NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = H.J.Assenbaum Found 9 matches. 1988AL24 Z.Phys. A330, 277 (1988) T.Altmeyer, E.Kolbe, T.Warmann, K.Langanke, H.J.Assenbaum On Discrepancies within the Experimental and Theoretical Low Energy 3H(α, γ)7Li Cross Sections NUCLEAR REACTIONS, ICPND 3H(α, γ), E ≈ 50-600 keV; calculated σ(E), S-factor vs E. Resonating group method.
1988AS03 Phys.Lett. 208B, 346 (1988) H.-J.Assenbaum, K.Langanke, G.Soff Vacuum Polarization Effects in Subbarrier Nuclear Fusion Reactions NUCLEAR REACTIONS 28Si, 16O(16O, X), 12C(12C, X), 28Si(28Si, X), E ≤ 20 MeV; calculated penetrability ratios.
doi: 10.1016/0370-2693(88)90626-0
1988KO29 Phys.Lett. 214B, 169 (1988) E.Kolbe, K.Langanke, H.J.Assenbaum Microscopic Study of the Low-Energy 7Be(p, γ)8B Reaction NUCLEAR REACTIONS, ICPND 7Be(p, γ), E < 500 keV; calculated astrophysical S-factor vs E.
doi: 10.1016/0370-2693(88)91462-1
1987AS01 Phys.Rev. C35, 755 (1987) H.J.Assenbaum, K.Langanke, A.Weiguny Electric Dipole Collectivity in Light Nuclear Systems NUCLEAR STRUCTURE 22Ne, 46,48,52Ti; calculated B(E1); deduced molecular sum rule fraction, E1 collectivity. Microscopic model, α clusters.
doi: 10.1103/PhysRevC.35.755
1987AS03 Phys.Rev. C36, 17 (1987) Low-Energy 2H(d, γ)4He Reaction and the D-State Admixture in the 4He Ground State NUCLEAR REACTIONS, ICPND 2H(d, γ), E(cm)=0.010-10 MeV; calculated σ(Eγ, E), capture σ, astrophysical S-factor vs E. 4He level deduced D-state admixture.
doi: 10.1103/PhysRevC.36.17
1987AS05 Z.Phys. A327, 461 (1987) H.J.Assenbaum, K.Langanke, C.Rolfs Effects of Electron Screening of Low-Energy Fusion Cross Sections NUCLEAR REACTIONS, ICPND 2H, 3He(d, p), E ≤ 50 keV; 3He(3He, 2p), 7Li, 18O, 11B, 15N(p, α), E ≤ 250 keV; calculated reaction σ, astrophysical S(E) factors. Electron screening effects.
1987BL12 Phys.Rev. C36, 21 (1987) G.Bluge, H.J.Assenbaum, K.Langanke Potential Model Analysis of Low Energy 2H(d, γ)4He Fusion Data NUCLEAR REACTIONS, ICPND 2H(d, γ), E(cm)=0.010-10 MeV; calculated σ(Eγ, E), capture σ, astrophysical S-factor vs E, phase shifts vs E. 4He level deduced D-state admixture nucleus-nucleus potential dependence.
doi: 10.1103/PhysRevC.36.21
1987KR03 Phys.Rev. C35, 1631 (1987) D.Krolle, H.J.Assenbaum, C.Funck, K.Langanke Possible Experiments to Distinguish between Different Methods of Treating the Pauli Principle in Nuclear Potential Models NUCLEAR REACTIONS 4He(α, αγ), E ≤ 15 MeV; calculated bremsstrahlung σ(E), σ(θ1, θ2), phase shifts. Finite Pauli repulsion model.
doi: 10.1103/PhysRevC.35.1631
1984AS04 Z.Phys. A318, 35 (1984) H.J.Assenbaum, K.Langanke, A.Weiguny Microscopic Study of the α - 14C Molecular-Dipole Degree of Freedom in the 18O Nucleus NUCLEAR STRUCTURE 18O; calculated rotational band, parity splitting, intrabrand E1 transitions. Molecular-dipole degree of freedom, (α)(14C) cluster.
doi: 10.1007/BF02117212
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