NSR Query Results
Output year order : Descending NSR database version of May 8, 2024. Search: Author = H.G.Reusch Found 4 matches. 1992TI03 Phys.Lett. 296B, 296 (1992) G.-R.Tillack, R.Reif, A.Schulke, P.Frobrich, H.J.Krappe, H.G.Reusch Light Particle Emission in the Langevin Dynamics of Heavy-Ion Induced Fission NUCLEAR REACTIONS 197Au(18O, F), E=159 MeV; calculated fission fragment total kinetic energy distribution, (fragment)n-coin, prescission particle multiplicities. 215Fr deduced light particle emission features. Langevin dynamics. NUCLEAR STRUCTURE 215Fr; calculated prescission fission induced light particle multiplicities; deduced light particle emission features. Langevin dynamics.
doi: 10.1016/0370-2693(92)91323-2
1990LA10 Z.Phys. A336, 403 (1990) K.Langanke, H.-G.Reusch, C.Rolfs Monte Carlo Simulations of the Lewis Effect NUCLEAR REACTIONS 27Al, 23Na, 26Mg(p, p), E ≤ 339 keV; calculated γ-yield curves. Nuclear, electronic energy loss curve Monte Carlo simulation.
1990RE07 Z.Phys. A336, 361 (1990) H.G.Reusch, K.Langanke, C.Rolfs Determination of Target Surface-Properties from High-Resolution Ion-Beam Experiments NUCLEAR REACTIONS, ICPND 23Na, 26Mg(p, γ), E ≈ resonance; analyzed thick target γ yield data; deduced target surface properties.
1989BL03 Z.Phys. A333, 219 (1989) G.Bluge, K.Langanke, H.G.Reusch, C.Rolfs The 3He(d, p)α Reaction at Astrophysical Energies NUCLEAR REACTIONS, ICPND 3He(d, p), E ≈ 0.01-1 MeV; calculated astrophysical S-factor vs E. Resonating group model, effective nucleon-nucleon interactions.
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