Experimental study of the key astrophysical 18Ne(α, p)21Na reaction

L. Y. Zhang, J. J. He, S. W. Xu, H. Yamaguchi, S. Kubono, Y. Wakabayashi, S. Z. Chen, J. Hu, P. Ma, Y. Togano, T. Hashimoto, D. Kahl, T. Teranishi, R. F. Chen, H. W. Wang, W. D. Tian, B. Guo, S. Hayakawa, N. Iwasa, T. YamadaT. Komatsubara

研究成果: Contribution to journalConference article査読

抄録

The 18Ne(α, p)21Na reaction is thought to be one of the key breakout reaction from the hot CNO cycle to the rp-process in X-ray bursts. We investigated the resonant properties of the compound nucleus 22Mg by measuring the resonant elastic scattering of 21Na+p. An 89 MeV 21Na radioactive beam was produced by CRIB and then bombarded a 93-μm-thick polyethylene target. The 21Na beam intensity was about 2× 105 pps, with a purity of about 70% on the target. The recoiled protons were measured by three sets of ΔE-E telescope respectively. A wide excitation energy range of 5.5-9.2 MeV in 22Mg was scanned with a thick-target method. Some preliminary results are shown.

本文言語英語
ジャーナルProceedings of Science
出版ステータス出版済み - 12 1 2012
イベント12th International Symposium on Nuclei in the Cosmos, NIC 2012 - Cairns, QLD, オーストラリア
継続期間: 8 5 20128 12 2012

All Science Journal Classification (ASJC) codes

  • 一般

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