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NSR database version of April 29, 2024.

Search: Author = E.Holub

Found 13 matches.

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1986HO01      Phys.Rev. C33, 143 (1986)

E.Holub, D.Hilscher, G.Ingold, U.Jahnke, H.Orf, H.Rossner, W.P.Zank, W.U.Schroder, H.Gemmeke, K.Keller, L.Lassen, W.Lucking

Preequilibrium Neutron Emission in Fusion of 165Ho + 12C at 25 MeV per Nucleon

NUCLEAR REACTIONS 165Ho(12C, nX), E=300 MeV; measured σ(fragment θ, θn, En), neutron multiplicity; deduced neutron emission mechanism. Fermi-jet model.

doi: 10.1103/PhysRevC.33.143
Citations: PlumX Metrics


1984KO22      Nuovo Cim. 81A, 31 (1984)

M.Korolija, E.Holub, N.Cindro, D.Hilscher

Pre-Equilibrium Emission of Nucleons from Reactions Induced by Medium-Energy Heavy Ions

NUCLEAR REACTIONS 165Ho(20Ne, xn), E=220, 292, 402 MeV; 158Gd(12C, xn), E=103, 124, 150 MeV; 157Gd(13C, xn), E=110, 140, 160 MeV; 154Sm(16O, xn), E=151.9 MeV; 238U(16O, xn), E=315 MeV; analyzed fast neutron spectra; deduced initial exciton number, degrees of freedom number near equality. Preequilibrium models.


1983CA23      Z.Phys. A313, 227 (1983)

R.Caplar, I.Udovicic, E.Holub, D.Pocanic, N.Cindro

Isotopic Effects in the (n, p) Reaction Cross Section on Heavy Targets and the Statistical Preequilibrium Model

NUCLEAR REACTIONS 122,124,126,128,130Te(n, p), E=14.6 MeV; 128,130,131,132,134Xe(n, p), E=14.4 MeV; 180,182,183,184,186W, 188,189,190,192Os(n, p), E=14.7 MeV; calculated σ; deduced proton, neutron separation energy role. Statistical preequilibrium model.


1983HO13      Phys.Rev. C28, 252 (1983)

E.Holub, D.Hilscher, G.Ingold, U.Jahnke, H.Orf, H.Rossner

Neutron Emission in Central Heavy-Ion Collisions of 165Ho + 20Ne at 11, 14.6, and 20.1 MeV/Nucleon

NUCLEAR REACTIONS 165Ho(20Ne, nX), E=220, 290, 402 MeV; measured σ(En, θn, fragment θ, fragment E); deduced prefission neutron multiplicity, multiple chance fission probability. Harp-Miller-Berne model.

doi: 10.1103/PhysRevC.28.252
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1983HO26      Z.Phys. A314, 347 (1983)

E.Holub, M.Korolija, N.Cindro

Preequilibrium Emission of Nucleons from Reactions Induced by Medium-Energy Heavy Ions

NUCLEAR REACTIONS 153Gd(12C, X), E=103, 124, 150 MeV; 157Gd(13C, X), E=110, 140, 160 MeV; 154Sm(16O, X), (16O, F), E=152 MeV; 238U(16O, X), (16O, F), E=315 MeV; 165Ho(20Ne, X), (20Ne, F), E=220, 292, 402 MeV; calculated (evaporation residue)(n)-, fission(fragment)(n)-coin spectra; deduced preequilibrium neutron emission energy dependence. Exciton, equilibration models.

doi: 10.1007/BF01412931
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1983RO09      Phys.Rev. C27, 2666 (1983)

H.Rossner, D.Hilscher, E.Holub, G.Ingold, U.Jahnke, H.Orf, J.R.Huizenga, J.R.Birkelund, W.U.Schroder, W.W.Wilcke

Angular Distributions of Fragments from Fission Induced by 220-MeV 20Ne on Targets of 165Ho, 197Au, and 209Bi

NUCLEAR REACTIONS 165Ho, 197Au, 209Bi(20Ne, F), E=220 MeV; measured fission fragment σ(θ). 197Ir, 211Ac, 223Np, 175Re, 207Fr, 219Pa; deduced prefission multi-neutron induced angular momentum dealignment effect. Liquid drop, rotating liquid drop models, incomplete fusion, prefission particle emission mechanisms.

