NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = W.Rapp Found 9 matches. 2008DI05 J.Phys.(London) G35, 014029 (2008) I.Dillmann, T.Rauscher, M.Heil, F.Kappeler, W.Rapp, F.-K.Thielemann p-Process simulations with a modified reaction library
doi: 10.1088/0954-3899/35/1/014029
2008RA19 Phys.Rev. C 78, 025804 (2008) W.Rapp, I.Dillmann, F.Kappeler, U.Giesen, H.Klein, T.Rauscher, D.Hentschel, S.Hilpp Cross section measurements of α-induced reactions on 92, 94Mo and 112Sn for p-process studies NUCLEAR REACTIONS 92,94Mo(α, n), 112Sn(α, γ), E=8.2-11.1 MeV; measured σ, astrophysical S-factors. Comparison with Hartree-Fock-Bogoliubov calculations.
doi: 10.1103/PhysRevC.78.025804
2007OZ01 Phys.Rev. C 75, 025801 (2007) N.Ozkan, G.Efe, R.T.Guray, A.Palumbo, J.Gorres, H.Y.Lee, L.O.Lamm, W.Rapp, E.Stech, M.Wiescher, Gy.Gyurky, Zs.Fulop, E.Somorjai Astrophysical S factor for α-capture on 112Sn in the p-process energy range NUCLEAR REACTIONS 112Sn(α, γ), (α, p), E(cm)=7.59-11.42 MeV; measured σ; deduced astrophysical S-factors. Activation technique.
doi: 10.1103/PhysRevC.75.025801
2006GY01 Phys.Rev. C 74, 025805 (2006) Gy.Gyurky, G.G.Kiss, Z.Elekes, Zs.Fulop, E.Somorjai, A.Palumbo, J.Gorres, H.Y.Lee, W.Rapp, M.Wiescher, N.Ozkan, R.T.Guray, G.Efe, T.Rauscher α-induced cross sections of 106Cd for the astrophysical p process NUCLEAR REACTIONS 106Cd(α, γ), (α, n), (α, p), E ≈ 7.5-12.5 MeV; measured σ; deduced S-factors. Comparison with statistical model predictions. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.74.025805
2006RA27 Astrophys.J. 653, 474 (2006) W.Rapp, J.Gorres, M.Wiescher, H.Schatz, F.Kappeler Sensitivity of p-process nucleosynthesis to nuclear reaction rates in a 25 M(.) supernova model
doi: 10.1086/508402
2005RA22 Nucl.Phys. A758, 545c (2005) W.Rapp, M.Wiescher, H.Schatz, F.Kappeler The Influence of Reaction Rates on the Final p-Abundances
doi: 10.1016/j.nuclphysa.2005.05.099
2003RA26 Phys.Rev. C 68, 015802 (2003) W.Rapp, P.E.Koehler, F.Kappeler, S.Raman 95Mo(n, α) cross section from 1 eV to 500 keV: A test of the α + nucleus optical potential used in calculating reaction rates for explosive nucleosynthesis NUCLEAR REACTIONS 95Mo(n, α), E=0.001-500 keV; measured σ; deduced resonance parameters. Determination of global α-nucleus potential parameters discussed.
doi: 10.1103/PhysRevC.68.015802
2002RA36 Phys.Rev. C66, 015803 (2002) W.Rapp, M.Heil, D.Hentschel, F.Kappeler, R.Reifarth, H.J.Brede, H.Klein, T.Rauscher α- and Neutron-Induced Reactions on Ruthenium Isotopes NUCLEAR REACTIONS 96Ru(α, γ), (α, p), 96,98Ru(α, n), E=7.0-10.6 MeV; 96,102,104Ru(n, γ), E=spectrum; measured σ. Activation technique, comparison with statistical model predictions, astrophysical implications discussed.
doi: 10.1103/PhysRevC.66.015803
2001RA24 Nucl.Phys. A688, 427c (2001) W.Rapp, H.J.Brede, M.Heil, D.Hentschel, F.Kappeler, H.Klein, R.Reifarth, T.Rauscher Alpha and Neutron Induced Reactions on Ruthenium NUCLEAR REACTIONS 96Ru(α, γ), (α, p), (α, n), 98Ru(α, n), E(cm)=7-11 MeV; measured Eγ, σ. Comparison with Statistical Model calculations, p-process discussed.
doi: 10.1016/S0375-9474(01)00745-X
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