强烈相互作用的物质在巨型中子星中表现出无限制的行为
Eemeli Annala1, Tyler Gorda2,3, Joonas Hirvonen4
1Department of Physics and Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, FI-00014, University of Helsinki, Finland.
Nature communications
|December 19, 2023
概括
中子星核可能包含极端密度的解密夸克物质. 这项研究表明,大质量中子星的状态方程与夸克物质一致,表明相位过渡.
科学领域:
- 核物理和天体物理学
- 高能量密度物理 高能量密度物理
背景情况:
- 中子星是超核密度物质的宇宙实验室.
- 中子星的核中可能存在从核物质到解封夸克物质的相变.
- 预计夸克物质具有近似的符合对称性,影响其状态方程 (EoS).
研究的目的:
- 量化物理中子星核中存在夸克物质的可能性.
- 为了研究大质量中子星的状态方程是否与解密的夸克物质一致.
主要方法:
- 将天体物理观测与理论计算结合起来.
- 采用贝叶斯推理来分析极端密度的状态方程.
- 评估了近似形态对称的恢复和活动自由度的数量.
主要成果:
- 极大质量中子星的状态方程与夸克物质一致.
- 在最高的探测密度下,发现大致的符合对称性恢复具有很高的可信性.
- 活跃的自由度的数量与未受限制的夸克物质的预测一致.
结论:
- 物理中子星,特别是最庞大的中子星,很可能在其核心中含有未被限制的夸克物质.
- 这些发现支持了夸克物质中近似合规对称性的理论预测.
- 这项研究提供了强有力的证据,证明中子星内部的阶段过渡到夸克物质.
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