The 17F( p,γ)18Ne reaction at stellar energies
✍ Scribed by M. Dufour; P. Descouvemont
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 248 KB
- Volume
- 730
- Category
- Article
- ISSN
- 0375-9474
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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
The energy averaged (n, c) cross sections of 58 Ni and 78 Se at a stellar energy of kT = 25 keV have been investigated with the so called activation technique, which represents a well established tool for measurements of stellar neutron cross sections. For both nuclides, offline decay counting is pr