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Astrophysical reaction rates of α-induced reactions for nuclei with 26≤Z≤83 from the new Atomki-V2 α-nucleus potential
Atomic Data and Nuclear Data Tables ( IF 1.8 ) Pub Date : 2021-08-06 , DOI: 10.1016/j.adt.2021.101453
P. Mohr 1 , Zs. Fülöp 1 , Gy. Gyürky 1 , G.G. Kiss 1 , T. Szücs 1 , A. Arcones 2, 3 , M. Jacobi 2 , A. Psaltis 2
Affiliation  

The new Atomki-V2 α-nucleus potential is applied to calculate astrophysical reaction rates NAσv of intermediate mass and heavy target nuclei from iron (Z=26) up to bismuth (Z=83). Overall, reaction rates of α-induced reactions are provided for 4359 target nuclei, covering as well neutron-deficient as extremely neutron-rich target nuclei from the proton to the neutron dripline. Contrary to previous rate compilations, these new calculations include all relevant exit channels with the dominating (α, xn) reactions for neutron-rich target nuclei.



中文翻译:

来自新 Atomki-V2 α 核势的 26≤Z≤83 原子核的 α 诱导反应的天体物理反应速率

新的 Atomki-V2 α- 应用核势来计算天体物理反应速率 N一种σv 来自铁的中等质量和重的目标原子核(Z=26) 直至铋 (Z=83)。总体而言,反应速率为α提供了 4359 个靶核的诱导反应,涵盖了从质子到中子滴管的中子缺乏和中子含量极高的靶核。与之前的汇率汇编相反,这些新的计算包括所有相关的退出渠道,其中占主导地位的是(α, xn) 富中子靶核的反应。

更新日期:2021-10-04
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