Directed Flow in Microscopic Models in Relativistic A+A Collisions

Evolution of directed flow of charged particles produced in relativistic heavy-ion collisions at energies 4 ≤ s ≤ 19.6 GeV is considered within two microscopic transport models, ultra-relativistic quantum molecular dynamics (UrQMD) and quark-gluon string model (QGSM). In both...

Full description

Bibliographic Details
Main Authors: Larissa Bravina, Yurii Kvasiuk, Sergey Sivoklokov, Oleksandr Vitiuk, Evgeny Zabrodin
Format: Article
Language:English
Published: MDPI AG 2019-03-01
Series:Universe
Subjects:
Online Access:http://www.mdpi.com/2218-1997/5/3/69
_version_ 1811262737652645888
author Larissa Bravina
Yurii Kvasiuk
Sergey Sivoklokov
Oleksandr Vitiuk
Evgeny Zabrodin
author_facet Larissa Bravina
Yurii Kvasiuk
Sergey Sivoklokov
Oleksandr Vitiuk
Evgeny Zabrodin
author_sort Larissa Bravina
collection DOAJ
description Evolution of directed flow of charged particles produced in relativistic heavy-ion collisions at energies 4 ≤ s ≤ 19.6 GeV is considered within two microscopic transport models, ultra-relativistic quantum molecular dynamics (UrQMD) and quark-gluon string model (QGSM). In both models, the directed flow of protons changes its sign at midrapidity from antiflow to normal flow with decreasing energy of collisions, whereas the flows of mesons and antiprotons remain antiflow-oriented. For lighter colliding systems, such as Cu+Cu or S+S, changing of the proton directed flow occurs at lower bombarding energies and for more central topologies compared to a heavy Au+Au system. The differences can be explained by dissimilar production zones of different hadrons and by the influence of spectators. Directed flows of most abundant hadronic species at midrapidity are found to be formed within t = 10–12 fm/c after the beginning of nuclear collision. The influence of hard and soft mean-field potentials on the directed flow is also studied.
first_indexed 2024-04-12T19:30:48Z
format Article
id doaj.art-9c56350bee7e44408768189e556fc228
institution Directory Open Access Journal
issn 2218-1997
language English
last_indexed 2024-04-12T19:30:48Z
publishDate 2019-03-01
publisher MDPI AG
record_format Article
series Universe
spelling doaj.art-9c56350bee7e44408768189e556fc2282022-12-22T03:19:20ZengMDPI AGUniverse2218-19972019-03-01536910.3390/universe5030069universe5030069Directed Flow in Microscopic Models in Relativistic A+A CollisionsLarissa Bravina0Yurii Kvasiuk1Sergey Sivoklokov2Oleksandr Vitiuk3Evgeny Zabrodin4Department of Physics, University of Oslo, PB 1048 Blindern, N-0316 Oslo, NorwayTaras Shevchenko National University of Kyiv, UA-01033 Kyiv, UkraineSkobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow RU-119991, RussiaTaras Shevchenko National University of Kyiv, UA-01033 Kyiv, UkraineDepartment of Physics, University of Oslo, PB 1048 Blindern, N-0316 Oslo, NorwayEvolution of directed flow of charged particles produced in relativistic heavy-ion collisions at energies 4 ≤ s ≤ 19.6 GeV is considered within two microscopic transport models, ultra-relativistic quantum molecular dynamics (UrQMD) and quark-gluon string model (QGSM). In both models, the directed flow of protons changes its sign at midrapidity from antiflow to normal flow with decreasing energy of collisions, whereas the flows of mesons and antiprotons remain antiflow-oriented. For lighter colliding systems, such as Cu+Cu or S+S, changing of the proton directed flow occurs at lower bombarding energies and for more central topologies compared to a heavy Au+Au system. The differences can be explained by dissimilar production zones of different hadrons and by the influence of spectators. Directed flows of most abundant hadronic species at midrapidity are found to be formed within t = 10–12 fm/c after the beginning of nuclear collision. The influence of hard and soft mean-field potentials on the directed flow is also studied.http://www.mdpi.com/2218-1997/5/3/69relativistic heavy-ion collisionsmicroscopic transport modelsdirected flowmean-field potentials
spellingShingle Larissa Bravina
Yurii Kvasiuk
Sergey Sivoklokov
Oleksandr Vitiuk
Evgeny Zabrodin
Directed Flow in Microscopic Models in Relativistic A+A Collisions
Universe
relativistic heavy-ion collisions
microscopic transport models
directed flow
mean-field potentials
title Directed Flow in Microscopic Models in Relativistic A+A Collisions
title_full Directed Flow in Microscopic Models in Relativistic A+A Collisions
title_fullStr Directed Flow in Microscopic Models in Relativistic A+A Collisions
title_full_unstemmed Directed Flow in Microscopic Models in Relativistic A+A Collisions
title_short Directed Flow in Microscopic Models in Relativistic A+A Collisions
title_sort directed flow in microscopic models in relativistic a a collisions
topic relativistic heavy-ion collisions
microscopic transport models
directed flow
mean-field potentials
url http://www.mdpi.com/2218-1997/5/3/69
work_keys_str_mv AT larissabravina directedflowinmicroscopicmodelsinrelativisticaacollisions
AT yuriikvasiuk directedflowinmicroscopicmodelsinrelativisticaacollisions
AT sergeysivoklokov directedflowinmicroscopicmodelsinrelativisticaacollisions
AT oleksandrvitiuk directedflowinmicroscopicmodelsinrelativisticaacollisions
AT evgenyzabrodin directedflowinmicroscopicmodelsinrelativisticaacollisions