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Astrophysical S factors determined from asymptotic normalization coefficients measured in peripheral transfer reactions

โœ Scribed by C.A. Gagliardi; A. Azhari; V. Burjan; F. Carstoiu; V. Kroha; A.M. Mukhamedzhanov; X. Tang; L. Trache; R.E. Tribble


Publisher
Elsevier Science
Year
2001
Tongue
English
Weight
162 KB
Volume
688
Category
Article
ISSN
0375-9474

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โœ A.M Mukhamedzhanov; A Azhari; V Burjan; C.A Gagliardi; V Kroha; A Sattarov; X Ta ๐Ÿ“‚ Article ๐Ÿ“… 2003 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 198 KB

The 13 C(p, ฮณ ) 14 N radiative capture reaction is analyzed within the R-matrix approach with the aim to determine the astrophysical S factor. The low-energy astrophysical S factor has important contributions from both resonant and nonresonant captures. The contribution of the nonresonant component