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作 者:HOU Su-qing CHEN Yong-shou WU Kai-su SHU Neng-chuan LI Zhi-hong
机构地区:[1]不详 [2]Beijing University of Chemical Technology, Beijing 100029, China
出 处:《Annual Report of China Institute of Atomic Energy》2009年第1期145-146,共2页中国原子能科学研究院年报(英文版)
基 金:Supported by National Natural Science Foundation of China(10447141,10775182);Major State Basic Research Development Program of China(2007CB815000);Youth Foundation of Beijing University of Chemical Technology(QN0622)
摘 要:Recently,the synthesis of CNO elements in BBN has attracted a great attention since the physics of stars formed from the collapse of the very first structure in the Universe may strongly depend onRecently, the synthesis of CNO elements in BBN has attracted a great attention since the physics of stars formed from the collapse of the very first structure in the Universe may strongly depend on the chemical composition of the clouds[1]. The present study reports a new important reaction chain which provides the main channel for production of CNO elements in standard BBN.
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