NSR Query Results
Output year order : Descending NSR database version of April 24, 2024. Search: Author = H.Oberhummer Found 73 matches. 2011BE47 Eur.Phys.J. A 47, 160 (2011) F.Belloni, M.Calviani, N.Colonna, P.Mastinu, P.M.Milazzo, U.Abbondanno, G.Aerts, H.Alvarez, F.Alvarez-Velarde, S.Andriamonje, J.Andrzejewski, L.Audouin, G.Badurek, M.Barbagallo, P.Baumann, F.Becvar, E.Berthoumieux, F.Calvino, D.Cano-Ott, R.Capote, C.Carrapico, P.Cennini, V.Chepel, E.Chiaveri, G.Cortes, A.Couture, J.Cox, M.Dahlfors, S.David, I.Dillmann, C.Domingo-Pardo, W.Dridi, I.Duran, C.Eleftheriadis, M.Embid-Segura, A.Ferrari, R.Ferreira-Marques, K.Fujii, W.Furman, I.Goncalves, E.Gonzalez-Romero, A.Goverdovski, F.Gramegna, C.Guerrero, F.Gunsing, B.Haas, R.Haight, M.Heil, A.Herrera-Martinez, M.Igashira, E.Jericha, F.Kappeler, Y.Kadi, D.Karadimos, D.Karamanis, M.Kerveno, P.Koehler, E.Kossionides, M.Krticka, C.Lamboudis, H.Leeb, A.Lindote, I.Lopes, M.Lozano, S.Lukic, J.Marganiec, S.Marrone, T.Martinez, C.Massimi, M.H.Meaze, A.Mengoni, C.Moreau, M.Mosconi, F.Neves, H.Oberhummer, S.O'Brien, J.Pancin, C.Papachristodoulou, C.Papadopoulos, C.Paradela, N.Patronis, A.Pavlik, P.Pavlopoulos, L.Perrot, M.T.Pigni, R.Plag, A.Plompen, A.Plukis, A.Poch, J.Praena, C.Pretel, J.Quesada, T.Rauscher, R.Reifarth, M.Rosetti, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, C.Santos, L.Sarchiapone, I.Savvidis, C.Stephan, G.Tagliente, J.L.Tain, D.Tarrio, L.Tassan-Got, L.Tavora, R.Terlizzi, G.Vannini, P.Vaz, A.Ventura, D.Villamarin, M.C.Vincente, V.Vlachoudis, R.Vlastou, F.Voss, S.Walter, M.Wiescher, K.Wisshak Measurement of the neutron-induced fission cross-section of 243Am relative to 235U from 0.5 to 20 MeV NUCLEAR REACTIONS 235U, 243Am(n, F), E=0.5-20 MeV; measured fission products using n_TOF fast ionization chamber; deduced σ; calculated σ using EMPIRE code. Compared with other data, ENDF/B-VII.0, JENDL-4.0, JEFF-3.1.1, ROSFOND, BROND-2.2.
doi: 10.1140/epja/i2011-11160-x
2011TA17 Phys.Rev. C 84, 015801 (2011) G.Tagliente, P.M.Milazzo, K.Fujii, U.Abbondanno, G.Aerts, H.Alvarez, F.Alvarez-Velarde, S.Andriamonje, J.Andrzejewski, L.Audouin, G.Badurek, P.Baumann, F.Becvar, F.Belloni, E.Berthoumieux, S.Bisterzo, F.Calvino, M.Calviani, D.Cano-Ott, R.Capote, C.Carrapico, P.Cennini, V.Chepel, E.Chiaveri, N.Colonna, G.Cortes, A.Couture, J.Cox, M.Dahlfors, S.David, I.Dillmann, C.Domingo-Pardo, W.Dridi, I.Duran, C.Eleftheriadis, M.Embid-Segura, A.Ferrari, R.Ferreira-Marques, W.Furman, R.Gallino, I.Goncalves, E.Gonzalez-Romero, F.Gramegna, C.Guerrero, F.Gunsing, B.Haas, R.Haight, M.Heil, A.Herrera-Martinez, E.Jericha, F.Kappeler, Y.Kadi, D.Karadimos, D.Karamanis, M.Kerveno, E.Kossionides, M.Krticka, C.Lamboudis, H.Leeb, A.Lindote, I.Lopes, M.Lozano, S.Lukic, J.Marganiec, S.Marrone, T.Martnez, C.Massimi, P.Mastinu, A.Mengoni, C.Moreau, M.Mosconi, F.Neves, H.Oberhummer, S.O'Brien, J.Pancin, C.Papachristodoulou, C.Papadopoulos, C.Paradela, N.Patronis, A.Pavlik, P.Pavlopoulos, L.Perrot, M.T.Pigni, R.Plag, A.Plompen, A.Plukis, A.Poch, J.Praena, C.Pretel, J.Quesada, T.Rauscher, R.Reifarth, M.Rosetti, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, C.Santos, L.Sarchiapone, I.Savvidis, C.Stephan, J.L.Tain, L.Tassan-Got, L.Tavora, R.Terlizzi, G.Vannini, P.Vaz, A.Ventura, D.Villamarin, M.C.Vincente, V.Vlachoudis, R.Vlastou, F.Voss, S.Walter, M.Wiescher, K.Wisshak Neutron capture on 94Zr: Resonance parameters and Maxwellian-averaged cross sections NUCLEAR REACTIONS 94Zr(n, γ), E=0.001-60 keV; measured E(n), I(n), capture yield using CERN n_TOF neutron source; deduced resonance parameters ER, gamma and neutron widths, capture kernels; calculated Maxwellian-averaged capture cross sections. 95Zr; deduced resonances, J, l-values, R-matrix analysis. Comparison with previous studies. Discussed astrophysical implications.
