发表机构
Technical University of Munich; Excellence Cluster ORIGINS（慕尼黑工业大学; ORIGINS卓越集群）
机构由 AI 辅助整理，请以论文原文为准。AI 中文总结
本文致敬Rho曼纽，延续其思想，回顾更新核子结构双尺度等早期概念，分析核子核心与云尺度，探讨其对致密核物质的意义并与中子星观测的贝叶斯推断结果对比。
AI 中文摘要
本文是对Rho曼纽（Mannque Rho）的纪念致敬，延续了他数十年来不断启发和塑造的一系列思想与理念：从低能核子结构的双尺度图像，到中子星核心中存在的致密冷重子物质。文中回顾了早期开创性概念，并通过近期对核子“核心”与“云”尺度的高级分析对其进行更新，随后讨论了这些概念对致密核物质的意义，并将其与中子星观测的贝叶斯推断分析所得的经验信息进行对比。
英文摘要
This memorial tribute to Mannque Rho follows a line of thoughts and ideas that he continuously inspired and shaped over many decades: from the two-scales picture of low-energy nucleon structure to dense and cold baryonic matter as it is realized in the cores of neutron stars. Early groundbreaking concepts are recalled and updated by recent advanced analyses of the `core' and `cloud' sizes of the nucleon. Implications for dense nuclear matter are then discussed and confronted with empirical information from Bayesian inference analyses of neutron star observables.
Comments12 pages, 12 figures
