On Kolmogorov wave turbulence in QCD

被引:46
作者
Mueller, A. H.
Shoshi, A. L. [1 ]
Wong, S. M. H.
机构
[1] Univ Bielefeld, Fak Phys, D-33501 Bielefeld, Germany
[2] Columbia Univ, Dept Phys, New York, NY 10027 USA
关键词
Kolmogorov wave turbulence; Kolmogorov spectra; instability; thermalization; heavy ion collisions;
D O I
10.1016/j.nuclphysb.2006.10.023
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We investigate Kolmogorov wave turbulence in QCD or, in other words, we calculate the spectrum of gluons as a function of time, f(k) (t), in the presence of a source which feeds in energy density in the infrared region at a constant rate. We find an early, an intermediate and a late time form for the gluon spectrum. Wave turbulence in QCD turns out to be somewhat different than the turbulence in the case phi(4)-type theories studied by Zakharov, L'vov and Falkovich. The hope is that a good understanding of QCD wave turbulence might lead to a better understanding of the instability problem in the early stages of the evolution after a heavy ion collision. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:145 / 165
页数:21
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