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arXiv 2602.03388nucl-thastro-ph.HE
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探索多Λ超核和中子星物质中的超子Skyrme力

Exploring Hyperon Skyrme Forces in Multi-$Λ$ Hypernuclei and Neutron Star Matter

Xiamen University(厦门大学);Nankai University(南开大学)

X. D. Sun, S. C. Han, J. N. Hu, A. Li

AI总结:

研究通过Skyrme Hartree-Fock框架分析ΛΛ和ΛΛN相互作用参数,结合核数据和天体观测约束,发现ΛΛ相互作用参数空间被紧密约束,而ΛΛN三体相互作用参数受天文输入影响,结果提升了中子星最大质量。

摘要:

中子星 strangeness-rich 内部建模的主要不确定性源于超子和核子之间两体和三体相互作用的约束不足。我们基于超核实验数据和天体观测,对ΛΛ和ΛΛN相互作用参数进行了全面的贝叶斯分析。结果显示,ΛΛ相互作用参数空间通过结合核数据和天体数据被紧密约束,而ΛΛN三体相互作用参数仍受天文输入影响。具体而言,局部、动量无关的两体相互作用参数λ₀被紧密约束且主要为吸引,而动量依赖参数λ₁和λ₂在高密度下产生排斥效应。ΛΛ势深在纯Λ物质中起关键作用,有效约束两体ΛΛ相互作用并调控低密度下的吸引与高密度下的排斥平衡。ΛΛ相互作用的排斥成分降低了超子分数,使超子丰富方程of state与观测到的~2M☉中子星相吻合,最大质量增加达22%。引入ΛΛN三体力进一步使EOS变刚,最大质量增加达~0.1M☉。本研究是实现广泛密度和 strangeness 组成范围内密集物质完整、实验基础描述的重要一步。

英文摘要:

A major source of uncertainty in modeling the strangeness-rich interiors of neutron stars arises from the poorly constrained two-body and three-body interactions among hyperons and nucleons. We perform a comprehensive Bayesian analysis of the $ΛΛ$ and $ΛΛN$ interaction parameters within the Skyrme Hartree-Fock framework, constrained by both hypernuclei experimental data and astrophysical observations. Our results show that the parameter space of the $ΛΛ$ interaction is tightly constrained by combining nuclear and astrophysical data, while the parameters of the $ΛΛN$ three-body interaction remain sensitive to astrophysical inputs alone. Specifically, the local, momentum-independent two-body interaction parameter $λ_0$ is tightly constrained and predominantly attractive, while the momentum-dependent parameters $λ_1$ and $λ_2$ contribute repulsive effects at high densities. A key role is played by the $ΛΛ$ potential depth in pure $Λ$ matter, which effectively constrains the two-body $ΛΛ$ interaction and governs the balance between attraction at low densities and repulsion at high densities. The repulsive components of $ΛΛ$ interactions then decrease hyperon fractions and reconcile hyperon-rich equations of state with the observed $\sim2\,M_{\odot}$ neutron stars, increasing the maximum mass by up to 22\%. The inclusion of $ΛΛN$ three-body forces further stiffens the EOS, raising the maximum mass by up to $\sim 0.1\,M_{\odot}$. Our study represents a promising step toward a complete, experimentally grounded description of dense matter across a wide range of densities and strangeness compositions.

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。

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