67 citations · 188 across the 8 of their papers we have counts for
8 papers
Measurement of the Tb(n, ) cross section at the CSNS Back-n facility
S. Zhang, G. Li, W. Jiang +19
The stellar (n, ) cross section data for the mass numbers around A 160 are of key importance to nucleosynthesis in the main component of the slow neutron capture proce…
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…
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…
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…
New determination of the 13C(a, n)16O reaction rate and its influence on the s-process nucleosynthesis in AGB stars
B. Guo, Z. H. Li, M. Lugaro +21
We present a new measurement of the -spectroscopic factor () and the asymptotic normalization coefficient (ANC) for the 6.356 MeV 1/2 subthreshold state of O thr…