Capture cross sections of ^(15)N(n,γ)^(16)N at astrophysical energies

作     者：樊广伟 马军兵 圣宗强 石国柱 田丰 王军 张超 Guang-Wei Fan Jun-Bing Ma Zong-Qiang Sheng Guo-Zhu Shi Feng Tian Jun Wang Chao Zhang

作者机构：School of Chemical Engineering Anhui University of Science and Technology Institute of Modern Physics Chinese Academy of Sciences Shanghai Institute of Applied Physics Chinese Academy of Sciences 

出 版 物：《Chinese Physics C》 (中国物理C（英文版）)

年 卷 期：2016年第40卷第12期

页      面：65-68页

核心收录：

学科分类：0709[理学-地质学] 07[理学] 0708[理学-地球物理学] 0804[工学-仪器科学与技术] 070401[理学-天体物理] 0827[工学-核科学与技术] 0703[理学-化学] 0704[理学-天文学] 0702[理学-物理学] 

基　　金：Support given by National Natural Science Foundation of China(11447236,11505002,11247001) Foundation of Anhui University of Science and Technology(11130,12608) 

主　　题：capture cross sections reaction cross sections 15N(n γ)16N Glauber model direct capture 

摘      要：We have reanalyzed reaction cross sections of 16N on a 12C target. The nucleon density distribution of 16N, especially surface density distribution, was extracted using the modified Glauber model. On the basis of dilute surface densities, the 15N（n, γ）16N reaction is discussed within the framework of the direct capture reaction mechanism. The calculations agree quite well with the experimental data.