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The relation between the deposit energies of the muons and their primary energies, and the relation between the deposit energies and their Cherenkov light yields in KM3 detector

机译:KM3探测器中介子的沉积能与其一次能之间的关系,以及沉积能与其契伦科夫光量之间的关系

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In the KM3 detector or pre-KM3 detector like AMANDA, one may recognize that [1] the deposit energiesof the muon produced in the detector by neutrino interaction are proportional to their primary muon energies and [2]these deposit energies are equivalent to Cherenkov light yield produced by the deposit energies. In these detectors inwhich high energy muons are detected via Cherenkov light, one may recognize that the primary energies of the muonsare uniquely determined by measuring Cherenkov yields in the detector under the prepositions of [1] and [2]. We havecarried out extensive numerical compute experiments for the examination on the validities of the prepositions [1] and [2].In our present paper, we discuss these validities quantitatively in detail.
机译:在像AMANDA这样的KM3探测器或KM3之前的探测器中,人们可能认识到[1]中微子相互作用在探测器中产生的μ子的沉积能与它们的主要μ子能成正比,[2]这些沉积能等于契伦科夫光沉积能量产生的产量。在这些通过切伦科夫光检测到高能μ子的探测器中,人们可能会认识到,通过在[1]和[2]的介词下通过测量探测器中的切伦科夫屈服来唯一确定μ子的一次能。我们对介词[1]和[2]的有效性进行了大量的数值计算实验。在本文中,我们对这些有效性进行了详细的定量讨论。

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