67 citations · 243 across the 9 of their papers we have counts for
9 papers
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…
Deep underground laboratory measurement of C(,)O in the Gamow windows of the - and -processes
B. Gao, T. Y. Jiao, Y. T. Li +71
The C(,)O reaction is the main neutron source for the slow-neutron-capture (s-) process in Asymptotic Giant Branch stars and for the intermediate (i-) process.…
Astrophysical factor of the reaction through the transfer reaction
Y. P. Shen, B. Guo, Z. H. Li +20
The reaction plays a key role in the evolution of stars with masses of 0.55 . The cross-section of the ${}^{12}\mathrm{C}(α…
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…
Proton widths of the low-lying 16F states from the 15N(7Li, 6Li)16N reaction
Z. D. Wu, B. Guo, Z. H. Li +24
All the 16F levels are unbound by proton emission. To date the four low-lying 16F levels below 1 MeV have been experimentally identified with well established spin-parity values an…
Constraining nova observables: direct measurements of resonance strengths in 33S(p,γ)34Cl
J. Fallis, A. Parikh, P. F. Bertone +32
The 33S(p,γ)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abu…