NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = C.J.Pethick Found 19 matches. 2022ZH31 Phys.Rev. C 105, 055807 (2022) Superfluid density in disordered pasta phases in neutron star crusts
doi: 10.1103/PhysRevC.105.055807
2021ZH28 Phys.Rev. C 103, 055807 (2021) Proton superconductivity in pasta phases in neutron star crusts
doi: 10.1103/PhysRevC.103.055807
2020PE05 Phys.Rev. C 101, 055802 (2020) C.J.Pethick, Z.-W.Zhang, D.N.Kobyakov Elastic properties of phases with nonspherical nuclei in dense matter
doi: 10.1103/PhysRevC.101.055802
2017KO30 Phys.Rev. C 96, 025805 (2017) D.N.Kobyakov, C.J.Pethick, S.Reddy, A.Schwenk Dispersion and decay of collective modes in neutron star cores
doi: 10.1103/PhysRevC.96.025805
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
2016KO36 Phys.Rev. C 94, 055806 (2016) Nucleus-nucleus interactions in the inner crust of neutron stars
doi: 10.1103/PhysRevC.94.055806
2014KO07 Phys.Rev.Lett. 112, 112504 (2014) Towards a Metallurgy of Neutron Star Crusts
doi: 10.1103/PhysRevLett.112.112504
2013KO12 Phys.Rev. C 87, 055803 (2013); Erratum Phys.Rev. C 94, 059902 (2016) Dynamics of the inner crust of neutron stars: Hydrodynamics, elasticity, and collective modes
doi: 10.1103/PhysRevC.87.055803
2009BA40 Phys.Rev. C 80, 032802 (2009) S.Bacca, K.Hally, C.J.Pethick, A.Schwenk Chiral effective field theory calculations of neutrino processes in dense matter
doi: 10.1103/PhysRevC.80.032802
2009PE27 Phys.Rev. C 80, 055805 (2009) Spin response of a normal Fermi liquid with noncentral interactions
doi: 10.1103/PhysRevC.80.055805
2008LY02 Phys.Rev. C 78, 045803 (2008) G.I.Lykasov, C.J.Pethick, A.Schwenk Unified approach to structure factors and neutrino processes in nucleon matter
doi: 10.1103/PhysRevC.78.045803
2005LY01 Phys.Rev. C 72, 025805 (2005) G.I.Lykasov, E.Olsson, C.J.Pethick Long-wavelength spin- and spin-isospin correlations in nucleon matter
doi: 10.1103/PhysRevC.72.025805
2004OL08 Phys.Rev. C 70, 025804 (2004) E.Olsson, P.Haensel, C.J.Pethick Static response of Fermi liquids with tensor interactions
doi: 10.1103/PhysRevC.70.025804
2002OL07 Phys.Rev. C 66, 065803 (2002) Multipair contributions to the spin response of nuclear matter
doi: 10.1103/PhysRevC.66.065803
1996PE17 Nucl.Phys. A606, 173 (1996) The Dependence of Neutron Skin Thickness and Surface Tension on Neutron Excess NUCLEAR STRUCTURE 40,48Ca; calculated nucleon densities. 40,42,44,46,48Ca, 46,48,50Ti; calculated nucleon radii, rms radii difference vs asymmetry parameter. 58,64Ni, 43Ca, 12C, 51V, 90Zr, 116,124Sn, 208Pb; calculated rms nucleon radii differences vs asymmetry parameter; deduced neutron skin thickness, surface tension dependence on neutron excess. Thermodynamically consistent approach.
doi: 10.1016/0375-9474(96)00216-3
1995PA40 Phys.Rev.Lett. 75, 4567 (1995) V.R.Pandharipande, C.J.Pethick, V.Thorsson Kaon Energies in Dense Matter
doi: 10.1103/PhysRevLett.75.4567
1995PE04 Nucl.Phys. A584, 675 (1995) C.J.Pethick, D.G.Ravenhall, C.P.Lorenz The Inner Boundary of a Neutron-Star Crust
doi: 10.1016/0375-9474(94)00506-I
1993HE23 Ann.Phys.(New York) 223, 37 (1993) H.Heiselberg, C.J.Pethick, D.G.Ravenhall Collective Behavior of Stable and Unstable Hot Fermi Systems
doi: 10.1006/aphy.1993.1026
1972RA09 Phys.Rev.Lett. 28, 978 (1972) D.G.Ravenhall, C.D.Bennett, C.J.Pethick Nuclear Surface Energy and Neutron-Star Matter
doi: 10.1103/PhysRevLett.28.978
Back to query form |