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Systematic study of \boldsymbol\mathcalα decay of nuclei around \boldsymbolZ=82, \boldsymbolN=126 shell closure within the cluster-formation model and proximity potential 1977 formalism

2018/04/17 by Jun-Gang Deng, Jie-Cheng Zhao, Peng-Cheng Chu +1 · 1 citation
Physics and Astronomy · #nucl-th #nucl-ex

paper · pdf · doi:10.1103/physrevc.97.044322

published as Phys. Rev. C 2018 · 4 figures, 7 tables; Accepted by Physical Review C

arxiv created 2018/04/17 · arxiv updated 2019/04/18

Abstract

In the present work, we systematically study the \mathcalα decay preformation factors Pα within the cluster-formation model and \mathcalα decay half-lives by the proximity potential 1977 formalism for nuclei around Z=82, N=126 closed shells. The calculations show that the realistic Pα is linearly dependent on the product of valance protons (holes) and valance neutrons (holes) NpNn. It is consistent with our previous works [X.-D. Sun et al., \hrefhttps://journals.aps.org/prc/abstract/10.1103/PhysRevC.94.024338 Phys. Rev. C 94, 024338 (2016), J.-G. Deng et al., \hrefhttps://journals.aps.org/prc/abstract/10.1103/PhysRevC.96.024318Phys. Rev. C 96, 024318 (2017)], which Pα are model-dependent and extracted from the ratios of calculated \mathcalα half-lives to experimental data. Combining with our previous works, we confirm that the valance proton-neutron interaction plays a key role in the \mathcalα preformation for nuclei around Z=82, N=126 shell closures whether the Pα is model-dependent or microcosmic. In addition, our calculated \mathcalα decay half-lives by using the proximity potential 1977 formalism taking Pα evaluated by the cluster-formation model can well reproduce the experimental data and significantly reduce the errors.

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