NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = A.Krauss Found 8 matches. 1989SC10 Nucl.Instrum.Methods Phys.Res. B40/41, 466 (1989) U.Schroder, S.Engstler, A.Krauss, K.Neldner, C.Rolfs, E.Somorjai, K.Langanke Search for Electron Screening of Nuclear Reactions at Sub-Coulomb Energies NUCLEAR REACTIONS, ICPND 3He(d, p), E=6-42 keV; measured σ(E); deduced astrophysical S-factor vs E, electron screening role. Atomic gas target.
doi: 10.1016/0168-583X(89)91022-7
1989SC43 Nucl.Instrum.Methods Phys.Res. B 40-41, 466 (1989) U.Schroeder, S.Engstler, A.Krauss, K.Neldner, C.Rolfs, E.Somorjai, K.Langanke Search for electron screening of nuclear reactions at sub-coulomb energies NUCLEAR REACTIONS 2H(3He, p), 3He(d, p), 6Li(p, 3He), 7Li(p, α), E=6.3-76 keV; measured products, 4He, Eπ, Iπ; deduced σ, σ(E). Data were imported from EXFOR entry A1291.
doi: 10.1016/0168-583x(89)91022-7
1988EN03 Phys.Lett. 202B, 179 (1988) S.Engstler, A.Krauss, K.Neldner, C.Rolfs, U.Schroder, K.Langanke Effects of Electron Screening on the 3He(d, p)4He Low-Energy Cross Sections NUCLEAR REACTIONS, ICPND 3He(d, p), E(cm)=5.9-41.6 keV; measured σ(E). Atomic gas target.
doi: 10.1016/0370-2693(88)90003-2
1987KR09 Nucl.Phys. A467, 273 (1987) A.Krauss, H.W.Becker, H.P.Trautvetter, C.Rolfs Astrophysical S(E) Factor of 3He(3He, 2p)4He at Solar Energies NUCLEAR REACTIONS, ICPND 3He(3He, 2p), E(cm)=17.9-342.5 keV; measured σ(E, θ); deduced reaction σ, astrophysical factor S(E). Windowless gas targets, beam calorimeter, cosmic background rejection, electronic shielding.
doi: 10.1016/0375-9474(87)90530-6
1987KR18 Nucl.Phys. A465, 150 (1987) A.Krauss, H.W.Becker, H.P.Trautvetter, C.Rolfs, K.Brand Low-Energy Fusion Cross Sections of D + D and D + 3He Reactions NUCLEAR REACTIONS, ICPND 2H(d, n), (d, p), E(cm)=2.98-162.5 keV; 3He(d, p), E(cm)=6.95-141.8 keV; measured σ(E, θ); deduced reaction σ, astrophysical S(E) factor. Windowless gas targets, beam calorimeter.
doi: 10.1016/0375-9474(87)90302-2
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
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