doi: 10.1103/PhysRevC.84.015801
2008DO05 J.Phys.(London) G35, 014020 (2008) C.Domingo-Pardo, U.Abbondanno, G.Aerts, H.Alvarez, F.Alvarez-Velarde, S.Andriamonje, J.Andrzejewski, P.Assimakopoulos, L.Audouin, G.Badurek, P.Baumann, F.Becvar, E.Berthoumieux, S.Bisterzo, F.Calvino, M.Calviani, D.Cano-Ott, R.Capote, C.Carrapico, P.Cennini, V.Chepel, N.Colonna, G.Cortes, A.Couture, J.Cox, M.Dahlfors, S.David, I.Dillmann, W.Dridi, I.Duran, C.Eleftheriadis, M.Embid-Segura, L.Ferrant, A.Ferrari, R.Ferreira-Marques, K.Fujii, W.Furman, R.Gallino, I.Goncalves, E.Gonzalez-Romero, F.Gramegna, C.Guerrero, F.Gunsing, B.Haas, R.Haight, M.Heil, A.Herrera-Martinez, M.Igashira, E.Jericha, Y.Kadi, F.Kappeler, D.Karadimos, D.Karamanis, M.Kerveno, P.Koehler, E.Kossionides, M.Krticka, C.Lamboudis, H.Leeb, A.Lindote, I.Lopes, M.Lozano, S.Lukic, J.Marganiec, S.Marrone, C.Massimi, P.Mastinu, A.Mengoni, P.M.Milazzo, M.Mosconi, F.Neves, H.Oberhummer, S.O'Brien, J.Pancin, C.Papachristodoulou, C.Papadopoulos, C.Paradela, N.Patronis, A.Pavlik, P.Pavlopoulos, L.Perrot, M.T.Pigni, R.Plag, A.Plompen, A.Plukis, A.Poch, C.Pretel, J.Quesada, T.Rauscher, R.Reifarth, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, C.Santos, L.Sarchiapone, I.Savvidis, C.Stephan, G.Tagliente, J.L.Tain, L.Tassan-Got, L.Tavora, R.Terlizzi, G.Vannini, P.Vaz, A.Ventura, D.Villamarin, M.C.Vincente, V.Vlachoudis, R.Vlastou, F.Voss, S.Walter, M.Wiescher, K.Wisshak The measurement of the 206Pb(n, γ) cross section and stellar implications NUCLEAR REACTIONS 206Pb(n, γ), E=0.001-1000 keV; measured Eγ, Iγ, capture cross sections. Deduced maxwellian averaged sections.
doi: 10.1088/0954-3899/35/1/014020
2003OB04 Nucl.Phys. A719, 283c (2003) H.Oberhummer, A.Csoto, M.Fairbairn, H.Schlattl, M.M.Sharma Temporal variation of coupling constants and nucleosynthesis
doi: 10.1016/S0375-9474(03)00933-3
2002BE37 Nucl.Phys. A705, 239 (2002) H.Beer, P.V.Sedyshev, W.Rochow, P.Mohr, H.Oberhummer Neutron Capture Measurements of the Noble Gas Isotopes 22Ne, 40Ar and 78, 80, 84, 86Kr in the keV Energy Region NUCLEAR REACTIONS 22Ne, 40Ar, 78,80,84,86Kr(n, γ), E=25-215 keV; measured capture σ; deduced astrophysical reaction rates. 85Kr deduced probability of isomeric state population. Activation technique, high-pressure gas targets.
doi: 10.1016/S0375-9474(02)00645-0
2001BO30 Nucl.Phys. A688, 493c (2001) I.N.Borzov, A.V.Avdeenkov, B.Grun, H.Oberhummer Direct Neutron Capture in a Microscopic Model NUCLEAR REACTIONS 124,132Sn, 208,232Pb(n, γ), E=30 keV; calculated non-resonant direct capture σ. Green's function formalism, comparison with other calculations and with data.
doi: 10.1016/S0375-9474(01)00766-7
2001CS04 Nucl.Phys. A688, 560c (2001) A.Csoto, H.Oberhummer, H.Schlattl Fine-Tuning the Basic Forces of Nature Through the Triple-Alpha Process in Red Giant Stars NUCLEAR STRUCTURE 12C; calculated 2nd 0+ resonance energy for different sets of nuclear potentials. Cluster model. NUCLEAR REACTIONS 8Be(α, γ), E=low; calculated reaction rate as function of 2nd 0+ resonance energy in 12C; deduced 12C abundance following network calculations.
doi: 10.1016/S0375-9474(01)00787-4
2001FO07 Phys.Rev. C64, 045801 (2001) O.Forstner, H.Herndl, H.Oberhummer, H.Schatz, B.A.Brown Thermonuclear Reaction Rate of 56Ni(p, γ)57Cu and 57Cu(p, γ)58Zn NUCLEAR REACTIONS 56Ni, 57Cu(p, γ), E=stellar; calculated reaction rates. Astrophysical implications discussed. NUCLEAR STRUCTURE 57,58Ni, 57Cu, 58Zn; calculated energy levels, level shifts. 57Cu, 58Zn; calculated shell model spectroscopic factors.
