Symmetry energy and neutron star properties in the saturated Nambu-Jona-Lasinio model

DOI10.1016/J.PHYSLETB.2016.10.019zbMath1370.85004arXiv1511.07144OpenAlexW2536977639MaRDI QIDQ2403599

Si-Na Wei, Wei-Zhou Jiang, Rong-Yao Yang, Dong-Rui Zhang

Publication date: 11 September 2017

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1511.07144

zbMATH Keywords

neutron starsNJL modelsymmetry energy

Mathematics Subject Classification ID

Model quantum field theories (81T10) Galactic and stellar structure (85A15)

Cites Work

• Non-perturbative methods for a chiral effective field theory of finite density nuclear systems
• Hidden pseudospin and spin symmetries and their origins in atomic nuclei
• The axial vector current in beta decay
• Quark–hadron phase transition in an extended Nambu–Jona-Lasinio model with scalar–vector interaction: Finite temperature and baryon chemical potential case
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• On Massive Neutron Cores
• The stability of nuclear matter in the Nambu-Jona-Lasinio model

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