Astrophysical reaction rate of 30S(p, γ)31Cl studied by Coulomb dissociation

Y. Togano, T. Motobayashi, N. Aoi, H. Baba, S. Bishop, X. Cai, P. Doornenbal, D. Fang, T. Furukawa, K. Ieki, N. Iwasa, T. Kawabata, S. Kanno, N. Kobayashi, Y. Kondo, T. Kuboki, N. Kume, K. Kurita, M. Kurokawa, Y. G. MaY. Matsuo, H. Murakami, M. Matsushita, T. Nakamura, K. Okada, S. Ota, Y. Satou, S. Shimoura, R. Shioda, K. N. Tanaka, S. Takeuchi, W. Tian, H. Wang, J. Wang, K. Yamada, Y. Yamada, K. Yoneda

Research output: Contribution to journalConference articlepeer-review

Fingerprint

Dive into the research topics of 'Astrophysical reaction rate of <sup>30</sup>S(p, γ)<sup>31</sup>Cl studied by Coulomb dissociation'. Together they form a unique fingerprint.

Physics & Astronomy