Particle ratios within EPOS, UrQMD and thermal models at AGS, SPS and RHIC energies

Author:

Hanafy Mahmoud12ORCID,Tawfik Abdel Nasser34,Maher Muhammad25,Scheinast Werner6

Affiliation:

1. Faculty of Science, Physics Department, Benha University 13518, Benha, Egypt

2. World Laboratory for Cosmology and Particle Physics (WLCAPP), 11571 Cairo, Egypt

3. Egyptian Center for Theoretical Physics (ECTP), Nile University, Juhayna Square off 26th-July-Corridor 12588 Giza, Egypt

4. Institute for Theoretical Physics, Goethe University, Max-von-Laue-Str. 1, D-60438 Frankfurt am Main, Germany

5. Faculty of Science, Physics Department, Helwan University, Ain Helwan, P. O. 11795, 11795 Cairo, Egypt

6. Joint Institute for Nuclear Research, Veksler and Baldin Laboratory of High Energy Physics, Moscow Region 141980 Dubna, Russia

Abstract

The particle ratios [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text] measured at AGS, SPS and RHIC energies are compared with large statistical ensembles of 100,000 events deduced from the CRMC EPOS [Formula: see text] and the Ultra-relativistic Quantum Molecular Dynamics (UrQMD) hybrid model. In the UrQMD hybrid model two types of phase transitions are taken into account. All these data are then confronted with the ideal Hadron Resonance Gas Model. The two types of phase transitions are apparently indistinguishable. Apart from [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text], the UrQMD hybrid model agrees well with the CRMC EPOS [Formula: see text]. We also conclude that the CRMC EPOS [Formula: see text] seems to largely underestimate [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text].

Publisher

World Scientific Pub Co Pte Ltd

Subject

General Physics and Astronomy,Nuclear and High Energy Physics

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