doi: 10.1103/PhysRevC.64.045801
2001FU19 Phys.Rev. C64, 065805 (2001) Zs.Fulop, Gy.Gyurky, Z.Mate, E.Somorjai, L.Zolnai, D.Galaviz, M.Babilon, P.Mohr, A.Zilges, T.Rauscher, H.Oberhummer, G.Staudt 92Mo(α, α)92Mo Scattering, the 92Mo-α Optical Potential, and the 96Ru(γ, α)92Mo Reaction Rate at Astrophysically Relevant Energies NUCLEAR REACTIONS 92Mo(α, α), E(cm) ≈ 13, 16, 19 MeV; measured σ(θ); deduced optical model parameters. 96Ru(γ, α), E not given; calculated astrophysical reaction rates.
doi: 10.1103/PhysRevC.64.065805
2001IV06 Eur.Phys.J. A 12, 87 (2001) A.N.Ivanov, V.A.Ivanova, H.Oberhummer, N.I.Troitskaya, M.Faber On the D-Wave State Component of the Deuteron in the Nambu-Jona-Lasinio Model of Light Nuclei NUCLEAR STRUCTURE 2H; calculated D-wave component admixture. Nambu-Jona-Lasinio model, comparison with data.
doi: 10.1007/s100500170041
2001MO20 Nucl.Phys. A688, 424c (2001) P.Mohr, M.Babilon, D.Galaviz, A.Zilges, Zs.Fulop, Gy.Gyurky, Z.Mate, E.Somorjai, L.Zolnai, H.Oberhummer α-Nucleus Potentials at Astrophysically Relevant Energies NUCLEAR REACTIONS 92Mo(α, α), E=14-20 MeV; measured σ(θ); deduced optical model parameters. Comparison with neighboring nuclei.
doi: 10.1016/S0375-9474(01)00744-8
2001OB02 Nucl.Phys. A689, 269c (2001) H.Oberhummer, A.Csoto, H.Schlattl Bridging the Mass Gaps at A = 5 and A = 8 in Nucleosynthesis
doi: 10.1016/S0375-9474(01)00841-7
2000CS08 Acta Phys.Hung.N.S. 12, 149 (2000) A.Csoto, H.Oberhummer, H.Schlattl At the Edge of Nuclear Stability: Nonlinear quantum amplifiers
2000IV04 Eur.Phys.J. A 7, 519 (2000) A.N.Ivanov, H.Oberhummer, N.J.Troitskaya, M.Faber The Nambu-Jona-Lasinio Model of Light Nuclei
doi: 10.1007/s100500050425
2000IV05 Eur.Phys.J. A 8, 125 (2000) A.N.Ivanov, H.Oberhummer, N.I.Troitskaya, M.Faber On the ΔΔ Component of the Deuteron in the Nambu-Jona-Lasinio Model of Light Nuclei NUCLEAR STRUCTURE 2H; calculated ΔΔ component contribution. Nambu-Jona-Lasinio model of light nuclei. Comparison with data.
doi: 10.1007/s100530050016
2000IV06 Eur.Phys.J. A 8, 223 (2000) A.N.Ivanov, H.Oberhummer, N.I.Troitskaya, M.Faber Dynamics of Low-Energy Nuclear Forces for Electromagnetic and Weak Reactions with the Deuteron in the Nambu-Jona-Lasinio Model of Light Nuclei NUCLEAR REACTIONS 1H(n, γ), E=thermal; 2H(γ, n), E=2.62-4.45 MeV; 2H(ν, e-p), E=4-10 MeV; calculated σ. 1H(p, X), E=low; calculated spectroscopic factor Spp(0). 2H(ν-bar, e+n), 2H(ν, nν), E not given; calculated σ averaged over antineutrino energy spectrum. Astrophysics relevance discussed.
doi: 10.1007/s100530050030
1999BI06 Nucl.Phys. A647, 3 (1999) R.Bieber, C.Wagemans, G.Goeminne, J.Wagemans, B.Denecke, M.Loiselet, M.Gaelens, P.Geltenbort, H.Oberhummer Thermal Neutron Induced (n, p) and (n, α) Reactions on 37Ar NUCLEAR REACTIONS 37Ar(n, α), (n, αγ), (n, p), E=thermal; measured α spectra, proton spectra; deduced reaction σ, (n, α0)/(n, α1) branching ratio. Comparison with previous data.
doi: 10.1016/S0375-9474(99)00013-5
1999HE33 Phys.Rev. C60, 064614 (1999) H.Herndl, R.Hofinger, J.Jank, H.Oberhummer, J.Gorres, M.Wiescher, F.-K.Thielemann, B.A.Brown Reaction Rates for Neutron Capture Reactions to C, N, and O Isotopes to the Neutron Rich Side of Stability NUCLEAR REACTIONS 13,14,15,16C, 15,16,17,18N, 18,19,20,21O(n, γ), E=stellar; analyzed data; deduced capture rates. Comparison with previous results.
doi: 10.1103/PhysRevC.60.064614
1999MO07 Phys.Rev. C59, 1790 (1999) P.Mohr, H.Oberhummer, Gy.Gyurky, E.Somorjai, A.Z.Kiss, I.Borbely-Kiss Absolute Measurement of the 5/2+ Resonance of 36Ar(p, γ)37K at Ep = 918 keV NUCLEAR REACTIONS 36Ar(p, γ), E=914-924 keV; measured Eγ, Iγ; deduced resonance absolute strength.
