论文标题
Mathusla意向书的更新:在HL-LHC上搜索长寿命的粒子
An Update to the Letter of Intent for MATHUSLA: Search for Long-Lived Particles at the HL-LHC
论文作者
论文摘要
我们报告了HL-LHC的拟议Mathusla Long Live粒子(LLP)检测器的最新进展,更新了原始意向书(LOI)中的信息,请参见CDS:LHCC-II-031,ARXIV:1811.00927。在LHC点5上已经确定了一个合适的位点,该位点比LOI中假定的更接近CMS相互作用点(IP)。衰减量已从20 m增加到25 m。为了将大部分衰减量定位在地下,已经进行了工程研究,从而使检测器更接近IP。随着这些变化,100 m x 100 m的检测器的物理学对于大c $τ$与200 m x 200 m检测器和其他研究中描述的相同。由于与IP的距离,因此小C $τ$的性能得到了改善。检测器技术在LOI中描述的电阻板室(RPC)中保留了带状传感器几何形状时也发展了。目前的设计使用使用波长移动纤维和硅光电层面(SIPM)读取的挤出闪烁杆。操作将变得更简单,更健壮,并且在不使用温室气体的情况下,操作电压较低。制造很简单,应节省成本。由于在2018年在Atlas上方运行的Mathusla测试站进行了新的模拟研究和测量值,对背景的理解也大大提高了。我们讨论了Mathusla协作的下一步步骤,并确定了新成员可以做出特别重要贡献的领域。
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$τ$ as the 200 m x 200 m detector described in the LoI and other studies. The performance for small c$τ$ 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.