| Issue |
EPJ Web Conf.
Volume 297, 2024
International Symposium on Nuclear Astrophysics (ISNA23)
|
|
|---|---|---|
| Article Number | 01017 | |
| Number of page(s) | 5 | |
| Section | Lectures | |
| DOI | https://doi.org/10.1051/epjconf/202429701017 | |
| Published online | 07 June 2024 | |
https://doi.org/10.1051/epjconf/202429701017
Nuclear Astrophysics with Exotic Beam; Thick-target Measurements at CRIB
1 Center for Nuclear Study (CNS), University of Tokyo, Wako, Japan
2 China Institute of Atomic Energy, Beijing, China
3 School of Nuclear Science and Technology, Lanzhou University, Lanzhou, China
4 Center for Exotic Nuclear Studies, Institute for Basic Science, Daejeon, Republic of Korea
5 Department of Physics, Ewha Womans University, Seoul, Republic of Korea
6 Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, China
* e-mail: yamag@cns.s.u-tokyo.ac.jp
Published online: 7 June 2024
Astrophysical reactions involving radioactive isotopes (RI) often play an important role in high-temperature stellar environments. The experimental information on those reactions is still limited mainly due to the technical difficulties in producing high-quality and intense RI beams. Although a direct measurement of those reactions at astrophysical energy would be still challenging, we may take several alternative approaches to determine the reaction rates, by applying other mesurement methods or improving the target and detectors. Here we mainly discuss the thick-target method in inverse kinematics (TTIK) based on the successful examples of experimental studies performed at Center for Nuclear Study, the University of Tokyo, using the low-energy RI beam separator CRIB.
© The Authors, published by EDP Sciences, 2024
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