https://doi.org/10.1140/epja/s10050-024-01259-w
Regular Article - Theoretical Physics
A global study of -clusters decay in heavy and superheavy nuclei with half-life and preformation factor
1
Department of Physics (H & S), Government Women Engineering College, 305002, Ajmer, India
2
Department of Physics, Faculty of Science, University of Zagreb, HR-10000, Zagreb, Croatia
3
Government Polytechnic College, 313324, Rajsamand, India
4
Department of Computer Science and Engineering, Malviya National Institute of Technology, 302016, Jaipur, India
Received:
9
November
2023
Accepted:
1
February
2024
Published online:
5
March
2024
A detailed study of -clusters decay is exhibited by incorporating crucial microscopic nuclear structure information into the estimations of half-life and preformation factor. For the first time, using the k-cross validation approach, two semi-empirical formulas for (1) -decay half-life and (2) -particle preformation factor, are picked out and subsequently modified by including shell, odd-nucleon blocking, and asymmetry effects along with the usual dependence on -decay energy () and angular momentum of -particle. Both the formulas are fitted for the two different regions separated by neutron number N 126, as from the experimental systematics the role of N 126 shell closure is found decisive in determining the trends of , -decay half-life, and -particle preformation factor. It is found that the inclusion of the above-mentioned degrees of freedom significantly reduces the errors in the estimations when compared with several other similar modified/refitted semi-empirical relations indicating the robustness of the proposed formulas. The predictions of -decay half-life throughout the periodic chart have been made including the unknown territory, future probable decay chain of self-conjugate nucleus Ba terminated on Sn, decay chain of Pa through new isotope Ac as well as decay chains of awaiting superheavy nuclei Og and 120. This article is expected to provide a systematic approach to selecting the formula by which reliable predictions can be made.
Supplementary Information The online version contains supplementary material available at https://doi.org/10.1140/epja/s10050-024-01259-w.
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© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.