ATLAS μ子触发“切片”

A. Sidoti, M. Bellomo, M. Biglietti, G. Carlino, G. Cataldi, F. Conventi, S. Cecco, A. Dimattia, C. Dionisi, S. Falciano, S. Giagu, E. Gorini, S. Grancagnolo, M. Inada, M. Kanaya, T. Kono, A. Krasznahorkay, H. Kiyamura, H. Kurashige, T. Kuwabara, C. Luci, L. Luminari, F. Marzano, A. Migliaccio, K. Nagano, A. Nisati, C. Omachi, N. Panikashvili, E. Pasqualucci, M. Primavera, M. Rescigno, I. Riu, P. Ryan, D. Scannicchio, G. Siragusa, S. Spagnolo, S. Tarem, Z. Tarem, K. Tokushuku, G. Usai, A. Ventura, V. Vercesi, Y. Yamazaki
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引用次数: 3

摘要

大型强子对撞机的ATLAS实验将面临在14 TeV质能中心的质子-质子碰撞中选择有趣的候选事件,同时拒绝大量背景事件的挑战。触发器系统架构分为三个层次。从40兆赫的串交叉率的第一级触发器,硬件实现,将降低到约75千赫的速率。然后,由二级触发器和事件滤波器组成的基于软件的高电平触发器(HLT)将频率降低到~ 200hz。HLT在商用cpu上使用基于通用ATLAS面向对象软件体系结构的框架实现。包容性触发器选择用于为ATLAS物理程序收集事件;具有μ子的最终态对于电弱精确测量以及希格斯和超对称性的搜索至关重要。在本文中,我们将介绍基于蒙特卡罗模拟的在线μ子选择的μ子切片、信号效率、背景抑制率和系统性能(执行时间等)的实现,以及在宇宙数据采集运行期间收集的真实事件中获得的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The ATLAS Muon Trigger "Slice"
The ATLAS experiment at the LHC will face the challenge of selecting interesting candidate events in proton-proton collisions at 14 TeV center of mass energy, while rejecting the enormous number of background events. The trigger system architecture is organized in three levels. From a bunch crossing rate of 40 MHz the First level trigger, hardware implemented, will reduce this rate to around ~75 kHz. Then the software based high level trigger (HLT), composed by the second level trigger and the event filter reduces the rate to ~ 200 Hz. HLT is implemented on commercial CPUs using a framework built on the common ATLAS object oriented software architecture. Inclusive trigger selections are used to collect events for the ATLAS physics program; final states with muons are crucial for electroweak precision measurements as well as Higgs and SUSY searches. In this paper we will present the implementation of the muon slice, signal efficiencies, background rejection rates and system performances (execution time,...) for online muon selection based on Monte Carlo simulations and results obtained on real events collected during cosmic data taking runs.
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