Momentum dependent potentials from a parity doubling CMF model in UrQMD: results on flow and particle production

被引:4
作者
Steinheimer, Jan [1 ,2 ]
Reichert, Tom [2 ,3 ,4 ]
Nara, Yasushi [5 ]
Bleicher, Marcus [1 ,3 ,4 ]
机构
[1] GSI Helmholtzzentrum Schwerionenforsch GmbH, Planckstr 1, D-64291 Darmstadt, Germany
[2] Frankfurt Inst Adv Studies FIAS, Ruth Moufang Str 1, D-60438 Frankfurt, Germany
[3] Goethe Univ Frankfurt, Inst Theoret Phys, Max von Laue Str 1, D-60438 Frankfurt, Germany
[4] GSI Helmholtzzentrum Schwerionenforsch GmbH, Helmholtz Res Acad Hesse FAIR HFHF, Campus Frankfurt,Max von Laue Str 12, D-60438 Frankfurt, Germany
[5] Akita Int Univ, Yuwa, Akita 0101292, Japan
基金
欧盟地平线“2020”;
关键词
high density equation of state; heavy ion collisions; chiral mean field model; UrQMD; PLUS AU COLLISIONS; QUANTUM MOLECULAR-DYNAMICS; HEAVY-ION COLLISIONS; QUARK-GLUON PLASMA; EQUATION-OF-STATE; NUCLEAR-EQUATION; PION-PRODUCTION; ELLIPTIC FLOW; MATTER; DENSITIES;
D O I
10.1088/1361-6471/adab0b
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The quantum molecular dynamics (QMD) part of the UrQMD model is extended to allow implementation of momentum dependent potentials from a parity doubling chiral mean field (CMF) model. Important aspects like energy conservation and effects on particle production and flow are discussed. It is shown, that this new implementation reproduces qualitatively and quantitatively available data over a wide range of beam energies and improves the description of observables without exception. In particular the description of hyperon and pion production at SIS18 energies is improved. From a comparison with HADES data one could conclude that the present parametrization of the CMF model leads to a slightly too weak momentum dependence. However, a more firm conclusion will require a systematic comparison with flow and multiplicity data over a range of beam energies and system sizes. Our work serves as an important step towards such future studies where the properties of dense QCD matter, through parameters of the CMF model, can be constraint using a comparison of the UrQMD model with high precision heavy ion data, finally also allowing direct comparisons with neutron star and neutron star merger observables.
引用
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页数:23
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