Measurement of the muon flux at the SND@LHC experiment

TheScatteringandNeutrinoDetectorattheLHC (SND@LHC) started taking data at the beginning of Run 3 of the LHC. The experiment is designed to perform measurements with neutrinos produced in proton-proton collisions at the LHC in an energy range between 100 GeV and 1 TeV. It covers a previously unexplor...

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Autores: Albanese, R.; Alexandrov, A.; Alicante, F.; Anokhina, A.; Asada, T.; Battilana, C.; Bay, A.; Betancourt, C.; Bick, D.; Garay Walls, Francisca; Castro, A. B.; Boccia, V.; Bogomilov, M.; Bonacorsi, D.; Bonivento, W. M.; Bordalo, P.; Boyarsky, A.; Buontempo, S.; Campanelli, M.; Camporesi, T.; Canale, V.; Castro, A.; Centanni, D.; Cerutti, F.; Chernyavskiy, M.; Choi, K. -.; Cholak, S.; Cindolo, F.; Climescu, M.; Conaboy, A. P.; Dallavalle, G. M.; Davino, D.; de Bryas, P. T.; De Lellis, G.; De Magistris, M.; De Roeck, A.; De Rújula, A.; De Serio, M.; De Simone, D.; Crescenzo, A. D.; Donà, R.; Durhan, O.; Fabbri, F.; Fedotovs, F.; Ferrillo, M.; Ferro-Luzzi, M.; Fini, R. A.; Fiorillo, A.; Fresa, R.; Funk, W.; Biswas, R.; Golovatiuk, A.; Golutvin, A.; Graverini, E.; Guler, A. M.; Guliaeva, V.; Haefeli, G. J.; Hagner, C.; Herrera, J. C. H.; van Herwijnen, E.; Iengo, P.; Ilieva, S.; Infantino, A.; Iuliano, A.; Jacobsson, R.; Kamiscioglu, C.; Kauniskangas, A. M.; Khalikov, E.; Kim, S. H.; Kim, Y. G.; Klioutchnikov, G.; Komatsu, M.; Konovalova, N.; Kuleshov, S.; Lacker, H. M.; Lantwin, O.; Manghi, F. L.; Lauria, A.; Lee, K. Y.; Lee, K. S.; Meo, S. L.; Loschiavo, V. P.; Marcellini, S.; Margiotta, A.; Mascellani, A.; Miano, A.; Mikulenko, A.; Montesi, M. C.; Navarria, F. L.; Ogawa, S.; Okateva, N.; Ovchynnikov, M.; Paggi, G.; Park, B. D.; Pastore, A.; Perrotta, A.; Podgrudkov, D.; Polukhina, N.; Prota, A.; Quercia, A.; Ramos, S.; Reghunath, A.; Roganova, T.; Ronchetti, F.; Rovelli, T.; Ruchayskiy, O.; Ruf, T.; Gilarte, M. S.; Sadykov, Z.; Samoilov, M.; Scalera, V.; Schmidt-Parzefall, W.; Schneider, O.; Sekhniaidze, G.; Serra, N.; Shaposhnikov, M.; Shevchenko, V.; Shchedrina, T.; Shchutska, L.; Shibuya, H.; Simone, S.; Siroli, G. P.; Sirri, G.; Soares, G.; Sohn, J. Y.; Sandoval, O. J. S.; Spurio, M.; Starkov, N.; Timiryasov, I.; Tioukov, V.; Tramontano, F.; Trippl, C.; Ursov, E.; Ustyuzhanin, A.; Vankova-Kirilova, G.; Verguilov, V.; Leonardo, N. V. G.; Vilela, C.; Visone, C.; Wanke, R.; Yaman, E.; Yazici, C.; Yoon, C. S.; Zaffaroni, E.; Saa, J. Z.
Tipo de documento: Artículo
Estado:Published version
Fecha de publicación:2024
País:Chile
Institución:Pontificia Universidad Católica de Chile
Repositorio:Pontificia Universidad Católica de Chile
OAI Identifier:oai:repositorio.uc.cl:11534/84650
Acceso en línea:https://doi.org/10.1140/epjc/s10052-023-12380-3
https://repositorio.uc.cl/handle/11534/84650
Nivel de acceso:Acceso abierto
Palabra clave:510
Matemática física y química
Sumario:TheScatteringandNeutrinoDetectorattheLHC (SND@LHC) started taking data at the beginning of Run 3 of the LHC. The experiment is designed to perform measurements with neutrinos produced in proton-proton collisions at the LHC in an energy range between 100 GeV and 1 TeV. It covers a previously unexplored pseudo-rapidity range of 7.2 <η<8.4. The detector is located 480m downstream of the ATLAS interaction point in the TI18 tunnel. It comprises a veto system, a target consisting of tungsten plates interleaved with nuclear emulsion and scintillating fiber (SciFi) trackers, followed by a muon detector (UpStream, US and DownStream, DS). In this article we report the measurement of the muon flux in three subdetectors: the emulsion, the SciFi trackers and the DownStream Muon detector. The muon flux per integrated luminosity through an 18×18cm2 area in the emulsion is: 1.5 ±0.1(stat) × 104 fb/cm2. The muon flux per integrated luminosity through a 31×31cm2 area in the centre of the SciFi is: 2.06 ±0.01(stat) ± 0.12(sys) × 104fb/cm2 The muon flux per integrated luminosity through a 52×52cm2 area in the centre of the downstream muon system is: 2.35 ±0.01(stat) ± 0.10(sys) × 104 fb/cm2 The total relative uncertainty of the measurements by the electronic detectors is 6% for the SciFi and 4% for the DS measurement. The Monte Carlo simulation prediction of these fluxes is 20–25% lower than the measured values.

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