NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = M.Hoeft Found 6 matches. 2005RU16 Nucl.Phys. A758, 170c (2005) G.Ruprecht, K.Czerski, D.Bemmerer, M.Hoeft, P.Heide Excitation of Giant Resonances in Deuteron Stripping Reactions on 10B far below the Coulomb Barrier NUCLEAR REACTIONS 10B(d, p), E(cm)=0-2.5 MeV; analyzed S-factors; deduced resonance contributions. 12C deduced hole-state contribution to GDR.
doi: 10.1016/j.nuclphysa.2005.05.172
2004RU10 Phys.Rev. C 70, 025803 (2004) G.Ruprecht, K.Czerski, D.Bemmerer, M.Hoeft, P.Heide Coherent resonance contributions in the reactions 6Li(d, α)4He and 10B(d, p0)11B at sub-Coulomb energies NUCLEAR REACTIONS 6Li(d, α), E(cm)=21-81 keV; measured angular distributions; 10B(d, p), E(cm)=100-300 keV; measured σ, angular distributions; deduced resonance contributions. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.70.025803
2001CZ01 Europhys.Lett. 54, 449 (2001) K.Czerski, A.Huke, A.Biller, P.Heide, M.Hoeft, G.Ruprecht Enhancement of the Electron Screening Effect for d + d Fusion Reactions in Metallic Environments NUCLEAR REACTIONS 2H(d, p), (d, n), E=5-60 MeV; measured angular distributions, thick-target yields for targets implanted in Al, Zr, and Ta; deduced possible electron screening effects.
doi: 10.1209/epl/i2001-00265-7
2001HO19 Nucl.Phys. A688, 390c (2001) Description of Star Formation in the Context of Cosmological Large-Scale Structure Formation
doi: 10.1016/S0375-9474(01)00733-3
2001HO22 Nucl.Phys. A688, 524c (2001) M.Hoeft, K.Czerski, P.Heide, M.Lang S-Factors for the 10B(d, p)11B and 10B(d, α)8Be Reactions in the Deuteron Energy Range from 120 to 340 keV NUCLEAR REACTIONS 10B(d, p), (d, α), E=120-340 keV; measured σ(θ), S-factor. Comparison with earlier data.
doi: 10.1016/S0375-9474(01)00776-X
2001RU08 Nucl.Phys. A688, 521c (2001) G.Ruprecht, D.Bemmerer, K.Czerski, P.Heide, M.Hoeft Interference Effects between Resonant and Direct Reaction Mechanisms for 6Li(d, α)4He NUCLEAR REACTIONS 6Li(d, α), E=40-2000 keV; calculated S-factor, σ(θ), anisotropy. Optical Model, DWBA.
doi: 10.1016/S0375-9474(01)00775-8
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