Primary Cosmic-ray Spectrum and the Intensity of Atmospheric Neutrinos

Simple item page
dc.creatorGaisser, Thomas K.
dc.date1998-11-12
dc.date.accessioned2026-07-07T04:05:43Z
dc.date.available2026-07-07T04:05:43Z
dc.descriptionMeasurements of the intensity of primary cosmic-ray protons reported in the last two years suggest a lower normalization than some earlier measurements. Here we comment on the measurements, compare them to assumptions made in two independent calculations of atmospheric neutrinos and discuss the possible consequences for interpretation of measurements of atmospheric neutrinos.
dc.description7 pages, LaTeX, 1 figure, talk given at the Symposium "New Era in Neutrino Physics", Tokyo Metropolitan University, Japan, 11-12 June, 1998
dc.identifierhttps://arxiv.org/abs/hep-ph/9811314
dc.identifierhttp://arxiv.org/abs/hep-ph/9811314
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48504
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePrimary Cosmic-ray Spectrum and the Intensity of Atmospheric Neutrinos
dc.typetext

Files

Collections

arXiv