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Antineutrino and gamma emission from the OSIRIS research reactor

机译:OSIRIS研究堆的反中微子和γ辐射

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For the first time, the summation method has been coupled with a complete reactor model, in order to predict the antineutrino emission of a research reactor. This work, discussed in the first part of this paper, allows us to predict the low energy part of the antineutrino spectrum, evidencing the important contribution of actinides to the antineutrino emission. Experimental conditions at short distance from research reactors are challenging, because the reactor itself produces huge gamma background that induce accidental and correlated backgrounds in an antineutrino target. The understanding of this background is of utmost importance and triggered the second part of the work presented here.
机译:求和方法首次与完整的反应堆模型相结合,以预测研究堆的反中微子发射。本文第一部分讨论的这项工作使我们能够预测抗中微子谱的低能部分,从而证明了in系元素对抗中微子发射的重要贡献。离研究反应堆不远的实验条件具有挑战性,因为反应堆本身会产生巨大的伽马背景,从而在反中微子目标中诱发偶然的和相关的背景。对这种背景的理解是至关重要的,并触发了此处介绍的第二部分工作。

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