Nuclear structure and astrophysics
Nuclear structure and astrophysics
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DOI：
10.1088/0034-4885/70/9/r02
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发表时间：
2007-08
影响因子：
18.1
通讯作者：
H. Grawe;K. Langanke;G. Martínez-Pinedo
中科院分区：
文献类型：
--
作者：
H. Grawe;K. Langanke;G. Martínez-Pinedo
本文评述了塞格雷星表中具有天体物理重要性的区域的核结构。主要的重点是放在那些核是相关的恒星核合成融合过程中，在慢中子捕获，都位于接近稳定，快速中子捕获接近中子滴线和快速质子捕获质子滴线附近。现代核结构的基本特征，它们的重要性和未来的潜力，天体物理学和它们的可预测性水平进行了批判性的讨论。最近的实验和理论结果壳演化远离稳定线和后果弱相互作用过程，质子和中子捕获的评论。
The nuclear structure in regions of the Segré chart which are of astrophysical importance is reviewed. The main emphasis is put on those nuclei that are relevant for stellar nucleosynthesis in fusion processes, and in slow neutron capture, both located close to stability, rapid neutron capture close to the neutron dripline and rapid proton capture near the proton dripline. The basic features of modern nuclear structure, their importance and future potential for astrophysics and their level of predictibility are critically discussed. Recent experimental and theoretical results for shell evolution far off the stability line and consequences for weak interaction processes, proton and neutron capture are reviewed.