Deformed magic numbers at N = 178 and Z = 120, 124 in the 112≤N≤190 superheavy region from Skyrme mean-field calculations
Year: 2025
Type: article
Abstract: Background: Various motivations for exploration of superheavy (SH) region revolve around the question on whether 126 is a spherical proton magic number, as is the case for neutrons. In exploring this region, identification of nuclei with relatively longer half-life as compared to its neighbors is crucial for experimental studies. Such information is provided from theoretical predictions, which are, however, heavily dependent on the theoretical model used and observable quantities under investigation. Purpose: Limiting ourselves to the Skyrme Hartree–Fock-plus-Bardeen–Cooper–Schrieffer approach, we aimed to analyze the appearance of a nuclear region with relatively high stability associated with emergence of spherical and deformed magic numbers in the region of [Formula: see text] ([Formula: see text]) based on various observables. Methods: Three Skyrme parametrizations, namely the SkM* frequently employed for fission calculations, and the SLy5 and SLy4 commonly used for SH region, are considered to provide comparisons within the Skyrme mean-field approach. We evaluated the variation of electric quadrupole deformation ([Formula: see text]), binding energy per nucleon (BE/A), two-nucleon separation energy differential ([Formula: see text]), alpha-decay energy ([Formula: see text]) and alpha-decay half-lives ([Formula: see text]). Conclusion: Our analyses suggest that neutron number [Formula: see text] is candidate for deformed magic number around proton number [Formula: see text]. For protons, [Formula: see text] and 124 appears to be a candidate for deformed magic number at around [Formula: see text]–178. Both sets of deformed magic numbers appear at oblate ground-state deformation.
Authors: W. Asous, Mastura Syamimi Abdullah, Meng-Hock Koh, Kok-Siong Khoo
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W4408946879