New insights into backbending in the symmetry-adapted shell-model framework

0575100 - ÚJF 2024 RIV US eng J - Článek v odborném periodiku
Heller, N. D. - Sargsyan, G. H. - Launey, K. D. - Johnson, C. W. - Dytrych, Tomáš - Draayer, J. P.
New insights into backbending in the symmetry-adapted shell-model framework.
Physical Review C. Roč. 108, č. 2 (2023), č. článku 024304. ISSN 2469-9985. E-ISSN 2469-9993
Grant CEP: GA ČR(CZ) GA22-14497S
Institucionální podpora: RVO:61389005
Klíčová slova: symmetry-adapted framework * no-core shell model * energy spectrum
Obor OECD: Nuclear physics
Impakt faktor: 3.1, rok: 2022
Způsob publikování: Omezený přístup
https://doi.org/10.1103/PhysRevC.108.024304

We provide insights into the backbending phenomenon within the symmetry-adapted framework which naturally describes the intrinsic deformation of atomic nuclei. For 20Ne, the canonical example of backbending in light nuclei, the ab initio symmetry-adapted no-core shell model shows that while the energy spectrum replicates the backbending from experimental energies under the rotor-model assumption, there is no change in the intrinsic deformation or intrinsic spin of the yrast band around the backbend. For the traditional example of 48Cr, computed in the valence shell with empirical interactions, we confirm a high-spin nucleus that is effectively near-spherical, in agreement with previous models. However, we find that this spherical distribution results, on average, from an almost equal mixing of deformed prolate shapes with deformed oblate shapes. Microscopic calculations confirm the importance of spin alignment and configuration mixing, but surprisingly unveil no anomalous increase in moment of inertia. This finding opens the path toward further understanding the rotational behavior and moment of inertia of medium-mass nuclei.
Trvalý link: https://hdl.handle.net/11104/0344958