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Technical Proposal: FASERnu

Authors :
FASER Collaboration
Abreu, Henso
Andreini, Marco
Antel, Claire
Ariga, Akitaka
Ariga, Tomoko
Bertone, Caterina
Boyd, Jamie
Buckley, Andy
Cadoux, Franck
Casper, David W.
Cerutti, Francesco
Chen, Xin
Coccaro, Andrea
Danzeca, Salvatore
Dougherty, Liam
Dozen, Candan
Denton, Peter B.
Favre, Yannick
Fellers, Deion
Feng, Jonathan L.
Ferrere, Didier
Gall, Jonathan
Galon, Iftah
Gibson, Stephen
Gonzalez-Sevilla, Sergio
Hsu, Shih-Chieh
Hu, Zhen
Iacobucci, Giuseppe
Jakobsen, Sune
Jansky, Roland
Kajomovitz, Enrique
Kling, Felix
Kose, Umut
Kuehn, Susanne
Lamont, Mike
Lefebvre, Helena
Levinson, Lorne
Li, Ke
McFayden, Josh
Meehan, Sam
Mladenov, Dimitar
Nakamura, Mitsuhiro
Nakano, Toshiyuki
Nessi, Marzio
Neuhaus, Friedemann
Osborne, John
Otono, Hidetoshi
Pelletier, Serge
Petersen, Brian
Pietropaolo, Francesco
Queitsch-Maitland, Michaela
Resnati, Filippo
Sabate-Gilarte, Marta
Salfeld-Nebgen, Jakob
Galan, Francisco Sanchez
Diaz, Pablo Santos
Sato, Osamu
Scampoli, Paola
Schmieden, Kristof
Schott, Matthias
Schulz, Holger
Sfyrla, Anna
Shively, Savannah
Smolinsky, Jordan
Soffa, Aaron M.
Takubo, Yosuke
Torrence, Eric
Trojanowski, Sebastian
Tufanli, Serhan
Zhang, Dengfeng
Zhang, Gang
Publication Year :
2020

Abstract

FASERnu is a proposed small and inexpensive emulsion detector designed to detect collider neutrinos for the first time and study their properties. FASERnu will be located directly in front of FASER, 480 m from the ATLAS interaction point along the beam collision axis in the unused service tunnel TI12. From 2021-23 during Run 3 of the 14 TeV LHC, roughly 1,300 electron neutrinos, 20,000 muon neutrinos, and 20 tau neutrinos will interact in FASERnu with TeV-scale energies. With the ability to observe these interactions, reconstruct their energies, and distinguish flavors, FASERnu will probe the production, propagation, and interactions of neutrinos at the highest human-made energies ever recorded. The FASERnu detector will be composed of 1000 emulsion layers interleaved with tungsten plates. The total volume of the emulsion and tungsten is 25cm x 25cm x 1.35m, and the tungsten target mass is 1.2 tonnes. From 2021-23, 7 sets of emulsion layers will be installed, with replacement roughly every 20-50 1/fb in planned Technical Stops. In this document, we summarize FASERnu's physics goals and discuss the estimates of neutrino flux and interaction rates. We then describe the FASERnu detector in detail, including plans for assembly, transport, installation, and emulsion replacement, and procedures for emulsion readout and analyzing the data. We close with cost estimates for the detector components and infrastructure work and a timeline for the experiment.<br />49 pages, 25 figures; submitted to the CERN LHCC on 28 October 2019

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....a73a3ce6ba3b1fa98c79bf92d2cf0934