跳到主要导航 跳到搜索 跳到主要内容

Determination of astrophysical nuclear reaction rates using light neutron-rich RNBs

  • H. Ishiyama
  • , T. Hashimoto
  • , T. Ishikawa
  • , K. Yamaguchi
  • , Y. X. Watanabe
  • , Y. Hirayama
  • , N. Imai
  • , H. Miyatake
  • , M. H. Tanaka
  • , N. Yoshikawa
  • , S. C. Jeong
  • , Y. Fuchi
  • , T. Nomura
  • , I. Katayama
  • , H. Kawakami
  • , S. Arai
  • , M. Okada
  • , M. Oyaizu
  • , S. Mitsuoka
  • , A. Osa
  • T. K. Sato, K. Nishio, M. Matsuda, S. Ichikawa, H. Ikezoe, Y. Mizoi, S. K. Das, T. Fukuda, T. Shimoda, K. Otsuki, T. Kajino
  • High Energy Accelerator Research Organization, Tsukuba
  • The University of Tokyo
  • University of Tsukuba
  • Japan Atomic Energy Agency
  • Osaka Electro-Communication University
  • The University of Osaka
  • GSI Helmholtz Centre for Heavy Ion Research
  • National Astronomical Observatory of Japan

科研成果: 期刊稿件会议文章同行评审

摘要

Excitation functions of 8Li(α, n), (d, t) and 12B(α, n) reactions were directly measured in the energy region of astrophysical interest using low-energy radioactive nuclear beams of 8Li and 12B. Each measured excitation function is strongly affected by one or more resonances through a compound nucleus. The measured excitation functions are presented. Dominant r-process paths through 8Li at various temperatures are discussed and our future experimental plan is also presented.

源语言英语
期刊Proceedings of Science
出版状态已出版 - 2008
已对外发布
活动10th Symposium on Nuclei in the Cosmos, NIC 2008 - Mackinac Island, MI, 美国
期限: 27 7月 20081 8月 2008

学术指纹

探究 'Determination of astrophysical nuclear reaction rates using light neutron-rich RNBs' 的科研主题。它们共同构成独一无二的学术指纹。

引用此