Structure of the Medium Formed in Heavy Ion Collisions

Author:

Alvarado García J. R.1ORCID,Rosales Herrera D.1ORCID,Fernández Téllez A.1ORCID,Díaz Bogar234ORCID,Ramírez J. E.5ORCID

Affiliation:

1. Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Apartado Postal 165, 72000 Puebla, Mexico

2. Departamento de Matemáticas, Universidad Carlos III de Madrid, Avenida de la Universidad 30, 28911 Leganés, Spain

3. Grupo de Teorías de Campos y Física Estadística, Instituto Gregorio Millán (UC3M), Unidad Asociada al Instituto de Estructura de la Materia, CSIC, Serrano 123, 28006 Madrid, Spain

4. Instituto de Ciencias Matemáticas (ICMAT), CSIC-UAM-UC3M-UCM, C. Nicolás Cabrera 13–15, 28049 Madrid, Spain

5. Centro de Agroecología, Instituto de Ciencias, Benemérita Universidad Autónoma de Puebla, Apartado Postal 165, 72000 Puebla, Mexico

Abstract

We investigate the structure of the medium formed in heavy ion collisions using three different models: the Color String Percolation Model (CSPM), the Core–Shell-Color String Percolation Model (CSCSPM), and the Color Glass Condensate (CGC) framework. We analyze the radial distribution function of the transverse representation of color flux tubes in each model to determine the medium’s structure. Our results indicate that the CSPM behaves as an ideal gas, while the CSCSPM exhibits a structural phase transition from a gas-like to a liquid-like structure. Additionally, our analysis of the CGC framework suggests that it produces systems that behave like non-ideal gases for AuAu central collisions at RHIC energies and liquid-like structures for PbPb central collisions at LHC energies.

Publisher

MDPI AG

Subject

General Physics and Astronomy

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