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arXiv 2602.19618hep-phhep-ex
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利用轻核在Spallation Neutron Source进行方向性反冲检测以测量CEvNS

Directional recoil detection for CEvNS measurements with light nuclei at the Spallation Neutron Source

The University of Sydney(悉尼大学);University of Hawaii(夏威夷大学);The University of Melbourne(墨尔本大学)

Ciaran A. J. O'Hare, Anirudh Chandra Shekar, Chiara Lisotti, Michael Litke, Nityasa Mishra, Jayden L. Newstead, Louis E. Strigari, Sven E. Vahsen

AI总结:

利用轻核在Spallation Neutron Source进行方向性反冲检测以测量CEvNS,通过高分割电荷读出的气体时间投影室实现反冲能量和散射角的测量,提升中微子能量重建精度。

摘要:

中微子与核的相干弹性散射,也称为CEvNS,已通过由中微子从停止π子衰变产生的Spallation Neutron Source(SNS)产生的中微子进行的COHERENT实验研究多年。我们提出了一种新的方法,用于在SNS上测量CEvNS,旨在以两种主要方式补充COHERENT实验:通过重建CEvNS诱导反冲的角分布,以及测量在较轻的目标核如氦、碳和氟上进行的CEvNS。所提出的探测器将采用气体时间投影室,具有高分割电荷读出,以实现由CEvNS诱导反冲产生的约10-500 keV电离轨迹的空间重建。这将使同时测量CEvNS反冲能量和散射角成为可能,从而实现事件级的中微子能量重建。我们估计,60:40氦:CF4气体混合物在大气压下在总目标质量和良好的方向性之间提供了良好的折中,甚至在悲观的背景条件下也能检测到CEvNS的角分布。我们对1和10立方米规模探测器的灵敏度进行了预测,包括:标准模型CEvNS截面的测量、中微子味依赖性中微子通量的重建、观测中微子诱导的Migdal效应、对超出标准模型中微子相互作用的限制,以及探测10电子伏级的中性中微子。

英文摘要:

The coherent elastic scattering of neutrinos on nuclei, also known as CEvNS, has been studied for several years by the COHERENT program of experiments using neutrinos from stopped-pion decays produced at the Spallation Neutron Source (SNS). We propose a new approach for CEvNS measurements at the SNS that aims to complement the COHERENT experiments in two main ways: by reconstructing the angular distribution of CEvNS-induced recoils, and by measuring CEvNS on much lighter target nuclei such as helium, carbon, and fluorine. The proposed detector would employ a gaseous time-projection chamber with a highly segmented charge readout to enable the spatial reconstruction of $\sim$10-500 keV ionisation tracks created by CEvNS-induced recoils. This would enable the simultaneous measurement of the CEvNS recoil energy and scattering angle, thereby allowing event-by-event reconstruction of the neutrino energy. We estimate that a 60:40 He:CF$_4$ gas mixture at atmospheric pressure offers a good trade-off between total target mass and good directionality and could deliver a detection of the angular distribution of CEvNS, even under pessimistic background conditions. We project the sensitivity of 1 and 10 m$^3$-scale detectors in the context of several physics cases, including: the measurement of the Standard Model CEvNS cross section, reconstruction of the flavour-dependent neutrino fluxes, observing the neutrino-induced Migdal effect, constraints on beyond-Standard Model neutrino interactions, and probing 10-eV-scale sterile neutrinos.

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