NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = C.J.Xia Found 6 matches. 2022XI02 Phys.Rev. C 105, 045803 (2022) C.-J.Xia, B.Y.Sun, T.Maruyama, W.-H.Long, A.Li Unified nuclear matter equations of state constrained by the in-medium balance in density-dependent covariant density functionals ATOMIC MASSES A=20-260; calculated binding energies, energy per baryon of finite nuclei. Thomas-Fermi approximation framework with two covariant density functionals DD-LZ1 and DD-ME2. Comparison with data from AME2016.
doi: 10.1103/PhysRevC.105.045803
2021LI01 Phys.Rev. C 103, 014616 (2021) Y.Liu, Y.Wang, Y.Cui, C.-J.Xia, Z.Li, Y.Chen, Q.Li, Y.Zhang Insights into the pion production mechanism and the symmetry energy at high density
doi: 10.1103/PhysRevC.103.014616
2021XI04 Phys.Rev. C 103, 055812 (2021) C.-J.Xia, T.Maruyama, N.Yasutake, T.Tatsumi, Y.-X.Zhang Nuclear pasta structures and symmetry energy NUCLEAR STRUCTURE 208Pb; calculated symmetry energy and its slope of nuclear matter, neutron skin thickness, proton and neutron density profiles using Thomas-Fermi approximation. Investigated nuclear pasta structures in a three-dimensional geometry with reflection symmetry using RMF model with Thomas-Fermi approximation; deduced similarity of droplets and bubbles in body-centered cubic (bcc) and face-centered cubic (fcc) lattices, with impact on properties of neutron stars, supernova dynamics, and binary neutron star mergers.
doi: 10.1103/PhysRevC.103.055812
2020ZH08 Phys.Rev. C 101, 034303 (2020) Y.Zhang, M.Liu, C.-J.Xia, Z.Li, S.K.Biswal Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars NUCLEAR REACTIONS 112,124Sn(124Sn, X), (112Sn, X), E=35, 50 MeV/nucleon; analyzed symmetry energy and related set of 22 nuclear matter parameters by comparing the isospin diffusion data to transport model calculations in five-dimensional parameter space. 208Pb; calculated neutron skin of 208Pb using the deduced nuclear matter parameter set and the restricted density variational (RDV) method. Calculated properties of a neutron star, such as the tidal deformability and maximum mass, and compared with the current constraints.
doi: 10.1103/PhysRevC.101.034303
2018LI43 Phys.Rev. C 98, 024316 (2018) Z.-X.Liu, C.-J.Xia, W.-L.Lu, Y.-X.Li, J.N.Hu, T.-T.Sun Relativistic mean-field approach for Λ, Ξ and Σ Hypernuclei NUCLEAR STRUCTURE 17O, 17N, 17F, 41Ca, 41K, 41Sc, 91Zr, 91Nb, 91Y, 209Pb, 209Tl, 209Bi; calculated mean-field potentials, single-particle levels, density distributions, energies, radii, tensor potentials, and binding energies for hyperons (Λ, Ξ and Σ) in the hypernuclei, starting with the core nuclei of 16O, 40Ca and 208Pb. Relativistic mean-field model. Comparison with available experimental data.
doi: 10.1103/PhysRevC.98.024316
2018SU02 Chin.Phys.C 42, 025101 (2018) T.-T.Sun, C.-J.Xia, S.-S.Zhang, M.S.Smith Massive neutron stars and Λ-hypernuclei in relativistic mean field models NUCLEAR STRUCTURE 208Pb, 139La, 89Y, 51V, 40Ca, 28Si, 16O; calculated predicted single binding energies of hypernuclei using the effective interactions PK1 and TM1. Comparison with the experimental data.
doi: 10.1088/1674-1137/42/2/025101
Back to query form |