𝔖 Bobbio Scriptorium
✦   LIBER   ✦

New determination of the astrophysical13C( p, γ)14N S(E) factors and reaction rates via the13C(7Li,6He)14N reaction

✍ Scribed by Y. J. Li; Z. H. Li; E. T. Li; X. X. Bai; J. Su; B. Guo; B. X. Wang; S. Q. Yan; S. Zeng; Z. C. Li; J. C. Liu; X. Liu; S. J. Jin; Y. B. Wang; L. Y. Zhang; X. Q. Yu; L. Li; G. Lian; Q. W. Fan; W. P. Liu


Book ID
119983530
Publisher
Springer
Year
2012
Tongue
English
Weight
818 KB
Volume
48
Category
Article
ISSN
1434-601X

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


Asymptotic normalization coefficients fr
✍ A.M Mukhamedzhanov; A Azhari; V Burjan; C.A Gagliardi; V Kroha; A Sattarov; X Ta 📂 Article 📅 2003 🏛 Elsevier Science 🌐 English ⚖ 198 KB

The 13 C(p, γ ) 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

New determinations of gamma-ray line int
✍ J Kiener; M Gros; V Tatischeff; D Attié; I Bailly; A Bauchet; C Chapuis; B Cordi 📂 Article 📅 2004 🏛 Elsevier Science 🌐 English ⚖ 539 KB

Gamma-ray angular distributions for the resonances at E p =550 and 1747 keV of the radiative capture reaction 13 C(p,g) 14 N have been measured, using intense proton beams on isotopically pure 13 C targets. Experimental gamma-ray spectra were obtained with three HP-Germanium detectors at four angles