NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = X.H.Wu Found 10 matches. 2024JI01 Phys.Lett. B 849, 138448 (2024) X.F.Jiang, X.H.Wu, P.W.Zhao, J.Meng Nuclear level density from relativistic density functional theory and combinatorial method NUCLEAR STRUCTURE 112Cd; calculated total state densities, nuclear level densities based on different formulas of moments of inertia using combinatorial method based on RHB with PC-PK1 and DD-PC1. Comparison with available data.
doi: 10.1016/j.physletb.2024.138448
2024WU03 Phys.Rev. C 109, 024310 (2024) X.H.Wu, C.Pan, K.Y.Zhang, J.Hu Nuclear mass predictions of the relativistic continuum Hartree-Bogoliubov theory with the kernel ridge regression
doi: 10.1103/PhysRevC.109.024310
2023DU07 Chin.Phys.C 47, 074108 (2023) X.-K.Du, P.Guo, X.-H.Wu, S.-Q.Zhang Examination of machine learning for assessing physical effects: Learning the relativistic continuum mass table with kernel ridge regression NUCLEAR STRUCTURE N<300; analyzed available data; deduced empirical proton-neutron interactions, odd-even mass differences, one- and two-neutron separation and binding energies extracted from the nuclear mass table obtained by the relativistic continuum Hartree-Bogoliubov theory. Comparison with available data.
doi: 10.1088/1674-1137/acc791
2022WU07 Phys.Rev. C 105, L031303 (2022) Nuclear energy density functionals from machine learning NUCLEAR STRUCTURE 4He, 16O, 40Ca; calculated rms radii, total energies, kinetic energies, ground-state densities. Self-consistent Kohn-Sham and machine-learning approaches. Comparison to available experimental data.
doi: 10.1103/PhysRevC.105.L031303
2021JI08 Astrophys.J. 915, 29 (2021) Sensitivity Study of r-process Abundances to Nuclear Masses ATOMIC MASSES A=120-210; analyzed available data; deduced impact of nuclear mass uncertainties on the r-process abundances.
doi: 10.3847/1538-4357/ac042f
2020WU06 Phys.Rev. C 101, 051301 (2020) Predicting nuclear masses with the kernel ridge regression ATOMIC MASSES Z=8-120; N=8-160; calculated mass excesses using WS4 mass model with kernel ridge regression (KRR) approach. Comparison with evaluated data in AME2012 and AME2016.
doi: 10.1103/PhysRevC.101.051301
2019WU08 Phys.Rev. C 99, 065802 (2019) Nuclear symmetry energy and hadron-quark mixed phase in neutron stars
doi: 10.1103/PhysRevC.99.065802
2018WU09 Phys.Rev. C 98, 064302 (2018) X.H.Wu, Q.B.Chen, P.W.Zhao, S.Q.Zhang, J.Meng Two-dimensional collective Hamiltonian for chiral and wobbling modes. II. Electromagnetic transitions
doi: 10.1103/PhysRevC.98.064302
2017WU10 Phys.Rev. C 96, 025802 (2017) Finite-size effects on the hadron-quark phase transition in neutron stars
doi: 10.1103/PhysRevC.96.025802
2004ZO01 Chin.Phys.Lett. 21, 43 (2004) H.-S.Zong, X.-H.Wu, F.-Y.Hou, E.-G.Zhao Explicit and Dynamical Chiral Symmetry Breaking in an Effective Quark-Quark Interaction Model
doi: 10.1088/0256-307X/21/1/013
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