MISC

2005年7月

Study of stellar reactions in explosive hydrogen burning with CRIB

NUCLEAR PHYSICS A
  • S Kubono
  • ,
  • T Teranishi
  • ,
  • M Notani
  • ,
  • H Yamaguchi
  • ,
  • A Saito
  • ,
  • JJ He
  • ,
  • M Wakabayashi
  • ,
  • H Fujikawa
  • ,
  • G Amadio
  • ,
  • H Baba
  • ,
  • T Fukuchi
  • ,
  • S Shimoura
  • ,
  • S Michimasa
  • ,
  • S Nishimura
  • ,
  • M Nishimura
  • ,
  • Y Gono
  • ,
  • A Odahara
  • ,
  • S Kato
  • ,
  • JY Moon
  • ,
  • JH Lee
  • ,
  • CS Lee
  • ,
  • JC Kim
  • ,
  • KI Hahn
  • ,
  • T Ishikawa
  • ,
  • T Hashimoto
  • ,
  • H Ishiyama
  • ,
  • YX Watanabe
  • ,
  • MH Tanaka
  • ,
  • H Miyatake
  • ,
  • Z Fulop
  • ,
  • Guimaraes, V
  • ,
  • R Lichtenthaler

758
開始ページ
733C
終了ページ
736C
記述言語
英語
掲載種別
DOI
10.1016/j.nuclphysa.2005.05.132
出版者・発行元
ELSEVIER SCIENCE BV

With using low-energy RI beams from an in-flight RIB separator, CRIB, the most crucial stellar reaction O-14(alpha,p)F-17 for the onset of the high-temperature rp-process was directly investigated and the transitions through the states at around 6.2 MeV in Ne-18 were first observed, confirming the importance predicted before. The (alpha,p) reaction leading to the first excited state in F-17 was also found to have a large contribution. A proton resonance search experiment of Mg-23 + p was also discussed, which is a part of our series of resonance search studies relevant to the early stage of the rp-process.


リンク情報
DOI
https://doi.org/10.1016/j.nuclphysa.2005.05.132
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000230660500159&DestApp=WOS_CPL

エクスポート
BibTeX RIS