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- W4385491014 endingPage "138112" @default.
- W4385491014 startingPage "138112" @default.
- W4385491014 abstract "Halo phenomena have long been an important frontier in both experimental and theoretical nuclear physics. $^{37}$Mg was identified as a halo nucleus in 2014 and remains the heaviest nuclear halo system to date. While the halo phenomenon in $^{37}$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 $^{37}$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 $p$-wave halo characteristics of $^{37}$Mg are well reproduced without any free parameters. In particular, the orbital occupied by the halo neutron in $^{37}$Mg, exhibiting $p$-wave components comparable to those suggested in experiments, remains consistent across various employed density functionals including PC-F1, PC-PK1, NL3*, and PK1. The DRHBc theory investigated only even-even magnesium isotopes in previous works and for that reason missed predicting $^{37}$Mg as a halo nucleus before 2014. Although the core and the halo of $^{37}$Mg are both prolate, higher-order shape decoupling on the hexadecapole and hexacontatetrapole levels is predicted." @default.
- W4385491014 created "2023-08-03" @default.
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- W4385491014 date "2023-09-01" @default.
- W4385491014 modified "2023-10-15" @default.
- W4385491014 title "Missed prediction of the neutron halo in 37Mg" @default.
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- W4385491014 doi "https://doi.org/10.1016/j.physletb.2023.138112" @default.
- W4385491014 hasPublicationYear "2023" @default.
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