MATHUSLA意向书:ATLAS或CMS之上的专用位移顶点检测器。

C. Alpigiani, A. Ball, L. Barak, J. Beacham, Yan Benhammo, T. Cao, P. Camarri, R. Cardarelli, M. Rodríguez-Cahuantzi, J. Chou, D. Curtin, M. Diamond, G. Sciascio, M. Drewes, S. Eno, E. Etzion, R. Essig, J. Evans, O. Fischer, S. Giagu, Brandon Gomes, A. Haas, Y. Heng, G. Iaselli, K. Johns, M. Karagoz, L. Kasper, A. Kvam, D. Lazic, Liang Li, B. Liberti, Zhen Liu, H. Lubatti, G. Marsella, M. McCullough, D. McKeen, P. Meade, G. Mizrachi, D. Morrissey, M. M. Moshe, K. S. Caballero-Mora, Piter A. Paye Mamani, A. Policicchio, M. Proffitt, M. Reggiani-Guzzo, J. Rothberg, R. Santonico, M. Schioppa, J. Shelton, B. Shuve, M. Vasquez, D. Stolarski, A. Roeck, A. F. Tellez, G. T. Muñoz, M. I. M. Hernández, Y. Silver, S. A. Thayil, E. Torró, Yuhsin Tsai, J. C. Arteaga-Velázquez, G. Watts, C. Young, J. Zurita
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引用次数: 65

摘要

在这份意向书(LOI)中,我们提议在ATLAS或CMS表面上为HL-LHC建造一个专用的大体积位移顶点探测器MATHUSLA (MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles)。这种探测器可以在HL-LHC升级之前利用现有技术和合理的预算建造,可以以比ATLAS或CMS高几个数量级的灵敏度搜索中性长寿命粒子(LLPs),同时也可以作为CERN的尖端宇宙射线望远镜,探索宇宙射线和天体粒子物理学中的许多悬而未决的问题。我们回顾了MATHUSLA的物理动机,总结了几种不同可能的探测器几何形状的LLP到达,并概述了宇宙射线物理程序。我们为MATHUSLA提供了几项最新的背景研究,这些研究有助于为第一个探测器设计概念提供信息,该概念利用电阻板室(rpc)作为主要跟踪技术的模块化结构。我们提出了第一个效率和重建研究,以验证这一设计概念的可行性,并探讨了其总成本的一些方面。最后,我们总结了MATHUSLA试验台的最新进展,这是一个目前在欧洲核子研究中心1号点采集数据的小规模示范实验,并对未来的工作进行了简短的评论。
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A Letter of Intent for MATHUSLA: a dedicated displaced vertex detector above ATLAS or CMS.
In this Letter of Intent (LOI) we propose the construction of MATHUSLA (MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles), a dedicated large-volume displaced vertex detector for the HL-LHC on the surface above ATLAS or CMS. Such a detector, which can be built using existing technologies with a reasonable budget in time for the HL-LHC upgrade, could search for neutral long-lived particles (LLPs) with up to several orders of magnitude better sensitivity than ATLAS or CMS, while also acting as a cutting-edge cosmic ray telescope at CERN to explore many open questions in cosmic ray and astro-particle physics. We review the physics motivations for MATHUSLA and summarize its LLP reach for several different possible detector geometries, as well as outline the cosmic ray physics program. We present several updated background studies for MATHUSLA, which help inform a first detector-design concept utilizing modular construction with Resistive Plate Chambers (RPCs) as the primary tracking technology. We present first efficiency and reconstruction studies to verify the viability of this design concept, and we explore some aspects of its total cost. We end with a summary of recent progress made on the MATHUSLA test stand, a small-scale demonstrator experiment currently taking data at CERN Point 1, and finish with a short comment on future work.
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