Three-Body Calculation of 4He（αα,γ）12C Reaction at Stellar Energies

作     者：Firoozabadi M. M. Sadeghi H. 

作者机构：Department of Physics University of Birjand Birjand Iran Department of Physics Faculty of Science Arak University Arak 8349-8-38156 Iran 

出 版 物：《Chinese Physics Letters》 (中国物理快报（英文版）)

年 卷 期：2015年第32卷第7期

页      面：25-28页

核心收录：

学科分类：07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

基　　金：Supported by the University of Birjand 

主　　题：Three-Body Calculation of C Reaction at Stellar Energies 

摘      要：The triple-alpha reaction is the key to our understanding about the nucleosynthesis and the observed abundance of 12C in stars. On the basis of our model, the triple-alpha radiative capture process is studied by using the three-body Faddeev approach as well as two- and three-body electromagnetic currents. The bound and resonance states of 12 C are calculated via an inverse process： three-a photodisintegration of a 12 C nucleus.