Astrophysical reaction rates of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e6953" altimg="si202.svg"><mml:mi>α</mml:mi></mml:math>-induced reactions for nuclei with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e6958" altimg="si8.svg"><mml:mrow><mml:mn>26</mml:mn><mml:mo linebreak="goodbreak" linebreakstyle="after">≤</mml:mo><mml:mi>Z</mml:mi><mml:mo linebreak="goodbreak" linebreakstyle="after">≤</mml:mo><mml:mn>83</mml:mn…
نویسندگان
چکیده
The new Atomki-V2 α-nucleus potential is applied to calculate astrophysical reaction rates NA〈σv〉 of intermediate mass and heavy target nuclei from iron (Z=26) up bismuth (Z=83). Overall, α-induced reactions are provided for 4359 nuclei, covering as well neutron-deficient extremely neutron-rich the proton neutron dripline. Contrary previous rate compilations, these calculations include all relevant exit channels with dominating (α, xn) nuclei.
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ژورنال
عنوان ژورنال: Atomic Data and Nuclear Data Tables
سال: 2021
ISSN: ['0092-640X', '1090-2090']
DOI: https://doi.org/10.1016/j.adt.2021.101453