Strangeness Enhancement at LHC Energies using the thermal model and EPOSLHC event-generator
Mahmoud Hanafy, Omnia S.A. Qandil, and Asmaa G. Shalaby

TL;DR
This study investigates strangeness enhancement at LHC energies using the thermal HRG model and EPOS event generators, showing good agreement with experimental data and estimating freeze-out parameters across different collision systems.
Contribution
It introduces a combined analysis of strangeness production using HRG and EPOS models across a wide energy range, including LHC energies, which is novel.
Findings
Strangeness enhancement appears at higher energies.
Both HRG and EPOS models accurately describe particle ratios.
Freeze-out parameters are estimated for various collision systems.
Abstract
The strangeness enhancement signature of QGP formation at LHC energies is carefully tackled in the present study. Based on HRG, the particle ratios of mainly strange and multi-strange particles are studied at energies from lower 0.001 up to 13 TeV. The strangeness enhancement clearly appeared at more higher energies, and the ratios are confronted to the available experimental data. The particle ratios are also studied using the Cosmic Ray Monte Carlo (CRMC) interface model with its two different event generators namely; EPOS and EPOSlhc which show a good agreement with the model calculations at the whole range of the energy. We utilize to produce some ratios. EPOS is used to estimate particle ratios at lower energies from AGS up to the Relativistic Heavy Ion Collider (RHIC) while EPOSlhc is used at LHC energies. The production of kaons and lambda particles…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsHigh-Energy Particle Collisions Research · Particle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions
