相干实验对加速器产生的暗物质的灵敏度

C. C. D. Akimov, Peibo An, C. Awe, P. Barbeau, B. Becker, V. Belov, M. Blackston, A. Bolozdynya, B. Cabrera-Palmer, N. Chen, E. Conley, R. Cooper, J. Daughhetee, M. D. V. Coello, J. Detwiler, M. Durand, Y. Efremenko, S. Elliott, L. Fabris, M. Febbraro, W. Fox, A. Galindo-Uribarri, M. Green, K. S. Hansen, M. Heath, S. Hedges, T. Johnson, M. Kaemingk, L. Kaufman, A. Khromov, A. Konovalov, E. Kozlova, A. Kumpan, L. Li, J. Librande, J. Link, J. Liu, K. Mann, D. Markoff, H. Moreno, P. Mueller, J. Newby, D. Parno, S. Penttila, D. Pershey, D. Radford, R. Rapp, H. Ray, J. Raybern, O. Razuvaeva, D. Reyna, G. Rich, D. Rudik, J. Runge, D. Salvat, K. Scholberg, A. Shakirov, G. Simakov, G. Sinev, W. Snow, V. Sosnovtsev, B. Suh, R. Tayloe, K. Tellez-Giron-Flores, R. Thornton, I. Tolstukhin, J. Vanderwerp, R. Varner, C. Virtue, G. Visser, C. Wiseman, T. Wongjirad, J. Yang, Y. Yen, J. Yoo, C.-H. Yu, J. Zettlemoyer
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引用次数: 39

摘要

相干实验很好地准备了测试亚gev暗物质模型,使用对相干弹性中微子核散射(CEvNS)敏感的低能反冲探测器,在由散裂中子源产生的$\pi$ -DAR中微子束中。我们展示了计划中的750公斤液态氩闪烁探测器将如何对标量光暗物质模型施加领先限制,超过暗物质质量的两个数量级,对于通过矢量和疏光门户产生的暗物质粒子,在没有其他超出标准模型的影响的情况下。$\pi$ -DAR波束的特征定时结构提供了一个独特的机会,可以在不期望信号的时间窗口中约束标准模型背景上的系统不确定性,从而提高期望灵敏度。此外,我们讨论了未来的前景,进一步增加CEvNS探测器的发现潜力。这样的方法将在一个数量级的暗物质质量上,测试矢量门户模型中所有耦合$\alpha'\leq1$计算出的热暗物质丰度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Sensitivity of the COHERENT experiment to accelerator-produced dark matter
The COHERENT experiment is well poised to test sub-GeV dark matter models using low-energy recoil detectors sensitive to coherent elastic neutrino-nucleus scattering (CEvNS) in the $\pi$-DAR neutrino beam produced by the Spallation Neutron Source. We show how a planned 750-kg liquid argon scintillation detector would place leading limits on scalar light dark matter models, over two orders of magnitude of dark matter mass, for dark matter particles produced through vector and leptophobic portals in the absence of other effects beyond the standard model. The characteristic timing structure of a $\pi$-DAR beam allows a unique opportunity for constraining systematic uncertainties on the standard model background in a time window where signal is not expected, enhancing expected sensitivity. Additionally, we discuss future prospects, further increasing the discovery potential of CEvNS detectors. Such methods would test the calculated thermal dark matter abundance for all couplings $\alpha'\leq1$ within the vector portal model over an order of magnitude of dark matter masses.
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