NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = E.Baldini-Neto Found 10 matches. 2006BA23 J.Phys.(London) G32, 655 (2006) E.Baldini-Neto, B.V.Carlson, D.Hirata Self-consistent Dirac quasi-particle blocking approximation applied to the α-decay scheme of the superheavy element 287115 NUCLEAR STRUCTURE 63,64,65,66,67,68Ga, 65,66,67,68,69,70Ge, 67,68,69,70,71,72As, 69,70,71,72,73Se, 72,73,74,75Br; calculated binding energies, radii, β2. 287,288Mc, 283,284Nh, 279,280Rg, 275,276Mt, 271,272Bh, 268Db; calculated binding energies, β2, level energies and configurations.Dirac-Hartree-Bogoliubov formalism. RADIOACTIVITY 287Mc, 283Nh, 279Rg, 275Mt(α); calculated Qα, T1/2. Dirac-Hartree-Bogoliubov formalism.
doi: 10.1088/0954-3899/32/5/005
2004BA18 Braz.J.Phys. 34, 773 (2004) E.Baldini-Neto, B.V.Carlson, R.A.Rego, M.S.Hussein p+6, 8He Elastic Scattering at Intermediate Energies NUCLEAR REACTIONS 6,8He(p, p), E ≈ 0.7 GeV; calculated σ(θ), analyzing power. Relativistic optical potential. NUCLEAR STRUCTURE 4,6,8He; calculated radii.
doi: 10.1590/s0103-97332004000500017
2004BA21 Braz.J.Phys. 34, 855 (2004) E.Baldini-Neto, B.V.Carlson, D.Hirata Dirac-Hartree-Bogoliubov Approximation for Finite Nuclei with Blocking NUCLEAR STRUCTURE O, Ni, Ca, Sn; calculated mass defects. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data. RADIOACTIVITY 277Cn, 273Ds, 269Hs, 265Sg, 261Rf, 257No, 253Fm, 249Cf(α); calculated Qα. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data.
doi: 10.1590/s0103-97332004000500039
2004BB18 Braz.J.Phys. 34, 773 (2004) E.Baldini-Neto, B.V.Carlson, R.A.Rego, M.S.Hussein p+6, 8He Elastic Scattering at Intermediate Energies NUCLEAR REACTIONS 6,8He(p, p), E ≈ 0.7 GeV; calculated σ(θ), analyzing power. Relativistic optical potential. NUCLEAR STRUCTURE 4,6,8He; calculated radii.
doi: 10.1590/S0103-97332004000500017
2004BB21 Braz.J.Phys. 34, 855 (2004) E.Baldini-Neto, B.V.Carlson, D.Hirata Dirac-Hartree-Bogoliubov Approximation for Finite Nuclei with Blocking NUCLEAR STRUCTURE O, Ni, Ca, Sn; calculated mass defects. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data. RADIOACTIVITY 277Cn, 273Ds, 269Hs, 265Sg, 261Rf, 257No, 253Fm, 249Cf(α); calculated Qα. Dirac-Hartree-Bogoliubov approximation with blocking, comparison with data.
doi: 10.1590/S0103-97332004000500039
2004LI29 Nucl.Phys. A735, 303 (2004) G.F.Lima, A.Lepine-Szily, A.C.C.Villari, W.Mittig, R.Lichtenthaler, M.Chartier, N.A.Orr, J.C.Angelique, G.Audi, E.Baldini-Neto, B.V.Carlson, J.M.Casandjian, A.Cunsolo, C.Donzaud, A.Foti, A.Gillibert, D.Hirata, M.Lewitowicz, S.Lukyanov, M.MacCormick, D.J.Morrissey, A.N.Ostrowski, B.M.Sherrill, C.Stephan, T.Suomijarvi, L.Tassan-Got, D.J.Vieira, J.M.Wouters Reaction cross section and matter radius measurements of proton-rich Ga, Ge, As, Se and Br nuclides NUCLEAR REACTIONS Si(63Ga, X), (64Ga, X), (65Ga, X), (66Ga, X), (67Ga, X), (68Ga, X), (65Ge, X), (66Ge, X), (67Ge, X), (68Ge, X), (69Ge, X), (70Ge, X), (67As, X), (68As, X), (69As, X), (70As, X), (71As, X), (72As, X), (69Se, X), (70Se, X), (71Se, X), (72Se, X), (73Se, X), (72Br, X), (73Br, X), (74Br, X), (75Br, X), E ≈ 50-60 MeV/nucleon; measured reaction σ. 63,64,65,66,67,68Ga, 65,66,67,68,69,70Ge, 67,68,69,70,71,72As, 69,70,71,72,73Se, 72,73,74,75Br; deduced matter radii. Glauber model analysis.
doi: 10.1016/j.nuclphysa.2004.01.125
2003BA19 Braz.J.Phys. 33, 250 (2003) E.Baldini-Neto, C.L.Lima, P.Van Isacker Binding Energies of Isoscalar and Isovector Ground States of N = Z Nuclei in the Interacting Boson Model NUCLEAR STRUCTURE 58Cu, 62Ga, 66As, 70Br, 74Rb, 78Y, 82Nb, 86Tc, 90Rh, 94Ag, 98In; calculated binding energies, level energies. Interacting boson model.
doi: 10.1590/s0103-97332003000200014
2003BA65 Nucl.Phys. A724, 345 (2003) E.Baldini-Neto, B.V.Carlson, R.A.Rego, M.S.Hussein p + 4, 6, 8He elastic scattering at intermediate energies NUCLEAR REACTIONS 4He(p, p), E=0.561, 0.8, 1.029 GeV; 6He(p, p), E=0.717 GeV; 8He(p, p), E=0.671 GeV; calculated σ(θ), analyzing power. Relativistic optical model, comparison with data and other models.
doi: 10.1016/S0375-9474(03)01540-9
2003BB19 Braz.J.Phys. 33, 250 (2003) E.Baldini-Neto, C.L.Lima, P.Van Isacker Binding Energies of Isoscalar and Isovector Ground States of N = Z Nuclei in the Interacting Boson Model NUCLEAR STRUCTURE 58Cu, 62Ga, 66As, 70Br, 74Rb, 78Y, 82Nb, 86Tc, 90Rh, 94Ag, 98In; calculated binding energies, level energies. Interacting boson model.
2002BA58 Phys.Rev. C65, 064303 (2002) E.Baldini-Neto, C.L.Lima, P.Van Isacker Binding Energies of T = 0 and T = 1 Ground States of N = Z Nuclei in the Interacting Boson Model NUCLEAR STRUCTURE 18F, 20Ne, 22Na, 24Mg, 26Al, 28Si, 30P, 32S, 34Cl, 36Ar, 38K, 58Cu, 60Zn, 62Ga, 64Ge, 66As, 68Se, 70Br, 72Kr, 74Rb, 76Sr, 78Y, 80Zr, 82Nb, 84Mo, 86Tc, 88Ru, 90Rh, 92Pd, 94Ag, 96Cd, 98In; calculated binding energies, energy differences between T=0 and T=1 states. Interacting boson model.
doi: 10.1103/PhysRevC.65.064303
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