Non-standard interactions of solar neutrinos in dark matter experiments

被引:48
|
作者
Dutta, Bhaskar [1 ]
Liao, Shu [1 ]
Strigari, Louis E. [1 ]
Walker, Joel W. [2 ]
机构
[1] Texas A&M Univ, Mitchell Inst Fundamental Phys & Astron, Dept Phys & Astron, College Stn, TX 77845 USA
[2] Sam Houston State Univ, Dept Phys, Huntsville, TX 77341 USA
基金
美国国家科学基金会;
关键词
D O I
10.1016/j.physletb.2017.08.031
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that non-standard neutrino interactions (NSI) can be probed in future direct dark matter detection experiments through both elastic neutrino-electron scattering and coherent neutrino-nucleus scattering. We show NSI can increase the event rate due to solar neutrinos, with a sharp increase for lower nuclear recoil energy thresholds. We also identify an interference range of NSI parameters for which the rate is reduced by approximately 40%. Finally, we show that the "dark side" solution for the solar neutrino mixing angle may be discovered at forthcoming experiments. (C) 2017 The Authors. Published by Elsevier B.V.
引用
收藏
页码:242 / 246
页数:5
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