Reactions with radioactive beams and explosive nucleosynthesis

被引:69
作者
Wiescher, M [1 ]
Schatz, H
Champagne, AE
机构
[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[2] Univ N Carolina, Dept Phys, Chapel Hill, NC USA
[3] Duke Univ, Triangle Univ Nucl Lab, Durham, NC USA
来源
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | 1998年 / 356卷 / 1744期
关键词
nucleosynthesis; supernovae; r-process; radioactive beam; luminosity;
D O I
10.1098/rsta.1998.0265
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
This paper summarizes our present understanding of nuclear reactions with short-lived particles, which are relevant for the nucleosynthesis and energy generation in explosive stellar scenarios. It discusses the need for data on reactions far off stability and presents a short description of the present possibilities for measurements with radioactive beams. The paper presents an overview of the nucleosynthesis aspects for different explosive burning scenarios. The possible influence of proton capture reactions on short-lived nuclei are discussed for explosive hydrogen burning in novae and X-ray bursts. Also discussed are various aspects of weak-interaction processes during the collapse phase of a type-II supernova. Finally, we present key reactions for the onset of the cr recombination in the neutrino-driven shock of type-II supernovae, and discuss nuclear structure effects for the r-process path.
引用
收藏
页码:2105 / 2136
页数:32
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