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Atmospheric neutrino oscillations with DeepCore

机译：DeepCore的大气中微子振荡

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摘要

IceCube DeepCore can study atmospheric neutrino oscillations through a combination of its low energy reach,as low as about 10 GeV, and its unprecedented statistical sample, of about 150,000 triggered atmospheric muon neutrinosper year. With the diameter of the earth as a baseline, the muon neutrino disappearance minimum and tau neutrinoappearance maximum are expected at about 25 GeV, which is considerably lower energy than typical IceCube neutrinoevents, but higher than the energies at which accelerator-based experiments have detected oscillations. We present herethe status of the newly developed low energy reconstruction algorithms, the expected experimental signatures, and theproposed approach fotrino oscillation measurements.
机译：IceCube DeepCore可通过其低能量范围（低至约10 GeV）和其空前的统计样本（每年约150,000个触发的大气μ子中微子）相结合来研究大气中微子振荡。以地球直径为基准，预计μ子中微子消失最小值和τ中微子外观最大值约为25 GeV，这比典型的IceCube中微子事件要低得多，但比基于加速器的实验检测到振荡时的能量要高。 。我们在这里介绍新近开发的低能量重建算法的状态，预期的实验特征以及拟议的方法振荡振荡测量。

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