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Fluxes of atmospheric neutrinos and related cosmic rays

โœ Scribed by T.K. Gaisser


Publisher
Elsevier Science
Year
1999
Tongue
English
Weight
553 KB
Volume
77
Category
Article
ISSN
0920-5632

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โœฆ Synopsis


The atmospheric neutrino beam simultaneously spans a range of pathlengths from ten to ten thousand kilometers, which correspond respectively to downward-and upward-going neutrinos. As with any neutrino oscillation experiment, also in this case the interpretation of the data depends on a detailed knowledge of the neutrino beam. The ingredients are the primary spectrum of cosmlc-ray nucleons, the geomagnetic fields in which the charged particles propagate and the properties of interactions of hadrons in the atmosphere. In this talk I review the status of calculations in light of the recent evidence for neutrino oscillations from Super-Kamiokande [1].


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Ultrahigh Energy Cosmic Rays and Neutrin
โœ A.V. Olinto; K. Kotera; D. Allard ๐Ÿ“‚ Article ๐Ÿ“… 2011 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 166 KB

The observation of neutrinos from cosmic accelerators will be revolutionary. High energy neutrinos are closely connected to ultrahigh energy cosmic rays and their sources. Cosmic ray sources are likely to produce neutrinos and the propagation of ultrahigh cosmic rays from distant sources can generat