Decay Characteristics of Neutron Excess Scandium Nuclei

Qeios Pub Date : 2024-05-24 DOI:10.32388/25ngqr
J. Bevelacqua
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Abstract

Bevelacqua Resources, 7531 Flint Crossing Circle SE, Owens Cross Roads, AL 35762 USA  bevelresou@aol.com      In neutron star mergers, neutron excess nuclei and the r-process are important factors governing the production of heavier nuclear systems. A single-particle model evaluation of Scandium nuclei suggests that the heaviest Z = 21 nucleus will have mass 71 with filling of the 1g9/2 neutron shell. A = 59 – 71 scandium isotopes have limited experimental half-life data, but the model predicts beta decay half-lives in the range of 0.312 – 7.60 ms. Based on previous calculations for Z = 9 - 20, 26, and 30 systems and comparisons to the 59Sc – 67Sc calculations, summarized in the Japanese Nuclear Data Compilation, the single-particle model results likely overestimate the half-lives of A = 59 – 71 neutron excess scandium nuclei. KEYWORDS: Nucleosynthesis, Neutron Excess Scandium Nuclei, Beta Decay, Nuclear Structure
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中子过剩钪核的衰变特性
Bevelacqua Resources, 7531 Flint Crossing Circle SE, Owens Cross Roads, AL 35762 USA bevelresou@aol.com 在中子星合并中,中子过剩核和r过程是产生较重核系统的重要因素。对钪核的单粒子模型评估表明,最重的 Z = 21 核在填满 1g9/2 中子壳后的质量为 71。A = 59 - 71钪同位素的实验半衰期数据有限,但模型预测β衰变半衰期在 0.312 - 7.60 毫秒之间。根据以前对 Z = 9 - 20、26 和 30 系统的计算,以及与《日本核数据汇编》中总结的 59Sc - 67Sc 计算的比较,单粒子模型的结果很可能高估了 A = 59 - 71 中子过剩钪核的半衰期。
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