The indirect measurement of O-17(p,alpha)N-14 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 F-18 at E-c.m.(R) = 65 keV and E-c.m.(R) = 183 keV play a significant role in the reaction rate determination.
|Titolo:||The 65 keV resonance in the O-17(p,alpha)N-14 thermonuclear reaction|
|Data di pubblicazione:||2010|
|Appare nelle tipologie:||1.1 Articolo in rivista|