- Open Access
Topological production of charmonia with event-shape engineering in collisions at using pythia8
Phys. Rev. D 113, 054032 – Published 23 March, 2026
DOI: https://doi.org/10.1103/dtgx-hrbp
Abstract
The production of heavy quarks (charm and beauty) in high-energy hadronic and nuclear collisions provides an excellent testing ground for the theory of strong interactions and validates models based on quantum chromodynamics (QCD). In this work, prompt and nonprompt production of in collisions at are studied as a function of the transverse spherocity using pythia8. is reconstructed via its electromagnetic decay to dielectrons and dimuons, in mid- and forward rapidity, respectively. Transverse spherocity, an event-shape observable, is used to distinguish hard-QCD events from the softer, isotropic ones. In pythia8, the production of can be influenced by the average number of multiple parton interactions (), owing to the underlying events, which have a dominant contribution to particle production at lower transverse momentum. Since transverse spherocity is correlated to , this can serve as an experimentally accessible tool for event selection to study the underlying QCD processes influencing the prompt and nonprompt production. This study reveals the correlation between heavy-flavor production dynamics and topological event selection in collisions using pythia8, whose relevance awaits experimental validation.
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References (55)
- S. A. Bass, M. Gyulassy, H. Stoecker, and W. Greiner, J. Phys. G 25, R1 (1999).
- J. C. Collins, D. E. Soper, and G. F. Sterman, Adv. Ser. Dir. High Energy Phys. 5, 1 (1989).
- N. Brambilla, S. Eidelman, B. K. Heltsley et al., Eur. Phys. J. C 71, 1534 (2011).
- J. Adam et al. (ALICE Collaboration), J. High Energy Phys. 07 (2015) 051.
- S. Acharya et al. (ALICE Collaboration), Eur. Phys. J. C 78, 466 (2018).
- A. M. Sirunyan et al. (CMS Collaboration), Eur. Phys. J. C 77, 269 (2017).
- D. Acosta et al. (CDF Collaboration), Phys. Rev. D 71, 032001 (2005).
- S. Prasad, N. Mallick, and R. Sahoo, Phys. Rev. D 109, 014005 (2024).
- B. Abelev et al. (ALICE Collaboration), Phys. Lett. B 712, 165 (2012).
- S. Acharya et al. (ALICE Collaboration), Phys. Lett. B 810, 135758 (2020).
- S. Acharya et al. (ALICE Collaboration), J. High Energy Phys. 06 (2022) 015.
- S. Acharya et al. (ALICE Collaboration), J. High Energy Phys. 07 (2025) 238.
- S. G. Weber, A. Dubla, A. Andronic, and A. Morsch, Eur. Phys. J. C 79, 36 (2019).
- S. Prasad, S. Tripathy, B. Sahoo, and R. Sahoo, arXiv:2506.03782.
- S. Prasad, B. Sahoo, S. Tripathy, N. Mallick, and R. Sahoo, Phys. Rev. C 111, 044902 (2025).
- K. Goswami, S. Prasad, N. Mallick, R. Sahoo, and G. B. Mohanty, Phys. Rev. D 110, 034017 (2024).
- S. Acharya et al. (ALICE Collaboration), J. High Energy Phys. 05 (2024) 184.
- J. Adam et al. (ALICE Collaboration), J. High Energy Phys. 09 (2015) 148.
- D. Thakur, S. De, R. Sahoo, and S. Dansana, Phys. Rev. D 97, 094002 (2018).
- S. Deb, D. Thakur, S. De, and R. Sahoo, Eur. Phys. J. A 56, 134 (2020).
- S. Acharya et al. (ALICE Collaboration), Eur. Phys. J. C 81, 630 (2021).
- S. Acharya et al. (ALICE Collaboration), Eur. Phys. J. C 79, 857 (2019).
- S. Prasad, N. Mallick, D. Behera, R. Sahoo, and S. Tripathy, Sci. Rep. 12, 3917 (2022).
- S. Prasad, N. Mallick, S. Tripathy, and R. Sahoo, Phys. Rev. D 107, 074011 (2023).
- S. Tripathy, S. Prasad, and R. Sahoo, Phys. Rev. D 112, 114012 (2025).
- S. Prasad, A. M. Kavumpadikkal Radhakrishnan, R. Sahoo, and N. Mallick, Phys. Lett. B 868, 139753 (2025).
- N. Mallick, R. Sahoo, S. Tripathy, and A. Ortiz, J. Phys. G 48, 045104 (2021).
- N. Mallick, S. Tripathy, and R. Sahoo, Eur. Phys. J. C 82, 524 (2022).
- A. Menon Kavumpadikkal Radhakrishnan, S. Prasad, S. Tripathy, N. Mallick, and R. Sahoo, Eur. Phys. J. Plus 140, 110 (2025).
- Available online at https://pythia.org/.
- C. Bierlich, S. Chakraborty, N. Desai, L. Gellersen, I. Helenius et al., SciPost Phys. Codebases 2022, 8 (2022).
- T. Sjostrand and P. Z. Skands, Eur. Phys. J. C 39, 129 (2005).
- R. Corke and T. Sjostrand, J. High Energy Phys. 03 (2011) 032.
- T. Sjostrand and M. van Zijl, Phys. Rev. D 36, 2019 (1987).
- T. Sjostrand and P. Z. Skands, J. High Energy Phys. 03 (2004) 053.
- B. Andersson, G. Gustafson, G. Ingelman, and T. Sjostrand, Phys. Rep. 97, 31 (1983).
- T. Sjostrand, Nucl. Phys. B248, 469 (1984).
- M. M. Aggarwal et al. (STAR Collaboration), Phys. Rev. C 84, 034909 (2011).
- J. R. Christiansen and P. Z. Skands, J. High Energy Phys. 08 (2015) 003.
- P. Schwaller, D. Stolarski, and A. Weiler, J. High Energy Phys. 05 (2015) 059.
- E. Norrbin and T. Sjostrand, Phys. Lett. B 442, 407 (1998).
- A. Banfi, G. P. Salam, and G. Zanderighi, J. High Energy Phys. 06 (2010) 038.
- B. Abelev et al. (ALICE Collaboration), J. High Energy Phys. 11 (2012) 065.
- S. Acharya et al. (ALICE Collaboration), J. High Energy Phys. 03 (2022) 190.
- M. Aaboud et al. (ATLAS Collaboration), Eur. Phys. J. C 78, 762 (2018).
- V. Khachatryan et al. (CMS Collaboration), Eur. Phys. J. C 71, 1575 (2011).
- S. Acharya et al. (ALICE Collaboration), Eur. Phys. J. C 80, 167 (2020).
- S. Acharya et al. (ALICE Collaboration), Phys. Lett. B 843, 137649 (2023).
- S. Acharya et al. (ALICE Collaboration), J. High Energy Phys. 05 (2024) 229.
- S. Acharya et al. (ALICE Collaboration), Phys. Rev. C 101, 044907 (2020).
- A. Ortiz, A. Paz, J. D. Romo, S. Tripathy, E. A. Zepeda, and I. Bautista, Phys. Rev. D 102, 076014 (2020).
- A. M. Sirunyan et al. (CMS Collaboration), J. High Energy Phys. 11 (2020) 001.
- S. Acharya et al. (ALICE Collaboration), Eur. Phys. J. C 81, 1121 (2021).
- R. Aaij et al. (LHCb Collaboration), J. High Energy Phys. 10 (2015) 172.
- S. Acharya et al. (ALICE Collaboration), J. High Energy Phys. 10 (2023) 092.