NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = W.G.Newton Found 20 matches. 2023NE03 Phys.Rev.Lett. 130, 112701 (2023) D.Neill, R.Preston, W.G.Newton, D.Tsang Constraining the Nuclear Symmetry Energy with Multimessenger Resonant Shattering Flares
doi: 10.1103/PhysRevLett.130.112701
2022NE01 Phys.Rev. C 105, 025806 (2022) W.G.Newton, S.Cantu, S.Wang, A.Stinson, M.A.Kaltenborn, J.R.Stone Glassy quantum nuclear pasta in neutron star crusts
doi: 10.1103/PhysRevC.105.025806
2022NE05 Eur.Phys.J. A 58, 69 (2022) W.G.Newton, L.Balliet, S.Budimir, G.Crocombe, B.Douglas, T.Head, Z.Langford, L.Rivera, J.Sanford Ensembles of unified crust and core equations of state in a nuclear-multimessenger astrophysics environment
doi: 10.1140/epja/s10050-022-00710-0
2022NE11 Phys.Lett. B 834, 137481 (2022) W.G.Newton, R.Preston, L.Balliet, M.Ross From neutron skins and neutron matter to the neutron star crust NUCLEAR STRUCTURE 208Pb; analyzed available data; deduced the first Bayesian inference of neutron star crust properties to incorporate neutron skin data, including the recent PREX measurement of the neutron skin of 208Pb, combined with recent chiral effective field theory predictions of pure neutron matter with statistical errors.
doi: 10.1016/j.physletb.2022.137481
2022SC17 J.Phys.(London) G49, 110502 (2022) H.Schatz, A.D.Becerril Reyes, A.Best, E.F.Brown, K.Chatziioannou, K.A.Chipps, C.M.Deibel, R.Ezzeddine, D.K.Galloway, C.J.Hansen, F.Herwig, A.P.Ji, M.Lugaro, Z.Meisel, D.Norman, J.S.Read, L.F.Roberts, A.Spyrou, I.Tews, F.X.Timmes, C.Travaglio, N.Vassh, C.Abia, P.Adsley, S.Agarwal, M.Aliotta, W.Aoki, A.Arcones, A.Aryan, A.Bandyopadhyay, A.Banu, D.W.Bardayan, J.Barnes, A.Bauswein, T.C.Beers, J.Bishop, T.Boztepe, B.Cote, M.E.Caplan, A.E.Champagne, J.A.Clark, M.Couder, A.Couture, S.E.de Mink, S.Debnath, R.J.deBoer, J.den Hartogh, P.Denissenkov, V.Dexheimer, I.Dillmann, J.E.Escher, M.A.Famiano, R.Farmer, R.Fisher, C.Frohlich, A.Frebel, C.Fryer, G.Fuller, A.K.Ganguly, S.Ghosh, B.K.Gibson, T.Gorda, K.N.Gourgouliatos, V.Graber, M.Gupta, W.C.Haxton, A.Heger, W.R.Hix, W.C.G.Ho, E.M.Holmbeck, A.A.Hood, S.Huth, G.Imbriani, R.G.Izzard, R.Jain, H.Jayatissa, Z.Johnston, T.Kajino, A.Kankainen, G.G.Kiss, A.Kwiatkowski, M.La Cognata, A.M.Laird, L.Lamia, P.Landry, E.Laplace, K.D.Launey, D.Leahy, G.Leckenby, A.Lennarz, B.Longfellow, A.E.Lovell, W.G.Lynch, S.M.Lyons, K.Maeda, E.Masha, C.Matei, J.Merc, B.Messer, F.Montes, A.Mukherjee, M.R.Mumpower, D.Neto, B.Nevins, W.G.Newton, L.Q.Nguyen, K.Nishikawa, N.Nishimura, F.M.Nunes, E.O'Connor, B.W.O'Shea, W.-J.Ong, S.D.Pain, M.A.Pajkos, M.Pignatari, R.G.Pizzone, V.M.Placco, T.Plewa, B.Pritychenko, A.Psaltis, D.Puentes, Y.-Z.Qian, D.Radice, D.Rapagnani, B.M.Rebeiro, R.Reifarth, A.L.Richard, N.Rijal, I.U.Roederer, J.S.Rojo, J.S K, Y.Saito, A.Schwenk, M.L.Sergi, R.S.Sidhu, A.Simon, T.Sivarani, A.Skuladottir, M.S.Smith, A.Spiridon, T.M.Sprouse, S.Starrfield, A.W.Steiner, F.Strieder, I.Sultana, R.Surman, T.Szucs, A.Tawfik, F.Thielemann, L.Trache, R.Trappitsch, M.B.Tsang, A.Tumino, S.Upadhyayula, J.O.Valle Martinez, M.Van der Swaelmen, C.Viscasillas Vazquez, A.Watts, B.Wehmeyer, M.Wiescher, C.Wrede, J.Yoon, R.G.T.Zegers, M.A.Zermane, M.Zingale, the Horizon 2020 Collaborations Horizons: nuclear astrophysics in the 2020s and beyond
doi: https://dx.doi.org/10.1088/1361-6471/ac8890
2021NE05 Phys.Rev. C 103, 064323 (2021) Nuclear symmetry energy from neutron skins and pure neutron matter in a Bayesian framework NUCLEAR STRUCTURE 48Ca, 112,114,116,118,120,122,124,126,128,130,132Sn, 208Pb; analyzed in Bayesian framework nuclear symmetry energy magnitudes from a combination of experimental data for neutron skin thicknesses on calcium, lead and tin isotopes from various experiments including electron scattering (PREX) experiments at Jefferson Laboratory, and theoretical information about pure neutron matter from chiral effective field theory calculations and theoretical neutron skin thicknesses from quantum Skyrme-Hartree-Fock approach using an extended Skyrme energy-density functional. Relevance to more direct modeling of the future experimental observables at Jefferson Laboratory and at Mainz about parity-violating asymmetry, electric dipole response, neutron distributions, etc.
