# Quark production, Bose-Einstein condensates and thermalization of the   quark-gluon plasma

**Authors:** Jean-Paul Blaizot, Bin Wu, and Li Yan

arXiv: 1402.5049 · 2014-10-23

## TL;DR

This study models the thermalization process of quark-gluon plasma, revealing how initial gluon distributions influence Bose-Einstein condensate formation and showing quark production delays thermalization.

## Contribution

It derives coupled transport equations for gluons and quarks, and explores the conditions leading to Bose-Einstein condensate formation during plasma thermalization.

## Key findings

- Different thermalization patterns depending on initial gluon density.
- Quark production extends the thermalization time significantly.
- Bose-Einstein condensate formation depends on initial conditions.

## Abstract

In this paper, we study the thermalization of gluons and N_f 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 = f_0 theta (1-p/Q_s) with Q_s the saturation momentum and f_0 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 f_0. In fact, we observe, depending on the value of f_0, three different patterns: (a) thermalization without gluon Bose-Einstein condensate (BEC) for f_0 < f_{0t}, (b) thermalization with transient BEC for f_{0t} < f_0 < f_{0c}, and (c) thermalization with BEC for f_{0c} < f_0. The values of f_{0t} and f_{0c} depend on N_f. When f_0> 1 > f_{0c}, the onset of BEC occurs at a finite time t_c ~ 1/((alpha_s f_0)^2 Q_s). We also find that quark production slows down the thermalization process: the equilibration time for N_f = 3 is typically about 5 to 6 times longer than that for N_f = 0 at the same Q_s.

## Full text

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## Figures

36 figures with captions in the complete paper: https://tomesphere.com/paper/1402.5049/full.md

## References

16 references — full list in the complete paper: https://tomesphere.com/paper/1402.5049/full.md

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Source: https://tomesphere.com/paper/1402.5049