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Nuclear astrophysics projects at the low-energy RI beam separator CRIB
- Authors
- Yamaguchi, H.; Kahl, D.; Hayakawa, S.; Yang, L.; Shimizu, H.; Sakaguchi, Y.; Abe, K.; Nakao, T.; Suhara, T.; Iwasa, N.; Kim, A.; Kim, D. H.; Cha, S. M.; Kwag, M. S.; Lee, J. H.; Lee, E. J.; Chae, K. Y.; Wakabayashi, Y.; Imai, N.; Kitamura, N.; Lee, P.; Moon, J. Y.; Lee, K. B.; Akers, C.; Jung, H. S.; Duy, N. N.; Khiem, L. H.; Lee, C. S.; Hashimoto, T.; Kubono, S.; Kawabata, T.; Teranishi, T.; Kwon, Y. K.; Binh, D. N.
- Issue Date
- Dec-2017
- Publisher
- E D P SCIENCES
- Citation
- NUCLEAR PHYSICS IN ASTROPHYSICS VIII (NPA8 2017), v.165
- Journal Title
- NUCLEAR PHYSICS IN ASTROPHYSICS VIII (NPA8 2017)
- Volume
- 165
- ISSN
- 2100-014X
- Abstract
- Studies on nuclear reactions relevant for astrophysics have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study (CNS), the University of Tokyo. A type of measurement to study astrophysical reactions at CRIB is by the elastic resonant scattering with the thick-target method in inverse kinematics. We introduce the alpha resonant scattering with Be-7 beam, related to the astrophysical Be-7(alpha,gamma) reactions, which is relevant in the hot p-p chain and nu p-process in supernovae. Other alpha resonant scattering measurements with S-30, Be-10, O-15, and Ne-18 beams have been performed at CRIB, using the thick-target method.
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Collections - College of Natural Sciences > Department of Physics > 1. Journal Articles
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