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Simulations of neutron background in a time projection chamber relevant to dark matter searches

机译:与暗物质搜索有关的时间投影室内中子背景的模拟

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Presented here are results of simulations of neutron background performed for a time projection chamber acting as a particle dark matter detector in an underground laboratory. The investigated background includes neutrons from rock and detector components, generated via spontaneous fission and (alpha,n) reactions, as well as those due to cosmic-ray muons. Neutrons were propagated to the sensitive volume of the detector and the nuclear recoil spectra were calculated. Methods of neutron background suppression were also examined and limitations to the sensitivity of a gaseous dark matter detector are discussed. Results indicate that neutrons should not limit sensitivity to WIMP-nucleon interactions down to a level of (I - 3) x 10(-8) pb in a 10 kg detector. (c) 2005 Elsevier B.V. All rights reserved.
机译:这里介绍的是在地下实验室中充当粒子暗物质探测器的时间投影室进行的中子本底模拟结果。研究的背景包括来自岩石和探测器成分的中子,这些中子是通过自发裂变和(α,n)反应产生的,以及由于宇宙射线μ子而产生的中子。中子传播到探测器的敏感体积,并计算核反冲谱。还研究了中子本底抑制方法,并讨论了气态暗物质探测器灵敏度的局限性。结果表明,中子不应在10 kg的检测器中将对WIMP-核子相互作用的敏感性降低到(I-3)x 10(-8)pb的水平。 (c)2005 Elsevier B.V.保留所有权利。

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