NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = A.Redder Found 7 matches. 1987PL03 Nucl.Phys. A465, 291 (1987) R.Plaga, H.W.Becker, A.Redder, C.Rolfs, H.P.Trautvetter, K.Langanke The Scattering of Alpha Particles from 12C and the 12C(α, γ)16O Stellar Reaction Rate NUCLEAR REACTIONS, ICPND 12C(α, α0), E=1-66 MeV; measured σ(E, θ); deduced astrophysical S-factor vs E, capture σ. 16O deduced level parameters. Enriched 12C targets.
doi: 10.1016/0375-9474(87)90436-2
1987RE02 Nucl.Phys. A462, 385 (1987) A.Redder, H.W.Becker, C.Rolfs, H.P.Trautvetter, T.R.Donoghue, T.C.Rinckel, J.W.Hammer, K.Langanke The 12C(α, γ)16O Cross Section at Stellar Energies NUCLEAR REACTIONS, ICPND 12C(α, γ), E=0.94-2.84 MeV; measured Eγ, Iγ, σ(E), σ(E, E(γ), θ); deduced astrophysical S-factor. Implanted 12C targets, NaI(Tl), Ge detectors.
doi: 10.1016/0375-9474(87)90555-0
1987SC18 Phys.Lett. 192B, 55 (1987) U.Schroder, A.Redder, C.Rolfs, R.E.Azuma, L.Buchmann, C.Campbell, J.D.King, T.R.Donoghue Astrophysical S Factor of 3H(α, γ)7Li NUCLEAR REACTIONS, ICPND 3H(α, γ), E(cm)=79-464 keV; measured Eγ, Iγ, branching ratio, σ(E), γ yield; deduced astrophysical S-factor vs E. Ge(Li) detectors.
doi: 10.1016/0370-2693(87)91141-5
1987SE13 Nucl.Instrum.Methods Phys.Res. A260, 33 (1987) S.Seuthe, H.W.Becker, A.Krauss, A.Redder, C.Rolfs, U.Schroder, H.P.Trautvetter, K.Wolke, S.Wustenbecker, R.W.Kavanagh, F.B.Waanders Production and Properties of Implanted Targets NUCLEAR REACTIONS, ICPND 12C(p, γ), E=220-340 keV; 12C(α, γ), E=2.65-2.85 MeV; 14N(p, γ), E=260-360 keV; 20Ne(p, γ), E=1165-1185 keV; 23Na(p, γ), E=300-400 keV; measured γ-ray yields. Implanted targets.
doi: 10.1016/0168-9002(87)90385-8
1985RE09 Phys.Rev.Lett. 55, 1262 (1985) A.Redder, H.W.Becker, J.Gorres, M.Hilgemeier, A.Krauss, C.Rolfs, U.Schroder, H.P.Trautvetter, K.Wolke, T.R.Donoghue, T.C.Rinckel, J.W.Hammer Capture Amplitudes in the Reaction 12C(α, γ)16O at Stellar Energies NUCLEAR REACTIONS 12C(α, γ), E(cm)=1.7-2.8 MeV; measured Eγ, Iγ, γ(θ); deduced nonnegligible E2 contribution to reaction rate at stellar energies, capture σ(E1)/σ(E2).
doi: 10.1103/PhysRevLett.55.1262
1984BU09 Nucl.Phys. A415, 93 (1984) L.Buchmann, M.Hilgemeier, A.Krauss, A.Redder, C.Rolfs, H.P.Trautvetter, T.R.Donoghue The Abundance of 26Al in the MgAl Cycle NUCLEAR REACTIONS, ICPND 26Al(p, γ), (p, p'γ), E=0.17-1.58 MeV; measured E(γ), I(γ)(E), γ yield vs E. 27Si deduced levels, absolute γ-transition strength, Γ, J, π, γ-branching ratios, astrophysical reaction rate. Artificially produced 26Al target, Ge(Li) detector.
doi: 10.1016/0375-9474(84)90601-8
1982RE06 Z.Phys. A305, 325 (1982) A.Redder, H.W.Becker, H.Lorenz-Wirzba, C.Rolfs, P.Schmalbrock, H.P.Trautvetter The 15N(p, α0)12C Reaction at Stellar Energies NUCLEAR REACTIONS 15N(p, α), E=78-810 keV; measured σ(E, θ); deduced astrophysical S-factor. 16O resonances deduced Γ, Γp, Γα.
doi: 10.1007/BF01419081
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