Recent studies indicate that aaa reaction rate is larger than the NACRE compilation. The rate at the temperature of ~0.1GK affects the evolution of the AGB stars, and at the temperature of ~1GK affects the synthesis of light p-nuclei in the supernovae nup-process.
In this workshop, we will discuss,
1. aaa reaction rate
2. Effect of new aaa rate on the evolution of AGB stars and the CNO cycle
3. Effect of new aaa rate on supernovae nup process
4. Future experiments in RIBF related to CNO and nup process
Contact person: Yasuhiro Togano
e-mail: togano at ribf.riken.jp (please change "at" to "@")
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