doi: 10.1103/PhysRevC.59.1790
1999MO16 Phys.Rev. C59, 3410 (1999) P.Mohr, P.V.Sedyshev, H.Beer, W.Stadler, H.Oberhummer, Yu.P.Popov, W.Rochow Neutron Capture of 46Ca at Thermonuclear Energies NUCLEAR REACTIONS 46Ca(n, γ), E ≈ thermal-200 keV; measured σ; deduced s-wave resonance role. Activation technique. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.59.3410
1999MO22 Phys.Rev. C60, 017603 (1999) P.Mohr, H.Beer, H.Oberhummer, W.Rochow, P.V.Sedyshev, S.Volz, A.Zilges Neutron Capture of 26Mg at kT = 52 keV and the Resonance at En = 68.7 keV NUCLEAR REACTIONS 26Mg(n, γ), E=spectrum; measured activation σ; deduced resonance strength, Maxwellian averaged capture σ.
doi: 10.1103/PhysRevC.60.017603
1999SE16 Phys.Rev. C60, 054613 (1999) P.V.Sedyshev, P.Mohr, H.Beer, H.Oberhummer, Yu.P.Popov, W.Rochow Measurement of Neutron Capture on 50Ti at Thermonuclear Energies NUCLEAR REACTIONS 50Ti(n, γ), E=25, 30, 52, 145 keV; measured capture σ; deduced Maxwellian averaged σ, stellar reaction rates. 51Ti deduced resonance width. Activation technique, enriched target, HPGe detector.
doi: 10.1103/PhysRevC.60.054613
1998EF05 Eur.Phys.J. A 1, 447 (1998) V.D.Efros, H.Oberhummer, A.Pushkin, I.J.Thompson Low-Energy Photodisintegration of 9Be and α + α + n ← → 9Be + γ Reactions at Astrophysical Conditions NUCLEAR REACTIONS 9Be(γ, n), E=1.6-2.2 MeV; calculated photodisintegration σ; deduced astrophysical reaction rates. Comparison with data. NUCLEAR STRUCTURE 9Be; calculated ground state, continuum wavefunctions. Three-body model.
doi: 10.1007/s100500050079
1998HE25 Phys.Rev. C58, 1798 (1998) H.Herndl, M.Fantini, C.Iliadis, P.M.Endt, H.Oberhummer Thermonuclear Reaction Rate of 23Mg(p, γ)24Al NUCLEAR REACTIONS 23Mg(p, γ), E not given; calculated reaction rate vs stellar temperature; deduced parameters. Comparison with previous results. Astrophysical implications.
doi: 10.1103/PhysRevC.58.1798
1998MO17 Phys.Rev. C58, 932 (1998) P.Mohr, H.Beer, H.Oberhummer, G.Staudt Neutron Capture of 26Mg at Thermonuclear Energies NUCLEAR REACTIONS 26Mg(n, γ), E=25-208 keV spectra; measured σ; deduced resonance features, astrophysical reaction rates. Fast cyclic activation technique.
doi: 10.1103/PhysRevC.58.932
1998RA08 Phys.Rev. C57, 2031 (1998) T.Rauscher, R.Bieber, H.Oberhummer, K.-L.Kratz, J.Dobaczewski, P.Moller, M.M.Sharma Dependence of Direct Neutron Capture on Nuclear-Structure Models NUCLEAR STRUCTURE 124,126,128,130,132,134,136,138,140,142,144Sn, 208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238Pb; calculated neutron capture σ. Several structure models compared.
doi: 10.1103/PhysRevC.57.2031
1998SO07 Astron.Astrophys. 333, 1112 (1998) E.Somorjai, Zs.Fulop, A.Z.Kiss, C.E.Rolfs, H.P.Trautvetter, U.Greife, M.Junker, S.Goriely, M.Arnould, M.Rayet, T.Rauscher, H.Oberhummer Experimental Cross Section of 144Sm(α, γ)148Gd and Implications for the p-Process NUCLEAR REACTIONS 144Sm(α, γ), E=10.5-13.4 MeV; measured σ; deduced astrophysical S-factors, stellar production ratio. Activation method. Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0416. 1998VA08 Phys.Rev. C57, 2711 (1998) G.Vancraeynest, P.Decrock, M.Gaelens, M.Huyse, P.Van Duppen, C.R.Bain, T.Davinson, R.D.Page, A.C.Shotter, P.J.Woods, F.Binon, P.Duhamel, J.Vanhorenbeeck, R.Coszach, Th.Delbar, W.Galster, J.Graulich, P.Leleux, E.Lienard, P.Lipnik, C.Michotte, A.Ninane, J.Vervier, H.Herndl, H.Oberhummer, Cs.Sukosd, M.Wiescher 19Ne(p, γ)20Na and 19Ne(d, n)20Na Reactions and Its Astrophysical Implications for the Transition of the Hot CNO Cycle to the rp Process NUCLEAR REACTIONS 1H(19Ne, γ), E(cm)=0.6-1.8 MeV; 2H(19Ne, n), E(cm)=0.6-1.8 MeV; measured σ; deduced astrophysical reaction rates. 20Na deduced resonance properties. DWBA analysis. Radioactive beam.
doi: 10.1103/PhysRevC.57.2711
1997BE42 Nucl.Phys. A621, 235c (1997) H.Beer, C.Coceva, R.Hofinger, P.Mohr, H.Oberhummer, P.V.Sedyshev, Yu.P.Popov Measurement of Direct Neutron Capture by Neutron-Rich Sulfur Isotopes NUCLEAR REACTIONS 34,36S(n, γ), E=reactor; measured Eγ, Iγ; deduced capture σ. 35,37S deduced levels, J, π, spectroscopic factors. Direct capture model.
doi: 10.1016/S0375-9474(97)00244-3
1997IV02 Nucl.Phys. A617, 414 (1997); Erratum Nucl.Phys. A625, 896 (1997) A.N.Ivanov, N.I.Troitskaya, M.Faber, H.Oberhummer On the Relativistic Field Theory Model of the Deuteron II NUCLEAR REACTIONS 1H(n, γ), E=low; 1H(p, X), E=low; calculated radiative capture, fusion σ respectively. Relativistic field theory model.
