Study of β+/EC-decay properties of sd shell nuclei using nuclear shell model
Abstract
Our study employs the nuclear shell model to systematically compute the half-lives of β -decay for nuclei in the mass range of A = 18-39, encompassing the majority of sd shell nuclei. This analysis utilizes the USDB and SDNN Hamiltonians. The theoretical outcomes contain calculations of various parameters such as Q -values, half-lives, excitation energy, logft values, and branching ratios. We explore these results with axial-vector coupling constant for weak interactions, denoted as gA(= 1.27), and value (= 6289). We perform calculations of Gamow Teller matrix elements for 116 decay processes to calculate the quenching factor; we found a quenching factor of q = 0.7940.05 for the USDB interaction and q = 0.8150.04 for the SDNN interaction. We have also calculated superallowed transitions 0+ → 0+ for seven nuclei. Further, we have also included the electron capture phase space factor for the required nuclei to calculate the half-lives. This inclusion leads to small contribution in results, particularly for nuclei where electron capture (EC) plays a significant role. The overall results are in agreement with the experimental data.
Turn this paper into a full lesson
ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.