NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = H.W.Drotleff Found 3 matches. 1996KU07 Phys.Rev. C53, 2486 (1996) R.Kunz, S.Barth, A.Denker, H.W.Drotleff, J.W.Hammer, H.Knee, A.Mayer Determination of the 9Be(α, n)12C Reaction Rate NUCLEAR REACTIONS, ICPND 9Be(α, n), E=0.5-3.5 MeV; measured yield, σ(E); deduced astrophysical S-factor vs E, reaction rate. 13C deduced resonances, Γ.
doi: 10.1103/PhysRevC.53.2486
1993DR08 Astrophys.J. 414, 735 (1993) H.W.Drotleff, A.Denker, H.Knee, M.Soine, G.Wolf, J.W.Hammer, U.Greife, C.Rolfs, H.P.Trautvetter Reaction Rates of the s-Process Neutron Sources 22Ne(α, n)25Mg and 13C(α, n)16O NUCLEAR REACTIONS, ICPND 13C(α, n), E(cm) ≈ 275-1075 keV; 22Ne(α, n), E=0.57-2.3 MeV; measured σ(E); deduced astrophysical S-factor, reaction rates at helium burning temperatures.
doi: 10.1086/173119
1991DR01 Z.Phys. A338, 367 (1991) H.W.Drotleff, A.Denker, J.W.Hammer, H.Knee, S.Kuchler, D.Streit, C.Rolfs, H.P.Trautvetter New 22Ne(α, n)25Mg-Resonances at Very Low Energies Relevant for the Astrophysical s-Process NUCLEAR REACTIONS, ICPND 22Ne(α, n), E ≈ 550-2100 keV; measured σ(E); deduced resonance structure relevant to s-process. Windowless gas target system, 4π neutron detector.
doi: 10.1007/BF01288203
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