Directed Flow in Heavy-Ion Collisions and Its Implications for Astrophysics

Directed Flow in Heavy-Ion Collisions and Its Implications for Astrophysics

Analysis of directed flow ( v 1 ) of protons, antiprotons and pions in heavy-ion collisions is performed in the range of collision energies s N N = 2.7–39 GeV. Simulations have been done within a three-fluid model employing a purely hadronic equation of state (EoS) and two versions...

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Bibliographic Details
Main Author:	Yuri B. Ivanov
Format:	Article
Language:	English
Published:	MDPI AG 2017-11-01
Series:	Universe
Subjects:	heavy-ion collisions directed flow hydrodynamics deconfinement hybrid stars
Online Access:	https://www.mdpi.com/2218-1997/3/4/79

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