doi: 10.1016/S0375-9474(97)00016-X
1997IV04 Z.Phys. A358, 81 (1997) A.N.Ivanov, N.I.Troitskaya, M.Faber, H.Oberhummer On the S-Wave πD-Scattering Length in the Relativistic Field Theory Model of the Deuteron NUCLEAR REACTIONS 2H(π, π), E not given; calculated S-wave scattering length; deduced importance of Δ-resonance.
doi: 10.1007/s002180050279
1997MO04 Phys.Rev. C55, 1523 (1997) P.Mohr, T.Rauscher, H.Oberhummer, Z.Mate, Zs.Fulop, E.Somorjai, M.Jaeger, G.Staudt 144Sm-α Optical Potential at Astrophysically Relevant Energies Derived from 144Sm(α, α)144Sm Elastic Scattering NUCLEAR REACTIONS 144Sm(α, α), E=20 MeV; measured σ(θ); deduced optical parameters at astrophysically relevant energy, very limited uncertainities.
doi: 10.1103/PhysRevC.55.1523
1997MO06 Phys.Rev. C55, 1591 (1997) P.Mohr, H.Herndl, H.Oberhummer Spectroscopic Factors for Bound s-Wave States Derived from Neutron Scattering Lengths NUCLEAR STRUCTURE 13,14C, 16N, 17,19O, 23Ne, 37,41Ar; calculated bound s-states associated neutron single-particle spectroscopic factors. Model independent method.
doi: 10.1103/PhysRevC.55.1591
1997MO17 Phys.Rev. C56, 1154 (1997) P.Mohr, H.Oberhummer, H.Beer, W.Rochow, V.Kolle, G.Staudt, P.V.Sedyshev, Yu.P.Popov Direct Neutron Capture of 48Ca at kT = 52 keV NUCLEAR REACTIONS 48Ca, 197Au(n, γ), E < 0.1 MeV; measured Eγ, Iγ; deduced neutron capture σ. Direct capture model. Activation technique.
doi: 10.1103/PhysRevC.56.1154
1997MO27 Phys.Rev.Lett. 79, 3837 (1997) R.Morlock, R.Kunz, A.Mayer, M.Jaeger, A.Muller, J.W.Hammer, P.Mohr, H.Oberhummer, G.Staudt, V.Kolle Halo Properties of the First (1/2)+ State in 17F from the 16O(p, γ)17F Reaction NUCLEAR REACTIONS, ICPND 16O(p, p), (p, γ), E(cm)=200-3750 keV; measured Eγ, Iγ, elastic, capture σ(E). 17F deduced halo state properties. Direct capture model.
doi: 10.1103/PhysRevLett.79.3837
1997MO33 Phys.Rev. C56, 3425 (1997) P.Mohr, H.Herndl, H.Oberhummer, G.Staudt Reply to ' Comment on ' Spectroscopic Factors for Bound s-Wave States Derived from Neutron Scattering Lengths ' '
doi: 10.1103/PhysRevC.56.3425
1997PI07 Nucl.Phys. A618, 55 (1997) R.Pichler, H.Oberhummer, A.Csoto, S.A.Moszkowski Three-Alpha Structure in 12C NUCLEAR STRUCTURE 12C; calculated three-body resonances, Γ. Microscopic cluster model, complex scaling method.
doi: 10.1016/S0375-9474(97)00057-2
1997RA23 Nucl.Phys. A621, 327c (1997) T.Rauscher, K.-L.Kratz, H.Oberhummer, J.Dobaczewski, P.Moller, M.Sharma Uncertainties in Direct Neutron Capture Calculations Due to Nuclear Structure Models NUCLEAR REACTIONS 124,126,128,130,132,134,136,138,140,142,144Sn(n, γ), E(cm)=30 keV; calculated capture σ; deduced accuracy of models far from stability. Optical potential, several models compared.
doi: 10.1016/S0375-9474(97)00265-0
1997SO19 Nucl.Phys. A621, 293c (1997) E.Somorjai, Zs.Fulop, A.Z.Kiss, C.Rolfs, H.-P.Trautvetter, U.Greife, M.Junker, M.Arnould, M.Rayet, H.Oberhummer Experimental Cross Section of 144Sm(α, γ)148Gd NUCLEAR REACTIONS, ICPND 144Sm(α, γ), E=10.5-13.4 MeV; measured residual nucleus α-decay; deduced production σ. Activation method, solid state nuclear track detectors. Statistical model calculations.
doi: 10.1016/S0375-9474(97)00258-3
1996BE53 Phys.Rev. C54, 2014 (1996) H.Beer, C.Coceva, P.V.Sedyshev, Yu.P.Popov, H.Herndl, R.Hofinger, P.Mohr, H.Oberhummer Measurement of Neutron Capture on 48Ca at Thermal and Thermonuclear Energies NUCLEAR REACTIONS 48Ca(n, γ), E=25.3 meV, 25-218 keV; measured capture σ, Eγ, Iγ. 49Ca levels deduced spectroscopic factors. Direct capture model, Saxon-Woods potential, folding potential, nuclear Ramsauer effect.
doi: 10.1103/PhysRevC.54.2014
1996CS02 Phys.Rev. C53, 1589 (1996) A.Csoto, H.Oberhummer, R.Pichler Searching for Three-Nucleon Resonances NUCLEAR STRUCTURE 3n; calculated phase shifts; deduced resonances, J, π. 3H deduced possible excited state.
