Missed prediction of the neutron halo in $^{37}$Mg
K. Y. Zhang, S. Q. Yang, J. L. An, S. S. Zhang, P. Papakonstantinou,, M.-H. Mun, Y. Kim, H. Yan

TL;DR
This paper presents a microscopic, self-consistent theoretical description of the neutron halo in $^{37}$Mg using the DRHBc model, successfully reproducing experimental data and clarifying the orbital structure, which was previously missed.
Contribution
It provides the first accurate, parameter-free prediction of the neutron halo in $^{37}$Mg using the deformed relativistic Hartree-Bogoliubov theory in continuum.
Findings
Reproduces neutron separation energies and matter radii of magnesium isotopes.
Identifies the $p$-wave orbital of the halo neutron consistent with experiments.
Predicts higher-order shape decoupling in $^{37}$Mg.
Abstract
Halo phenomena have long been an important frontier in both experimental and theoretical nuclear physics. Mg was identified as a halo nucleus in 2014 and remains the heaviest nuclear halo system to date. While the halo phenomenon in Mg was not predicted before the discovery, its description has been still challenging afterwards. In this Letter, we report a microscopic and self-consistent description of the neutron halo in Mg using the deformed relativistic Hartree-Bogoliubov theory in continuum (DRHBc) that was developed in 2010. The experimental neutron separation energies and empirical matter radii of neutron-rich magnesium isotopes as well as the deformed -wave halo characteristics of Mg are well reproduced without any free parameters. In particular, the orbital occupied by the halo neutron in Mg, exhibiting -wave components comparable to…
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Taxonomy
TopicsNuclear Physics and Applications · Nuclear physics research studies · Atomic and Subatomic Physics Research
