论文标题

Gran Sasso表面实验室的环境子-MEV中子测量,具有超细颗粒核乳液检测器

Environmental sub-MeV neutron measurement at the Gran Sasso surface laboratory with a super-fine-grained nuclear emulsion detector

论文作者

Shiraishi, T., Akamatsu, S., Naka, T., Asada, T., De Lellis, G., Tioukov, V., Rosa, G., Kobayashi, R., Ambrosio, N., Alexandrov, A., Sato, O.

论文摘要

环境中子的测量在寻找新物理学(例如暗物质颗粒)中尤其重要,因为中子构成了通常毫无疑问的背景来源。从技术上讲,在亚M-EV量表上的中子能谱的测量很困难,因为它需要非常好的能量分辨率和非常高的$γ$ - 射线排斥能力。在这项研究中,我们使用了一种称为Nano Imaging Tracker(NIT)的超细颗粒核乳液作为中子检测器。中子的主要目标是乳液膜的氢(质子)含量。通过拓扑分析,可以检测到由中子散射引起的质子后坐力,作为具有亚微米准确性的轨道。该方法显示了极高的$γ$ - 射线拒绝功率,$ 5 \ times 10^7〜γ/\ rm {cm}^2 $,相当于环境$γ$ - 砂的5年积累,即使在Sub-Mev Energy地区也是非常好的能量和方向分辨率。为了使用足够的统计数据进行此测量,我们升级了自动扫描系统,以达到250 g/ear/naker的速度。我们用880 KEV单色中子校准了该系统的检测器性能:发现所有相关运动学变量的期望与期望非常好。开发的方法应用于在Infn Gran Sasso表面实验室暴露的样品中的应用,首次测量了$(7.6 \ pm 1.7)\ times 10^{ - 3} \ rm {cm {cm}^{cm}^{-2} { - 2} \ rmmm {s}^reton to pots of neconon and 1 n 0.能量范围在0.25至10 meV之间),与预测一致。中子能量和方向分布也显示出良好的一致性。

The measurement of environmental neutrons is particularly important in the search for new physics, such as dark matter particles, because neutrons constitute an often-irreducible background source. The measurement of the neutron energy spectra in the sub-MeV scale is technically difficult because it requires a very good energy resolution and a very high $γ$-ray rejection power. In this study, we used a super-fine-grained nuclear emulsion, called Nano Imaging Tracker (NIT), as a neutron detector. The main target of neutrons is the hydrogen (proton) content of emulsion films. Through a topological analysis, proton recoils induced by neutron scattering can be detected as tracks with sub-micrometric accuracy. This method shows an extremely high $γ$-ray rejection power, at the level of $5 \times 10^7 ~ γ/\rm{cm}^2$, which is equivalent to 5 years accumulation of environmental $γ$-rays, and a very good energy and direction resolution even in the sub-MeV energy region. In order to carry out this measurement with sufficient statistics, we upgraded the automated scanning system to achieve a speed of 250 g/year/machine. We calibrated the detector performance of this system with 880 keV monochromatic neutrons: a very good agreement with the expectation was found for all the relevant kinematic variables. The application of the developed method to a sample exposed at the INFN Gran Sasso surface laboratory provided the first measurement of sub-MeV environmental neutrons with a flux of $(7.6 \pm 1.7) \times 10^{-3} \rm{cm}^{-2} \rm{s}^{-1}$ in the proton energy range between 0.25 and 1 MeV (corresponds to neutron energy range between 0.25 and 10 MeV), consistent with the prediction. The neutron energy and direction distributions also show a good agreement.

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