核物质散装粘度的对称性-能量依赖性
Yumu Yang1, Mauricio Hippert2,3, Enrico Speranza4
1University of Illinois Urbana-Champaign, Illinois Center for Advanced Studies of the Universe and Department of Physics, Urbana, Illinois 61801, USA.
Physical review letters
|December 12, 2025
概括
核对称能量及其斜率显著影响中子星物质的总粘度和放松时间. 这些特性影响中子星的潮反应,在引力波中可能可观察到.
科学领域:
- 核物理 核物理 核物理
- 天体物理学 天体物理学
- 引力波天文学 引力波天文学
背景情况:
- 中微子透明的npe物质属性对于理解中子星至关重要.
- 散装粘度 (ζ) 和放松时间 (τΠ) 是关键的运输量.
- 核对称能量 (S) 和它的斜率 (L) 是核物质的基本参数.
研究的目的:
- 为了澄清体积粘度和放松时间对核对称能量的依赖.
- 为了研究核物质特性对中子星潮变形能力的影响.
- 探索引力波信号对限制核物理学的潜力.
主要方法:
- 运输系数的理论计算.
- 在和密度下进行状态方程分析.
- 中子星潮反应的建模.
主要成果:
- 批量粘度和放松时间由核对称能 (S) 和其在和密度下的斜率 (L) 确定.
- 斜率 (L) 的变化可以导致散装粘度的数量级变化.
- 这些变化显著影响中子星的消散和保守的潮反应.
结论:
- 核对称能量及其斜率对于确定中子星物质的质量属性至关重要.
- 从二进制中子星启发的引力波签名可能会对核对称能量提供约束.
- 在GW中结合保守和消散效应可以提供对核物理学的见解.
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