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An Update to the Letter of Intent for MATHUSLA: Search for Long-Lived Particles at the HL-LHC

Authors :
Alpigiani, Cristiano
Arteaga-Velázquez, Juan Carlos
Ball, Austin
Barak, Liron
Barron, Jared
Batell, Brian
Beacham, James
Benhammo, Yan
Caballero-Mora, Karen Salomé
Camarri, Paolo
Cardarelli, Roberto
Chou, John Paul
Cui, Wentao
Curtin, David
Diamond, Miriam
Dienes, Keith R.
Dougherty, Liam Andrew
Di Sciascio, Giuseppe
Drewes, Marco
Etzion, Erez
Essig, Rouven
Evans, Jared
Téllez, Arturo Fernández
Fischer, Oliver
Freeman, Jim
Gall, Jonathan
Garabaglu, Ali
Giagu, Stefano
Greenberg, Stephen Elliott
Gomber, Bhawna
Guida, Roberto
Haas, Andy
Heng, Yuekun
Hsu, Shih-Chieh
Iaselli, Giuseppe
Johns, Ken
Kvam, Audrey
Lazic, Dragoslav
Li, Liang
Liberti, Barbara
Liu, Zhen
Lubatti, Henry
Luo, Lillian
Marsella, Giovanni
Hernández, Mario Iván Martínez
McCullough, Matthew
McKeen, David
Meade, Patrick
Mizrachi, Gilad
Morales-Olivares, O. G.
Morrissey, David
Moshe, Meny Raviv
Policicchio, Antonio
Proffitt, Mason
Ramirez, Dennis Cazar
Reece, Matthew
Robertson, Steven H.
Rodríguez-Cahuantzi, Mario
de Roeck, Albert
Roepe, Amber
Rothberg, Joe
Russell, James John
Russell, Heather
Santonico, Rinaldo
Schioppa, Marco
Shelton, Jessie
Shuve, Brian
Silver, Yiftah
Di Stante, Luigi
Stolarski, Daniel
Strauss, Mike
Strom, David
Stupak, John
Vasquez, Martin A. Subieta
Swain, Sanjay Kumar
Muñoz, Guillermo Tejeda
Thayil, Steffie Ann
Thomas, Brooks
Tsai, Yuhsin
Torro, Emma
Watts, Gordon
Young, Charles
Zurita, Jose
Publication Year :
2020

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. We discuss next steps for the MATHUSLA collaboration, and identify areas where new members can make particularly important contributions.<br />Comment: 22 pages + references, 12 Figures

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2009.01693
Document Type :
Working Paper