Bounds on non-standard neutrino interactions using PINGU

被引:34
|
作者
Choubey, Sandhya [1 ,2 ]
Ohlsson, Tommy [1 ]
机构
[1] KTH Royal Inst Technol, AlbaNova Univ Ctr, Sch Engn Sci, Dept Theoret Phys, S-10691 Stockholm, Sweden
[2] Harish Chandra Res Inst, Allahabad 211019, Uttar Pradesh, India
基金
瑞典研究理事会; 美国国家科学基金会;
关键词
MASSLESS NEUTRINOS; OSCILLATIONS;
D O I
10.1016/j.physletb.2014.11.010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the impact of non-standard neutrino interactions (NSIs) on atmospheric neutrinos using the proposed PINGU experiment. In particular, we focus on the matter NSI parameters epsilon(mu tau) and vertical bar epsilon(tau tau)-epsilon(mu mu)vertical bar that have previously been constrained by the Super-Kamiokande experiment. First, we present approximate analytical formulas for the difference of the muon neutrino survival probability with and without the above-mentioned NSI parameters. Second, we calculate the atmospheric neutrino events at PINGU in the energy range (2-100) GeV, which follow the trend outlined on probability level. Finally, we perform a statistical analysis of PINGU. Using three years of data, we obtain bounds from PINGU given by -0.0043 (-0.0048) < epsilon(mu tau) < 0.0047 (0.0046) and -0.03 (-0.016) < epsilon(tau tau) < 0.017 (0.032) at 90% confidence level for normal (inverted) neutrino mass hierarchy, which improve the Super-Kamiokande bounds by one order of magnitude. In addition, we show the expected allowed contour region in the epsilon-ettplane if NSIs exist in Nature and the result suggests that there is basically no correlation between epsilon(mu tau) and epsilon(tau tau). (C) 2014 The Authors. Published by Elsevier B.V.
引用
收藏
页码:357 / 364
页数:8
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