The indirect measurement of 17O(p,α)14N cross section was performed by means of the Trojan Horse Method. This approach allowed to investigate the ultra-low energy range (Ec.m. 0-300 keV) relevant for several astrophysics environments, where two resonant levels of 18F at ERc.m. 65 keV and ER c.m. 183 keV play a significant role in the reaction rate determination.
ASJC Scopus subject areas
- Physics and Astronomy(all)