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- W2756455104 abstract "The astrophysical p-process is an important way of nucleosynthesis to produce the stable and proton-rich nuclei beyond Fe which can not be reached by the s- and r-processes. In the present study, the astrophysical reaction rates of (γ,n), (γ,p), and (γ,α) reactions are computed within the modern reaction code TALYS for about 3000 stable and proton-rich nuclei with 12 Ru(γ,p) and 96 Ru(γ,α) are performed. It is shown that the experiments of photonuclear reactions in p-process based on ELI-NP are quite promising." @default.
- W2756455104 created "2017-09-25" @default.
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- W2756455104 date "2017-01-01" @default.
- W2756455104 modified "2023-10-18" @default.
- W2756455104 title "Photonuclear reactions in astrophysical p-process: Theoretical calculations and experiment simulation based on ELI-NP" @default.
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- W2756455104 doi "https://doi.org/10.1051/epjconf/201714601015" @default.
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