Non-standard interactions of solar neutrinos in dark matter experiments

被引：51

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

来源：

PHYSICS LETTERS B | 2017年 / 773卷

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

页码：242 / 246

页数：5

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