Year-end Sale % OFF 
Abstract
ABSTRACT A new astrophysical reaction rate for 12C(α, γ)16O has been evaluated on the basis of a global R-matrix fitting to the available experimental data. The reaction rates of 12C(α, γ)16O 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) × 1015 cm3 mol−1 s−1, where stellar helium burning occurs.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
