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17O(p,α)14N reaction measurement at astrophysical energies
- Source :
- AIP Conference Proceedings.
- Publication Year :
- 2014
- Publisher :
- AIP Publishing LLC, 2014.
-
Abstract
- The 17O(p,α)14N reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the 17O(p,α)14N reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of narrow resonance in the ultra-low energy region.
- Subjects :
- Physics
Stars
Supernova
Nucleosynthesis
0202 electrical engineering, electronic engineering, information engineering
Nuclear astrophysics
Resonance
Asymptotic giant branch
020206 networking & telecommunications
020201 artificial intelligence & image processing
02 engineering and technology
Astrophysics
Resonance strength
Subjects
Details
- ISSN :
- 0094243X
- Database :
- OpenAIRE
- Journal :
- AIP Conference Proceedings
- Accession number :
- edsair.doi...........65436876193c6141e8cb44100c35963d
- Full Text :
- https://doi.org/10.1063/1.4875312