Halo structure of $^6$He from $\textit{ab initio}$ two-nucleon spatial correlations
Mengyao Huang, Tobias Frederico, Peng Yin, Robert A. M. Basili, Patrick J. Fasano, James P. Vary

TL;DR
This study uses ab initio no-core shell model calculations to analyze two-nucleon spatial correlations in helium isotopes, revealing the halo structure of $^6$He and the dominant spin-singlet configuration of its valence neutrons.
Contribution
It provides a detailed ab initio analysis of two-nucleon correlations and halo structure in $^6$He, highlighting the role of off-centering effects and specific two-body correlations.
Findings
Valence neutrons in $^6$He form a spin-singlet state.
Pair separations between core and halo neutrons are about 80% larger than within the core.
Off-centering of the halo neutrons explains increased point-proton radius in $^6$He.
Abstract
We evaluate pairwise correlations using ground state wave functions for He and He obtained by no-core shell model (NCSM) calculations with the Daejeon16 nucleon-nucleon interaction plus Coulomb interaction, to characterize the structures of these two systems. We demonstrate that two-nucleon spatial correlations, specifically the pair-number operator and the square-separation operator projected on two-body spin and isospin -components encode important details of the halo structure of He. We also analyze the single-particle state occupancies and the two-body state occupancies for the ground state of He and He. Our results indicate that the two valence neutrons in the ground state of He dominantly form a spin-singlet configuration. The rms pair separations between core nucleons and halo neutrons of He is about 80% larger…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNuclear physics research studies · Quantum Chromodynamics and Particle Interactions · Pulsars and Gravitational Waves Research
