Measurement of γ detector backgrounds in the energy range of 3-8 MeV at Jinping underground laboratory for nuclear astrophysics

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 chann...

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Bibliographic Details
Published in:	Science China. Physics, mechanics & astronomy Vol. 60; no. 10; pp. 63 - 66
Main Authors:	Shen, YangPing, Su, Jun, Liu, WeiPing, Lian, Gang, Gan, Lin, Qiao, LvHua, Yan, ShengQuan, Zhou, Yong, Yue, Qian, Zeng, Zhi, Hu, QingDong, Mi, YuHao, Zhao, Wei
Format:	Journal Article
Language:	English
Published:	Beijing Science China Press 01-10-2017 Springer Nature B.V
Subjects:	Astronomy Classical and Continuum Physics Letter to the Editor Nuclear astrophysics Observations and Techniques Physics Physics and Astronomy γ探测器反应速率地下实验室总横截面核天体物理测量电子能量范围
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Summary:	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：
Bibliography:	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 11-5849/N
ISSN:	1674-7348 1869-1927
DOI:	10.1007/s11433-017-9049-3