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

Abstract

The Coulomb dissociation of the proton-rich nucleus 31Cl was studied experimentally using a 31Cl beam at 58 MeV/nucleon with a lead target. The relative energy spectrum between 30S ions and protons was obtained from the measured momentum vectors of the reaction products detected in coincidence by the invariant mass method. The first excited state in 31Cl was observed which is relevant to the resonant capture in the stellar 30S(p, γ)31Cl reaction. Discussion for another observed state is also given.

Original languageEnglish
JournalProceedings of Science
Publication statusPublished - 2010
Event11th Symposium on Nuclei in the Cosmos, NIC 2010 - Heidelberg, Germany
Duration: 2010 Jul 192010 Jul 23

ASJC Scopus subject areas

  • General

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.

Cite this