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Автор Nicolao Fornengo
Автор M. Concha Gonzalez-Garcia
Автор Jose W. Furtado Valle
Дата выпуска 2000-07-01
dc.description Flavour changing (FC) neutrino-matter interactions have been proposed as a solution to the atmospheric neutrino anomaly. Here we perform the analysis of the full set of the recent 52 kTy SUPER-KAMIOKANDE atmospheric neutrino data, including the zenith angle distribution of the contained events as well as the higher energy upward-going stopping and through-going muon events. Our results show that the FC mechanism can describe the full data sample with a χ<sup>2</sup><sub>min</sub> = 44/33 d.o.f. which is acceptable only at the 90.5 confidence level, while the ν<sub>μ</sub>ν<sub>τ</sub> oscillation scenario gives a χ<sup>2</sup><sub>min</sub> = 23.5/33 d.o.f. which is valid at the 11 CL. The combined analysis confines the amount of FC to be either close to maximal or to the level of about (10-50).
Формат application.pdf
Издатель Institute of Physics Publishing
Название On the interpretation of the atmospheric neutrino data in terms of flavor changing neutrino interactions
Тип paper
DOI 10.1088/1126-6708/2000/07/006
Electronic ISSN 1029- 8479
Print ISSN 1126-6708
Журнал Journal of High Energy Physics
Том 2000
Первая страница 6
Последняя страница 006
Выпуск 07

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