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arXiv 2212.03466hep-phastro-ph.CO
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宇宙QCD转变——从夸克到奇异子和核子

Cosmic QCD transition-from quark to strangeon and nucleon

School of Physics, Peking University(北京大学物理学院);Kavli Institute for Astronomy and Astrophysics, Peking University(北京大学科维理天文与天体物理研究所);School of Science, Xi’an Jiaotong University(西安交通大学理学院);MOE Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter,Xi’an Jiaotong University(西安交通大学凝聚态物质非平衡合成与调控教育部重点实验室)

Xuhao Wu, Weibo He, Yudong Luo, Guo-Yun Shao, Renxin Xu

AI总结:

研究早期宇宙中QCD相变,通过非微扰耦合形成稳定奇异子nuggets,其热力学贡献微弱,可能解释冷暗物质。

摘要:

在早期宇宙中,研究了一个交叉型QCD相变,涉及稳定奇异子 nuggets 的形成场景。应用Polyakov-Nambu-Jona-Lasinio模型来计算包含u、d、s夸克的QCD相的热力学性质,并用相对论平均场模型描述核物质。夸克到核子的交叉相变发生在宇宙温度约为170 MeV时,这两个相在三窗口模型中相连。由于夸克的非微扰耦合,在转变过程中,具有净奇异性的夸克簇(即奇异子)以及奇异子 nuggets 可能形成。引入了一个 nugget 质子数分布函数来描述 nuggets 的数量密度。所有具有A>A_c的奇异子 nuggets 被认为是稳定的,其中临界数A_c由弱相互作用和强相互作用共同决定。应用非相对论方程状态来计算稳定 nuggets 的热力学性质。计算显示,稳定奇异子 nuggets 的热力学贡献(压力、熵等)是微不足道的。最终的奇异子 nuggets 的质量密度与暗物质相当,这表明可能提供了一种解释冷暗物质的可能,而无需引入超出标准模型的任何奇异粒子。

英文摘要:

A crossover QCD phase transition in the early Universe, involving a formation scenario of stable strangeon nuggets is studied. The Polyakov-Nambu-Jona-Lasinio model is applied to calculate the thermodynamics of the QCD phase with u, d, s quarks, and the relativistic mean-field model describes the hadronic matter. The crossover phase transition from quarks to hadrons occurred at cosmic temperature of T~170 MeV, and those two phases are connected in a three-window model. Due to quark's non-perturbative coupling, quark clusters with net strangeness (i.e., strangeons) and then strangeon nuggets could form during the transition process. A distribution function of the nugget baryon number, A, is introduced to describe the nuggets' number density. All the strangeon nuggets with A>A_c are considered to be stable, where the critical number, A_c, is determined by both the weak and strong interactions. A non-relativistic equation of state is applied to calculate the thermodynamics of stable nuggets. The calculation shows that the thermodynamical contributions (pressure, entropy, etc.) of the stable strangeon nuggets are negligible. The resultant mass density of the strangeon nuggets survival from the early Universe is comparable to the dark matter, that indicates a possible explanation of the cold dark matter without introducing any exotic particles beyond the standard model.

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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