The quark mean field model with pion and gluon corrections
arXiv:1609.04911 · doi:10.1103/PhysRevC.94.044308
Abstract
The properties of nuclear matter and finite nuclei are studied within the quark mean field (QMF) model by taking the effects of pion and gluon into account at the quark level. The nucleon is described as the combination of three constituent quarks confined by a harmonic oscillator potential. To satisfy the spirit of QCD theory, the contributions of pion and gluon on the nucleon structure are treated in second-order perturbation theory. For the nuclear many-body system, nucleons interact with each other by exchanging mesons between quarks. With different constituent quark mass, , we determine three parameter sets about the coupling constants between mesons and quarks, named as QMF-NK1, QMF-NK2, and QMF-NK3 by fitting the ground-state properties of several closed-shell nuclei. It is found that all of the three parameter sets can give satisfactory description on properties of nuclear matter and finite nuclei, meanwhile they can also predict the larger neutron star mass around without the hyperon degrees of freedom.
arXiv comment19 pages, 6 figures, 4 tables, accepted to Phys. Rev. C
References in corpus (30)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- The Shell Model as Unified View of Nuclear Structure
- Quantum Monte Carlo Calculations of Light Nuclei
- The role of nucleon structure in finite nuclei
- A quark-meson model for nuclear and neutron matter
- Nucleon and hadron structure changes in the nuclear medium and impact on observables
- Cold uniform matter and neutron stars in the quark-mesons-coupling model
- Self-consistent description of finite nuclei based on a relativistic quark model
- Variation of hadron masses in finite nuclei
- Complete relativistic equation of state for neutron stars
- The Nolen-Schiffer anomaly and isospin symmetry breaking in nuclear matter
- Hybrid stars in the quark-meson coupling model with superconducting quark matter
- Hot Nuclear Matter in the Quark Meson Coupling Model
- Quark-Meson Coupling Model, Nuclear Matter Constraints and Neutron Star Properties
- Fock terms in the quark-meson coupling model
- Quark mean field model for nuclear matter and finite nuclei
- Strange quark matter in a chiral SU(3) quark mean field model
- Effect of Nucleon Structure Variation in Super-allowed Fermi Beta-decay
- Naturalness in the quark-meson coupling model
- Extended quark mean-field model for neutron stars
- Quark-meson coupling model with the cloudy bag
- Study of hypernuclei in the quark mean field model
- Compact stars within an asy-soft quark-meson-coupling model
- Warm asymmetric matter in the Quark Meson Coupling Model
- New treatment of the chiral SU(3) quark mean field model
- Nuclear symmetry energy in a modified quark meson coupling model
- Liquid-gas phase transition and Coulomb instability of asymmetric nuclear systems
- Quark mean-field model for single and double and hypernuclei
- Liquid-gas phase transition in nuclear matter including strangeness
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- Note on neutron star equation of state in the light of GW170817