Comparing EPOS-4, EPOS-LHC, and SMASH for identified-hadron observables in the NICA energy range
Murad Badshah, Haifa I. Alrebdi, Sana Raza Khan, Muhammad Ajaz

TL;DR
This study compares three simulation models—EPOS-LHC, EPOS-4, and SMASH—for their predictions of identified hadron production in Au+Au collisions at NICA energies, highlighting differences in strange hadron yields, spectra, and flow scaling.
Contribution
It provides a systematic comparison of these models' predictions for hadron observables at NICA energies, revealing model-dependent differences especially in strangeness production and flow.
Findings
EPOS-4 predicts highest strange hadron yields and hardest spectra.
EPOS-LHC shows better NCQ scaling of elliptic flow.
Model separation increases with collision energy from 6 to 8 GeV.
Abstract
We present a systematic simulation study of identified hadron production in minimum bias Au+Au collisions at sqrt(sNN) = 6, 7, and 8 GeV. The event samples were generated with three modern frameworks based on different microscopic pictures: EPOS-LHC, EPOS-4, and the purely hadronic transport model SMASH. We compare observables that probe baryon stopping, transverse dynamics, hadron formation, and strangeness production: rapidity densities dN/dy, transverse momentum spectra dN/dpT, two dimensional pT-y distributions, v2/nq versus pT/nq, and the yield ratios pi-/pi+, K-/K+, pbar/p, K+/pi+, K-/pi-, p/pi+, and Lambda/pi+. For charged and neutral pions, the three models give broadly similar yields and spectral shapes in both dN/dy and dN/dpT. At these energies, resonance decays and isospin constraints reduce the sensitivity to early stage dynamics. In contrast, strange mesons and baryons…
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Taxonomy
TopicsHigh-Energy Particle Collisions Research · Particle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions
