Damping signatures in future neutrino oscillation experiments

被引:46
作者
Blennow, M
Ohlsson, T
Winter, W
机构
[1] Royal Inst Technol, Sch Engn Sci,AlbaNova Univ Ctr, Dept Phys, Div Math Phys, S-10691 Stockholm, Sweden
[2] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2005年 / 06期
基金
美国国家科学基金会;
关键词
solar and atmospheric neutrinos; neutrino physics;
D O I
10.1088/1126-6708/2005/06/049
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We discuss the phenomenology of damping signatures in the neutrino oscillation probabilities, where either the oscillating terms or the probabilities can be damped. This approach is a possibility for tests of damping effects in future neutrino oscillation experiments, where we mainly focus on reactor and long-baseline experiments. We extensively motivate different damping signatures due to small corrections by neutrino decoherence, neutrino decay, oscillations into sterile neutrinos, or other mechanisms, and classify these signatures according to their energy ( spectral) dependencies. We demonstrate, at the example of short baseline reactor experiments, that damping can severely alter the interpretation of results, e. g., it could fake a value of sin(2)(2 theta(13)) smaller than the one provided by Nature. In addition, we demonstrate how a neutrino factory could constrain different damping models with emphasis on how these different models could be distinguished, i.e., how easily the actual type of effect could be identified. We find that the damping models cluster in different categories, which can be much better distinguished from each other than models within the same cluster.
引用
收藏
页码:1095 / 1125
页数:32
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