Measurement of the muon flux at the SND@LHC experiment

Albanese, R.; Alexandrov, A.; Alicante, F.; Anokhina, A.; Asada, T.; Battilana, C.; Bay, A.; Betancourt, C.; Bick, D.; Biswas, R.; Castro, A.; 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.-Y.; 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.; Donà, R.; Durhan, O.; Fabbri, F.; Fedotovs, F.; Ferrillo, M.; Ferro-Luzzi, M.; Fini, R.A.; Fiorillo, A.; Fresa, R.; Funk, W.; Walls, F.; Golovatiuk, A.; Golutvin, A.; Graverini, E.; Guler, ALİ; Guliaeva, V.; Haefeli, G.J.; Hagner, C.; Herrera, J.; 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.; Lauria, A.; Lee, K.Y.; Lee, K.S.; Meo, S.; 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.; 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.; Spurio, M.; Starkov, N.; Timiryasov, I.; Tioukov, V.; Tramontano, F.; Trippl, C.; Ursov, E.; Ustyuzhanin, A.; Vankova-Kirilova, G.; Verguilov, V.; Leonardo, N.; Vilela, C.; Visone, C.; Wanke, R.; Yaman, E.; Yazici, C.; Yoon, C.S.; Zaffaroni, E.; Saa, J.

doi:10.1140/epjc/s10052-023-12380-3

Measurement of the muon flux at the SND@LHC experiment

Atıf İçin Kopyala

Albanese R., Alexandrov A., Alicante F., Anokhina A., Asada T., Battilana C., ...Daha Fazla

European Physical Journal C, cilt.84, sa.1, 2024 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 84 Sayı: 1
Basım Tarihi: 2024
Doi Numarası: 10.1140/epjc/s10052-023-12380-3
Dergi Adı: European Physical Journal C
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, Aerospace Database, Chemical Abstracts Core, Communication Abstracts, INSPEC, zbMATH, Directory of Open Access Journals
Orta Doğu Teknik Üniversitesi Adresli: Evet

Özet

The Scattering and Neutrino Detector at the LHC (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 480 m 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 × 18 cm 2 area in the emulsion is: 1.5±0.1(stat)×104fb/cm2. The muon flux per integrated luminosity through a 31 × 31 cm 2 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 × 52 cm 2 area in the centre of the downstream muon system is: 2.35±0.01(stat)±0.10(sys)×104fb/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.