NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = B.J.Cai Found 15 matches. 2024QI01 Phys.Lett. B 849, 138435 (2024) M.Qiu, B.-J.Cai, L.-W.Chen, C.-X.Yuan, Zh.Zhang Bayesian model averaging for nuclear symmetry energy from effective proton-neutron chemical potential difference of neutron-rich nuclei NUCLEAR STRUCTURE 48Ca, 68Ni, 88Sr, 132Sn, 208Pb; analyzed available data; deduced symmetry energy using the data-driven Bayesian model averaging is a rigorous statistical approach to combining multiple models for a unified prediction.
doi: 10.1016/j.physletb.2023.138435
2022CA13 Phys.Rev. C 105, 064607 (2022) Investigating effects of relativistic kinematics, dimensionality, interactions, and short-range correlations on the ratio of quartic over quadratic nuclear symmetry energies
doi: 10.1103/PhysRevC.105.064607
2022CA24 Phys.Rev. C 106, 044319 (2022) B.-J.Cai, R.Wang, Z.Zhang, L.-W.Chen High-order isospin-dependent surface tension contribution to the fourth-order symmetry energy of finite nuclei
doi: 10.1103/PhysRevC.106.044319
2021CA12 Phys.Rev. C 103, 034607 (2021) Intrinsic correlations among characteristics of neutron-rich matter imposed by the unbound nature of pure neutron matter
doi: 10.1103/PhysRevC.103.034607
2021CA15 Phys.Rev. C 103, 054611 (2021) Auxiliary function approach for determining symmetry energy at suprasaturation densities
doi: 10.1103/PhysRevC.103.054611
2019CA18 Phys.Rev. C 100, 024303 (2019) Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
doi: 10.1103/PhysRevC.100.024303
2018CA13 Phys.Rev. C 97, 054322 (2018) Neutron matter within QCD sum rules
doi: 10.1103/PhysRevC.97.054322
2018LI08 Prog.Part.Nucl.Phys. 99, 29 (2018) B.-An.Li, B.-J.Cai, L.-W.Chen, J.Xu Nucleon effective masses in neutron-rich matter
doi: 10.1016/j.ppnp.2018.01.001
2016CA04 Phys.Rev. C 93, 014619 (2016) Symmetry energy of cold nucleonic matter within a relativistic mean field model encapsulating effects of high-momentum nucleons induced by short-range correlations
doi: 10.1103/PhysRevC.93.014619
2016CA40 Phys.Rev. C 94, 061302 (2016) Proton skins in momentum space and neutron skins in coordinate space in heavy nuclei NUCLEAR STRUCTURE 208Pb; calculated reduced nucleon momentum distribution of neutron-rich nucleonic matter, correlation between neutron skin and proton skin using high-momentum tail (HMT)-experimental and HMT-self-consistent Green's function (SCGF) parameter sets; deduced protons move faster than neutrons in neutron skins of heavy nuclei, neutron-proton (np) (isospin) asymmetry dependence of nuclear equation of state (EOS).
doi: 10.1103/PhysRevC.94.061302
2015CA11 Phys.Rev. C 92, 011601 (2015) Isospin quartic term in the kinetic energy of neutron-rich nucleonic matter
doi: 10.1103/PhysRevC.92.011601
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
2012CA08 Phys.Rev. C 85, 024302 (2012) Nuclear matter fourth-order symmetry energy in the relativistic mean field models
doi: 10.1103/PhysRevC.85.024302
2012CH08 Phys.Rev. C 85, 024305 (2012) R.Chen, B.-J.Cai, L.-W.Chen, B.-A.Li, X.-H.Li, C.Xu Single-nucleon potential decomposition of the nuclear symmetry energy
doi: 10.1103/PhysRevC.85.024305
2009CH34 Phys.Rev. C 80, 014322 (2009) L.-W.Chen, B.-J.Cai, C.M.Ko, B.-A.Li, C.Shen, J.Xu Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
doi: 10.1103/PhysRevC.80.014322
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