https://doi.org/10.1140/epjp/s13360-026-07443-9
Regular Article
Modelling identified hadrons in
at SPS energies with Pythia 8 Angantyr: subcollision acceptance and string-end topology
Physics Department, Faculty of Science, Umm Al-Qura University, PO Box 715, 21421, Makkah, Saudi Arabia
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Received:
20
October
2025
Accepted:
16
February
2026
Published online:
25
February
2026
Abstract
We study identified hadron production (p,
,
) in inelastic proton–proton collisions at
, 31, 40, 80, and
using Pythia 8.315 with Angantyr, confronted with NA61/SHINE rapidity spectra. Four ingredients are varied in a controlled way: (i) the accepted mix of NN subcollisions via two post-classification settings, DS4-lite
and DS4-strong (0.6, 0.4, 0.4, 0.4); (ii) the string-end hadron formation pattern (diquark vs. popcorn, allowing one intermediate meson); (iii) the level of soft activity through a gentle low-energy MPI retune with elastic-like remnants filtered; and (iv) hadronic rescattering (HR).
At 20–
, DS4-lite suppresses the midrapidity proton excess and restores the observed “U” shape, with HR providing a modest additional deepening; DS4-strong improves the central
and
normalizations. At 80 and
, the popcorn option smooths unphysical forward spikes for protons, enhances forward
and
, and slightly moderates
, while the DS4 strength chiefly controls midrapidity levels. A persistent feature remains at intermediate energies: the large-y
tail (
) is underestimated at 31 and
, pointing to missing forward-baryon/associated-strangeness dynamics rather than to overall soft activity or rescattering effects.
With these minimal, transparent adjustments—DS acceptance plus a controlled string-end topology—the simulations closely follow NA61/SHINE across species and energies in the SPS window.
This study paves the way to a consistent, data-anchored pp baseline for Angantyr extrapolations to p A and A+A, while quantitatively constraining the midrapidity balance of soft activity and baryon stopping across SPS energies.
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© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2026
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.

