[Submitted on 12 Aug 2025]
Exact Calculation of Strongly Correlated Nucleonic Matter
Rongzhe Hu🇨🇳 · Shaoliang Jin🇨🇳 · Xin Zhen🇨🇳 · Haoyu Shang🇨🇳 · Junchen Pei🇨🇳 · Furong Xu🇨🇳 · Francesco Marino🇩🇪
Dense nucleonic matter is of vital importance for understanding compact stars and inferring the transition into deconfined quark phase. We present exact calculations of infinite nucleonic matter with the state-of-the-art full configuration-interaction quantum Monte Carlo method, enabling us to rigorously benchmark many-body methods and assess the degree to which the nucleonic matter is correlated. Our method has been numerically validated against exact diagonalization within a small model space. Calculations of nucleonic matter using chiral nuclear forces reveal that symmetric nuclear matter is strikingly strongly correlated, raising questions on previous calculations of nuclear matter with many-body expansion truncations and offering insights into simultaneous descriptions of finite nuclei and infinite nucleonic matter from first principles.
- Comments:
- 6 pages, 4 figures, published version
- Subjects:
- Nuclear Theory (nucl-th); High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Experiment (nucl-ex)
- arXiv:
- 2508.09252 [pdf]