A direct detection view of the neutrino NSI landscape

被引:9
|
作者
Amaral, Dorian [1 ,2 ]
Cerdeno, David [3 ,4 ]
Cheek, Andrew [5 ]
Foldenauer, Patrick [1 ,3 ]
机构
[1] Univ Durham, Inst Particle Phys Phenomenol, Durham DH1 3LE, England
[2] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA
[3] Univ Autonoma Madrid, Inst Fis Teor, Madrid 28049, Spain
[4] Univ Autonoma Madrid, Dept Fis Teor, Madrid 28049, Spain
[5] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Astrocent, Ul Rektorska 4, PL-00614 Warsaw, Poland
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2023年 / 07期
基金
美国国家科学基金会;
关键词
Neutrino Interactions; Non-Standard Neutrino Properties; DARK-MATTER; NONSTANDARD INTERACTIONS; SOLAR NEUTRINOS; OSCILLATIONS; PHYSICS; MODELS;
D O I
10.1007/JHEP07(2023)071
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
In this article, we study the potential of direct detection experiments to explore the parameter space of general non-standard neutrino interactions (NSI) via solar neutrino scattering. Due to their sensitivity to neutrino-electron and neutrino-nucleus scattering, direct detection provides a complementary view of the NSI landscape to that of spallation sources and neutrino oscillation experiments. In particular, the large admixture of tau neutrinos in the solar flux makes direct detection experiments well-suited to probe the full flavour space of NSI. To study this, we develop a re-parametrisation of the NSI framework that explicitly includes a variable electron contribution and allows for a clear visualisation of the complementarity of the different experimental sources. Using this new parametrisation, we explore how previous bounds from spallation source and neutrino oscillation experiments are impacted. For the first time, we compute limits on NSI from the first results of the XENONnT and LUX-ZEPLIN experiments, and we obtain projections for future xenon-based experiments. These computations have been performed with our newly developed software package, SNuDD. Our results demonstrate the importance of using a more general NSI parametrisation and indicate that next generation direct detection experiments will become powerful probes of neutrino NSI.
引用
收藏
页数:50
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