Reaction rates for Neutron Capture Reactions to C-, N- and O-isotopes to the neutron rich side of stability

Reaction rates for Neutron Capture Reactions to C-, N- and O-isotopes to the neutron rich side of stability
复制标题

C、N 和 O 同位素的中子俘获反应的反应速率达到稳定的富中子一侧

DOI:
10.1103/physrevc.60.064614
复制
发表时间:
1999
期刊:
影响因子:
3.1
通讯作者:
B. A. Brown
B. A. Brown
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
H. Herndl;R. Hofinger;J. Jank;H. Oberhummer;J. Goerres;M. Wiescher;F. Thielemann;B. A. Brown

文献摘要

被引文献

相似文献

中子俘获轻核反应的反应速率对于可靠地模拟各种恒星场景中的核合成是重要的。在混合化合物和直接俘获模型的框架下,计算了富中子C-、N-和O-同位素的中子俘获反应速率。将结果制成表格,并与以前的计算结果以及与实验结果进行比较。
The reaction rates of neutron capture reactions on light nuclei are important for reliably simulating nucleosynthesis in a variety of stellar scenarios. Neutron capture reaction rates on neutron-rich C-, N-, and O-isotopes are calculated in the framework of a hybrid compound and direct capture model. The results are tabulated and compared with the results of previous calculations as well as with experimental results.