A new astrophysical reaction rate for 12 C( α , γ ) 16 O has been evaluated on the basis of a global R -matrix fitting to the available experimental data. The reaction rates of 12 C( α , γ ) 16 O for stellar temperatures between 0.04 ≤ T 9 ≤ 10 are provided in a tabular form and by an analytical fitting expression. At T 9 = 0.2, the reaction rate is (7.83 ± 0.35) × 10 15 cm 3 mol −1 s −1 , where stellar helium burning occurs.
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An et al. (2016) studied this question.
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