doi: 10.1103/PhysRevC.103.064323
2015CA14 Phys.Rev. C 92, 015802 (2015) B.-J.Cai, F.J.Fattoyev, B.-A.Li, W.G.Newton Critical density and impact of Δ (1232) resonance formation in neutron stars
doi: 10.1103/PhysRevC.92.015802
2015HE03 Phys.Rev. C 91, 015810 (2015) X.-T.He, F.J.Fattoyev, B.-A.Li, W.G.Newton Impact of the equation-of-state-gravity degeneracy on constraining the nuclear symmetry energy from astrophysical observables
doi: 10.1103/PhysRevC.91.015810
2015ST02 Phys.Rev. C 91, 015804 (2015) A.W.Steiner, S.Gandolfi, F.J.Fattoyev, W.G.Newton Using neutron star observations to determine crust thicknesses, moments of inertia, and tidal deformabilities
doi: 10.1103/PhysRevC.91.015804
2014FA05 Eur.Phys.J. A 50, 45 (2014) F.J.Fattoyev, W.G.Newton, B.-A.Li Probing the high-density behavior of symmetry energy with gravitational waves
doi: 10.1140/epja/i2014-14045-6
2014FA12 Phys.Rev. C 90, 022801 (2014) F.J.Fattoyev, W.G.Newton, B.-A.Li Quantifying correlations between isovector observables and the density dependence of the nuclear symmetry energy away from saturation density NUCLEAR STRUCTURE 48Ca, 208Pb; calculated correlations between nuclear symmetry energy S(ρ) and its slope L(ρ), neutron skin thickness, radii of neutron stars, and the crust-core transition pressure for different densities using Skyrme models SLy4 and NRAPR.
doi: 10.1103/PhysRevC.90.022801
2014NE02 Eur.Phys.J. A 50, 41 (2014) W.G.Newton, J.Hooker, M.Gearheart, K.Murphy, D.-H.Wen, F.J.Fattoyev, B.-A.Li Constraints on the symmetry energy from observational probes of the neutron star crust
doi: 10.1140/epja/i2014-14041-x
2014PA54 Phys.Rev. C 90, 065802 (2014) Phase transitions in core-collapse supernova matter at sub-saturation densities
doi: 10.1103/PhysRevC.90.065802
2013FA02 Phys.Rev. C 87, 015806 (2013) F.J.Fattoyev, J.Carvajal, W.G.Newton, B.-A.Li Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars
doi: 10.1103/PhysRevC.87.015806
2012FA09 Phys.Rev. C 86, 025804 (2012) F.J.Fattoyev, W.G.Newton, J.Xu, B.-A.Li Generic constraints on the relativistic mean-field and Skyrme-Hartree-Fock models from the pure neutron matter equation of state NUCLEAR STRUCTURE 112,114,116,118,120,122,124,126,128,130,132Sn, 208Pb; calculated nuclear symmetry energy, neutron skin thickness. Microscopic pure neutron matter (PNM) calculations using relativistic mean-field (RMF) and Skyrme-Hartree-Fock (SHF) models with IU-FSU and SkIU-FSU parametrizations. 40,48Ca, 78Ni, 90Zr, 132Sn, 208Pb; analyzed relative deviation of the binding energies and charge radii. Comparison with experimental data. Discussed predictions of neutron skin thicknesses and neutron star radii.
doi: 10.1103/PhysRevC.86.025804
2012WE01 Phys.Rev. C 85, 025801 (2012) Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energy
doi: 10.1103/PhysRevC.85.025801
2011LI54 J.Phys.:Conf.Ser. 312, 042006 (2011) B.-A.Li, L.-W.Chen, M.Gearheart, J.Hooker, C.M.Ko, P.G.Krastev, W.-K.Lin, W.G.Newton, D.-H.Wen, C.Xu, J.Xu Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
doi: 10.1088/1742-6596/312/4/042006
2009NE06 Phys.Rev. C 79, 055801 (2009) Modeling nuclear "pasta" and the transition to uniform nuclear matter with the 3D Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovae NUCLEAR STRUCTURE 16O, 40Ca, 56Fe; calculated binding energies and rms radii. A=100-2000; calculated free energy functions versus nucleon number, neutron density profiles and energy deformation surfaces. Implications for Core-collapse supernovae. Three-dimensional finite temperature Skyrme-Hatree-Fock+BCS calculations for inhomogeneous phase of bulk nuclear matter using computer code TAMAR.
doi: 10.1103/PhysRevC.79.055801
2009NE15 Phys.Rev. C 80, 065809 (2009) Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear data
doi: 10.1103/PhysRevC.80.065809
2004ST06 Int.J.Mod.Phys. E13, 181 (2004) P.D.Stevenson, M.R.Strayer, J.Rikovska Stone, W.G.Newton Giant resonances from TDHF NUCLEAR STRUCTURE 16O; calculated giant resonance strength functions. TDHF approach.
doi: 10.1142/S0218301304001928
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