European Physical Journal C: Particles and Fields (Jan 2024)

Measurement of the muon flux at the SND@LHC experiment

  • R. Albanese,
  • A. Alexandrov,
  • F. Alicante,
  • A. Anokhina,
  • T. Asada,
  • C. Battilana,
  • A. Bay,
  • C. Betancourt,
  • D. Bick,
  • R. Biswas,
  • A. Blanco Castro,
  • V. Boccia,
  • M. Bogomilov,
  • D. Bonacorsi,
  • W. M. Bonivento,
  • P. Bordalo,
  • A. Boyarsky,
  • S. Buontempo,
  • M. Campanelli,
  • T. Camporesi,
  • V. Canale,
  • A. Castro,
  • D. Centanni,
  • F. Cerutti,
  • M. Chernyavskiy,
  • K. -Y. Choi,
  • S. Cholak,
  • F. Cindolo,
  • M. Climescu,
  • A. P. Conaboy,
  • G. M. Dallavalle,
  • D. Davino,
  • P. T. de Bryas,
  • G. De Lellis,
  • M. De Magistris,
  • A. De Roeck,
  • A. De Rújula,
  • M. De Serio,
  • D. De Simone,
  • A. Di Crescenzo,
  • R. Donà,
  • O. Durhan,
  • F. Fabbri,
  • F. Fedotovs,
  • M. Ferrillo,
  • M. Ferro-Luzzi,
  • R. A. Fini,
  • A. Fiorillo,
  • R. Fresa,
  • W. Funk,
  • F. M. Garay Walls,
  • A. Golovatiuk,
  • A. Golutvin,
  • E. Graverini,
  • A. M. Guler,
  • V. Guliaeva,
  • G. J. Haefeli,
  • C. Hagner,
  • J. C. Helo Herrera,
  • E. van Herwijnen,
  • P. Iengo,
  • S. Ilieva,
  • A. Infantino,
  • A. Iuliano,
  • R. Jacobsson,
  • C. Kamiscioglu,
  • A. M. Kauniskangas,
  • E. Khalikov,
  • S. H. Kim,
  • Y. G. Kim,
  • G. Klioutchnikov,
  • M. Komatsu,
  • N. Konovalova,
  • S. Kuleshov,
  • H. M. Lacker,
  • O. Lantwin,
  • F. Lasagni Manghi,
  • A. Lauria,
  • K. Y. Lee,
  • K. S. Lee,
  • S. Lo Meo,
  • V. P. Loschiavo,
  • S. Marcellini,
  • A. Margiotta,
  • A. Mascellani,
  • A. Miano,
  • A. Mikulenko,
  • M. C. Montesi,
  • F. L. Navarria,
  • S. Ogawa,
  • N. Okateva,
  • M. Ovchynnikov,
  • G. Paggi,
  • B. D. Park,
  • A. Pastore,
  • A. Perrotta,
  • D. Podgrudkov,
  • N. Polukhina,
  • A. Prota,
  • A. Quercia,
  • S. Ramos,
  • A. Reghunath,
  • T. Roganova,
  • F. Ronchetti,
  • T. Rovelli,
  • O. Ruchayskiy,
  • T. Ruf,
  • M. Sabate Gilarte,
  • Z. Sadykov,
  • M. Samoilov,
  • V. Scalera,
  • W. Schmidt-Parzefall,
  • O. Schneider,
  • G. Sekhniaidze,
  • N. Serra,
  • M. Shaposhnikov,
  • V. Shevchenko,
  • T. Shchedrina,
  • L. Shchutska,
  • H. Shibuya,
  • S. Simone,
  • G. P. Siroli,
  • G. Sirri,
  • G. Soares,
  • J. Y. Sohn,
  • O. J. Soto Sandoval,
  • M. Spurio,
  • N. Starkov,
  • I. Timiryasov,
  • V. Tioukov,
  • F. Tramontano,
  • C. Trippl,
  • E. Ursov,
  • A. Ustyuzhanin,
  • G. Vankova-Kirilova,
  • V. Verguilov,
  • N. Viegas Guerreiro Leonardo,
  • C. Vilela,
  • C. Visone,
  • R. Wanke,
  • E. Yaman,
  • C. Yazici,
  • C. S. Yoon,
  • E. Zaffaroni,
  • J. Zamora Saa

DOI
https://doi.org/10.1140/epjc/s10052-023-12380-3
Journal volume & issue
Vol. 84, no. 1
pp. 1 – 10

Abstract

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Abstract 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 $$7.2<\eta <8.4$$ 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 $$\times $$ × 18 cm $$^{2}$$ 2 area in the emulsion is: $$\begin{aligned} 1.5 \pm 0.1(\text {stat}) \times 10^4\,\text {fb/cm}^{2}. \end{aligned}$$ 1.5 ± 0.1 ( stat ) × 10 4 fb/cm 2 . The muon flux per integrated luminosity through a 31 $$\times $$ × 31 cm $$^{2}$$ 2 area in the centre of the SciFi is: $$\begin{aligned} 2.06\pm 0.01(\text {stat})\pm 0.12(\text {sys}) \times 10^{4} \text {fb/cm}^{2} \end{aligned}$$ 2.06 ± 0.01 ( stat ) ± 0.12 ( sys ) × 10 4 fb/cm 2 The muon flux per integrated luminosity through a 52 $$\times $$ × 52 cm $$^{2}$$ 2 area in the centre of the downstream muon system is: $$\begin{aligned} 2.35\pm 0.01(\text {stat})\pm 0.10(\text {sys}) \times 10^{4}\,\text {fb/cm}^{2} \end{aligned}$$ 2.35 ± 0.01 ( stat ) ± 0.10 ( sys ) × 10 4 fb/cm 2 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.