論文

査読有り
2015年4月

Different mechanism of two-proton emission from proton-rich nuclei Al-23 and Mg-22

PHYSICS LETTERS B
  • Y. G. Ma
  • D. Q. Fang
  • X. Y. Sun
  • P. Zhou
  • Y. Togano
  • N. Aoi
  • H. Baba
  • X. Z. Cai
  • X. G. Cao
  • J. G. Chen
  • Y. Fu
  • W. Guo
  • Y. Hara
  • T. Honda
  • Z. G. Hu
  • K. Ieki
  • Y. Ishibashi
  • Y. Ito
  • N. Iwasa
  • S. Kanno
  • T. Kawabata
  • H. Kimura
  • Y. Kondo
  • K. Kurita
  • M. Kurokawa
  • T. Moriguchi
  • H. Murakami
  • H. Ooishi
  • K. Okada
  • S. Ota
  • A. Ozawa
  • H. Sakurai
  • S. Shimoura
  • R. Shioda
  • E. Takeshita
  • S. Takeuchi
  • W. D. Tian
  • H. W. Wang
  • J. S. Wang
  • M. Wang
  • K. Yamada
  • Y. Yamada
  • Y. Yasuda
  • K. Yoneda
  • G. Q. Zhang
  • T. Motobayashi
  • 全て表示

743
開始ページ
306
終了ページ
309
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.physletb.2015.02.066
出版者・発行元
ELSEVIER SCIENCE BV

Two-proton relative momentum (q(pp)) and opening angle (theta(pp)) distributions from the three-body decay of two excited proton-rich nuclei, namely Al-23 --> p + p + Na-21 and Mg-22 --> p + p + Ne-20, have been measured with the projectile fragment separator (RIPS) at the RIKEN RI Beam Factory. An evident peak at q(pp) similar to 20 MeV/c as well as a peak in theta(pp) around 30 degrees are seen in the two-proton break-up channel from a highly-excited Mg-22. In contrast, such peaks are absent for the Al-23 case. It is concluded that the two-proton emission mechanism of excited Mg-22 is quite different from the Al-23 case, with the former having a favorable diproton emission component at a highly excited state and the latter dominated by the sequential decay process. (C) 2015 The Authors. Published by Elsevier B.V.

リンク情報
DOI
https://doi.org/10.1016/j.physletb.2015.02.066
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000352147500047&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.physletb.2015.02.066
  • ISSN : 0370-2693
  • eISSN : 1873-2445
  • Web of Science ID : WOS:000352147500047

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