逆流非阿贝尔流体中的新型不稳定性

Subramanya Bhat K.N. , Amita Das , V. Ravishankar , Bhooshan Paradkar
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引用次数: 0

摘要

强相互作用粒子的动力学受杨-米尔斯(Y-M)理论支配,该理论是麦克斯韦电动力学(ED)的自然概括。它的量子化版本被称为量子色动力学(QCD)(Gross and Wilczek, 1973; Politzer, 1973; 't Hooft, 1972[1], [2], [3]),研究得非常深入。事实证明,经典 Y-M 理论同样令人感兴趣,因为它在描述夸克-胶子等离子体(QGP)物理学中发挥着核心作用--夸克-胶子等离子体在早期宇宙中非常普遍,在相对论重离子碰撞实验中也会产生。这就需要对经典 Y-M 理论进行系统研究。对经典 Y-M 动力学的深入了解,最好是将 Y-M 结果与其对应的 ED 结果进行比较和对比。本文首先考虑了 Y-M 流体中的流不稳定性。我们发现,除了类似于 ED 的不稳定性之外,还出现了新的非阿贝尔模式,反映了相互作用固有的非阿贝尔性质。新模式表现出传播/增长,其增长率可能大于我们在 ED 中发现的增长率。有趣的是,我们还发现了一种不受介质影响而传播的模式。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Novel instabilities in counter-streaming nonabelian fluids

The dynamics of strongly interacting particles are governed by Yang–Mills (Y–M) theory, which is a natural generalization of Maxwell Electrodynamics (ED). Its quantized version is known as quantum chromodynamics (QCD) (Gross and Wilczek, 1973; Politzer, 1973; ’t Hooft, 1972[1], [2], [3]) and has been very well studied. Classical Y–M theory is proving to be equally interesting because of the central role it plays in describing the physics of quark–gluon plasma (QGP) — which was prevalent in the early universe and is also produced in relativistic heavy ion collision experiments. This calls for a systematic study of classical Y–M theories. A good insight into classical Y–M dynamics would be best obtained by comparing and contrasting the Y–M results with their ED counterparts. In this article, a beginning has been made by considering streaming instabilities in Y–M fluids. We find that in addition to analogues of ED instabilities, novel nonabelian modes arise, reflecting the inherent nonabelian nature of the interaction. The new modes exhibit propagation/ growth, with growth rates that can be larger than what we find in ED. Interestingly, we also find a mode that propagates without getting affected by the medium.

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