W. Rapp

activity

20042008

most citedSensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model

182 citations · 322 across the 3 of their papers we have counts for

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astro-ph2008★ 52 cited

Cross section measurements of $α$ -induced reactions on $^{92, 94}$ Mo and $^{112}$ Sn for $p$ -process studies

W. Rapp, I. Dillmann, F. Käppeler +5

The $^{92}$ Mo( $α, n$ ) $^{95}$ Ru, $^{94}$ Mo( $α, n$ ) $^{97}$ Ru, and $^{112}$ Sn( $α, γ$ ) $^{116}$ Te cross sections were measured at the upper end of the $p$ -process Gamow window between 8.2…

astro-ph2006★ 182 cited

Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model

W. Rapp, J. Goerres, M. Wiescher +2

The astrophysical p process, which is responsible for the origin of the proton rich stable nuclei heavier than iron, was investigated using a full nuclear reaction network for a ty…

astro-ph2004

The Influence of Reaction Rates on the Final p-Abundances

W. Rapp, M. Wiescher, H. Schatz +1

The astrophysical p-process is responsible for the origin of the proton rich nuclei,which are heavier than iron. A huge network involving thousands of reaction rates is necessary t…

Cross section measurements of α-induced reactions on 92,94Mo and 112Sn for p-process studies

Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model

The Influence of Reaction Rates on the Final p-Abundances

Cross section measurements of $α$ -induced reactions on $^{92, 94}$ Mo and $^{112}$ Sn for $p$ -process studies