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Study of stellar reactions in explosive hydrogen burning with CRIB
- Authors
- Kubono, S.; Teranishi, T.; Notani, M.; Yamaguchi, H.; Saito, A.; He, J.J.; Wakabayashi, M.; Fujikawa, H.; Amadio, G.; Baba, H.; Fukuchi, T.; Shimoura, S.; Michimasa, S.; Nishimura, S.; Nishimura, M.; Gono, Y.; Odahara, A.; Kato, S.; Moon, J.Y.; Lee, J.H.; Lee, C.S.; Kim, J.C.; Hahn, K.I.; Ishikawa, T.; Hashimoto, T.; Ishiyama, H.; Watanabe, Y.X.; Tanaka, M.H.; Miyatake, H.; Fulop, Z.; Guimaraes, V.; Lichtenthaler, R.
- Issue Date
- Jul-2005
- Publisher
- ELSEVIER SCIENCE BV
- Citation
- NUCLEAR PHYSICS A, v.758, no.1-4 SPEC. ISS., pp 733C - 736C
- Journal Title
- NUCLEAR PHYSICS A
- Volume
- 758
- Number
- 1-4 SPEC. ISS.
- Start Page
- 733C
- End Page
- 736C
- ISSN
- 0375-9474
1873-1554
- Abstract
- 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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