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NEW STELLAR REACTION RATE FOR ~(12)C(α, γ)~(16)O

机译:〜(12)C(α,γ)〜(16)O的新恒星反应速率

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摘要

The ~(12)C(α, γ)~(16)O reaction rate has been reevaluated using recently published cross section estimates. The results suggest that the temperature dependence of the reaction rate as given by Caughlan & Fowler should be revised, even though the absolute cross section of ~(12)C(α, γ)~(16)O still needs a better determination at low energies. Values for the stellar reaction rate of ~(12)C(α, γ)~(16)O have been calculated for a recommended cross section as well as for the experimental upper and lower limits of the cross section. In addition, analytic expressions for these reaction rates are given for 0.03 ≤ T_9 ≤ 2.
机译:〜(12)C(α,γ)〜(16)O反应速率已使用最近发表的截面估计值进行了重新评估。结果表明,即使〜(12)C(α,γ)〜(16)O的绝对截面在低温下仍需要更好的测定,仍应修正Caughlan&Fowler给出的反应速率对温度的依赖性。能量。已针对推荐的横截面以及实验的横截面上限和下限计算了〜(12)C(α,γ)〜(16)O的恒星反应速率值。另外,给出了这些反应速率的解析表达式,其值为0.03≤T_9≤2。

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