Publication data of Newton, William G.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion200420062008201020122014201620182020202220240500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications201020202005201520250102030405001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20042006200820102012201420162018202020222024051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestEfficacy of crustal superfluid neutrons in pulsar glitch modelsObservational constraints on neutron star crust–core coupling during glitchesNuclear symmetry energy from neutron skins and pure neutron matter in a Bayesian frameworkNuclear symmetry energy from neutron skins and pure neutron matter in a …The state of matter in simulations of core-collapse supernovae -- Reflections and recent developmentsThe state of matter in simulations of core-collapse supernovae -- Reflections a…The cooling of the Cassiopeia A neutron star as a probe of the nuclear symmetry energy and nuclear pastaThe cooling of the Cassiopeia A neutron star as a probe of the nuclear symm…Impact of the equation-of-state–gravity degeneracy on constraining the nuclear symmetry energy from astrophysical observablesImpact of the equation-of-state–gravity degeneracy on constraining the nucl…Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear dataConstraining the gravitational binding energy of PSR J0737-3039B using terr…Constraints on the symmetry energy from observational probes of the neutron star crustConstraints on the symmetry energy from observational probes of the neutro…How tightly is the nuclear symmetry energy constrained by a unitary Fermi gas?How tightly is the nuclear symmetry energy constrained by a unitary Fermi g…Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energySensitivity of the neutron star r-mode instability window to the density depe…Generic constraints on the relativistic mean-field and Skyrme-Hartree-Fock models from the pure neutron matter equation of stateGeneric constraints on the relativistic mean-field and Skyrme-Hartree-Fock m…Neutron–proton effective mass splitting in neutron-rich matter at normal density from analyzing nucleon–nucleus scattering data within an isospin dependent optical modelNeutron–proton effective mass splitting in neutron-rich matter at normal den…Critical density and impact of Δ(1232) resonance formation in neutron starsUpper limits on the observational effects of nuclear pasta in neutron starsConstraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron starsConstraining the high-density behavior of the nuclear symmetry energy with…The Double pulsar J0737-3039: Testing the neutron star equation of stateA survey of the parameter space of the compressible liquid drop model as applied to the neutron star inner crustA survey of the parameter space of the compressible liquid drop model as ap…Using Neutron Star Observations to Determine Crust Thicknesses, Moments of Inertia, and Tidal DeformabilitiesUsing Neutron Star Observations to Determine Crust Thicknesses, Moments o…Modeling nuclear 'pasta' and the transition to uniform nuclear matter with the D-3 Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovaeModeling nuclear 'pasta' and the transition to uniform nuclear matter with th…200420062008201020122014201620182020202220240500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Efficacy of crustal superfluid neutrons in pulsar glitch modelsObservational constraints on neutron star crust–core coupling during glitchesNuclear symmetry energy from neutron skins and pure neutron matter in a Bayesian frameworkNuclear symmetry energy from neutron skins and pure neutron matter in a …The state of matter in simulations of core-collapse supernovae -- Reflections and recent developmentsThe state of matter in simulations of core-collapse supernovae -- Reflections a…The cooling of the Cassiopeia A neutron star as a probe of the nuclear symmetry energy and nuclear pastaThe cooling of the Cassiopeia A neutron star as a probe of the nuclear symm…Impact of the equation-of-state–gravity degeneracy on constraining the nuclear symmetry energy from astrophysical observablesImpact of the equation-of-state–gravity degeneracy on constraining the nucl…Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear dataConstraining the gravitational binding energy of PSR J0737-3039B using terr…Constraints on the symmetry energy from observational probes of the neutron star crustConstraints on the symmetry energy from observational probes of the neutro…How tightly is the nuclear symmetry energy constrained by a unitary Fermi gas?How tightly is the nuclear symmetry energy constrained by a unitary Fermi g…Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energySensitivity of the neutron star r-mode instability window to the density depe…Generic constraints on the relativistic mean-field and Skyrme-Hartree-Fock models from the pure neutron matter equation of stateGeneric constraints on the relativistic mean-field and Skyrme-Hartree-Fock m…Neutron–proton effective mass splitting in neutron-rich matter at normal density from analyzing nucleon–nucleus scattering data within an isospin dependent optical modelNeutron–proton effective mass splitting in neutron-rich matter at normal den…Critical density and impact of Δ(1232) resonance formation in neutron starsUpper limits on the observational effects of nuclear pasta in neutron starsConstraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron starsConstraining the high-density behavior of the nuclear symmetry energy with…The Double pulsar J0737-3039: Testing the neutron star equation of stateA survey of the parameter space of the compressible liquid drop model as applied to the neutron star inner crustA survey of the parameter space of the compressible liquid drop model as ap…Using Neutron Star Observations to Determine Crust Thicknesses, Moments of Inertia, and Tidal DeformabilitiesUsing Neutron Star Observations to Determine Crust Thicknesses, Moments o…Modeling nuclear 'pasta' and the transition to uniform nuclear matter with the D-3 Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovaeModeling nuclear 'pasta' and the transition to uniform nuclear matter with th…200420062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average20042006200820102012201420162018202020222024050100150200250