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Nuclear matter and neutron star properties with the extendedNambu-Jona-Lasinio model 被引量:1

Nuclear matter and neutron star properties with the extendedNambu-Jona-Lasinio model
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摘要 An extended Nambu-Jona-Lasinio(eNJL) model with nucleons as the degrees of freedom is used to investigate properties of nuclear matter and neutron stars(NSs),including the binding energy and symmetry energy of the nuclear matter, the core-crust transition density, and mass-radius relation of NSs. The fourth-order symmetry energy at saturation density is also investigated. When the bulk properties of nuclear matter at saturation density are used to determine the model parameters, the double solutions of parameters are obtained for a given nuclear incompressibility. It is shown that the isovector-vector interaction has a significant influence on the nuclear matter and NS properties, and the sign of isovector-vector coupling constant is critical in the determination of the trend of the symmetry energy and equation of state. The effects of the other model parameters and symmetry energy slope at saturation density are discussed. An extended Nambu-Jona-Lasinio(eNJL) model with nucleons as the degrees of freedom is used to investigate properties of nuclear matter and neutron stars(NSs),including the binding energy and symmetry energy of the nuclear matter, the core-crust transition density, and mass-radius relation of NSs. The fourth-order symmetry energy at saturation density is also investigated. When the bulk properties of nuclear matter at saturation density are used to determine the model parameters, the double solutions of parameters are obtained for a given nuclear incompressibility. It is shown that the isovector-vector interaction has a significant influence on the nuclear matter and NS properties, and the sign of isovector-vector coupling constant is critical in the determination of the trend of the symmetry energy and equation of state. The effects of the other model parameters and symmetry energy slope at saturation density are discussed.
作者 Yan-Jun Chen 陈晏军(Department of Physics and Electronic Science, Changsha University of Science and Technology;Hunan Provincial Key Laboratory of Flexible Electronic Materials Genome Engineering)
出处 《Chinese Physics C》 SCIE CAS CSCD 2019年第3期82-90,共9页 中国物理C(英文版)
基金 Supported by Hunan Provincial Natural Science Foundation of China(2015JJ2005) the Science Research Foundation of Education Department of Hunan Province(15C0029) the National Natural Science Foundation of China(11103001) the construct program of the key discipline in Hunan province
关键词 NEUTRON stars nuclear MATTER EXTENDED Nambu-Jona-Lasinio model SYMMETRY energy neutron stars nuclear matter extended Nambu-Jona-Lasinio model symmetry energy
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