Abstract
The cross section for the 18F(p,α) 15O reaction has been obtained in reverse kinematics ( 18F beam on CH 2 target) between 550 and 740 keV above threshold, i.e. in a region of astrophysical interest. The reaction yield is dominated by a wide resonant state whose spin, parity, total width and partial widths were deduced from the analysis of the α-particle and elastic proton data.
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