致密星中的致密物质-教学介绍
Dense matter in compact stars - A pedagogical introduction
摘要：
在致密恒星的内部可以发现冷而致密的核物质和/或夸克物质。由于量子色动力学的强耦合性质，确定这种物质的基态和性质是非常具有挑战性的。我给一个教学介绍微观计算的基础上唯象模型，有效的理论和微扰QCD。我将讨论这些计算的结果如何与天体物理观测相关联，以潜在地排除或确认致密物质的候选阶段。
英文摘要：
Cold and dense nuclear and/or quark matter can be found in the interior of compact stars. It is very challenging to determine the ground state and properties of this matter because of the strong-coupling nature of QCD. I give a pedagogical introduction to microscopic calculations based on phenomenological models, effective theories, and perturbative QCD. I discuss how the results of these calculations can be related to astrophysical observations to potentially rule out or confirm candidate phases of dense matter.
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。
