What can we learn from the directed flow in heavy-ion collisions at BES RHIC energies?
YB Ivanov, AA Soldatov - The European Physical Journal A, 2016 - Springer
YB Ivanov, AA Soldatov
The European Physical Journal A, 2016•SpringerAnalysis of directed flow (v_1) of protons, antiprotons and pions in heavy-ion collisions is
performed in the range of collision energies s_NN=2.7--39 GeV. Simulations have been
done within a three-fluid model employing a purely hadronic equation of state (EoS) and two
versions of the EoS with deconfinement transitions: a first-order phase transition and a
smooth crossover transition. The crossover EoS is unambiguously preferable for the
description of the most part of experimental data in this energy range. The directed flow …
performed in the range of collision energies s_NN=2.7--39 GeV. Simulations have been
done within a three-fluid model employing a purely hadronic equation of state (EoS) and two
versions of the EoS with deconfinement transitions: a first-order phase transition and a
smooth crossover transition. The crossover EoS is unambiguously preferable for the
description of the most part of experimental data in this energy range. The directed flow …
Abstract
Analysis of directed flow () of protons, antiprotons and pions in heavy-ion collisions is performed in the range of collision energies GeV. Simulations have been done within a three-fluid model employing a purely hadronic equation of state (EoS) and two versions of the EoS with deconfinement transitions: a first-order phase transition and a smooth crossover transition. The crossover EoS is unambiguously preferable for the description of the most part of experimental data in this energy range. The directed flow indicates that the crossover deconfinement transition takes place in semicentral Au+Au collisions in a wide range of collision energies GeV. The obtained results suggest that the deconfinement EoS’s in the quark-gluon sector should be stiffer at high baryon densities than those used in the calculation. The latter finding is in agreement with that discussed in astrophysics.
Springer