Abstract
Systematic study of superheavy nuclei 296 Og and its possibilities to emit alpha particle and heavier clusters are studied using Modified Generalized Liquid Drop Model (MGLDM) with Q value dependent preformation factor. Half-lives and branching ratio of all possible cluster emission of 296 Og is checked and only those cluster which are within the experimental half-lives limit (less than 10 30 s) and branching ratio limit (down to 10 -19 ) are considered. Among this, 88 Kr is found to be the most probable heavy cluster, leading to doubly magic 208 Pb daughter nuclei, with half-lives comparable with alpha decay half-lives. Thus the role of doubly magic daughter nuclei in cluster decay is highlighted here. Again the decay modes of 296 Og are also studied by comparing alpha decay half-lives using MGLDM with spontaneous fission half-lives proposed by Bao et al. , and from this, it is found that for superheavy element 296 Og, decays by 3 alpha chains followed by spontaneous fission. We hope that this study would help when this emission is experimentally detected in near future.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have