The (85)Rb(p,n)(85)Sr reaction and the modified proton optical potential

Kiss, G. G., Gyuerky, Gy., Simon, A., Fueloep, Zs., Somorjai, E. and Rauscher, T. (2009) The (85)Rb(p,n)(85)Sr reaction and the modified proton optical potential. In: 13th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics, 2008-08-25 - 2008-08-29.

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The cross sections of the astrophysically relevant (85)Rb(p,n)(85)Sr(g,m) reaction have been measured between E(c.m). = 2.16 and 3.96 MeV. The cross sections have been derived by measuring the gamma radiation following the beta decay of the reaction products. A comparison with the predictions of Hauser-Feshbach calculations using the NON-SMOKER code confirms a recently derived modification of the global optical proton potential.

Item Type	Conference or Workshop Item (Other)
Keywords	nucleosynthesis in novae, energies, capture cross-sections, 59 <= a <= 89, gamma-processes, p-process, statistical compound-nucleus reactions, model, supernovae, rates, relevant, and other explosive environments, finite nuclei, hard-core interaction
Date Deposited	15 May 2025 16:32
Last Modified	10 Jul 2025 23:30