NSR Query Results


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NSR database version of May 24, 2024.

Search: Author = H.Oberhummer

Found 73 matches.

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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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23148.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23330. Data from this article have been entered in the XUNDL database. For more information, click here.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22984.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22808.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0375.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0375.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22427.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22500.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22485.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22419.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22446.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0525.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22416.


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
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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
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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
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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
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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
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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
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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
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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
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1996EF03      Phys.Rev. C54, 1485 (1996)

V.D.Efros, H.Oberhummer

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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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1993OB01      Yad.Fiz. 56, No 7, 129 (1993); Phys.Atomic Nuclei 56, 928 (1993)

H.Oberhummer, T.Rauscher

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
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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
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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
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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
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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
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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
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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
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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
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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
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1981ED02      Acta Phys.Austr. 53, 79 (1981)

G.Eder, H.Oberhummer

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
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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)

H.Oberhummer

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
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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
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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
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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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