in the atmosphere derived from the latest JACEE, MSU, SOKOL and CRN primary spectrum using Z-factors for p-air collisions estimated from Fermi national accelerator data.

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ncimc..19..355b&link_type=abstract

Nuovo Cimento C, Vol. 19C, N. 3, p. 355 - 366

Physics

1

Cosmic Rays: Neutrinos

Scientific paper

The absolute spectra of atmospheric neutrinos in the vertical direction
and at large zenith angle have been estimated directly from the primary
cosmic-ray nucleon spectrum based on the latest JACEE, MSU, SOKOL and
CRN data surveyed by Swordy.

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