NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = H.Leiste Found 7 matches. 2012IM02 Phys.Rev. C 85, 065810 (2012), Erratum Phys.Rev. C 86, 039902 (2012) G.Imbriani, R.J.de Boer, A.Best, M.Couder, G.Gervino, J.Gorres, P.J.LeBlanc, H.Leiste, A.Lemut, E.Stech, F.Strieder, E.Uberseder, M.Wiescher Measurement of γ rays from 15N(p, γ)16O cascade and 15N(p, α1γ)12C reactions NUCLEAR REACTIONS 15N(p, γ)16O, 15N(p, αγ)12C, E=0.14-1.80 MeV; measured Eγ, Iγ, S factors, cross section. 12C, 16O; deduced levels, J, π, widths. R-matrix analysis. Comparison with previous studies.
doi: 10.1103/PhysRevC.85.065810
2011DI11 Phys.Rev. C 84, 015802 (2011) I.Dillmann, L.Coquard, C.Domingo-Pardo, F.Kappeler, J.Marganiec, E.Uberseder, U.Giesen, A.Heiske, G.Feinberg, D.Hentschel, S.Hilpp, H.Leiste, T.Rauscher, F.-K.Thielemann Cross sections for proton-induced reactions on Pd isotopes at energies relevant for the γ process NUCLEAR REACTIONS 102,104Pd(p, γ), 105Pd(p, n), E=2.75-9 MeV; measured Eγ, Iγ, total cross sections. 104Pd(p, n), 105Pd(p, γ)106mAg, 106Pd(p, n)106mAg, 110Pd(p, n)110mAg, E=2.75-9 MeV; measured Eγ, Iγ, partial cross sections; deduced S factors. Activation method. Relevant cross sections measured close to the astrophysical Gamow window of the γ process. Comparison with previous measurements and theoretical predictions from Hauser-Feshbach model "NON-SMOKER". RADIOACTIVITY 104Ag(EC); measured precise Iγ.
doi: 10.1103/PhysRevC.84.015802
2010LE21 Phys.Rev. C 82, 055804 (2010), Erratum Phys.Rev. C 84, 019902 (2011) P.J.LeBlanc, G.Imbriani, J.Gorres, M.Junker, R.Azuma, M.Beard, D.Bemmerer, A.Best, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, M.Couder, R.deBoer, Z.Elekes, S.Falahat, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, F.Kappeler, A.Kontos, R.Kuntz, H.Leiste, A.Lemut Q.Li, B.Limata, M.Marta, C.Mazzocchi, R.Menegazzo, S.O'Brien, A.Palumbo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, E.Stech, O.Straniero, F.Strieder, W.Tan, F.Terrasi, H.P.Trautvetter, E.Uberseder, M.Wiescher Constraining the S factor of 15N(p, γ)16O at astrophysical energies NUCLEAR REACTIONS 15N(p, γ), E=130-1800 keV; measured Ep, Ip, Eγ, Iγ, σ(E), σ(θ); deduced resonances, branching ratios, astrophysical S factors and reaction rates. Multilevel R-matrix analysis. Implications for the first and second cycles of the CNO cycles.
doi: 10.1103/PhysRevC.82.055804
2003DA19 Phys.Rev. C 68, 025801 (2003) S.Dababneh, M.Heil, F.Kappeler, J.Gorres, M.Wiescher, R.Reifarth, H.Leiste Stellar He burning of 18O: A measurement of low-energy resonances and their astrophysical implications NUCLEAR REACTIONS 18O(α, γ), E ≈ 470-770 keV; measured Eγ, Iγ; deduced resonance strengths, branching ratios, reaction rates. HPGe and BGO detectors. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.68.025801
2003GO21 Nucl.Phys. A718, 155c (2003) J.Gorres, S.Dababneh, A.Couture, M.Heil, F.Kappeler, H.Leiste, M.Lugaro, C.Ugalde, M.Wiescher Nucleosynthesis in TP-AGB Stars and the Production of 19F NUCLEAR REACTIONS 18O(α, γ), E ≈ 470, 566 MeV; measured Eγ, Iγ, γγ-coin; deduced resonance strengths, reaction rate. Implications for 19F nucleosynthesis discussed.
doi: 10.1016/S0375-9474(03)00707-3
2001GO28 Nucl.Phys. A688, 225c (2001) J.Gorres, C.Arlandini, U.Giesen, M.Heil, F.Kappeler, H.Leiste, E.Stech, M.Wiescher Topics in Stellar He Burning NUCLEAR REACTIONS 14N(α, γ), E=low; measured σ, resonance energy and strength, reaction rates. Comparison with earlier data, network calculations.
doi: 10.1016/S0375-9474(01)00703-5
2000GO43 Phys.Rev. C62, 055801 (2000) J.Gorres, C.Arlandini, U.Giesen, M.Heil, F.Kappeler, H.Leiste, E.Stech, M.Wiescher Low-Energy Resonances in 14N(α, γ)18F and Their Astrophysical Implications NUCLEAR REACTIONS 14N(α, γ), E=550-1300 keV; measured Eγ, Iγ(t), resonance yields; deduced astrophysical reaction rates. 18F deduced resonance energies, strengths. Implications for isotopic abundances discussed.
doi: 10.1103/PhysRevC.62.055801
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