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Neutrino mass spectrum with nu(mu)->nu(s) oscillations of atmospheric neutrinos

机译:大气中微子的nu(mu)-> nu(s)振荡的中微子质谱

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摘要

We consider the "standard" spectrum of the active neutrinos (characterized by strong mass hierarchy and small mixing) with additional sterile neutrino, nu(s). The sterile neutrino mixes strongly with the muon neutrino, so that nu(mu) <--> nu(s) oscillations solve the atmospheric neutrino problem. We show that the parametric enhancement of the nu(mu) <--> nu(s) oscillations occurs for the high energy atmospheric neutrinos which cross the core of the Earth. This can be relevant for the anomaly observed by the MACRO experiment. Solar neutrinos are converted both to nu(mu) and nu(s). The heaviest neutrino (approximate to nu(tau)) may compose the hot dark matter of the Universe. The phenomenology of this scenario is elaborated and crucial experimental signatures are identified. We also discuss properties of the underlying neutrino mass matrix. (C) 1998 Published by Elsevier Science B.V. [References: 74]
机译:我们考虑到活性中微子的“标准”谱图(以强质量等级和少量混合为特征)以及其他无菌中微子nu。无菌中微子与μon中微子强烈混合,因此nu(mu)--- nu(s)振荡解决了大气中微子问题。我们表明,对于穿过地球核心的高能大气中微子而言,nu(μ)<-> nu(s)振荡的参数增强发生了。这可能与MACRO实验观察到的异常有关。太阳中微子都被转换为nu(mu)和nu(s)。最重的中微子(近似于nu(tau))可能构成了宇宙的炽热暗物质。详细阐述了这种情况的现象学,并确定了关键的实验特征。我们还将讨论基础中微子质量矩阵的性质。 (C)1998年,由Elsevier Science B.V.出版[参考文献:74]

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