EPJ Web Conf.
Volume 165, 2017Nuclear Physics in Astrophysics VIII (NPA8 2017)
|Number of page(s)||4|
|Published online||30 December 2017|
Nuclear astrophysics projects at the low-energy RI beam separator CRIB
1 Center for Nuclear Study (CNS), University of Tokyo, RIKEN campus, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
2 School of Physics and Astronomy, the University of Edinburgh, Peter Guthrie Tait Road, Edinburgh EH9 3BF, UK
3 China Institute of Atomic Energy, P.O. Box 275(10), Beijing 102413, China
4 Advanced Science Research Center, Japan Atomic Energy Agency, Tokai, Ibaraki 319-1195, Japan
5 Matsue College of Technology, Matsue, Shimane 690-8518, Japan
6 Department of Physics, Tohoku University, Aoba, Sendai, Miyagi 980-8578, Japan
7 Department of Physics, Sungkyunkwan University, 2066 Seobu-ro, Jangan-gu, Suwon, Korea
8 Department of Physics, Ewha Womans University, Seoul 120-750, Korea
9 The Institute of Physical and Chemical Research (RIKEN), 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
10 Department of Physics, Chung-Ang University, Seoul 156-756, Korea
11 Institute for Basic Science, 70, Yuseong-daero 1689-gil, Yuseong-gu, Daejeon 305-811, Korea
12 Wako Nuclear Science Center (WNSC), KEK, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
13 Institute of Physics, Vietnam Academy of Science and Technology, 10 Dao Tan, Ba Dinh, Hanoi, Vietnam
1 Dong Nai University, Le Quy Don Street, Tan Hiep Ward, Bien Hoa City, Dong Nai, Vietnam
1 Department of Physics, Kyoto University, Kita-Shirakawa, Kyoto 606-8502, Japan
1 Department of Physics, Kyushu University, 6-10-1 Hakozaki, Fukuoka 812-8581, Japan
1 30 MeV Cyclotron Center, Tran Hung Dao Hospital, Hoan Kiem District, Hanoi, Vietnam
* e-mail: firstname.lastname@example.org
Published online: 30 December 2017
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 α resonant scattering with 7Be beam, related to the astrophysical 7Be(α, γ) reactions, which is relevant in the hot p-p chain and νp-process in supernovae. Other α resonant scattering measurements with 30S, 10Be, 15O, and 18Ne beams have been performed at CRIB, using the thick-target method.
© The Authors, published by EDP Sciences, 2017
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