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High energy neutrino production by cosmic ray interactions in the Sun
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Nuclear and Particle Physics.
1996 (English)In: PHYSICAL REVIEW D, ISSN 0556-2821, Vol. 54, no 7, 4385-4392 p.Article in journal (Refereed) Published
Abstract [en]

The flux of neutrinos originating from cosmic ray interactions with matter in the Sun has been calculated based on Monte Carlo models for high energy particle interactions. The resulting flux at the Earth (within the Sun's solid angle) is higher than the

Place, publisher, year, edition, pages
1996. Vol. 54, no 7, 4385-4392 p.
Keyword [en]
ATMOSPHERIC NEUTRINOS; OSCILLATIONS; MATTER; SPECTROSCOPY; SPECTRUM; PHYSICS; SEARCH; MODEL
Identifiers
URN: urn:nbn:se:uu:diva-26767OAI: oai:DiVA.org:uu-26767DiVA: diva2:54661
Note
Addresses: Ingelman G, UNIV UPPSALA, DEPT RADIAT SCI, BOX 535, S-75121 UPPSALA, SWEDEN. DESY, D-22603 HAMBURG, GERMANY.Available from: 2008-05-25 Created: 2008-05-25 Last updated: 2011-01-15

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http://arXiv.org/abs/hep-ph/9604288

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Ingelman, Gunnar

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