https://doi.org/10.1140/epjp/s13360-025-06415-9
Regular Article
Hadron production models’ prediction for
distribution of charged hadrons in pp interactions at LHC energies
1
Department of Physics, Abdul Wali Khan University Mardan, 23200, Mardan, Pakistan
2
Department of Physics, College of Science, Princess Nourah bint Abdulrahman University, P.O. Box 84428, 11671, Riyadh, Saudi Arabia
3
Hubei Key Laboratory of Energy Storage and Power Battery, School of Optoelectronic Engineering, School of New Energy, Hubei University of Automotive Technology, 442002, Shiyan, China
4
Department of Mathematics, Physics and Statistics, Faculty of Natural Sciences, University of Guyana, 101110, Georgetown, Guyana
a
20220073@huat.edu.cn
b
ajaz@awkum.edu.pk
Received:
10
September
2024
Accepted:
9
May
2025
Published online:
12
June
2025
In this work, we present transverse momentum () spectra of identified charged hadrons and their ratios in proton–proton (pp) collisions at
TeV and 13 TeV using Monte Carlo models. The study employs Pythia8.3 (including variants Pythia8.3_CR and Pythia8.3_noCR) and EPOS (including EPOS
, EPOS
, and EPOSLHC). Results are measured at mid-rapidity (
) in the
range
GeV/c (CMS analysis) and
GeV/c (ALICE analysis). Comparisons with CMS and ALICE data reveal that EPOSLHC reproduces the spectra well for all identified charged hadrons and pion yields. However, it underestimates kaon yields and overestimates (anti-)proton yields. EPOS
agrees well with data for pions and (anti-)protons but overestimates kaons. Its agreement for all hadrons is limited to the high-
region. EPOS
fails to describe most hadrons, except for pions at high
. For Pythia8.3 variants: Pythia8.3_CR successfully predicts pion yields but underestimates (anti-)protons at high
. It improves predictions for kaons, (anti-)protons, and their ratios (
,
), though it fails for high-
pions. Pythia8.3_noCR matches pion yields but underestimates kaons and (anti-)protons, albeit with smaller discrepancies. The success of EPOSLHC is attributed to hadronic rescattering and flow effects. EPOS
benefits from hadronic cascades, core-corona effects, microcanonical decays, and rescattering, unlike EPOS
, which lacks these features. Pythia8.3_CR outperforms Pythia8.3_noCR due to color reconnection (CR) and multiple parton interaction (MPI) parameters.
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Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.