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W. Rapp

4 papers hereh-index 12671 citations31 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3
  • middle author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • nucl-ex1

identity via Semantic Scholar / OpenAlex

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

collaborators

4 papers

astro-ph2008★ 52 cited

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

W. Rapp, I. Dillmann, F. Käppeler +5

The 92Mo(α,n)95Ru, 94Mo(α,n)97Ru, and 112Sn(α,γ)116Te 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…

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

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…

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