Quark stars in the pure pseudo-Wigner phase

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Li-Qun Su, Chao Shi, Yong-Feng Huang, Yan Yan, Cheng-Ming Li, Wen-Li Yuan, Hong-Shi Zong
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Abstract

In this paper, we consider the scenario of a pure quark star which is completely composed of quarks in the pseudo-Wigner phase. The equation of state (EoS) of deconfined quark stars is studied in the framework of the two-flavor NJL model, and the self-consistent mean field approximation is employed by introducing a parameter \(\alpha \) combining the original Lagrangian and the Fierz-transformed Lagrangian, \(\mathcal{L}_{R}= (1-\alpha )\mathcal{L}+\alpha \mathcal{L}_{F}\), to measure the weights of different interaction channels. We assume deconfinement phase transition happens along with the chiral phase transition. Thus, due to the lack of description of confinement in the NJL model, the vacuum pressure is set to confine quarks at low densities, which is the pressure corresponding to the critical point of chiral phase transition. We find that the bag constant shifts from \((130\text{ MeV})^{4}\) to \((150 \text{ MeV})^{4}\) as \(\alpha \) grows. When \(\alpha \) is around 0.9, the mass-radius relations of deconfined quark stars can meet the requirement of pulsar observations. In addition, the tidal deformability \(\Lambda \) is found to range in 253 – 482, which satisfies the astronomical constraint of \(\Lambda <800\) for 1.4-solar-mass neutron stars.

纯伪维格纳阶段的夸克星
本文考虑了完全由处于伪维格纳相的夸克组成的纯夸克星的情形。在双味NJL模型框架下研究了去封闭夸克星的状态方程,并通过引入一个参数(\α \)结合原始拉格朗日和费尔兹变换拉格朗日,采用了自洽平均场近似、\(\mathcal{L}_{R}= (1-\alpha )\mathcal{L}+\alpha \mathcal{L}_{F}\),来测量不同相互作用通道的权重。我们假设去抵消相变与手性相变同时发生。因此,由于 NJL 模型缺乏对约束的描述,我们将真空压力设定为在低密度下约束夸克,也就是手性相变临界点对应的压力。我们发现,随着 \(α \) 的增长,包常数从 \((130 \text{ MeV})^{4}\) 变为 \((150 \text{ MeV})^{4}\) 。当(α)在0.9左右时,去束缚夸克星的质量-半径关系可以满足脉冲星观测的要求。此外,潮汐变形率(\Lambda \)的范围在253 - 482之间,满足1.4太阳质量中子星的天文约束条件(\\Lambda <800\)。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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