doi: 10.1103/PhysRevC.53.1589
1996EF02 Z.Phys. A355, 101 (1996) V.D.Efros, W.Balogh, H.Herndl, R.Hofinger, H.Oberhummer Reaction Rate for Two-Neutron Capture by 4He NUCLEAR REACTIONS 5He(n, γ), E ≤ 1 MeV; 6He(γ, n), E ≈ 2-8 MeV; calculated σ(E); 6He(γ, 2n), E not given; calculated photodisintegration reaction rate vs temperature; comparison with 6He(α, n) reaction rate. Two-step mechanism, 4He(2n, γ) reaction rate also evaluated.
doi: 10.1007/s002180050084
1996EF03 Phys.Rev. C54, 1485 (1996) Ground-State Energies and Widths of 5He and 5Li Nuclei NUCLEAR REACTIONS 3H, 3He(d, γ), E not given; analyzed data analyses. 5He, 5Li deduced level energy, Γ. Comparison with other work.
doi: 10.1103/PhysRevC.54.1485
1996FU11 Z.Phys. A355, 203 (1996) Zs.Fulop, A.Z.Kiss, E.Somorjai, C.E.Rolfs, H.P.Trautvetter, T.Rauscher, H.Oberhummer 70Ge(α, γ)74Se Cross Section Measurements at Energies of Astrophysical Interest NUCLEAR REACTIONS, ICPND 70Ge(α, γ), E=5.05-7.8 MeV; measured Eγ, Iγ, γγ-coin; deduced σ(E), astrophysical S-factor vs E, (α, γ), (γ, α) reaction rates. Statistical model comparison.
doi: 10.1007/s002180050099
1996KR01 Phys.Rev. C53, 469 (1996) E.Krausmann, W.Balogh, H.Oberhummer, T.Rauscher, K.-L.Kratz, W.Ziegert Direct Neutron Capture for Magic-Shell Nuclei NUCLEAR REACTIONS 48Ca(n, γ), E ≤ 1 MeV; calculated capture, Maxwellian-averaged σ(E). Also evaluated 50Ca(n, γ) reaction σ.
doi: 10.1103/PhysRevC.53.469
1995BE55 Phys.Rev. C52, 3442 (1995) H.Beer, P.V.Sedyshev, Yu.P.Popov, W.Balogh, H.Herndl, H.Oberhummer Cross Section of 36S(n, γ)37S NUCLEAR REACTIONS 36S(n, γ), E=25, 151, 176, 218 keV; measured σ(n, γ), direct capture; deduced stellar reaction rate factor. Fast cyclic activation technique. Samples of elemental sufur enriched in 36S.
doi: 10.1103/PhysRevC.52.3442
1994KW03 J.Phys.(London) G20, 1919 (1994) E.Kwasniewicz, H.Herndl, H.Oberhummer Spectroscopic Amplitudes for One-Nucleon Transfer between 1p0f-Shell Nuclei NUCLEAR STRUCTURE 42,47,41,43,45Ca, 44,46Sc; calculated one-nucleon transfer spectroscopic factors. Shell model approach.
doi: 10.1088/0954-3899/20/12/008
1994MO17 Phys.Rev. C50, 1543 (1994) P.Mohr, V.Kolle, S.Wilmes, U.Atzrott, G.Staudt, J.W.Hammer, H.Krauss, H.Oberhummer Direct Capture in the 3+ Resonance of 2H(α, γ)6Li NUCLEAR REACTIONS, ICPND 2H(α, γ), E=2-2.5 MeV; measured Eγ, Iγ; deduced σ(E), folding potential parameters.
doi: 10.1103/PhysRevC.50.1543
1994MO27 Z.Phys. A349, 339 (1994) P.Mohr, H.Abele, V.Kolle, G.Staudt, H.Oberhummer, H.Krauss Properties of 8Be and 12C Deduced from the Folding-Potential Model NUCLEAR REACTIONS, ICPND 4He(α, α), E ≈ 7-35 MeV; analyzed σ(θ); deduced model potential parameters. 4He(α, γ), E(cm)=1.5-3.5 MeV; 8Be(α, γ), E not given; calculated σ(E), astrophysical S-factor, Γγ. Double-folded potential. NUCLEAR STRUCTURE 8Be, 12C; calculated levels, B(λ). α-cluster states, double-folded potential.
doi: 10.1007/BF01288987
1994OB03 Z.Phys. A349, 241 (1994) H.Oberhummer, H.Krauss, K.Grun, T.Rauscher, H.Abele, P.Mohr, G.Staudt Alpha Clustering and the Stellar Nucleosynthesis of Carbon NUCLEAR REACTIONS 12C(γ, α), E=low; calculated triple-α process reaction rate. Direct capture, α-clustering.
doi: 10.1007/BF01288967
1993DE25 Phys.Rev. C48, 2057 (1993) P.Decrock, M.Gaelens, M.Huyse, G.Reusen, G.Vancraeynest, P.Van Duppen, J.Wauters, Th.Delbar, W.Galster, P.Leleux, I.Licot, E.Lienard, P.Lipnik, C.Michotte, J.Vervier, H.Oberhummer Study of the 13N(d, n)14O Reaction Cross Section and Its Astrophysical Implications for the 13N Proton Capture Reaction NUCLEAR REACTIONS, ICPND 2H(13N, n), E=8.2-28.5 MeV; measured Eγ, Iγ; deduced 13N(d, n) reaction σ(E), astrophysical implications. 14O level deduced spectroscopic factor. 13C, 13N(p, γ), E(cm) ≤ 1 MeV; calculated astrophysical S-factor.
