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NSR database version of May 1, 2024.

Search: Author = R.J.Donangelo

Found 4 matches.

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2017RA17      Phys.Rev. C 96, 034602 (2017)

H.A.Radi, J.O.Rasmussen, R.J.Donangelo

Semiclassical calculations for the 156Gd (p, d) reaction

NUCLEAR REACTIONS 156Gd(p, d), (p, p), E=25 MeV; calculated real optical potentials (central + spin-orbit) for protons and deuterons, final deflection angles of 276, 983 protons and deuterons with respect to proton impact parameter, imaginary optical potentials protons and deuteron, survival probability as a function of impact parameter for protons and deuterons, angular distributions for deuterons and elastically scattered protons. 156,158Gd(p, d), E=25 MeV; calculated σ(θ) for L=0 transfer for deuterons corresponding to dominant 1/2[400] configuration, and compared with experimental data, and with DWBA calculations. Semiclassical calculations for neutron-pickup and proton elastic scattering, and three-body quantum approach.

doi: 10.1103/PhysRevC.96.034602
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1994AB32      Int.J.Mod.Phys. E3, 783 (1994)

G.Abal, L.F.Canto, R.J.Donangelo

A Mass Parameter for Nuclear Collective Motion from the Generator Coordinate Method

NUCLEAR STRUCTURE A=12-100; calculated mass parameter; deduced shell effects evidence. Generator coordinate method.

doi: 10.1142/S0218301394000218
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1990CA21      Phys.Lett. 241B, 295 (1990)

L.F.Canto, R.J.Donangelo, M.W.Guidry, A.F.Farhan, J.O.Rasmussen, P.Ring, M.A.Stoyer

Alder-Winther-De Boer Method Applied to Diabolical Two-Neutron Transfer

NUCLEAR REACTIONS 160Dy(208Pb, X), E=1100 MeV; calculated nucleon transfer probability fpr X=206Pb; deduced Berry phase signature.

doi: 10.1016/0370-2693(90)91645-R
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1981RH01      Phys.Rev. C24, 2747 (1981)

M.J.Rhoades-Brown, R.J.Donangelo, M.W.Guidry, R.E.Neese

Quantum-Mechanical and Classical-Limit Coupled-Channels Calculations for very Heavy Systems

NUCLEAR REACTIONS 160Gd(40Ar, 40Ar'), E=120-180 MeV; calculated collective state excitation probabilities. Coupled-channels calculation, quantum, classical limits.

doi: 10.1103/PhysRevC.24.2747
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