Abstract
A new improved quark mass density-dependent model including u, d quarks, σ mesons, ω mesons and ρ mesons is presented. By employing this model, the properties of nuclear matter, neutron matter and neutron star are studied. After introducing the isovector ρ mesons, the isospin effect for asymmetric nuclear matter is considered. Under mean field approximation, we find that our model can describe the properties of asymmetric nuclear matter, in particular the neutron matter, successfully. The results given by the new improved quark mass density-dependent model and by the quark–meson coupling model are compared.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Journal of Physics G: Nuclear and Particle Physics
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
