NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = S.Engstler Found 7 matches. 1993AN06 Z.Phys. A345, 231 (1993) C.Angulo, S.Engstler, G.Raimann, C.Rolfs, W.H.Schulte, E.Somorjai The Effects of Electron Screening and Resonances in (p, α) Reactions on 10B and 11B at Thermal Energies NUCLEAR REACTIONS, ICPND 11,10B(p, α), E(cm)=17-134 keV; measured spectra, α yield. 11B(p, γ), E=140-260 keV; 1H(19F, αγ), E ≈ 6.23-7.83; measured thick target yield; deduced absolute astrophysical S-factor vs E, electron screening role.
doi: 10.1007/BF01293350
1992EN01 Phys.Lett. 279B, 20 (1992) S.Engstler, G.Raimann, C.Angulo, U.Greife, C.Rolfs, U.Schroder, E.Somorjai, B.Kirch, K.Langanke Test for Isotopic Dependence of Electron Screening in Fusion Reactions NUCLEAR REACTIONS, ICPND 7,6Li(p, α), 6Li(d, α), E(cm)=10-1004 keV; measured σ(θ, E); deduced astrophysical S-factor vs E, electron screening potential energy.
doi: 10.1016/0370-2693(92)91833-U
1992EN04 Z.Phys. A342, 471 (1992) S.Engstler, G.Raimann, C.Angulo, U.Greife, C.Rolfs, U.Schroder, E.Somorjai, B.Kirch, K.Langanke Isotopic Dependence of Electron Screening in Fusion Reactions NUCLEAR REACTIONS, ICPND 1,2H(6Li, α), 1H(7Li, α), E(cm)=10-1450 keV; 6Li(p, α), (d, α), 7Li(p, α), E(cm)=10-450 keV; measured σ(Eα), σ(θ), astrophysical S-factor vs E. LiF solid targets, hydrogen molecular gas targets.
doi: 10.1007/BF01294958
1990RA28 Phys.Lett. 249B, 191 (1990) G.Raimann, B.Bach, K.Grun, H.Herndl, H.Oberhummer, S.Engstler, C.Rolfs, H.Abele, R.Neu, G.Staudt Evidence for Direct Reaction Mechanism in 7Li(p, α)4He at Thermonuclear Energies NUCLEAR REACTIONS, ICPND 7Li(p, α), E(cm)=0.013-1 MeV; analyzed σ(θ), astrophysical S-factor vs E; deduced reaction mechanism at thermonuclear energy. DWBA analysis.
doi: 10.1016/0370-2693(90)91241-3
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
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