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首页> 外文期刊>Physical review, D >Foraging for dark matter in large volume liquid scintillator neutrino detectors with multiscatter events
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Foraging for dark matter in large volume liquid scintillator neutrino detectors with multiscatter events

机译:在具有多重散射事件的大容量液体闪烁器中微子探测器中寻找暗物质

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We show that dark matter with a per-nucleon scattering cross section ? 10 ? 28 ? ? cm 2 could be discovered by liquid scintillator neutrino detectors like Borexino, SNO + , and JUNO. Due to the large dark matter fluxes admitted, these detectors could find dark matter with masses up to 1 0 21 ? ? GeV , surpassing the mass sensitivity of current direct detection experiments (such as XENON1T and PICO) by over 2 orders of magnitude. We derive the spin-independent and spin-dependent cross section sensitivity of these detectors using existing selection triggers, and we propose an improved trigger program that enhances this sensitivity by 2 orders of magnitude. We interpret these sensitivities in terms of three dark matter scenarios: (1)?effective contact operators for scattering, (2)?QCD-charged dark matter, and (3)?a recently proposed model of Planck-mass baryon-charged dark matter. We calculate the flux attenuation of dark matter at these detectors due to the earth overburden, taking into account the earth’s density profile and elemental composition, as well as nuclear spins.
机译:我们证明暗物质具有每个核子的散射截面? 10? 28? ?液体闪烁体中微子探测器(例如Borexino,SNO +和JUNO)可以发现cm 2。由于允许大量的暗物质通量,这些探测器可以发现质量最高为1 0 21?的暗物质。 ? GeV超过当前直接检测实验(例如XENON1T和PICO)的质量灵敏度超过2个数量级。我们使用现有的选择触发器得出这些检测器的自旋无关和自旋相关截面灵敏度,并且我们提出了一种改进的触发器程序,可以将该灵敏度提高2个数量级。我们从三种暗物质的情况来解释这些敏感性:(1)用于散射的有效接触算子,(2)QCD带电的暗物质,以及(3)最近提出的普朗克质量重子带电暗物质模型。考虑到地球的密度分布和元素组成以及核自旋,我们计算了由于地球覆盖而导致的这些探测器的暗物质通量衰减。

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