Abstract
Motivated by the need of spectroscopic data to better understand the astrophysical rp-process, we developed a new experimental method using the Grand Raiden magnet spectrometer to study protin rich nuclei with α and 3He induced reactions. First results of the 24Mg( 4He, 6He) 22Mg reaction at 206 MeV and 0° are presented, showing states relevant for resonant reaction rate calculations of the proton capture 21Na(p,γ) 22Mg and the 18Ne(α,p) 21Na reaction which controls the break-out of the hot CNO cycles at X-ray burst conditions.
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