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.
American Institute of Physics (AIP).
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 | Other |
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Uncontrolled 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 | 18 Nov 2024 12:20 |
Last Modified | 18 Nov 2024 12:20 |
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