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Kinetic evolution of the glasma and thermalization in heavy-ion collisions

机译:重离子碰撞中玻璃的动力学演化和​​热化

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In relativistic heavy-ion collisions, a highly occupied gluonic matter is created shortly after initial impact, which is in a nonthermal state and often referred to as the Glasma. Successful phenomenology suggests that the glasma evolves rather quickly toward the thermal quark-gluon plasma (QGP) and a hydrodynamic behavior emerges at a very early time ~?(1) fm/c. Exactly how such "apparent thermalization" occurs and connects the initial conditions to the hydrodynamic onset, remains a significant challenge for theory as well as phenomenology. We briefly review various ideas and recent progress in understanding the approach of the glasma to the thermalized QGP, with an emphasis on the kinetic theory description for the evolution of such far-from-equilibrium and highly overpopulated, thus weakly-coupled yet strongly interacting glasma.
机译:在相对论重离子碰撞中,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态,通常称为格拉斯马。成功的现象学表明,玻璃纤维向热夸克-胶子等离子体(QGP)的演化相当快,并且流体动力学行为在很早的时间(?)fm / c出现。这种“表观热化”的确切发生方式以及将初始条件与流体动力学的开始联系起来,仍然是理论和现象学的重大挑战。我们简要回顾了各种观点以及在了解玻璃质热化QGP方法方面的最新进展,重点是动力学理论描述了这种远离平衡和高度过剩,弱耦合但相互作用强的玻璃质的演化。

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