https://doi.org/10.1140/epja/i2006-08-050-5
Nuclear Physics in Astrophysics II
Nuclear astrophysics at the east drip line
1
Center for Nuclear Study (CNS), University of Tokyo, Wako Branch at RIKEN, Hirosawa 2-1, 351-0198, Wako, Saitama, Japan
2
Department of Physics, Kyushu University, 812-8581, Fukuoka, Japan
3
Physics Division, Argonne National Laboratory, 60439, IL, USA
4
RIKEN, 351-0198, Saitama, Japan
5
Rikkyo University, 171-0021, Toshima, Tokyo, Japan
6
Nishi-Nippon Institute of Technology, 800-0394, Fukuoka, Japan
7
Department of Physics, Yamagata University, 999-8560, Yamagata, Japan
8
Department of Physics, Chung-Ang University, 156-756, Seoul, Korea
9
Ewha Womens' University, 120-750, Seoul, Korea
10
Institute of Nuclear Research (ATOMKI), H-4001, Debrecen, Hungary
11
Departmento de Fysica Nuclear, Universidade de S ao Paulo, S ao Paulo, Brazil
* e-mail: kubono@cns.s.u-tokyo.ac.jp
Received:
28
June
2005
Accepted:
20
December
2005
Published online:
23
March
2006
In the first half of the paper, the nuclear astrophysics activities in Japan, especially in experimental studies are briefly overviewed. A variety of beams have been developed and used for nuclear astrophysics experiments in Japan. The activities include the RI beam facilities at low energies by the in-flight method at the Center for Nuclear Study (CNS), University of Tokyo and by the ISOL-based method at the JAERI tandem facility, and the RI beam facility at intermediate energies at RIKEN. Other activities include a study of the 12C(α,γ)16O reaction exclusively at the tandem accelerator at the Kyushu University, and studies at the neutron facility at Tokyo Institute of Technology and at the photon facility at AIST (Sanso-ken). Research opportunities in the future at RIBF, J-PARC, and SPRING8 are also discussed. A discussion on the research activities at CNS has been specifically extended in the latter half, including various possibilities in collaboration at the RI beam factory at RIKEN.
PACS: 25.70.Ef Resonances – / 25.60.-t Reactions induced by unstable nuclei – / 26.30.+k Nucleosynthesis in novae, supernovae and other explosive environments – / 29.25.Rm Sources of radioactive nuclei –
© Società Italiana di Fisica and Springer-Verlag, 2006