利用宇宙射线事件评价目标探测器ν-Angra实验

G. Lopes, D. M. Souza, I. A. Costa, M. Paschoal, A. S. Lopes, M. Migliorini, R. Nobrega, J. Anjos, H. Lima, G. Cernicchiaro, I. Pepe, D. Ribeiro, P. Chimenti, G. Guedes, L. Gonzales, E. Kemp
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引用次数: 0

摘要

v-Angra实验计划开发一种探测器,通过测量中微子事件的速率来推断核反应堆的耗散功率,该系统安装在离核芯几十米远的海平面上。目标探测器是v-安格拉实验及其触发系统的关键组成部分,因为它的信号被发送到触发电子设备,触发电子设备利用它们来选择要存储的事件。此外,宇宙射线代表了它的主要背景噪声,因此,它与探测器相互作用时的特征应该是众所周知的,以便使实验能够开发出有效的事件选择算法。本文对TARGET探测器中宇宙射线事件的特性进行了研究,以期为触发系统的开发提供有价值的信息。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
TARGET detector evaluation using cosmic ray events for the ν-Angra Experiment
The v-Angra Experiments intends to develop a detector capable of inferring the dissipated power of nuclear reactors by means of measuring the rate of neutrinos events detected by a system installed at sea level a few tens of meters away from the nuclear core. The TARGET detector is a key component of the v-Angra Experiment and of its trigger system since its signals are sent to the trigger electronics which makes use of them to select events for storage. Alongside, cosmic rays represent its main background noise and, consequently, its characteristics when interacting with the detector should be well known in order to enable the experiment to develop an efficient events-selection algorithm. This work presents a study of the characteristics of cosmic rays events in the TARGET detector in order to acquire valuable information for the development of trigger system.
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