Constraining relativistic models through heavy ion collisions

Details Constraining relativistic models through heavy ion collisions Constraining relativistic models through heavy ion collisions

2007-08-24

arxiv.org/abs/0708.3380v1

Phys.Rev.C76:064902,2007

Physics

High Energy Physics

High Energy Physics - Phenomenology

9 pages, 1 figure, 3 tables

Scientific paper

10.1103/PhysRevC.76.064902

Relativistic models can be successfully applied to the description of compact star properties in nuclear astrophysics as well as to nuclear matter and finite nuclei properties, these studies taking place at low and moderate temperatures. Nevertheless, all results are model dependent and so far it is unclear whether some of them should be discarded. Moreover, in the regime of hot hadronic matter very few calculations exist using these relativistic models, in particular when applied to particle yields in heavy ion collisions. In the present work we comment on the known constraints that can help the selection of adequate models in this regime and investigate the main differences that arise when the particle production during a Au+Au collision at RHIC is calculated with different models.

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