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NSR database version of May 6, 2024.

Search: Author = P.Bano

Found 3 matches.

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2023BA18      Phys.Rev. C 108, 015802 (2023)

P.Bano, S.P.Pattnaik, M.Centelles, X.Vinas, T.R.Routray

Correlations between charge radii differences of mirror nuclei and stellar observables

NUCLEAR STRUCTURE 34,36S, 34,38Ar, 36Ca, 38Ca, 54Fe, 54Ni; calculated rms proton radii differences of mirror nuclei and correlation with neutron skin thickness, slope of the symmetry energy, tidal deformability and neutron star radius correlation to charge radii difference in mirror pairs and neutron skin thickness. Investigated isospin-symmetry breaking effect leading to a linear correlation between the proton rms radii difference in mirror pairs and neutron skin thickness. Simple effective interaction (SEI) finite-range model.

doi: 10.1103/PhysRevC.108.015802
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2022BA29      Phys.Rev. C 106, 024313 (2022)

P.Bano, X.Vinas, T.R.Routray, M.Centelles, M.Anguiano, L.M.Robledo

Finite-range simple effective interaction including tensor terms

NUCLEAR STRUCTURE 68,70,72,74,76,78Ni; calculated ground-state energies, neutron and proton single-particle levels around the Fermi level. 58,59,60,61,62,63,64,65,66,67,68,69,70Ni; calculated rms charge radii, isotope shifts. 69,71,73,75,77,79Cu; calculated ground-state energies. 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132Sn; calculated energy differences between 1h11/2 and 1g7/2 proton orbitals, single-particle neutron energies and their occupation probabilities. 132Sn, 134Te, 136Xe, 138Ba, 140Ce, 142Nd, 144Sm, 146Gd, 148Dy, 150Er; calculated energy differences between 1i13/2 and 1h9/2 neutron single-particle levels, and single-particle proton energies and their occupation probabilities in N=82 isotones. 91Zr, 93Mo, 95Ru, 97Pd, 99Cd, 101Sn; calculated neutron single-particle levels in N=51 isotones relative to the 2d5/2 level. Calculations based on simple effective interaction (SEI) with and without the addition of a short-range tensor force to SEI and SIII-T, SLy5-T, SAMi-T Skyrme and D1MTd Gogny effective interaction. Comparison with available experimental data.

doi: 10.1103/PhysRevC.106.024313
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2021RO19      Phys.Rev. C 104, L011302 (2021)

T.R.Routray, P.Bano, M.Anguiano, M.Centelles, X.Vinas, L.M.Robledo

Reexamination of the N=50 and Z=28 shell closure

NUCLEAR STRUCTURE 68,70,72,74,76,78Ni; calculated proton single-particle levels around the Fermi level. 69,71,73,75,77,79Cu; calculated energies and spins of the ground states, and energies of the first excited states. Quasilocal density functional theory (QLDFT) using Skyrme forces SAMi-T and SLy5 with the tensor part, D1M Gogny force, and simple effective interaction (SEI) model. Comparison with HFB calculations, and with experimental energies and spins of the first excited states.

doi: 10.1103/PhysRevC.104.L011302
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