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Volumn 58, Issue 7, 1998, Pages 0730051-07300512

Comparison of vν ↔ ν τ and ν μ ↔ νs oscillations as solutions of the atmospheric neutrino problem

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EID: 0001065795     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.073005     Document Type: Article
Times cited : (81)

References (60)
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    • Note in the lower panels of Figs. 5 and 6 that the suppression factor for v -> v, transitions, if studied in great detail shows a complex dependence on the zenith angle that can be compared with the oscillation probability curves in Fig. 3.
    • Note in the lower panels of Figs. 5 and 6 that the suppression factor for v -> v, transitions, if studied in great detail shows a complex dependence on the zenith angle that can be compared with the oscillation probability curves in Fig. 3.
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    • note
    • We note that in [17] the authors have considered only the case of positive Am2. Matter effects allow to distinguish the case of positive and negative squared mass differences, and the allowed region for Aw2< 0 is somewhat larger than in the other case, because of the MSW resonance present for the neutrinos.
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    • The acceptance for the muon flux increases with the area (as opposed to the volume) of the detector: SK does not dominate the other experiments as for the contained neutrino events.
    • The acceptance for the muon flux increases with the area (as opposed to the volume) of the detector: SK does not dominate the other experiments as for the contained neutrino events.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.