- ELSEVIER SCIENCE BV
With using low-energy RI beams from an in-flight RIB separator, CRIB, the most crucial stellar reaction O-14(alpha,p)F-17 for the onset of the high-temperature rp-process was directly investigated and the transitions through the states at around 6.2 MeV in Ne-18 were first observed, confirming the importance predicted before. The (alpha,p) reaction leading to the first excited state in F-17 was also found to have a large contribution. A proton resonance search experiment of Mg-23 + p was also discussed, which is a part of our series of resonance search studies relevant to the early stage of the rp-process.
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