论文标题
大型中子星的核心是什么？
What's in the core of massive neutron stars?
论文作者
论文摘要
当强度的变化以高于核问题密度$ N_0 $的两倍的拓扑变化而表达的强子夸克的连续性可以用大量紧凑型恒星的核心来描述，这既不像纯baryons of pure baryons offers of pure baryon电荷的准颗粒。隐藏的对称性（局部规格和伪符号（或刻度））出现并引起长期以来的核Gamow-teller tellients $ \ sim n_0 $的Qu_a $ g_a $，并引起了伪内形式的声音速度$ V_ {PCS}^2/C^2/c^2 $ et $ 1/3 $ gs $ gs $ gs。这些特性面临着最近观察到的超纯游戏转换和天体物理观察中的观察结果。
When hadron-quark continuity is formulated in terms of a topology change at a density higher than twice the nuclear matter densiy $n_0$ the core of massive compact stars can be described in terms of quasiparticles of fractional baryon charges, behaving neither like pure baryons nor deconfined quarks. Hidden symmetries, both local gauge and pseudo-conformal (or broken scale), emerge and give rise to the long-standing quenched $g_A$ in nuclear Gamow-Teller transitions at $\sim n_0$ and to the pseudo-conformal sound velocity $v_{pcs}^2/c^2\approx 1/3$ at $\gsim 3n_0$. These properties are confronted with the recent observations in superallowed Gamow-Teller transitions and in astrophysical observations.
