52 citations · 136 across the 9 of their papers we have counts for
9 papers
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).…
Measurement of F(,)Ne reaction suggests CNO break-out in first stars
Liyong Zhang, Jianjun He, Richard J. deBoer +33
The origin of calcium production in the first stars (Pop III stars), which formed out of the primordial matter of the Big Bang, and their fates, remain most fascinating mysteries i…
Temperature of the hot -source: a guidance to probe the Bose-Einstein condensation of clusters in the heavy-ion collision
Jun Su, Long Zhu
Recent experimental efforts were made to explore the Bose-Einstein condensation in multi- system using the heavy-ion collisions. This Letter provides a explanation why no signat…
Transport Model Comparison Studies of Intermediate-Energy Heavy-Ion Collisions
Hermann Wolter, Maria Colonna, Dan Cozma +49
Transport models are the main method to obtain physics information from low to relativistic-energy heavy-ion collisions. The Transport Model Evaluation Project (TMEP) has been purs…
Examination of the role of the O(,)F reaction rate in type I x-ray bursts
J. Hu, J. J. He, A. Parikh +17
The O(,)F reaction is one of the key reactions involved in the breakout from the hot-CNO cycle to the rp-process in type I x-ray bursts (XRBs). The resonant pro…
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…
A confirmative spin-parity assignment for the key 6.15 MeV state in Ne of astrophysical importance
J. Hu, J. J. He, S. W. Xu +14
Proton resonant states in Ne have been investigated by the resonant elastic scattering of F+. The F beam was separated by the CNS radioactive ion beam separ…
Determination of astrophysical 12N(p,g)13O reaction rate from the 2H(12N, 13O)n reaction and its astrophysical implications
B. Guo, J. Su, Zhihong Li +20
The evolution of massive stars with very low-metallicities depends critically on the amount of CNO nuclides which they produce. The N(,\,)O reaction is an impor…
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…