The Sun is a source of high energy neutrinos (E > 10 GeV) produced by cosmic ray interactions in the solar atmosphere. We study the impact of three-flavor oscillations on the solar atmosphere neutrino fluxes observable at Earth. We find that peculiar matter oscillation effects in the Sun do exist, b
β¦ LIBER β¦
Solar neutrino oscillations
β Scribed by W.C. Haxton
- Publisher
- Elsevier Science
- Year
- 1994
- Tongue
- English
- Weight
- 754 KB
- Volume
- 570
- Category
- Article
- ISSN
- 0375-9474
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