Effects of equation of state on hydrodynamic expansion, spectra, flow harmonics and two-pion interferometry

Author:

Dudek Danuce M.1,Qian Wei-Liang23,Wu Chen4,Socolowski Otávio5,Padula Sandra S.6,Krein Gastão6,Hama Yogiro7,Kodama Takeshi89

Affiliation:

1. Universidade Federal Fronteira Sul - Campus Realeza, 85770-000 Realeza, PR, Brazil

2. Escola de Engenharia de Lorena, Universidade de São Paulo, 12602-810 Lorena, SP, Brazil

3. Faculdade de Engenharia de Guaratinguetá, Universidade Estadual Paulista, 12516-410 Guaratinguetá, SP, Brazil

4. Shanghai Institute of Applied Physics, 201800, Shanghai, P. R. China

5. Instituto de Matemática Estatística e Física, Universidade Federal do Rio Grande, 96201-900 Rio Grande, RS, Brazil

6. Instituto de Física Teórica, Universidade Estadual Paulista, 01140-070 São Paulo, SP, Brazil

7. Instituto de Física, Universidade de São Paulo, 05389-970 São Paulo, SP, Brazil

8. Instituto de Física, Universidade Federal do Rio de Janeiro, 21941-972 Rio de Janeiro, RJ, Brazil

9. Instituto de Física, Universidade Federal Fluminense, 24210-346 Niterói, RJ, Brazil

Abstract

We perform an extensive study of the role played by the equation of state (EoS) in the hydrodynamic evolution of the matter produced in relativistic heavy ion collisions. By using the same initial conditions and freeze-out scenario, the effects of different equations of state are compared by calculating their respective hydrodynamical evolution, particle spectra, harmonic flow coefficients [Formula: see text], [Formula: see text] and [Formula: see text] and two-pion interferometry radius parameters. The equations of state investigated contain distinct features, such as the nature of the phase transition, as well as strangeness and baryon density contents, which are expected to lead to different hydrodynamic responses. The results of our calculations are compared to the data recorded at two RHIC energies, 130[Formula: see text]GeV and 200[Formula: see text]GeV. The three equations of state used in the calculations are found to describe the data reasonably well. Differences can be observed among the studied observables, but they are quite small. In particular, the collective flow parameters are found not to be sensitive to the choice of the EOS, whose implications are discussed.

Funder

Fundação de Amparo à Pesquisa do Estado de São Paulo

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior

Fundação de Amparo à Pesquisa do Estado de Minas Gerais

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Nuclear and High Energy Physics

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