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 dr...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:展开更多
基金the National Natural Science Foundation of China(Grant Nos.11490560,and 11321064)the National Basic Research Program of China(Grant No.2013CB834406)
文摘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: