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ICARUS at the Fermilab Short-Baseline Neutrino program: initial operation

  • P. Abratenko
  • , A. Aduszkiewicz
  • , F. Akbar
  • , M. Artero Pons
  • , J. Asaadi
  • , M. Aslin
  • , M. Babicz
  • , W. F. Badgett
  • , L. F. Bagby
  • , B. Baibussinov
  • , B. Behera
  • , V. Bellini
  • , O. Beltramello
  • , R. Benocci
  • , J. Berger
  • , S. Berkman
  • , S. Bertolucci
  • , R. Bertoni
  • , M. Betancourt
  • , M. Bettini
  • S. Biagi, K. Biery, O. Bitter, M. Bonesini, T. Boone, B. Bottino, A. Braggiotti, D. Brailsford, J. Bremer, S. J. Brice, V. Brio, C. Brizzolari, J. Brown, H. S. Budd, F. Calaon, A. Campani, D. Carber, M. Carneiro, I. Caro Terrazas, H. Carranza, D. Casazza, L. Castellani, A. Castro, S. Centro, G. Cerati, M. Chalifour, P. Chambouvet, A. Chatterjee, D. Cherdack, S. Cherubini, N. Chithirasreemadam, M. Cicerchia, V. Cicero, T. Coan, A. G. Cocco, M. R. Convery, S. Copello, E. Cristaldo, A. A. Dange, I. de Icaza Astiz, A. De Roeck, S. Di Domizio, L. Di Noto, C. Di Stefano, D. Di Ferdinando, M. Diwan, S. Dolan, L. Domine, S. Donati, R. Doubnik, F. Drielsma, J. Dyer, S. Dytman, C. Fabre, F. Fabris, A. Falcone, C. Farnese, A. Fava, H. Ferguson, A. Ferrari, F. Ferraro, N. Gallice, F. G. Garcia, M. Geynisman, M. Giarin, D. Gibin, S. G. Gigli, A. Gioiosa, W. Gu, M. Guerzoni, A. Guglielmi, G. Gurung, S. Hahn, K. Hardin, H. Hausner, A. Heggestuen, C. Hilgenberg, M. Hogan, B. Howard, R. Howell, J. Hrivnak, M. Iliescu, G. Ingratta, C. James, W. Jang, M. Jung, Y. J. Jwa, L. Kashur, W. Ketchum, J. S. Kim, D. H. Koh, U. Kose, J. Larkin, G. Laurenti, G. Lukhanin, S. Marchini, C. M. Marshall, S. Martynenko, N. Mauri, A. Mazzacane, K. S. McFarland, D. P. Méndez, A. Menegolli, G. Meng, O. G. Miranda, D. Mladenov, A. Mogan, N. Moggi, E. Montagna, C. Montanari, A. Montanari, M. Mooney, G. Moreno-Granados, J. Mueller, D. Naples, M. Nebot-Guinot, M. Nessi, T. Nichols, M. Nicoletto, B. Norris, S. Palestini, M. Pallavicini, V. Paolone, R. Papaleo, L. Pasqualini, L. Patrizii, R. Peghin, G. Petrillo, C. Petta, V. Pia, F. Pietropaolo, J. Poirot, F. Poppi, M. Pozzato, M. C. Prata, A. Prosser, G. Putnam, X. Qian, G. Rampazzo, A. Rappoldi, G. L. Raselli, R. Rechenmacher, F. Resnati, A. M. Ricci, G. Riccobene, L. Rice, E. Richards, A. Rigamonti, M. Rosenberg, M. Rossella, C. Rubbia, P. Sala, P. Sapienza, G. Savage, A. Scaramelli, A. Scarpelli, D. Schmitz, A. Schukraft, F. Sergiampietri, G. Sirri, J. S. Smedley, A. K. Soha, M. Spanu, L. Stanco, J. Stewart, N. B. Suarez, C. Sutera, H. A. Tanaka, M. Tenti, K. Terao, F. Terranova, V. Togo, D. Torretta, M. Torti, F. Tortorici, N. Tosi, Y. T. Tsai, S. Tufanli, M. Turcato, T. Usher, F. Varanini, S. Ventura, F. Vercellati, M. Vicenzi, C. Vignoli, B. Viren, D. Warner, Z. Williams, R. J. Wilson, P. Wilson, J. Wolfs, T. Wongjirad, A. Wood, E. Worcester, M. Worcester, M. Wospakrik, H. Yu, J. Yu, A. Zani, P. G. Zatti, J. Zennamo, J. C. Zettlemoyer, C. Zhang, S. Zucchelli, M. Zuckerbrot

Research output: Contribution to journalArticlepeer-review

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Abstract

The ICARUS collaboration employed the 760-ton T600 detector in a successful 3-year physics run at the underground LNGS laboratory, performing a sensitive search for LSND-like anomalous νe appearance in the CERN Neutrino to Gran Sasso beam, which contributed to the constraints on the allowed neutrino oscillation parameters to a narrow region around 1 eV 2 . After a significant overhaul at CERN, the T600 detector has been installed at Fermilab. In 2020 the cryogenic commissioning began with detector cool down, liquid argon filling and recirculation. ICARUS then started its operations collecting the first neutrino events from the booster neutrino beam (BNB) and the Neutrinos at the Main Injector (NuMI) beam off-axis, which were used to test the ICARUS event selection, reconstruction and analysis algorithms. ICARUS successfully completed its commissioning phase in June 2022. The first goal of the ICARUS data taking will be a study to either confirm or refute the claim by Neutrino-4 short-baseline reactor experiment. ICARUS will also perform measurement of neutrino cross sections with the NuMI beam and several Beyond Standard Model searches. After the first year of operations, ICARUS will search for evidence of sterile neutrinos jointly with the Short-Baseline Near Detector, within the Short-Baseline Neutrino program. In this paper, the main activities carried out during the overhauling and installation phases are highlighted. Preliminary technical results from the ICARUS commissioning data with the BNB and NuMI beams are presented both in terms of performance of all ICARUS subsystems and of capability to select and reconstruct neutrino events.

Original languageEnglish
Article number467
JournalEuropean Physical Journal C
Volume83
Issue number6
DOIs
StatePublished - Jun 2023
Externally publishedYes

Funding

This document was prepared by the ICARUS collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by the US Department of Energy, INFN, EU Horizon 2020 Research and Innovation Program under the Marie Sklodowska-Curie Grant Agreement Nos. 734303, 822185, 858199, and 101003460 and Horizon Europe Program research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 101081478. Part of the work resulted from the implementation of the research Project No. 2019/33/N/ST2/02874 funded by the National Science Centre, Poland. The ICARUS Collaboration would like to thank the MINOS Collaboration for having provided the Side CRT panels as well as Double Chooz (University of Chicago) for the Bottom CRT panels. We also acknowledge the contribution of many SBND colleagues, in particular for the development of a number of simulation, reconstruction and analysis tools which are shared within the SBN program. Finally, our experiment could not have been carried out without the major support of CERN in the detector overhauling within the Neutrino Platform framework and of Fermilab in the detector installation and commissioning, and in providing the BNB and NuMI beams.

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