混合星中的强子-夸克混合相区
Region of hadron-quark mixed phase in hybrid stars
摘要：
强子-夸克混合相在混合星内部结构的广泛区域中存在。然而，我们表明，强子-夸克混合相应限制在一个较窄的区域，因为电荷屏蔽效应。混合相的窄区域似乎解释了中子星的强磁场和毛刺现象等物理现象，并给出了新的中子星冷却曲线。
英文摘要：
Hadron--quark mixed phase is expected in a wide region of the inner structure of hybrid stars. However, we show that the hadron--quark mixed phase should be restricted to a narrower region to because of the charge screening effect. The narrow region of the mixed phase seems to explain physical phenomena of neutron stars such as the strong magnetic field and glitch phenomena, and it would give a new cooling curve for the neutron star.
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。
