NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = P.Avogadro Found 8 matches. 2013AV01 Phys.Rev. C 87, 014331 (2013) Efficient calculation for the quasiparticle random-phase approximation matrix NUCLEAR STRUCTURE 120Sn; calculated isoscalar monopole strength function. 208,210,212,214,216,218,220,222,224Pb; calculated chemical potentials, average pairing gaps, neutron pair transfer strengths. Iterative finite-amplitude (i-FAM) QRPA matrix finite-amplitude (m-FAM) methods. Discussed computational aspects of different FAM approaches.
doi: 10.1103/PhysRevC.87.014331
2013AV06 Phys.Rev. C 88, 044319 (2013) Role of pairing in the description of giant monopole resonances NUCLEAR STRUCTURE 90,92,94Zr, 92,96Mo, 106,108,110,112,114,116Cd, 112,114,116,118,120,122,124,174Sn, 144Sm, 204,206,208Pb; calculated centroids of isoscalar giant monopole resonances (ISGMR), pairing strengths. Fully self-consistent quasi-particle random phase approximation on top of Hartree Fock Bogoliubov, including density dependence of pairing interactions (HFB+QRPA+DDDI). Skyrme functionals (SLy5, SkM* and Skxs20). Comparison with experimental data.
doi: 10.1103/PhysRevC.88.044319
2012NA28 J.Phys.:Conf.Ser. 387, 012015 (2012) T.Nakatsukasa, S.Ebata, P.Avogadro, L.Guo, T.Inakura, K.Yoshida Density functional approaches to nuclear dynamics NUCLEAR STRUCTURE 120Sn; calculated isoscalar monopole γ strength function. 132,134,136,138,140Xe; calculated B(E1) strength distribution. Density functional approach.
doi: 10.1088/1742-6596/387/1/012015
2011AV06 Phys.Rev. C 84, 014314 (2011) Finite amplitude method for the quasiparticle random-phase approximation NUCLEAR STRUCTURE 174Sn; calculated transition strengths for isoscalar monopole 0+ excitation. Quasiparticle random-phase approximation (QRPA) with finite amplitude method.
doi: 10.1103/PhysRevC.84.014314
2011NA03 Acta Phys.Pol. B42, 609 (2011) T.Nakatsukasa, P.Avogadro, S.Ebata, T.Inakura, K.Yoshida Self-consistent Description of Nuclear Photoabsorption Cross-sections NUCLEAR REACTIONS 154Sm(γ, X), E<40 MeV; calculated σ. QRPA and FAM calculations, comparison with experimental data. NUCLEAR STRUCTURE 50Ca; calculated isoscalar monopole strength distribution. QRPA and FAM calculations.
doi: 10.5506/APhysPolB.42.609
2008AV05 Nucl.Phys. A811, 378 (2008) P.Avogadro, F.Barranco, R.A.Broglia, E.Vigezzi Vortex-nucleus interaction in the inner crust of neutron stars
doi: 10.1016/j.nuclphysa.2008.07.010
2007AV01 Phys.Rev. C 75, 012805 (2007) P.Avogadro, F.Barranco, R.A.Broglia, E.Vigezzi Quantum calculation of vortices in the inner crust of neutron stars
doi: 10.1103/PhysRevC.75.012805
2007AV05 Nucl.Phys. A788, 130c (2007) P.Avogadro, F.Barranco, R.A.Broglia, E.Vigezzi Microscopic quantal calculation of the vortex-nucleus interaction in the inner crust of neutron stars
doi: 10.1016/j.nuclphysa.2007.01.058
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