用于宇宙射线研究的闪烁探测器的研究与开发

Saikat Biswas
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引用次数: 0

摘要

在玻色研究所,Debendra Mohan Bose教授和他的同事在宇宙射线领域做出了全球公认的贡献,包括首次记录μ介子轨迹。博斯教授和比瓦·乔杜里博士在博斯研究所大吉岭校区(以及山打普和法利宗)进行了宇宙射线实验。目前,大吉岭校区拥有一个国家天体粒子物理和空间科学设施。加尔各答还有一个天体粒子物理和空间科学中心。在这两个校区,我们仍在致力于研究宇宙射线的塑料闪烁探测器的研发,以保存博士博士的遗产。由7个塑料闪烁体探测器组成的印度东部唯一的宇宙射线空气阵雨阵列于2018年1月底在喜马拉雅山东部(大吉岭)海拔约2200~米的高度(a.s.l)投入使用。宇宙射线空气阵雨阵列呈六边形,六个探测器分别位于六边形的顶点和中心。两个连续探测器之间的距离为8米。每个探测元件由4个尺寸为50~cm × 50~cm × 1~cm的塑料闪烁体组成,从而形成1~m × 2 ×的总活跃面积。这些闪烁体是在印度奥蒂的TIFR宇宙射线实验室(CRL)本土制造的。探测器的所有四个闪烁体都使用波长移位(WLS)光纤与单个光倍增管(PMT)耦合。一个带有7个输入的定制模块用于生成多重触发器。自2018年1月底以来,对宇宙射线气雨数量的测量一直在进行。在大吉岭实验室,利用塑料闪烁体的三倍重合技术记录了二次宇宙射线通量及其随时间的变化。实验设置的所有细节,测量技术都在前面报道过。本文介绍了结果的更新。本文综述了近五年来我国为研究宇宙射线而进行的塑料闪烁探测器的研发计划。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Research and development of scintillation detectors for the study of cosmic ray
At Bose Institute Prof. Debendra Mohan Bose and his co-workers made globally recognised contributions in the field of cosmic rays including the first recording of mu-meson tracks. Prof. D. M. Bose and Dr. Biva Choudhury did their cosmic ray experiments at the Darjeeling campus of Bose Institute (along with Sandakphu and Pharijong). Presently the Darjeeling campus hosts a National facility for Astroparticle Physics and Space Science. In Kolkata also there is a Centre for Astroparticle Physics and Space Science (CAPSS). In these two campuses, we are still working on the R\&D of plastic scintillation detectors for the study of the cosmic rays to preserve the legacy of Prof. D. M. Bose. The only cosmic ray air shower array in the eastern part of India, consisting of seven plastic scintillator detectors is commissioned at an altitude of about 2200~meters above sea level (a.s.l.) in the Eastern Himalayas (Darjeeling) at the end of January 2018. The cosmic ray air shower array has a hexagon shape with six detectors kept at the vertices ofthe hexagon and one at the center of it. The distance between two consecutive detectors is 8 meters. Each detectorelement is made up of four plastic scintillators of dimension 50~cm~$\times$~50~cm~$\times$~1~cm thereby forming a totalactive area of 1~m$^2$. These scintillators are fabricated indigenously in the Cosmic RayLaboratory (CRL), TIFR, Ooty, India. All four scintillators of a detector are coupled with a singlePhoto Multiplier Tube (PMT) using wavelength shifting (WLS) fibers. A custom-built module withseven inputs is used to generate a multi-fold trigger. Measurement of the number of cosmic ray airshower is going on since the end of January 2018. The secondary cosmic ray flux and its variation overtime are also recorded at the laboratory in Darjeeling using a three-fold coincidence technique withplastic scintillators. All the details of the experimental setup, techniques of measurement are reported earlier. The updates in the results are presented in this article. In this review article, the details of the R\&D program of plastic scintillation detectors carried out during the last five years, for the study of cosmic ray is reported.
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