NSR Query Results
Output year order : Descending NSR database version of May 1, 2024. Search: Author = B.T.Reed Found 6 matches. 2024RE05 Phys.Rev. C 109, 035803 (2024) B.T.Reed, F.J.Fattoyev, C.J.Horowitz, J.Piekarewicz Density dependence of the symmetry energy in the post-PREX-CREX era
doi: 10.1103/PhysRevC.109.035803
2021RE05 Phys.Rev.Lett. 126, 172503 (2021) B.T.Reed, F.J.Fattoyev, C.J.Horowitz, J.Piekarewicz Implications of PREX-2 on the Equation of State of Neutron-Rich Matter NUCLEAR STRUCTURE 208Pb; analyzed available data for the neutron skin thickness; deduced the slope of the symmetry energy, the impact of stiff symmetry energy on some critical neutron-star observables.
doi: 10.1103/PhysRevLett.126.172503
2020FA09 Phys.Rev. C 102, 065805 (2020) F.J.Fattoyev, C.J.Horowitz, J.Piekarewicz, B.Reed GW190814: Impact of a 2.6 solar mass neutron star on the nucleonic equations of state
doi: 10.1103/PhysRevC.102.065805
2020HO16 Phys.Rev. C 102, 044321 (2020) C.J.Horowitz, J.Piekarewicz, B.Reed Insights into nuclear saturation density from parity-violating electron scattering NUCLEAR STRUCTURE 208Pb; calculated charge density, saturation density of nuclear matter, baryon density, extrapolation factor as a function of the neutron skin thickness for several nonrelativistic and relativistic energy density functionals (EDFs) using PREX experimental result for the weak radius of 208Pb, and symmetrized two parameter Fermi function. Comparison with other theoretical predictions.
doi: 10.1103/PhysRevC.102.044321
2020RE08 Phys.Rev. C 101, 045803 (2020) Large sound speed in dense matter and the deformability of neutron stars
doi: 10.1103/PhysRevC.101.045803
2020RE16 Phys.Rev. C 102, 064308 (2020) B.T.Reed, Z.Jaffe, C.J.Horowitz, C.Sfienti Measuring the surface thickness of the weak charge density of nuclei NUCLEAR REACTIONS 48Ca, 208Pb(polarized e-, e-), E=855, 950, 2220 MeV; calculated differential σ(θ) and parity violating asymmetry including Coulomb distortions, radius and surface thickness parameters, weak charge density versus radius for 855 MeV beam energy, log derivative of parity violating asymmetry with respect to the log of the surface thickness parameter or the log of the weak radius versus scattering angle; evaluated statistical uncertainties and figure of merit (FOM) for proposed experiments at the A1 spectrometer facility of the MAMI accelerator to measure the surface thickness of the weak charge density of a heavy nucleus, further to present PREX-II and CREX parity violating electron scattering experiments probing the weak charge densities. Fermi function fit with relativistic and non-relativistic mean field models.
doi: 10.1103/PhysRevC.102.064308
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