arXivDaily arXiv每日学术速递 周一至周五更新
arXiv周末暂无论文更新,休息一下吧,周末愉快~~
arXiv 1010.4928nucl-ex
收藏

30秒束流发展与X射线爆发

30S Beam Development and X-ray Bursts

D. Kahl, A. A. Chen, S. Kubono, D. N. Binh, J. Chen, T. Hashimoto, S. Hayakawa, D. Kaji, A. Kim, Y. Kurihara, N. H. Lee, S. Nishimura, Y. Ohshiro, K. Setoodeh n… 展开作者

D. Kahl, A. A. Chen, S. Kubono, D. N. Binh, J. Chen, T. Hashimoto, S. Hayakawa, D. Kaji, A. Kim, Y. Kurihara, N. H. Lee, S. Nishimura, Y. Ohshiro, K. Setoodeh nia, Y. Wakabayashi, H. Yamaguchi

摘要:

在过去的三年里,我们一直致力于开发一个良好的特点30 S放射性核束,用于未来的实验,旨在直接测量30 S(α,p)恒星反应速率的伽莫夫窗口内的I型X射线爆发。讨论了~(30)S(α,p)反应对X射线爆发的重要性。鉴于天体物理学的动机,成功的结果和挑战涉及生产的低能量30 S光束进行了详细说明。最后,我们的未来计划的概述,关于这个正在进行的项目。

英文摘要:

Over the past three years, we have worked on developing a well-characterized 30S radioactive beam to be used in a future experiment aiming to directly measure the 30S(alpha,p) stellar reaction rate within the Gamow window of Type I X-ray bursts. The importance of the 30S(alpha,p) reaction to X-ray bursts is discussed. Given the astrophysical motivation, the successful results of and challenges involved in the production of a low-energy 30S beam are detailed. Finally, an overview of our future plans regarding this on-going project are presented.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