用RI光束进行恒星反应的实验方法-氢燃烧实验概述-
Experimental Approach to Stellar Reactions with RI Beams - Overview of Experiments on Hydrogen Burning -
摘要：
在简要回顾了自上届NN会议以来天体物理学的最新进展之后，重新回顾了以RI束为主的核天体物理学的实验工作，特别是与缺中子核有关的工作，这是由Reynam在这次会议上回顾的核图表的另一半。在过去的几年里，人们讨论了一个新的有趣的认识，即爆发性氢燃烧过程在II型超新星极早期阶段的重要作用。还讨论了从观测和核天体物理学两方面对第一代恒星进行研究的一个新的、不断扩大的研究领域。
英文摘要：
After a short review on resent developments achieved in astrophysics in the past years since last NN conference, experimental efforts in nuclear astrophysics primarily with RI beams were revisited, especially on the works relevant to neutron-deficient nuclei, the other half of the nuclear chart reviewed by Rehm in this conference. A new interesting recognition discussed in the past years is the important role of explosive hydrogen burning process in the very early stage of type II supernovae. A new broadening research field related to the first generation stars both from observations as well as from nuclear astrophysics was also discussed.
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。
