Abstract
Studies on nuclear astrophysics and nuclear structure have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam separator CRIB of the University of Tokyo. Recent studies on astrophysical reactions in high-temperature stellar environments at CRIB are discussed. We conducted a series of \(\alpha \) resonant scattering measurements with RI beams and the thick-target method, mainly to evaluate astrophysical reaction rates of \(\alpha \)-induced reactions. Experimental projects based on other experimental techniques, such as the Trojan horse method or RI-implanted target, are also ongoing.
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Acknowledgements
The experiments were performed at RI Beam Factory operated by RIKEN Nishina Center and CNS, the University of Tokyo. We are grateful to the RIKEN and CNS accelerator staff for their help. This work was partly supported by JSPS KAKENHI (Nos. 15K17662, 16K05369, and 16H03980) from the Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan.
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Yamaguchi, H., Hayakawa, S., Yang, L., Shimizu, H., Kahl, D., CRIB Collaboration. (2019). Study on Explosive Nucleosynthesis with Low-Energy RI Beams at CRIB. In: Formicola, A., Junker, M., Gialanella, L., Imbriani, G. (eds) Nuclei in the Cosmos XV. Springer Proceedings in Physics, vol 219. Springer, Cham. https://doi.org/10.1007/978-3-030-13876-9_44
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