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Muon energy reconstruction and atmospheric neutrino spectrum unfolding with the ANTARES detector

机译:利用ANTARES探测器进行μon能量重建和大气中微子谱展开

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Measurement of the atmospheric muon neutrino spectrum is important since it is a test on the expected con-ventionalatmospheric neutrino fluxes as well as on the prompt contribution from charm decay. In addition to that, itforms the irreducible background for high energy cosmic neutrinos searches. A number of methods have been developedwithin the ANTARES collaboration for the estimation of the energy of muon tracks traversing the detector. These includea maximum likelihood method, an approach based on neural networks as well as an estimator based on the energy loss ofthe muon along its track. The reconstructed muon energy can be used to calculate the energy spectrum of the atmosphericneutrinos by using a singular value decomposition approach on regularized unfolding. The most recent results on theenergy reconstruction and spectrum deconvolution will be presented.
机译:大气μon中微子谱的测量很重要,因为它是对预期的常规大气中微子通量以及魅力衰减的迅速贡献的测试。除此之外,它还为高能宇宙中微子搜索形成了不可约的背景。在ANTARES协作范围内,已经开发了许多方法来估计穿过探测器的μ子轨道的能量。其中包括最大似然法,一种基于神经网络的方法以及一种基于μ子沿其轨迹的能量损耗的估计器。通过对正则展开采用奇异值分解方法,重构的μ子能可用于计算大气中微子的能谱。将介绍有关能量重构和频谱去卷积的最新结果。

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