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探测暗物质EFT:QUEST-DMC项目:投影灵敏度和衰减上限

Probing the Dark Matter EFT with QUEST-DMC: Projected Sensitivities and Attenuation Ceilings

Royal Holloway University of London(伦敦大学皇家霍洛威学院);Lancaster University(兰卡斯特大学);University of Oxford(牛津大学);University of Liverpool(利物浦大学);RIKEN(理化学研究所);UKRI STFC Rutherford Appleton Laboratory(英国研究与创新部科学和技术设施委员会鲁瑟福阿普尔顿实验室)
DMC Collaboration, N. Darvishi, S. Autti, L. Bloomfield, A. Casey, N. Eng, P. Franchini, R. P. Haley, P. J. Heikkinen, A. Jennings, A. Kemp, E. Leason, J. March… 展开作者

DMC Collaboration, N. Darvishi, S. Autti, L. Bloomfield, A. Casey, N. Eng, P. Franchini, R. P. Haley, P. J. Heikkinen, A. Jennings, A. Kemp, E. Leason, J. March-Russell, A. Mayer, J. Monroe, D. Munstermann, M. T. Noble, J. R. Prance, X. Rojas, T. Salmon, J. Saunders, J. Smirnov, R. Smith, M. D. Thompson, A. Thomson, A. Ting, V. Tsepelin, S. M. West, L. Whitehead, D. E. Zmeev

AI总结:

QUEST-DMC实验通过超流³He和纳米机械谐振器探测暗物质,利用低反冲能量阈值探测亚GeV暗物质,并在非相对论EFT框架下预测探测范围及耦合结构。

摘要:

本文总结了QUEST-DMC概念所预测的约束,这是一个基于表面的直接探测实验,使用在毫开尔文以下运行的超流³He,并配备由SQUID读出的纳米机械谐振器。低反冲能量阈值(对于SQUID配置降至亚电子伏特)使该实验能够探测跨多种相互作用结构的亚GeV暗物质,超越了标准的自旋无关和自旋相关限制。我们以非相对论有效场论(EFT)框架提出预测,扫描标准的十四种伽利略不变算符,并以有效暗物质-核子(或暗物质-中子)截面表达探测范围。由于QUEST-DMC在地表运行,我们还考虑了由于大气和地球中的散射导致的入射通量抑制,这在大耦合情况下会产生依赖相互作用的灵敏度上限。最后,我们概述了非相对论结果如何映射到代表性的相对论EFT暗物质-核子双线性项,从而以紫外动机的耦合结构形式简洁地解释预测的探测范围。

英文摘要:

This proceedings contribution summarises projected constraints from the QUEST-DMC concept, a surface-based direct-detection experiment using superfluid $^3$He operated below the millikelvin regime and instrumented with nanomechanical resonators read out by SQUIDs. The low recoil-energy threshold (down to sub-eV for the SQUID configuration) enables sensitivity to sub-GeV dark matter across a wide set of interaction structures beyond the canonical spin-independent and spin-dependent limits. We present projections in the non-relativistic Effective Field Theory (EFT) framework, scanning the standard set of fourteen Galilean-invariant operators and expressing reach in terms of effective dark matter-nucleon (or dark matter-neutron) cross sections. Because QUEST-DMC operates at the surface, we also account for suppression of the incident flux due to scattering in the atmosphere and Earth, which produces an interaction-dependent sensitivity ceiling at large couplings. Finally, we outline how the non-relativistic results map onto representative relativistic EFT dark matter-nucleon bilinears, enabling a compact interpretation of the projected reach in terms of UV-motivated coupling structures.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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