NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = F.V.De Blasio Found 17 matches. 1998DE19 Nucl.Phys. A633, 391 (1998) Lattice Defects in the Crust of a Neutron Star
doi: 10.1016/S0375-9474(98)00123-7
1997DE31 Phys.Rev. C56, 2332 (1997) F.V.De Blasio, M.Hjorth-Jensen, O.Elgaroy, L.Engvik, G.Lazzari, M.Baldo, H.-J.Schulze Coherence Length of Neutron Superfluids
doi: 10.1103/PhysRevC.56.2332
1996DE24 Z.Phys. A355, 113 (1996) Pinning Mechanism and Vortex Trap Region in Neutron Star Crusts
doi: 10.1007/s002180050087
1996DE45 Phys.Lett. 384B, 1 (1996) Vibrations of Slabs and Cylindrical Nuclei
doi: 10.1016/0370-2693(96)00684-3
1996LA32 Nuovo Cim. 109A, 1691 (1996) Protons in Non-Spherical Nuclear Phases of a Neutron Star Crust NUCLEAR STRUCTURE A=130-180; calculated protonic gap vs mass number, cylinder, slab-like neutron star crust nuclear phase regions.
doi: 10.1007/BF02773549
1995DE25 Phys.Rev. C52, 418 (1995) Unusual Nuclear Shapes and Neutron Specific Heat of Neutron Star Crusts
doi: 10.1103/PhysRevC.52.418
1995LA12 Z.Phys. A352, 9 (1995) Pairing Properties of Clustered Protons in Neutron Star Crusts
doi: 10.1007/BF01292754
1995LA23 Z.Phys. A353, 13 (1995) Vortex Pinning with Non-Spherical Nuclei
doi: 10.1007/BF01297720
1995LA24 Z.Phys. A353, 235 (1995) Specific Heat of Protons in Non-Spherical Nuclei
doi: 10.1007/BF01292325
1995LA28 Int.J.Mod.Phys. E4, 843 (1995) Proton Superfluidity in Neutron Star Matter with an Effective Interaction
doi: 10.1142/S0218301395000304
1994BO11 Nucl.Phys. A569, 237c (1994) P.F.Bortignon, C.Riva, M.Braguti, F.V.De Blasio, R.A.Broglia, W.Cassing, M.Tohyama Limiting Temperature for the Existence of Collective Motion in Highly Excited Nuclei ( Question ) NUCLEAR STRUCTURE 16O, 40Ca; analyzed dipole, quadrupole motion time evolution vs temperature; deduced GDR spreading width temperature independence role.
doi: 10.1016/0375-9474(94)90114-7
1994DE49 Nuovo Cim. 107A, 1579 (1994) Mean-Field Calculations of Bulk Properties in Neutron-Rich Nuclei NUCLEAR STRUCTURE 110,120,130,140,150,160,170,176Sn; calculated proton, neutron density diffusivities, density profiles, BCS formalism, Hartree-Fock approximation.
doi: 10.1007/BF02780692
1994LA24 Z.Phys. A349, 7 (1994) Specific Heat of the Superfluid Neutron Matter in Neutron Star Crusts
doi: 10.1007/BF01296326
1994LA30 Acta Phys.Pol. B25, 1467 (1994) Non-Uniform Pairing Gap of the Superfluid Neutrons in the Crust of Neutron Stars
1994LA34 Z.Phys. A350, 177 (1994) Neutron Superfluidity and Unusual Nuclear Shapes in Neutron Stars Crusts
doi: 10.1007/BF01289576
1993BO10 Acta Phys.Pol. B24, 129 (1993) P.F.Bortignon, F.V.De Blasio, W.Cassing, M.Tohyama, R.A.Broglia Collective Motion in Very Excited Nuclei NUCLEAR STRUCTURE 40Ca, 16O; calculated quadrupole, dipole moments, modes widths. TDHF, time-dependent density-matrix approaches.
1992DE06 Phys.Rev.Lett. 68, 1663 (1992) F.V.De Blasio, W.Cassing, M.Tohyama, P.F.Bortignon, R.A.Broglia Nonperturbative Study of the Damping of Giant Resonances in Hot Nuclei NUCLEAR STRUCTURE 16O, 40Ca; calculated dipole, quadrupole resonance width vs temperature. Mean field theory.
doi: 10.1103/PhysRevLett.68.1663
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