doi: 10.1103/PhysRevC.48.2057
1993KR18 Ann.Phys.(Leipzig) 2, 258 (1993) H.Krauss, K.Grun, T.Rauscher, H.Oberhummer The Astrophysical S-Factor of the Reaction 7Be(p, γ)8B in the Direct Capture Model NUCLEAR REACTIONS, ICPND 7Be(p, γ), E(cm) ≤ 2 MeV; calculated σ(E), astrophysical S-factor vs E. 7Li(n, γ), E(cm) ≤ 1 MeV; calculated σ(E). Direct capture model.
doi: 10.1002/andp.19935050304
1993MO11 Phys.Rev. C48, 1420 (1993) P.Mohr, H.Abele, R.Zwiebel, G.Staudt, H.Krauss, H.Oberhummer, A.Denker, J.W.Hammer, G.Wolf Alpha Scattering and Capture Reactions in the A = 7 System at Low Energies NUCLEAR REACTIONS, ICPND 4He(3He, 3He), E=1.2-3 MeV; measured σ(θ). 4He(3He, 3He), (t, t), E ≤ 10 MeV; analyzed phase shifts data. 3H, 3He(α, γ), E(cm) ≤ 1 MeV; calculated astrophysical S-factor vs E; deduced multipole contributions.
doi: 10.1103/PhysRevC.48.1420
1993OB01 Yad.Fiz. 56, No 7, 129 (1993); Phys.Atomic Nuclei 56, 928 (1993) Reaction Mechanisms for Astrophysically Relevant Nuclear Processes NUCLEAR REACTIONS 8Li(α, n), E=low; compiled different analyses of reaction rates. Different mechanisms.
1992RA04 Phys.Rev. C45, 1996 (1992) T.Rauscher, K.Grun, H.Krauss, H.Oberhummer, E.Kwasniewicz Analysis of 8Li(α, n)11B Below the Coulomb Barrier in the Potential Model NUCLEAR REACTIONS, ICPND 8Li(α, n), E(cm) ≤ 1 MeV; calculated astrophysical S-factor vs E, reaction rates. DWBA, folding potentials.
doi: 10.1103/PhysRevC.45.1996
1992WI09 J.Phys.(London) G18, L147 (1992) S.Winkler, H.Krauss, K.Grun, T.Rauscher, H.Oberhummer, H.Abele, G.Staudt Calculation of the 3He(3He, 2p)4He and 3H(3H, 2n)4He Astrophysical S Factor at Low Energies NUCLEAR REACTIONS, ICPND 3He(3He, 2p), E(cm) ≤ 1 MeV; analyzed astrophysical S-factor vs E. 3H(t, 2n), E ≤ 0.35 MeV; analyzed σ(E), astrophysical S-factor vs E. Potential model.
doi: 10.1088/0954-3899/18/8/004
1991HE16 Phys.Rev. C44, R952 (1991) H.Herndl, H.Abele, G.Staudt, B.Bach, K.Grun, H.Scsribany, H.Oberhummer, G.Raimann Direct Reaction Analysis of 19F(p, α)16O Below the Coulomb Barrier NUCLEAR REACTIONS, ICPND 19F(p, α), E=150-900 keV; analyzed σ(θ) vs E; deduced astrophysical S-factor, reaction mechanism. DWBA.
doi: 10.1103/PhysRevC.44.R952
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
1988WA10 J.Phys.(London) G14, L91 (1988) M.Walz, R.Neu, G.Staudt, H.Oberhummer, H.Cech Absolute Magnitude of (p, α) and (α, p) Cross Sections - New Results Concerning a Long-Standing Problem NUCLEAR REACTIONS 27Al(polarized p, α), E=35 MeV; calculated σ(θ), analyzing power vs θ. 27Al(p, p), E=24.5-46 MeV; 24Mg(α, α), E=28-50.1 MeV; 27Al(p, α), E=24-45 MeV; 42Ca(p, p), E=26.5 MeV; 40Ca(α, α), E=36.2 MeV; 40Ca(α, p), E=35.6 MeV; calculated σ(θ). Double-folded α-potentials.
doi: 10.1088/0305-4616/14/5/005
1985HO02 Phys.Rev. C31, 17 (1985) F.Hoyler, H.Oberhummer, T.Rohwer, G.Staudt, H.V.Klapdor Microscopic and Semimicroscopic Analysis of the Reaction 27Al(p, α)24Mg in the Energy Range between 20 and 45 MeV NUCLEAR REACTIONS 27Al(p, α), E=20, 24, 30.5, 45 MeV; measured σ(Eα, θ); deduced normalization factors. Microscopic, semi-microscopic DWBA analysis.
doi: 10.1103/PhysRevC.31.17
1983BR07 Nucl.Phys. A398, 84 (1983) F.Brunner, H.H.Muller, C.Dorninger, H.Oberhummer Absolute Normalisation in Microscopic DWBA Analysis of the Three-Nucleon Transfer-Reaction Cross Sections NUCLEAR REACTIONS 94,92,90Zr, 89Y, 58Ni, 56Fe, 55Mn, 27Al(p, α), E not given; analyzed data; deduced normalization constants. Microscopic, zero-range, finite-range DWBA analyses.
doi: 10.1016/0375-9474(83)90648-6
1983OB01 Nucl.Phys. A401, 415 (1983) H.Oberhummer, W.Pfeifer, F.Brunner, H.H.Muller Microscopic Model for the Transfer Reactions (N, α) and (α, N) using the Isospin Formalism NUCLEAR REACTIONS 27Al(polarized p, α), E=34.73 MeV; measured σ(Eα, θ), analyzing power vs Eα, θ. 27Al, 24Mg deduced wave functions. Enriched target. Microscopic model, three-nucleon transfer.
