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作者机构:Department of Physics Institute for Fundamental Science University of Oregon Eugene Oregon97403 United States Oho 1-1 Ibaraki Tsukuba305-0801 Japan Tsukuba305-0801 Japan Kavli Institute for the Physics and Mathematics of the Universe WPI The University of Tokyo Institutes for Advanced Study The University of Tokyo Chiba Kashiwa277-8583 Japan 1-1 Oho Ibaraki Tsukuba305-0801 Japan Center for Cosmology and Particle Physics Department of Physics New York University New YorkNY10003 United States
出 版 物:《arXiv》 (arXiv)
年 卷 期:2023年
核心收录:
主 题:Neutrons
摘 要:Next generation direct dark matter (DM) detection experiments will have unprecedented capabilities to explore coherent neutrino-nucleus scattering (CEνNS) complementary to dedicated neutrino experiments. We demonstrate that future DM experiments can effectively probe nonstandard neutrino interactions (NSI) mediated by scalar fields in the scattering of solar and atmospheric neutrinos. We set first limits on S1 leptoquark models that result in sizable µ − d and τ − d sector neutrino NSI CEνNS contributions using LUX-ZEPLIN (LZ) data. As we show, near future DM experiments reaching ∼ O(100)ton-year exposure, such as argon-based ARGO and xenon-based DARWIN, can probe parameter space of leptoquarks beyond the reach of current and planned collider facilities. We also analyze for the first time prospects for testing NSI in lead-based detectors. We discuss the ability of leptoquarks in the parameter space of interest to also explain the neutrino masses and (g−2)µ observations. © 2023, CC BY.