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arXiv 2407.09754hep-phhep-thnucl-th
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重离子碰撞预平衡阶段磁场诱导的各向异性胶子压力的影响:通往各向同性化的更快速路径

Influence of magnetic field-induced anisotropic gluon pressure during pre-equilibrium in heavy-ion collisions: A faster road towards isotropization

A. Ayala, A. Mizher

AI总结:

本研究针对重离子碰撞预平衡阶段的强磁场效应,采用强场近似结合有效动力学理论分析磁场诱导的胶子压力各向异性,发现该效应可加快约1 fm固有时下的各向同性化进程。

摘要:

在周边高能重离子碰撞中可产生高强度磁场。尽管其强度下降迅速,且目前尚不清楚这些磁场的持续时间是否足以在夸克-胶子等离子体阶段诱导磁化,但大多数模型和模拟预测,存在可观强度的磁场可持续至反应开始后约1 fm的固有时,这正是流体动力学阶段启动的典型时间。该时间段被称为预平衡阶段。因此,预平衡阶段的反应演化很可能受到这些磁场的影响。在本研究中,我们采用强场近似来研究磁场诱导的各向异性对胶子压力的影响。我们将这种各向异性纳入通过有效动力学理论(Effective Kinetic Theory)得到的描述中,并探究其对在约1 fm固有时达到各向同性化的影响。我们表明,当纳入磁场效应时,各向同性化的实现速度更快。

英文摘要:

Magnetic fields of a large intensity can be generated in peripheral high-energy heavy-ion collisions. Although their intensity drops fast and, moreover, it is not clear whether these fields last long enough to induce a magnetization during the quark-gluon plasma phase, most of the models and simulations predict a significant intensity that lasts up to proper times of order 1 fm after the beginning of the reaction, which is a typical time for the hydrodynamical phase to start. This interval of time is referred to as the pre-equilibrium stage. The evolution of the reaction during pre-equilibrium is thus likely to be influenced by these fields. In this work we adopt a strong field approximation to study the effects of the magnetic field-induced anisotropy on the gluon pressure. We include this anisotropy within the description obtained by means of Effective Kinetic Theory and explore the consequences to reach isotropization at proper times of order 1 fm. We show that when including the magnetic field effects, isotropization is achieved faster.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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