26 citations · 89 across the 7 of their papers we have counts for
7 papers
Design and commissioning of a windowless gas-target system for high-current beams at JUNA
Xuyang Wang, Fuqiang Cao, Weike Nan +20
Windowless gas targets avoid the beam-energy loss and straggling introduced by entrance foils and are therefore well suited for direct measurements of low-energy nuclear reactions.…
A cryogenic gas target for high-intensity radioactive ion beam production at HIRFL-RIBLL
Xiao Fang, Shiwei Xu, Longhui Ru +21
A liquid-nitrogen-cooled cryogenic gas target system has been developed and installed for radioactive ion beam (RIB) production at the Radioactive Ion Beam Line in Lanzhou (RIBLL).…
New determination of the spectroscopic factor of Be ground state and the Li()Be astrophysical S(E) factors
Zhi-Hong Li, Er-Tao Li, Jun Su +6
The `lithium problem' in Big Bang Nucleosynthesis (BBN) has recently focused on the reactions involving Be. The Li()Be reaction can provide us not only the inform…
A proposed direct measurement of cross section at Gamow window for key reaction F(,)O in Asymptotic Giant Branch stars with a planned accelerator in CJPL
J. J. He, S. W. Xu, S. B. Ma +16
In 2014, the National Natural Science Foundation of China (NSFC) approved the Jinping Underground Nuclear Astrophysics laboratory (JUNA) project, which aims at direct cross-section…
Spectroscopic factors for low-lying 16N levels and the astrophysical 15N(n,gamma)16N reaction rate
B. Guo, Z. H. Li, Y. J. Li +23
Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditions within stars. The astrophysical site to produce fluorine is suggest…
Neutron spectroscopic factors of 7Li and astrophysical 6Li(n,g)7Li reaction rates
Jun Su, Zhihong Li, Bing Guo +12
Angular distributions of the 7Li(6Li,6Li)7Li elastic scattering and the 7Li(6Li,7Li_{g.s.})6Li, 7Li(6Li,7Li*_{0.48})6Li transfer reactions at Ec.m. = 23.7 MeV were measured with th…
The 13N(d,n)14O Reaction and the Astrophysical 13N(p,g)14O Reaction Rate
Z. H. Li, B. Guo, S. Q. Yan
N()O is one of the key reactions in the hot CNO cycle which occurs at stellar temperatures around 0.1. Up to now, some uncertainties still exist for…