NSR Query Results
Output year order : Descending NSR database version of May 2, 2024. Search: Author = P.M.Pizzochero Found 9 matches. 2023KL02 Phys.Rev. C 108, 035808 (2023) P.Klausner, F.Barranco, P.M.Pizzochero, X.Roca-Maza, E.Vigezzi Microscopic calculation of the pinning energy of a vortex in the inner crust of a neutron star
doi: 10.1103/PhysRevC.108.035808
2004DO10 Nucl.Phys. A742, 363 (2004) Fully consistent semi-classical treatment of vortex-nucleus interaction in rotating neutron stars
doi: 10.1016/j.nuclphysa.2004.07.002
2004VI04 Eur.Phys.J. A 20, 101 (2004) E.Vigezzi, F.Barranco, R.A.Broglia, P.M.Pizzochero Superfluidity in the inner crust of neutron stars
doi: 10.1140/epja/i2002-10331-2
2003VI12 Acta Phys.Pol. B34, 2185 (2003) E.Vigezzi, F.Barranco, R.A.Broglia, P.M.Pizzochero Neutron superfluidity and the cooling of neutron stars
1997BI07 Phys.Rev. C56, R1675 (1997) M.Bianchetti, M.R.Quaglia, G.Colo, P.M.Pizzochero, R.A.Broglia, P.F.Bortignon Competition between Particle-Hole and Particle-Particle Correlations in Forbidden Electron Capture: The case of 123Te RADIOACTIVITY 123Te(EC); calculated K-electron capture T1/2 lower limit. Proton-neutron QRPA, Skyrme effective interactions.
doi: 10.1103/PhysRevC.56.R1675
1997PO06 Z.Phys. A357, 325 (1997) A.Polleri, R.A.Broglia, P.M.Pizzochero, N.N.Scoccola Rho Meson Properties in the Nambu-Jona-Lasinio Model
doi: 10.1007/s002180050249
1995OR01 Phys.Lett. 345B, 343 (1995) W.E.Ormand, P.M.Pizzochero, P.F.Bortignon, R.A.Broglia Neutrino Capture Cross Sections for 40Ar and β-Decay of 40Ti NUCLEAR REACTIONS 40Ar(ν, X), E=solar; calculated absorption σ. Shell model. RADIOACTIVITY 40Ti(β+); calculated β-decay matrix elements, T1/2, branching ratios. Shell model.
doi: 10.1016/0370-2693(94)01605-C
1994DO14 Phys.Rev.Lett. 72, 2835 (1994) P.Donati, P.M.Pizzochero, P.F.Bortignon, R.A.Broglia Temperature Dependence of the Nucleon Effect Mass and the Physics of Stellar Collapse NUCLEAR STRUCTURE 98Mo, 64Zn, 64Ni; calculated nucleon effective mass vs temperature; deduced consequences on level density parameter symmetry energy, stellar collapse implications. Dynamic mean field.
doi: 10.1103/PhysRevLett.72.2835
1993OR02 Phys.Lett. 308B, 207 (1993) W.E.Ormand, P.M.Pizzochero, P.F.Bortignon, R.A.Broglia The Solar Neutrino Capture Cross Section for 23Na NUCLEAR REACTIONS 23Na(ν, e-), (ν-bar, e+), E ≈ 3-15 MeV; calculated solar neutrino absorption rate, capture σ vs E. Standard solar model.
doi: 10.1016/0370-2693(93)91272-O
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