Bounds on new neutrino interactions from the first CEνNS data at direct detection experiments

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Valentina De Romeri, Dimitrios K. Papoulias and Christoph A. Ternes
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Abstract

Recently, two dark matter direct detection experiments have announced the first indications of nuclear recoils from solar 8B neutrinos via coherent elastic neutrino-nucleus scattering (CEνNS) with xenon nuclei. These results constitute a turning point, not only for dark matter searches that are now entering the neutrino fog, but they also bring out new opportunities to exploit dark matter facilities as neutrino detectors. We investigate the implications of recent data from the PandaX-4T and XENONnT experiments on both Standard Model physics and new neutrino interactions. We first extract information on the weak mixing angle at low momentum transfer. Then, following a phenomenological approach, we consider Lorentz-invariant interactions (scalar, vector, axial-vector, and tensor) between neutrinos, quarks and charged leptons. Furthermore, we study the U(1)B-L scenario as a concrete example of a new anomaly-free vector interaction. We find that despite the low statistics of these first experimental results, the inferred bounds are in some cases already competitive. For the scope of this work we also compute new bounds on some of the interactions using CEνNS data from COHERENT and electron recoil data from XENONnT, LUX-ZEPLIN, PandaX-4T, and TEXONO. It seems clear that while direct detection experiments continue to take data, more precise measurements will be available, thus allowing to test new neutrino interactions at the same level or even improving over dedicated neutrino facilities.
直接探测实验中第一个CEνNS数据的新中微子相互作用边界
最近,两个暗物质直接探测实验宣布了太阳8B中微子通过与氙核的相干弹性中微子核散射(CEνNS)产生核反冲的第一个迹象。这些结果构成了一个转折点,不仅是现在进入中微子迷雾的暗物质搜索,而且还带来了利用暗物质设施作为中微子探测器的新机会。我们研究了PandaX-4T和XENONnT实验的最新数据对标准模型物理和新中微子相互作用的影响。首先提取低动量传递时的弱混合角信息。然后,根据现象学方法,我们考虑了中微子、夸克和带电轻子之间的洛伦兹不变相互作用(标量、矢量、轴矢量和张量)。此外,我们研究了U(1)B-L情景作为一个新的无异常矢量相互作用的具体例子。我们发现,尽管这些第一个实验结果的统计数据很低,但在某些情况下,推断的界限已经具有竞争力。对于这项工作的范围,我们还使用来自XENONnT, LUX-ZEPLIN, PandaX-4T和TEXONO的相干CEνNS数据和电子反冲数据计算了一些相互作用的新边界。很明显,当直接探测实验继续收集数据时,更精确的测量将会出现,从而允许在相同水平上测试新的中微子相互作用,甚至改进专用的中微子设施。
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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