伽玛射线空间天文学用溴化镧三维成像量热计的研制

A. Gostojić, V. Tatischeff, J. Kiener, C. Hamadache, N. Karkour, D. Linget, G. Sedes, S. Blin, P. Barrillon
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引用次数: 4

摘要

新一代高光输出无机闪烁体即掺铈溴化镧(LaBr3:Ce)作为天基γ射线量热计具有广阔的应用前景。它的内部特性,如良好的能量分辨率或辐射耐受性,非常适合探测MeV范围内的γ射线,从而提供了迄今为止在核合成、活跃太阳或天体物理致密物体等物理学中尚未得到充分研究的问题。为此,在创建新型康普顿望远镜原型的项目下,我们研究了由5×5 cm2面积和1 cm厚的LaBr3:Ce晶体闪烁体耦合到ASIC MAROC读出的64通道多阳极光电倍增管的探测模块的响应。各种放射源的测量结果已经与详细的GEANT4模拟进行了比较,其中包括对闪烁晶体中产生的近紫外光子的跟踪。利用人工神经网络研究了γ射线入射第一相互作用点的定位。与其他测量特性一起,我们获得的位置分辨率使这个探测器模块对在中能量γ射线域中工作的下一代太空望远镜非常有趣。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Development of a 3D imaging calorimeter in lanthanum bromide for gamma-ray space astronomy
The new generation of high light-output inorganic scintillators i.e. cerium-doped lanthanum(III) bromide (LaBr3:Ce) show a promising future in application as a space-based γ-ray calorimeter. Its internal qualities such as good energy resolution or radiation tolerance are well suited for detection of γ-rays in the MeV range, thus providing access to, so far, understudied questions in physics of nucleosynthesis, the active Sun or astrophysical compact objects. For this purpose, under the project of creating a new Compton telescope prototype, we have studied the response of a detection module comprising a 5×5 cm2 area and 1 cm thick LaBr3:Ce crystal scintillator coupled to a 64 channel multi-anode photomultiplier read out by the ASIC MAROC. Measurements with various radioactive sources have been compared with detailed GEANT4 simulations that include the tracking of the near-UV photons produced in the scintillation crystal. The localization of the first interaction point of incident γ-rays have been studied from the measured charge distributions using an artificial neural network. Together with the other measured properties, the position resolution that we obtain makes this detector module very interesting for the next generation of space telescopes operating in the medium-energy γ-ray domain.
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