Abstract
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 ( E c . m . = 0 − 300 keV ) relevant for several astrophysics environments, where two resonant levels of 18F at E c . m . R = 65 keV and E c . m . R = 183 keV play a significant role in the reaction rate determination.
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