C. Alpigiani, J. C. Arteaga-Vel'azquez, A. Ball, L. Barak, Jared Barron, B. Batell, J. Beacham, Yan Benhammo, K. Caballero-Mora, P. Camarri, R. Cardarelli, J. Chou, Wentao Cui, D. Curtin, M. Diamond, K. Dienes, L. Dougherty, G. Sciascio, M. Drewes, E. Etzion, R. Essig, J. Evans, A. F. T'ellez, O. Fischer, J. Freeman, J. Gall, Ali Garabaglu, S. Giagu, S. Greenberg, B. Gomber, R. Guida, A. Haas, Y. Heng, S. Hsu, G. Iaselli, K. Johns, A. Kvam, D. Lazic, Liang Li, B. Liberti, Zhen Liu, H. Lubatti, Lillian Luo, G. Marsella, Mario Iv'an Mart'inez Hern'andez, M. McCullough, D. McKeen, P. Meade, G. Mizrachi, O. G. Morales-Olivares, D. Morrissey, M. M. Moshe, A. Policicchio, M. Proffitt, D. C. Ramirez, M. Reece, S. Robertson, M. Rodr'iguez-Cahuantzi, A. Roeck, A. Roepe, J. Rothberg, J. J. Russell, H. Russell, R. Santonico, M. Schioppa, J. Shelton, B. Shuve, Y. Silver, L. D. Stante, D. Stolarski, M. Strauss, D. Strom, J. Stupak, M. Vasquez, S. Swain, G. T. Muñoz, S. A. Thayil, B. Thomas, Yuhsin Tsai, E. Torró, G. W
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Vasquez, S. Swain, G. T. Muñoz, S. A. Thayil, B. Thomas, Yuhsin Tsai, E. Torró, G. W","doi":"10.2172/1659442","DOIUrl":null,"url":null,"abstract":"We report on recent progress in the design of the proposed MATHUSLA Long Lived Particle (LLP) detector for the HL-LHC, updating the information in the original Letter of Intent (LoI), see CDS:LHCC-I-031, arXiv:1811.00927. A suitable site has been identified at LHC Point 5 that is closer to the CMS Interaction Point (IP) than assumed in the LoI. The decay volume has been increased from 20 m to 25 m in height. Engineering studies have been made in order to locate much of the decay volume below ground, bringing the detector even closer to the IP. With these changes, a 100 m x 100 m detector has the same physics reach for large c$\\tau$ as the 200 m x 200 m detector described in the LoI and other studies. The performance for small c$\\tau$ is improved because of the proximity to the IP. Detector technology has also evolved while retaining the strip-like sensor geometry in Resistive Plate Chambers (RPC) described in the LoI. The present design uses extruded scintillator bars read out using wavelength shifting fibers and silicon photomultipliers (SiPM). Operations will be simpler and more robust with much lower operating voltages and without the use of greenhouse gases. Manufacturing is straightforward and should result in cost savings. Understanding of backgrounds has also significantly advanced, thanks to new simulation studies and measurements taken at the MATHUSLA test stand operating above ATLAS in 2018. 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引用次数: 50
摘要
我们报告了用于HL-LHC的MATHUSLA长寿命粒子(LLP)探测器设计的最新进展,更新了原始意向书(LoI)中的信息,见CDS: lhc - i -031, arXiv:1811.00927。在LHC第5点确定了一个合适的位置,该位置比LoI中假设的更接近CMS相互作用点(IP)。衰减体的高度从20米增加到25米。工程研究已经进行,以确定大部分衰减量在地下,使探测器更接近IP。有了这些变化,100米× 100米的探测器具有与LoI和其他研究中描述的200米× 200米探测器相同的大c$\tau$物理达到。由于靠近IP,小c$\tau$的性能得到了改善。探测器技术也得到了发展,同时保留了LoI中描述的电阻板室(RPC)中的条形传感器几何形状。本设计采用挤压式闪烁体条,通过波长移动光纤和硅光电倍增管读出。操作将更简单,更可靠,工作电压更低,不使用温室气体。制造是直截了当的,应该会节省成本。由于2018年在ATLAS上方运行的MATHUSLA测试台进行了新的模拟研究和测量,对背景的理解也得到了显着提高。我们讨论了MATHUSLA合作的下一步,并确定了新成员可以做出特别重要贡献的领域。
An Update to the Letter of Intent for MATHUSLA: Search for Long-Lived Particles at the HL-LHC
We report on recent progress in the design of the proposed MATHUSLA Long Lived Particle (LLP) detector for the HL-LHC, updating the information in the original Letter of Intent (LoI), see CDS:LHCC-I-031, arXiv:1811.00927. A suitable site has been identified at LHC Point 5 that is closer to the CMS Interaction Point (IP) than assumed in the LoI. The decay volume has been increased from 20 m to 25 m in height. Engineering studies have been made in order to locate much of the decay volume below ground, bringing the detector even closer to the IP. With these changes, a 100 m x 100 m detector has the same physics reach for large c$\tau$ as the 200 m x 200 m detector described in the LoI and other studies. The performance for small c$\tau$ is improved because of the proximity to the IP. Detector technology has also evolved while retaining the strip-like sensor geometry in Resistive Plate Chambers (RPC) described in the LoI. The present design uses extruded scintillator bars read out using wavelength shifting fibers and silicon photomultipliers (SiPM). Operations will be simpler and more robust with much lower operating voltages and without the use of greenhouse gases. Manufacturing is straightforward and should result in cost savings. Understanding of backgrounds has also significantly advanced, thanks to new simulation studies and measurements taken at the MATHUSLA test stand operating above ATLAS in 2018. We discuss next steps for the MATHUSLA collaboration, and identify areas where new members can make particularly important contributions.