2014/02/28 by Jean-Paul Blaizot, Bin Wu, Li Yan · 7 citations
Physics and Astronomy · #Cosmology and Gravitation Theories #High-Energy Particle Collisions Research #Quantum Chromodynamics and Particle Interactions #hep-ph #nucl-th
paper · pdf · doi:10.1016/j.nuclphysa.2014.07.041
published as Nucl.Phys. A930 (2014) 139-162 · 32 pages, 25 figures, minor modifications, Final version published in NPA
openalex publication_date 2014/08/04 · arxiv created 2014/10/22 · arxiv updated 2014/10/23 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
In this paper, we study the thermalization of gluons and Nf flavors of massless quarks and antiquarks in a spatially homogeneous system. First, two coupled transport equations for gluons and quarks (and antiquarks) are derived within the diffusion approximation of the Boltzmann equation, with only 2<-> 2 processes included in the collision term. Then, these transport equations are solved numerically in order to study the thermalization of the quark-gluon plasma. At initial time, we assume that no quarks or antiquarks are present and we choose the gluon distribution in the form f = f0 theta (1-p/Qs) with Qs the saturation momentum and f0 a constant. The subsequent evolution of systems may, or may not, lead to the formation of a (transient) Bose condensate, depending on the value of f0. In fact, we observe, depending on the value of f0, three different patterns: (a) thermalization without gluon Bose-Einstein condensate (BEC) for f0 < f0t, (b) thermalization with transient BEC for f0t < f0 < f0c, and (c) thermalization with BEC for f0c < f0. The values of f0t and f0c depend on Nf. When f0> 1 > f0c, the onset of BEC occurs at a finite time tc ~ 1/((alphas f0)2 Qs). We also find that quark production slows down the thermalization process: the equilibration time for Nf = 3 is typically about 5 to 6 times longer than that for Nf = 0 at the same Qs.