THERMALIZATION IN ULTRARELATIVISTIC NUCLEAR COLLISIONS .1. PARTON KINETICS AND QUARK-GLUON PLASMA FORMATION

被引:139
作者
GEIGER, K
机构
[1] School of Physics and Astronomy, University of Minnesota, Minneapolis
关键词
D O I
10.1103/PhysRevD.46.4965
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A relativistic kinetic formulation of the time evolution of parton distributions during the early preequilibrium stage of nucleus-nucleus collisions at the BNL Relativistic Heavy Ion Collider (RHIC) and CERN Large Hadron Collider (LHC) is presented to study the microscopic dynamics and equilibration of the system. The nuclear collision is described as a sequence of multiple hard and soft parton-parton collisions and associated parton emission and absorption processes. Important aspects for the space-time evolution of the partonic system are the balance between emissive and absorptive processes, dilated formation of gluon radiation, and the effects of soft gluon interference. The time evolution of central S-32+S-32 and Au-197+Au-197 Collisions at RHIC (square-root s = 200A GeV) is studied in complete phase space and the approach to equilibrium is investigated. The results obtained imply the formation of hot quark-gluon plasmas in these collisions with estimated equilibration times, temperatures, and energy densities Of tau(eq) congruent-to 1.2 (1.8) fm/c, T congruent-to 290 (325) MeV, and epsilion congruent-to 17 (31) GeV/fm3 for S-32+S-32 (Au-197+Au-197). The consequences of such rather high temperatures and energy densities should be clear quark-gluon plasma signatures, observable in the production of charm, strangeness, direct photons, and dileptons.
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页码:4965 / 4985
页数:21
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