EAS thermal neutron detection with the PRISMA-LHAASO-16 experiment

EAS thermal neutron detection with the PRISMA-LHAASO-16 experiment
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使用 PRISMA-LHAASO-16 实验进行 EAS 热中子探测

DOI:
10.1088/1748-0221/12/12/p12028
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发表时间:
2017-08
期刊:
JINST
影响因子:
--
通讯作者:
R. Zhou
R. Zhou
中科院分区:
其他
文献类型:
--
作者:
B.-B. Li;V.V. Alekseenko;S.-w Cui;T.-L. Chen;Dangzengluobu;S.-H. Feng;Q. Gao;Y. Liu;Q.-C. Huang;Y.-Y. He;M.-Y. Liu;X.-H. Ma;E.I. Pozdnyakov;O.B. Shchegolev;F.-Z. Shen;Yu.V. Stenkin;V.I. Stepanov;Ya.V. Yanin;J.-D. Yao;R. Zhou

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EAS(广泛空气簇射)热中子测量有利于研究初级宇宙射线的能量和质量组成,特别是在膝部区域。 PRISMA-YBJ实验成功后,我们于2017年3月在中国拉萨西藏大学(海拔3700米)建造了一个新的EAS热中子探测阵列。这个原型阵列被称为“PRISMA-LHAASO-16”,由16个EAS EN探测器(“EN”是电子和中子的缩写)组成,测量两个主要的EAS成分:强子和电磁成分。与 PRISMA-YBJ 不同,这些探测器使用薄层与天然硼化合物合金化的新型 ZnS(Ag) 闪烁体来捕获热中子。 PRISMA-LHAASO-16将在不久的将来转移到LHAASO现场。本文介绍了检测技术的原理、阵列的部署以及阵列的测试结果。
EAS (extensive air shower) thermal neutron measurement gives advantages to study energy and mass composition of primary cosmic rays especially in the knee region. After the success of the PRISMA-YBJ experiment, we build a new EAS thermal neutron detection array at Tibet University, Lhasa, China (3700 m a.s.l.) in March, 2017. This prototype array so called "PRISMA-LHAASO-16" consists of 16 EAS EN-detectors ("EN" is abbreviation for electron and neutron) measuring two main EAS components: hadronic and electromagnetic ones. Different from PRISMA-YBJ, these detectors use a thin layer of a novel type of ZnS(Ag) scintillator alloyed with natural boron compound for thermal neutron capture. PRISMA-LHAASO-16 will be moved to the LHAASO site in the near future. In this paper, we introduce principle of the detection technique, deployment of the array, and the test results of the array.
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