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• W2897515575 abstract "Photodisintegration reaction rates involving charged particles are of relevance to the p-process nucleosynthesis that aims at explaining the production of the stable neutron-deficient nuclides heavier than iron. In this study, the cross sections and astrophysical rates of (g,p) and (g,a) reactions for about 3000 target nuclei with 10<Z<100 ranging from stable to proton dripline nuclei are computed. To study the sensitivity of the calculations to the optical model potentials (OMPs), both the phenomenological Woods-Saxon and the microscopic folding OMPs are taken into account. The systematic comparisons show that the reaction rates, especially for the (g,a) reaction, are dramatically influenced by the OMPs. Thus the better determination of the OMP is crucial to reduce the uncertainties of the photodisintegration reaction rates involving charged particles. Meanwhile, a gamma-beam facility at ELI-NP is being developed, which will open new opportunities to experimentally study the photodisintegration reactions of astrophysics interest. Considering both the important reactions identified by the nucleosynthesis studies and the purpose of complementing the experimental results for the reactions involving p-nuclei, the measurements of six (g,p) and eight (g,a) reactions based on the gamma-beam facility at ELI-NP and the ELISSA detector for the charged particles detection are proposed, and the GEANT4 simulations are correspondingly performed. The minimum required energies of the gamma-beam to measure these reactions are estimated. It is shown that the direct measurements of these photonuclear reactions within the Gamow windows at T_9=2.5 for p-process are fairly feasible and promising at ELI-NP. The expected experimental results will be used to constrain the OMPs of the charged particles, which can eventually reduce the uncertainties of the reaction rates for the p-process nucleosynthesis." @default.
• W2897515575 created "2018-10-26" @default.
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• W2897515575 date "2018-11-01" @default.
• W2897515575 modified "2023-09-25" @default.
• W2897515575 title "Determination of the photodisintegration reaction rates involving charged particles: Systematic calculations and proposed measurements based on the facility for Extreme Light Infrastructure–Nuclear Physics" @default.
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• W2897515575 cites W1979964403 @default.
• W2897515575 cites W1981244505 @default.
• W2897515575 cites W1982098627 @default.
• W2897515575 cites W1982819416 @default.
• W2897515575 cites W1990217236 @default.
• W2897515575 cites W1995519529 @default.
• W2897515575 cites W1999395010 @default.
• W2897515575 cites W2002361842 @default.
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• W2897515575 cites W2013458172 @default.
• W2897515575 cites W2021556327 @default.
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• W2897515575 cites W2025777340 @default.
• W2897515575 cites W2038400049 @default.
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• W2897515575 cites W2044823649 @default.
• W2897515575 cites W2048122918 @default.
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• W2897515575 cites W2101531975 @default.
• W2897515575 cites W2103010404 @default.
• W2897515575 cites W2113536251 @default.
• W2897515575 cites W2121234839 @default.
• W2897515575 cites W2143978162 @default.
• W2897515575 cites W2146873882 @default.
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• W2897515575 cites W2213630128 @default.
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• W2897515575 doi "https://doi.org/10.1103/physrevc.98.054601" @default.
• W2897515575 hasPublicationYear "2018" @default.
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