期刊论文、会议论文

Xu, Y.

英文

EPJ Web of Conferences

2100-014X

2018

178

04007-

16th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics (CGS)

EPJ Web of Conferences

SEP 18-22, 2017

Shanghai, PEOPLES R CHINA

[Xu, Y.;Balabanski, D. L.;Chesnevskaya, S.;Guardo, G. L.;Lattuada, D.;Matei, C.] Extreme Light Infrastruct Nucl Phys, RO-077125 Magurele, Iifov, Romania.^[Goriely, S.] Univ Libre Bruxelles, Inst Astron & Astrophys, CP-226, B-1050 Brussels, Belgium.^[La Cognata, M.] INFN, Lab Nazl Sud, Via Santa Sofia 62, I-95123 Catania, Italy.^[Lan, H. Y.;Luo, W.] Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.

Sun, Y

17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE

E D P SCIENCES

10.1051/epjconf/201817804007

本校为其他机构

The astrophysical p-process is an important way of nucleosynthesis to produce the stable and protonrich nuclei beyond Fe which can not be reached by the s- and r-processes. In the present study, the impact of nuclear ingredients, especially the nuclear potential, level density and strength function, to the astrophysical reaction rates of (p,γ), (α,γ), (γ,p), and (γ,α) reactions are systematically studied. The calculations are performed basad on the modern reaction code TALYS for about 3000 stable and proton-rich nuclei with 12≤Z≤110. In...