摘要
The astrophysical reaction rate of the charged-particleinduced reaction is dominated by the cross section within the Gamow window.The total cross section σ(E)of a chargedparticle-induced reaction is known to drops steeply with decreasing energy owing to the Coulomb barrier in the entrance channel:
The astrophysical reaction rate of the charged-particleinduced reaction is dominated by the cross section within the Gamow window. The total cross section o-（E） of a charged- particle-induced reaction is known to drops steeply with decreasing energy owing to the Coulomb barrier in the entrance channel：
基金
the National Natural Science Foundation of China(Grant Nos.11490560,and 11321064)
the National Basic Research Program of China(Grant No.2013CB834406)
