NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = K.Grun Found 6 matches. 1994OB03 Z.Phys. A349, 241 (1994) H.Oberhummer, H.Krauss, K.Grun, T.Rauscher, H.Abele, P.Mohr, G.Staudt Alpha Clustering and the Stellar Nucleosynthesis of Carbon NUCLEAR REACTIONS 12C(γ, α), E=low; calculated triple-α process reaction rate. Direct capture, α-clustering.
doi: 10.1007/BF01288967
1993KR18 Ann.Phys.(Leipzig) 2, 258 (1993) H.Krauss, K.Grun, T.Rauscher, H.Oberhummer The Astrophysical S-Factor of the Reaction 7Be(p, γ)8B in the Direct Capture Model NUCLEAR REACTIONS, ICPND 7Be(p, γ), E(cm) ≤ 2 MeV; calculated σ(E), astrophysical S-factor vs E. 7Li(n, γ), E(cm) ≤ 1 MeV; calculated σ(E). Direct capture model.
doi: 10.1002/andp.19935050304
1992RA04 Phys.Rev. C45, 1996 (1992) T.Rauscher, K.Grun, H.Krauss, H.Oberhummer, E.Kwasniewicz Analysis of 8Li(α, n)11B Below the Coulomb Barrier in the Potential Model NUCLEAR REACTIONS, ICPND 8Li(α, n), E(cm) ≤ 1 MeV; calculated astrophysical S-factor vs E, reaction rates. DWBA, folding potentials.
doi: 10.1103/PhysRevC.45.1996
1992WI09 J.Phys.(London) G18, L147 (1992) S.Winkler, H.Krauss, K.Grun, T.Rauscher, H.Oberhummer, H.Abele, G.Staudt Calculation of the 3He(3He, 2p)4He and 3H(3H, 2n)4He Astrophysical S Factor at Low Energies NUCLEAR REACTIONS, ICPND 3He(3He, 2p), E(cm) ≤ 1 MeV; analyzed astrophysical S-factor vs E. 3H(t, 2n), E ≤ 0.35 MeV; analyzed σ(E), astrophysical S-factor vs E. Potential model.
doi: 10.1088/0954-3899/18/8/004
1991HE16 Phys.Rev. C44, R952 (1991) H.Herndl, H.Abele, G.Staudt, B.Bach, K.Grun, H.Scsribany, H.Oberhummer, G.Raimann Direct Reaction Analysis of 19F(p, α)16O Below the Coulomb Barrier NUCLEAR REACTIONS, ICPND 19F(p, α), E=150-900 keV; analyzed σ(θ) vs E; deduced astrophysical S-factor, reaction mechanism. DWBA.
doi: 10.1103/PhysRevC.44.R952
1990RA28 Phys.Lett. 249B, 191 (1990) G.Raimann, B.Bach, K.Grun, H.Herndl, H.Oberhummer, S.Engstler, C.Rolfs, H.Abele, R.Neu, G.Staudt Evidence for Direct Reaction Mechanism in 7Li(p, α)4He at Thermonuclear Energies NUCLEAR REACTIONS, ICPND 7Li(p, α), E(cm)=0.013-1 MeV; analyzed σ(θ), astrophysical S-factor vs E; deduced reaction mechanism at thermonuclear energy. DWBA analysis.
doi: 10.1016/0370-2693(90)91241-3
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