- Open Access
Multiplicities of positive and negative pions, kaons, and unidentified hadrons from deep-inelastic scattering of muons off a liquid hydrogen target
Phys. Rev. D 112, 012002 – Published 2 July, 2025
DOI: https://doi.org/10.1103/q4rb-bhcg
Abstract
The multiplicities of positive and negative pions, kaons, and unidentified hadrons produced in deep-inelastic scattering are measured in bins of the Bjorken scaling variable , the relative virtual-photon energy , and the fraction of the virtual-photon energy transferred to the final-state hadron . Data were obtained by the COMPASS Collaboration using a 160 GeV muon beam of both electric charges and a liquid hydrogen target. These measurements cover the kinematic domain with photon virtuality , , , and , in accordance with the kinematic domain used in earlier published COMPASS multiplicity measurements with an isoscalar target. The calculation of radiative corrections was improved by using the Monte Carlo generator djangoh, which results in up to 12% larger corrections in the low- region.
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References (32)
- R. Barate et al. (ALEPH Collaboration), Phys. Rep. 294, 1 (1998); P. Abreu et al. (DELPHI Collaboration), Eur. Phys. J. C 5, 585 (1998); R. Akers et al. (OPAL Collaboration), Z. Phys. C 63, 181 (1994).
- K. Abe et al. (SLD Collaboration), Phys. Rev. D 69, 072003 (2004); J. P. Lees et al. (BABAR Collaboration), 88, 032011 (2013).
- M. Leitgab et al. (Belle Collaboration), Phys. Rev. Lett. 111, 062002 (2013).
- A. Airapetian et al. (HERMES Collaboration), Phys. Rev. D 87, 074029 (2013).
- J. Ashman et al. (EMC Collaboration), Z. Phys. C 52, 361 (1991).
- C. Adolph et al. (COMPASS Collaboration), Phys. Lett. B 764, 1 (2017).
- C. Adolph et al. (COMPASS Collaboration), Phys. Lett. B 767, 133 (2017).
- S. S. Adler et al. (PHENIX Collaboration), Phys. Rev. Lett. 91, 241803 (2003); J. Adams et al. (STAR Collaboration), 97, 152302 (2006); I. Arsene et al. (BRAHMS Collaboration), 98, 252001 (2007); B. I. Abelev et al. (STAR Collaboration), Phys. Rev. C 75, 064901 (2007).
- D. de Florian, R. Sassot, and M. Stratmann, Phys. Rev. D 75, 114010 (2007).
- M. Hirai, S. Kumano, T.-H. Nagai, and K. Sudoh, Phys. Rev. D 75, 094009 (2007).
- E. Leader, A. V. Sidorov, and D. Stamenov, Phys. Rev. D 93, 074026 (2016).
- D. de Florian, R. Sassot, M. Epele, R. J. Hernández-Pinto, and M. Stratmann, Phys. Rev. D 91, 014035 (2015).
- D. de Florian, M. Epele, R. J. Hernández-Pinto, R. Sassot, and M. Stratmann, Phys. Rev. D 95, 094019 (2017).
- V. Bertone, S. Carrazza, N. P. Hartland, E. R. Nocera, and J. Rojo, Eur. Phys. J. C 77, 516 (2017).
- E. Moffat, W. Melnitchouk, T. C. Rogers, and N. Sato, Phys. Rev. D 104, 016015 (2021).
- I. Borsa, R. Sassot, D. de Florian, M. Stratmann, and W. Vogelsang, Phys. Rev. Lett. 129, 012002 (2022).
- D. de Florian, M. Stratmann, and W. Vogelsang, Phys. Rev. D 57, 5811 (1998).
- P. Abbon et al., Nucl. Instrum. Methods Phys. Res., Sect. A 631, 26 (2011).
- R. Akhunzyanov et al. (COMPASS Collaboration), Phys. Lett. B 786, 390 (2018).
- M. G. Alexeev et al. (COMPASS Collaboration), Phys. Lett. B 807, 135600 (2020).
Note that the number of kaons quoted in Ref. [7] is incorrect; the value after all selections was about .
- G. Ingelman, A. Edin, and J. Rathsman, Comput. Phys. Commun. 101, 108 (1997).
- T. Sjöstrand, Reports No. LU-TP-95-20, No. CERN-TH-7112-93-REV, arXiv:hep-ph/9508391.
- C. Adolph et al. (COMPASS Collaboration), Phys. Lett. B 718, 922 (2013).
- S. Agostinelli et al. (GEANT4 Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 506, 250 (2003).
- A. Sandacz and P. Sznajder, arXiv:1207.0333.
- S. V. Goloskokov and P. Kroll, Eur. Phys. J. C 53, 367 (2008).
- A. A. Akhundov, D. Bardin, L. Kalinovskaya, and T. Riemann, Fortschr. Phys. 44, 373 (1996).
- E. C. Aschenauer, T. Burton, M. Stratmann, T. Martini, and H. Spiesberger, Phys. Rev. D 88, 114025 (2013).
- The Durham hepdata project, http://durpdg.dur.ac.uk/.
It is worth noting that the unusual shape of the HERMES data as a function of can be represented as a straight line as a function of . The observed slope can be influenced by radiative corrections. Since the values of RC in Ref. [4] are not provided, we cannot compare them to those we can currently obtain using djangoh-mc for HERMES kinematics.
- https://www.universe-cluster.de/.