doi: 10.1016/0375-9474(83)90358-5
1981CE03 Nucl.Phys. A357, 191 (1981) H.Cech, H.Jasicek, H.Oberhummer, F.Brunner, H.H.Muller An Investigation of the Importance of Multi-Step Processes in the Three-Nucleon (p, α) Transfer Reactions NUCLEAR REACTIONS 56Fe, 55Mn(p, α), 92Zr(polarized p, α), E=35 MeV; calculated σ(θ); deduced role of multi-step processes. DWBA, sequential, inelastic transfers.
doi: 10.1016/0375-9474(81)90633-3
1981ED02 Acta Phys.Austr. 53, 79 (1981) A Single Particle Potential for Bound States in Spherical Nuclei NUCLEAR STRUCTURE 40,48Ca, 88Sr, 208Pb; calculated charge distributions; 40,48Ca, 60Ni, 88Sr, 114,120Sn, 140Ce, 208Pb, 238U; calculated nucleon, charge distribution rms radii. Nonlocal Saxon-Woods potential.
1980BR07 J.Phys.(London) G6, 473 (1980) F.Brunner, H.Cech, H.H.Muller, G.Ratel, H.Jasicek, H.Oberhummer A Finite-Range Cluster-Model Description of the Three-Nucleon Transfer Reaction (p, α) NUCLEAR REACTIONS 27Al(p, α), 92Zr(polarized p, α), E=35 MeV; analyzed σ(θ), A(θ); deduced finite-range effects in cluster model. Exact finite-range DWBA, cluster model form factor.
doi: 10.1088/0305-4616/6/4/016
1980BR32 Helv.Phys.Acta 53, 310 (1980) F.Brunner, H.H.Muller, W.Reichart, P.Schober, H.Jasicek, H.Oberhummer, W.Pfeifer Microscopic Analysis of the Three-Nucleon Transfer Reaction 27Al(p, α)24Mg Induced with Polarized Protons NUCLEAR REACTIONS 27Al(polarized p, α), E=34.73 MeV; measured σ(θ), analyzing power vs θ. DWBA, shell model form factors.
1980MU15 Helv.Phys.Acta 53, 314 (1980) H.H.Muller, P.Schober, K.Preisinger, H.Jasicek, H.Oberhummer, P.Riehs An Investigation of Shell Model Wave Functions of 56Fe and 53Mn by the (p, α)-Reaction using a Full Microscopic Description NUCLEAR REACTIONS 56Fe(p, α), E=34 MeV; measured σ(θ); deduced form factor interference effects. DWBA, shell model form factors.
1980OB02 Nuovo Cim. A55, 253 (1980) A Microscopic Finite-Range Analysis of (N, α) and (α, N) Reactions NUCLEAR REACTIONS 92Zr(polarized p, α), E=35 MeV; analyzed σ(θ), analyzing power vs θ. Microscopic finite range analysis.
doi: 10.1007/BF02902463
1979PR13 Nucl.Phys. A332, 278 (1979) K.Preisinger, H.Jasicek, H.Oberhummer, P.Riehs, H.H.Muller, P.Schober An Investigation of Shell Model Wave Functions of 56Fe and 53Mn by the (p, α) Reaction Using a Full Microscopic Description NUCLEAR REACTIONS 56Fe(p, α), E=34 MeV; measured σ(Eα, θ). 56Fe, 53Mn deduced wave functions. Enriched target.
doi: 10.1016/0375-9474(79)90002-2
1978FA14 Acta Phys.Aust. 49, 125 (1978) M.Faber, H.Jasicek, H.Oberhummer Schalenkorrekturen zur Deformationsenergie fur rotierende Kerne NUCLEAR STRUCTURE 240Pu; calculated dynamical moment of inertia. Saxon-Woods potential. Compared with geometrical value, Nilsson model.
1978GU17 Phys.Rev. C18, 1626 (1978) H.Guyer, V.Meyer, H.H.Muller, W.Reichart, H.Jasicek, H.Oberhummer, P.Riehs, R.Wagner, W.Pfeifer Microscopic Analysis of the Three-Particle Transfer Reaction 92Zr(p, α)89Y NUCLEAR REACTIONS 92Zr(p, α), E=35 MeV; measured σ(θ). Microscopic DWBA analysis.
doi: 10.1103/PhysRevC.18.1626
1978GU20 Helv.Phys.Acta 51, 97 (1978) H.Guyer, V.Meyer, H.H.Muller, W.Reichart, P.Schober, H.Jasicek, H.Oberhummer, P.Riehs, R.Wagner, W.Pfeifer A Microscopic Analysis of the Low Lying Levels in 86Sr with the Reaction 89Y(p, α)86Sr NUCLEAR REACTIONS 89Y(p, α), E=34 MeV; measured σ(θ). 88Sr levels deduced configurations. DWBA analysis with microscopic form factors.
1978RA19 Lett.Nuovo Cim. 23, 241 (1978) G.Ratel, V.Meyer, H.H.Muller, W.Reichart, P.Schober, H.Jasicek, H.Oberhummer, P.Riehs, R.Wagner Analysis of the Three-Nucleon Transfer Reaction (p, α) Induced with Polarized Protons NUCLEAR REACTIONS 92Zr(polarized p, α), E=35 MeV; measured σ(θ), A(Eα, θ).
doi: 10.1007/BF02778080
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