Development of the prototype of a large-volume liquid scintillation detector with photosensors based on silicon photomultiplayers

I. Dzaparova, A. Yanin, E. Gorbacheva, A. Kurenya, V. Petkov, I. Unatlokov, A. Shikhin
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Abstract

At present, the Institute for Nuclear Research of RAS carries out work on the creation of a large-volume scintillation detector at the Baksan Neutrino Observatory (BNO) to register natural low-energy neutrino fluxes, including from astrophysical sources. One of the prototypes of such a detector being developed at the BNO is an acrylic sphere with a diameter of 500 mm filled with a liquid scintillator. Matrices of silicon photomultipliers (SiPM) as photosensors are used to measure the total light output from the interaction of particles in the scintillator and to obtain images of such events. This approach makes it possible to separate useful events from background ones and thereby to lower the background when monitoring Supernova explosions in our Galaxy. The paper describes the prototype of a large-volume detector and presents the measurement results. The Multifaceted Universe: Theory Observations
基于硅光电多播放器的大体积液体闪烁探测器原型机的研制
目前,RAS核研究所正在巴克桑中微子天文台(BNO)建造一个大容量闪烁探测器,以记录自然低能中微子通量,包括来自天体物理源的中微子通量。BNO正在开发的这种探测器的原型之一是一个直径为500毫米的丙烯酸球体,里面充满了液体闪烁体。硅光电倍增管(SiPM)矩阵作为光传感器用于测量闪烁体中粒子相互作用产生的总光输出并获得此类事件的图像。这种方法可以将有用的事件从背景事件中分离出来,从而在监测银河系中的超新星爆炸时降低背景。本文介绍了一种大体积探测器的样机,并给出了测量结果。多面宇宙:理论观测
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