The shell model embedded in the continuum is applied to calculate the astrophysical S-factor and the reaction rate for the radiative proton capture reaction 17 F(p, γ ) 18 Ne. The dominant contribution to the cross-section at very low-energies is due to M1 transitions J π i = 2 + → J π f = 2 + 1 who
✦ LIBER ✦
The 17F(p, γ)18Ne direct capture cross section
✍ Scribed by J.C. Blackmon; D.W. Bardayan; C.R. Brune; F. Carstoiu; A.E. Champagne; R. Crespo; T. Davinson; J.C. Fernandes; C.A. Gagliardi; U. Greife; C.J. Gross; P.A. Hausladen; C. Iliadis; C.C. Jewett; R.L. Kozub; T.A. Lewis; F. Liang; B.H. Moazen; A.M. Mukhamedzhanov; C.D. Nesaraja; F.M. Nunes; P.D. Parker; D.C. Radford; L. Sahin; J.P. Scott; D. Shapira; M.S. Smith; J.S. Thomas; L. Trache; R.E. Tribble; P.J. Woods; C.-H. Yu
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 153 KB
- Volume
- 746
- Category
- Article
- ISSN
- 0375-9474
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