doi: 10.1103/PhysRevC.27.2666
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1982JA01      Phys.Rev.Lett. 48, 17 (1982)

U.Jahnke, H.H.Rossner, D.Hilscher, E.Holub

Global Increase of Near- and Below-Barrier Fusion for Heavier Systems

NUCLEAR REACTIONS 12C, 16O, 58,60,62,64Ni, 104,110Pd, 118,124Sn, 130Te(40Ar, xn), E(cm)=90-120 MeV; 154,144Sm, 110Pd(16O, xn), E(cm)=55-70 MeV; 110Pd, 124Sn, 130Te(12C, xn), 58,62,64Ni(86Kr, xn), E not given; measured neutron production σ; deduced σ(fusion, E), barrier dependence, shape distortions.

doi: 10.1103/PhysRevLett.48.17
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1981DR01      Phys.Lett. B98, 36 (1981)

D.M.Drake, M.Cates, N.Cindro, D.Pocanic, E.Holub

Gross Structure and Resonant Behaviour of 14C + 14C Elastic Scattering

NUCLEAR REACTIONS 14C(14C, 14C), E=23.4-58.4 MeV; measured σ(θ, E); deduced gross structure, resonant behavior. Optial model analysis.

doi: 10.1016/0370-2693(81)90362-2
Citations: PlumX Metrics


1981PO05      J.Phys.(London) G7, 389 (1981)

D.Pocanic, G.Vourvopoulos, X.Aslanoglou, E.Holub

Possible Evidence for the Existence of Intermediate Resonant Structure in the 9Be + 13C Heavy-Ion System

NUCLEAR REACTIONS 13C(9Be, α), E=8-22.75; measured σ(E, θ). 22Ne deduced possible intermediate resonances. Statistical analysis.

doi: 10.1088/0305-4616/7/3/014
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2155.


1980HO23      Z.Phys. A296, 341 (1980)

E.Holub, D.Pocanic, R.Caplar, N.Cindro

A Consistent Study of Precompound and Compound-Nucleus Emission Mechanisms in Neutron-Induced Reactions

NUCLEAR REACTIONS 45Sc, 55Mn, 56Fe, 59Co, 89Y, 93Nb, 103Rh, 169Tm, 175Lu, 181Ta, 197Au, 209Bi(n, n'), (n, p), (n, 2n), (n, 3n), E=4-24 MeV; calculated σ(E); deduced exciton model parameter K. Weisskopf-Ewing evaporation, precompound exciton models.

doi: 10.1007/BF01438529
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1979HO03      Z.Phys. A289, 421 (1979)

E.Holub, N.Cindro, O.Bersillon, J.Jary

Investigation of (n, 2n) Reactions by the Evaporation Process

NUCLEAR REACTIONS 45Sc, 56Fe, 59Co, 89Y, 93Nb, 103Rh, 148,150,152,154Sm, 169Tm, 175Lu, 197Au, 209Bi(n, 2n), E=5-20 MeV; calculated σ. Evaporation model; deduced reaction mechanism.

doi: 10.1007/BF01409395
Citations: PlumX Metrics


1977CI01      Phys.Rev.Lett. 39, 1135 (1977)

N.Cindro, F.Cocu, J.Uzureau, Z.Basrak, M.Cates, J.M.Fieni, E.Holub, Y.Patin, S.Plattard

Evidence for a Rotational Band in 24Mg and its Fragmentation: A Rotation-Vibration Coupling (Question)

NUCLEAR REACTIONS 12C(12C, α), E(cm)=6.85-15 MeV; measured σ(Eα, θ). 24Mg deduced resonances, J, π.

doi: 10.1103/PhysRevLett.39.1135
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1976HO15      J.Phys.(London) G2, 405 (1976)

E.Holub, N.Cindro

Study of Some Systematic Trends and Non-Equilibrium Effects in (n, 2n) Reactions for Nuclei Far from the Symmetry Line

NUCLEAR REACTIONS 84,86,88Sr, 93Nb, 113In, 134,136Ba(n, 2n), E=14.6 MeV; measured activation σ, isomeric σ ratios. Systematics. Natural targets; enriched, natural In target; Ge(Li) detector.

doi: 10.1088/0305-4616/2/6/009
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset30348.


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