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International audienceThe 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 ERc.m. = 183 keV play a significant role in the reaction rate determination

Indirect measurement of17O(p,α)14N cross section at ultra-low energies

Indirect measurement of¹⁷O(p,α)¹⁴N cross section at ultra-low energies