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arXiv · 2001.03073

Technical Proposal: FASERnu

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.

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FASER Collaboration, Henso Abreu, Marco Andreini, Claire Antel, Akitaka Ariga, Tomoko Ariga, Caterina Bertone, Jamie Boyd, Andy Buckley, Franck Cadoux, David W. Casper, Francesco Cerutti, Xin Chen, Andrea Coccaro, Salvatore Danzeca, Liam Dougherty, Candan Dozen, Peter B. Denton, Yannick Favre, Deion Fellers, Jonathan L. Feng, Didier Ferrere, Jonathan Gall, Iftah Galon, Stephen Gibson, Sergio Gonzalez-Sevilla, Shih-Chieh Hsu, Zhen Hu, Giuseppe Iacobucci, Sune Jakobsen, Roland Jansky, Enrique Kajomovitz, Felix Kling, Umut Kose, Susanne Kuehn, Mike Lamont, Helena Lefebvre, Lorne Levinson, Ke Li, Josh McFayden, Sam Meehan, Dimitar Mladenov, Mitsuhiro Nakamura, Toshiyuki Nakano, Marzio Nessi, Friedemann Neuhaus, John Osborne, Hidetoshi Otono, Serge Pelletier, Brian Petersen, Francesco Pietropaolo, Michaela Queitsch-Maitland, Filippo Resnati, Marta Sabate-Gilarte, Jakob Salfeld-Nebgen, Francisco Sanchez Galan, Pablo Santos Diaz, Osamu Sato, Paola Scampoli, Kristof Schmieden, Matthias Schott, Holger Schulz, Anna Sfyrla, Savannah Shively, Jordan Smolinsky, Aaron M. Soffa, Yosuke Takubo, Eric Torrence, Sebastian Trojanowski, Serhan Tufanli, Dengfeng Zhang, Gang Zhang. 2020-01-09. Technical Proposal: FASERnu. https://arxiv.org/abs/2001.03073

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