activity
20042008
most citedSensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model

182 citations · 356 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2008★ 52 cited

Cross section measurements of -induced reactions on Mo and Sn for -process studies

W. Rapp, I. Dillmann, F. Käppeler +5

The Mo()Ru, Mo()Ru, and Sn()Te cross sections were measured at the upper end of the -process Gamow window between 8.2…

astro-ph2008★ 29 cited

-Process simulations with a modified reaction library

I. Dillmann, T. Rauscher, M. Heil +3

We have performed -process simulations with the most recent stellar cross sections from the "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" project (versi…

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…

nucl-ex2006★ 88 cited

Alpha-induced cross sections of 106Cd for the astrophysical p-process

Gy. Gyurky, G. G. Kiss, Z. Elekes +11

The 106Cd(alpha,gamma)110Sn reaction cross section has been measured in the energy range of the Gamow window for the astrophysical p-process scenario. The cross sections for 106Cd(…

astro-ph2004★ 5 cited

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…