NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = G.Watanabe Found 16 matches. 2022MI17 Phys. Rev. Res. 4, 033141 (2022) Effects of pairing gap and band gap on superfluid density in the inner crust of neutron stars
doi: 10.1103/PhysRevResearch.4.033141
2020UO01 Phys.Rev. C 102, 014604 (2020) Y.Uozumi, Y.Fukuda, Y.Yamaguchi, G.Watanabe, M.Nakano Direct pickup and knockout processes in inclusive (p, αx) reactions from 42 to 300 MeV NUCLEAR REACTIONS 12C(p, αX), E=42, 62, 68 MeV; 27Al(p, αX), E=28.8, 42, 61.7, 68, 90, 120, 160, 200 MeV; 58Ni, 90Zr(p, αX), E=42, 68, 90 MeV; 59Co(p, αX), E=120, 160, 200 MeV; 89Y(p, αX), E=61.5 MeV; 93Nb(p, αX), E=100 MeV; 109Ag(p, αX), E=300 MeV; 197Au(p, αX), E=61.7, 68, 120, 160, 200 MeV; 209Bi(p, αX), E=38.7, 42, 61.7, 90 MeV; analyzed experimental data for inclusive σ(E) and double differential σ(E, θ) (DDX) of direct pickup, knockout, and indirect pickup channels using intranuclear cascade (INC) model.
doi: 10.1103/PhysRevC.102.014604
2018UO01 Phys.Rev. C 97, 034630 (2018) Y.Uozumi, Y.Yamaguchi, G.Watanabe, Y.Fukuda, R.Imamura, M.Ja.Kobra, M.Nakano Direct pickup and knockout processes in inclusive (P, dx) reactions at 42-392 MeV NUCLEAR REACTIONS 27Al(d, pX), E=42, 68, 90, 300, 392 MeV; calculated double-differential σ(E) data by intranuclear cascade (INC) model, and compared with experimental data; deduced roles of direct pickup and knockout.
doi: 10.1103/PhysRevC.97.034630
2017WA25 Phys.Rev.Lett. 119, 062701 (2017) Superfluid Density of Neutrons in the Inner Crust of Neutron Stars: New Life for Pulsar Glitch Models
doi: 10.1103/PhysRevLett.119.062701
2008SO03 Phys.Rev. C 77, 035806 (2008), Erratum Phys.Rev. C 81, 049902 (2010) H.Sonoda, G.Watanabe, K.Sato, K.Yasuoka, T.Ebisuzaki Phase diagram of nuclear "pasta" and its uncertainties in supernova cores NUCLEAR STRUCTURE 56Fe, 90Zr, 208Pb, 238U; calculated binding energies, central nucleon density, surface diffusiveness parameters, surface tension, nucleon distributions, phase diagrams. Quantum-molecular dynamics (QMD) model.
doi: 10.1103/PhysRevC.77.035806
2007SO08 Phys.Rev. C 75, 042801 (2007) H.Sonoda, G.Watanabe, K.Sato, T.Takiwaki, K.Yasuoka, T.Ebisuzaki Impact of nuclear "pasta" on neutrino transport in collapsing stellar cores
doi: 10.1103/PhysRevC.75.042801
2004WA15 Phys.Rev. C 69, 055805 (2004), Erratum Phys.Rev. C 81, 049901 (2010) G.Watanabe, K.Sato, K.Yasuoka, T.Ebisuzaki Phases of hot nuclear matter at subnuclear densities
doi: 10.1103/PhysRevC.69.055805
2003WA17 Phys.Rev. C 68, 035806 (2003) G.Watanabe, K.Sato, K.Yasuoka, T.Ebisuzaki Structure of cold nuclear matter at subnuclear densities by quantum molecular dynamics
doi: 10.1103/PhysRevC.68.035806
2003WA22 Nucl.Phys. A718, 700c (2003) G.Watanabe, K.Sato, K.Yasuoka, T.Ebisuzaki Microscopic study of nuclear "pasta": Quantum molecular dynamics approach
doi: 10.1016/S0375-9474(03)00893-5
2003WA25 Phys.Rev. C 68, 045801 (2003) Electron screening in the liquid-gas mixed phases of nuclear matter
doi: 10.1103/PhysRevC.68.045801
2002II01 Prog.Theor.Phys.(Kyoto), Suppl. 146, 514 (2002) Formation of Nuclear "Pasta" in Cold Neutron Star Matter
doi: 10.1143/PTPS.146.514
2002WA21 Phys.Rev. C66, 012801 (2002) G.Watanabe, K.Sato, K.Yasuoka, T.Ebisuzaki Microscopic Study of Slablike and Rodlike Nuclei: Quantum molecular dynamics approach
doi: 10.1103/PhysRevC.66.012801
2002WA30 Prog.Theor.Phys.(Kyoto), Suppl. 146, 638 (2002) G.Watanabe, K.Sato, K.Yasuoka, T.Ebisuzaki Microscopic Study of Nuclear "Pasta" by Quantum Molecular Dynamics
doi: 10.1143/PTPS.146.638
2001II01 Prog.Theor.Phys.(Kyoto) 106, 551 (2001); Erratum Prog.Theor.Phys.(Kyoto) 110, 847 (2003) Formation of Nuclear ' Pasta ' in Cold Neutron Star Matter
doi: 10.1143/PTP.106.551
2001WA15 Nucl.Phys. A687, 512 (2001); Erratum Nucl.Phys. A726, 357 (2003) Effects of Neutrino Trapping on Thermodynamic Properties of Nuclear ' Pasta '
doi: 10.1016/S0375-9474(00)00585-6
2000WA27 Nucl.Phys. A676, 455 (2000); Erratum Nucl.Phys. A726, 357 (2003) Thermodynamic Properties of Nuclear ' Pasta ' in Neutron Star Crusts
doi: 10.1016/S0375-9474(00)00197-4
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