In relativistic heavy ion collisions, a highly occupied gluonic matter iscreated shortly after initial impact, which is in a non-thermal state and oftenreferred to as the Glasma. Successful phenomenology suggests that the glasmaevolves rather quickly toward the thermal quark-gluon plasma and a hydrodynamicbehavior emerges at very early time $\sim \hat{o}(1)$ fm/c. Exactly how such"apparent thermalization" occurs and connects the initial conditions to thehydrodynamic onset, remains a significant challenge for theory as well asphenomenology. We briefly review various ideas and recent progress inunderstanding the approach of the glasma to the thermalized quark-gluon plasma,with an emphasis on the kinetic theory description for the evolution of suchfar-from-equilibrium and highly overpopulated, thus weakly-coupled yet stronglyinteracting glasma.
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机译:在相对论性重离子碰撞中,初始撞击后不久便产生了一个高度占据的胶质物质,该胶质物质处于非热状态,通常称为格拉斯马。成功的现象学表明,玻璃体向热夸克-胶子等离子体的演化相当快,并且在很早的时间就出现了流体动力学行为。\\ sim \ hat {o}(1)$ fm / c。确切地说,如何发生这种“表观热化”并将初始条件与流体动力学发生联系起来,仍然是理论和现象学的重大挑战。我们简要回顾了各种认识和了解玻璃对热夸克-胶子等离子体的处理方法的最新进展,重点介绍了从远处平衡和高度过剩,因此弱耦合但相互作用强的玻璃的演化的动力学理论描述。 。
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