P o S ( N I C X I ) 2 2 8 Astrophysical reaction rate of 30 S ( p , γ ) 31 Cl studied by Coulomb dissociation

Y. Togano ∗1, T. Motobayashi 1, N. Aoi 1, H. Baba1, S. Bishop 1, X. Cai2, P. Doornenbal 1, D. Fang2, T. Furukawa 1, K. Ieki 3, N. Iwasa4, T. Kawabata 5, S. Kanno 1, N. Kobayashi 6, Y. Kondo 1, T. Kuboki 7, N. Kume 4, K. Kurita 3, M. Kurokawa 1, Y. G. Ma2, Y. Matsuo 1, H. Murakami 1, M. Matsushita 3, T. Nakamura 6, K. Okada 3, S. Ota5, Y. Satou 6, S. Shimoura 5, R. Shioda 3, K. N. Tanaka 6, S. Takeuchi 1, W. Tian2, H. Wang2, J. Wang 8, K. Yamada 1, Y. Yamada3, and K. Yoneda 1 1RIKEN Nishina Center, Saitama 351-0198, Japan 2Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China 3Department of Physics, Rikkyo University, Tokyo 171-8501, Japan 4Department of Physics, Tohoku University, Miyagi 980-8578, Japan 5Center for Nuclear Study, University of Tokyo, Saitama 351-0198, Japan 6Department of Physics, Tokyo Institute of Technology, Tokyo 152-8551, Japan 7Department of Physics, Saitama University, Saitama 338-8570, Japan 8Institute of Modern Physics, Chinese Academy of Scienc es, Lanzhou 730000, China