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arXiv 2312.08758nucl-th
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从夸克-介子耦合强子物质到退禁闭夸克物质的混合星相变效应

Effects of phase transition in hybrid stars from quark-meson coupling hadronic matter to deconfined quark matter

Yida Yang, Chen Wu, Ji-Feng Yang

AI总结:

本研究探究混合星内强子-夸克相变类型与夸克模型对星体性质的影响,发现交叉相变结合热力学校正可使混合星最大质量符合脉冲星PSR J0952-0607的观测约束。

摘要:

近零温高密度下,强子到夸克的不同类型相变可能发生在混合星的内核中。我们研究了相变类型与夸克模型对混合星及夸克核性质的影响。采用夸克-介子耦合(QMC)模型描述强子物质,同时使用MIT袋模型以及Nambu-Jona-Lasinio(NJL)模型描述夸克物质以作对比。从通过物态方程(EOS)得到的质量-半径曲线中我们发现,在一级相变情形下,强子物质的物态方程对混合星的最大质量具有决定性影响,而在交叉相变情形下,夸克物质的物态方程对结果的影响更大。本研究还发现,由插值方案产生的热力学校正会显著使物态方程变硬。因此,交叉型相变通常会形成质量更高的混合星。特别地,通过使用QMC模型和NJL模型构建带热力学校正的交叉物态方程,我们发现混合星的最大质量能够满足PSR J0952-0607近期的质量观测约束,即$2.35\neq0.17M_\text{odot}$。

英文摘要:

Different types of phase transition from hadron to quark at high density near zero temperature may occur in the inner core of hybrid stars. We investigate the impacts of phase transition types and quark models on properties of hybrid star and quark cores. The quark-meson coupling (QMC) model is used to describe hadronic matter, and the MIT bag model as well as the Nambu-Jona-Lasinio (NJL) model are employed to describe quark matter for comparison. From the mass-radius curves obtained by using equations of state (EOS), we find that EOSs of hadron matter have a decisive influence on the maximum mass of a hybrid star in the first-order phase transition case, while quark matter EOSs have more impacts on results in the crossover transition case. It is also found in the present work that the thermodynamic correction arising from an interpolation scheme considerably stiffens the EOSs. Therefore the crossover type phase transition generally leads to hybrid stars with higher masses. In particular, by using the QMC model and the NJL model to construct crossover EOSs with thermodynamic correction, we discover that the maximum masses of hybrid stars can meet the recent observational constraint on mass from PSR J0952-0607, i.e., $2.35\pm0.17M_\odot$.

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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