面向国际空间站安装的面包板型伽玛暴偏振计的评估

Yuma Oikawa, S. Gunji, T. Nakamori, M. Takakura, T. Ueda, Tatsuya Kishikawa, S. Daigle, J. Gaskin, B. Ramsey, C. Wilson-Hodge, R. Preece, M. McConnell, P. Bloser, J. Legere, D. Yonetoku, T. Mihara, K. Hayashida, Y. Kishimoto, S. Kishimoto, H. Takahashi, Y. Yatsu, K. Toma, T. Sakamoto
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引用次数: 0

摘要

为了阐明伽马射线暴的辐射机制,我们正在研制由分段塑料闪烁体和GAGG(Ce)闪烁体组成的偏振计,它们分别与多阳极光电倍增管和雪崩光电二极管相连。用36片塑料闪烁体和24片GAGG(Ce)闪烁体构建面包板模型,在日本KEK光子工厂进行了光束实验。同时,我们还进行了计算机仿真,并将实验数据与仿真结果进行了比较。结果表明,实验得到的调制因子与仿真得到的调制因子基本一致。另一方面,虽然实验得到的检测效率与仿真得到的检测效率大致一致,但检测效率的数值却不能很好地合理解释。这种差异可能是由于塑料闪烁体的能量校准不完整所致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evaluation of a bread board model gamma-ray burst polarimeter toward installation on the international space station
To elucidate the radiation mechanism of gamma ray bursts, we are developing the polarimeter which consists of segmented plastic scintillators and GAGG(Ce) scintillators attached with multi-anode photomultipliers and avalanche photodiodes, respectively. Constructing the bread board model with 36 pieces of plastic scintillator and 24 pieces of GAGG(Ce) scintillator, we have carried out the beam experiments at the KEK Photon Factory in Japan. At the same time, we carried out also computer simulation and we compared the experimental data with results of simulations. As the results, it was recognized that the modulation factor by the experiments is consistent with that by the simulations. On the other hand, though the detection efficiency obtained by the experiments is in rough agreement with that by the simulation, the value of the detection efficiency can not be well explained reasonably. This discrepancy is likely due to the incomplete energy calibration of the plastic scintillators.
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