Local thermodynamical equilibrium and the equation of state of hot, dense matter created in Au+Au collisions at AGS

被引:65
作者
Bravina, LV
Gorenstein, MI
Belkacem, M
Bass, SA
Bleicher, M
Brandstetter, M
Hofmann, M
Soff, S
Spieles, C
Weber, H
Stocker, H
Greiner, W
机构
[1] Univ Frankfurt, Inst Theoret Phys, D-6000 Frankfurt, Germany
[2] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel
[3] Duke Univ, Dept Phys, Durham, NC 27706 USA
[4] Gesell Schwerionenforsch, Darmstadt, Germany
关键词
statistical model; equation of state; thermalization; Monte Carlo model for relativistic heavy ion collisions;
D O I
10.1016/S0370-2693(98)00624-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Local kinetic and chemical equilibration is studied for Au + Au collisions at 10.7 AGeV in the microscopic Ultrarelativistic Quantum Molecular Dynamics model (UrQMD). The UrQMD model exhibits dramatic derivations from equilibrium during the high density phase of the collision. Thermal and chemical equilibration of the hadronic matter seems to be established in the later stages during a quasi-isentropic expansion, observed in the central reaction cell with volume 125 fm(3). For t greater than or equal to 10 fm/c the hadron energy spectra in the cell are nicely reproduced by Boltzmann distributions with a common rapidly dropping temperature. Hadron yields change drastically and at the late expansion stage follow closely those of an ideal gas statistical model. The equation of state seems to be simple at late times: P congruent to 0.12 epsilon. The time evolution of other thermodynamical variables in the cell is also presented. (C) 1998 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:379 / 387
页数:9
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