
TL;DR
This paper discusses theoretical predictions of superheavy elements' stability, shapes, and decay properties, highlighting potential 'magic islands' of stability around specific proton and neutron numbers, and presents calculations of alpha-decay half-lives.
Contribution
The study provides new theoretical calculations of alpha-decay half-lives of superheavy nuclei using a WKB approach with density-dependent M3Y interaction, aligning well with experimental data.
Findings
Predicted superheavy nuclei with N=184 are spherical in ground states.
Fission-survived Sg nuclei with Z=106, N=162 have the longest alpha-decay half-life (~3.2 hours).
Neutron-rich superheavy nuclei with Z>118 have very short half-lives of microseconds or less.
Abstract
Recent microscopic calculation based on the density functional theory predicts long-lived superheavy elements in a variety of shapes, including spherical, axial and triaxial configurations. Only when N=184 is approached one expects superheavy nuclei that are spherical in their ground states. Magic islands of extra-stability have been predicted to be around Z=114, 124 or, 126 with N=184, and Z=120, with N=172. However, the question of whether the fission-survived superheavy nuclei with high Z and N would live long enough for detection or, undergo alpha-decay in a very short time remains open. In this talk I shall present results of our calculations of alpha-decay half lives of heavy and superheavy nuclei. Calculations, carried out in a WKB framework using density-dependent M3Y interaction, have been found to reproduce the experimental data quite well. Fission survived Sg nuclei with…
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