NOvA Muon Energy Scale Systematic

M. Strait, S. Bending, K. Kephart, P. L. U. O. Minnesota, University College London, F. N. Laboratory
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引用次数: 2

Abstract

The systematic uncertainty on the correspondence between muon range and energy is developed for the NOvA neutrino experiment. NOvA consists of two detectors, the Near Detector at Fermilab and the Far Detector in northern Minnesota. Total errors are developed for the Near Detector, with its Muon Catcher treated separately, the Far Detector, and all combinations of correlated and uncorrelated errors between these three detectors. The absolute errors for the Near Detector (1.0%), the Far Detector (0.9%), and the fully correlated error shared by them (0.9%) are strongly dominated by Geant4's treatment of the Bethe density effect. At the Near Detector, the next biggest uncertainty is from stray hits caused by neutron capture pile-up. Other contributions are marginally significant, with the biggest, in descending order, being due to external measurements of the mean excitation energies of elements, detector mass accounting, and modification of energy loss by chemical binding. For the Muon Catcher, the absolute error is expressed as an offset instead of a percentage: 21 MeV. The density effect (at higher energies) and neutron capture pile-up (at lower energies) are the strongly dominant errors. The relative error between the Near and Far Detectors is 0.4% and is strongly dominated by neutron capture pile-up at the Near Detector, with a subdominant contribution from detector mass accounting.
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新星介子能量刻度系统
为NOvA中微子实验建立了介子范围与能量对应关系的系统不确定度。NOvA由两个探测器组成,费米实验室的近距离探测器和明尼苏达州北部的远距离探测器。总误差开发了近探测器,其μ子捕获器单独处理,远探测器,以及这三个探测器之间相关和不相关误差的所有组合。Geant4对贝特密度效应的处理在很大程度上主导了近探测器(1.0%)、远探测器(0.9%)的绝对误差,以及它们共享的完全相关误差(0.9%)。在近距离探测器上,下一个最大的不确定性来自中子捕获堆积引起的散射撞击。其他贡献也不太重要,最大的贡献(按降序排列)是由于元素平均激发能的外部测量、探测器质量计算和化学结合对能量损失的修正。对于μ子捕集器,绝对误差表示为偏移量而不是百分比:21兆电子伏特。密度效应(高能量)和中子俘获堆积(低能量)是主要的误差。近、远探测器之间的相对误差为0.4%,近探测器的中子捕获堆积在很大程度上占主导地位,而探测器质量核算则占次要地位。
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