Quark mean field model with pion and gluon corrections for $\Lambda,~\Xi^0$ hypernuclei and neutron stars

@article{Xing2017QuarkMF,
  title={Quark mean field model with pion and gluon corrections for \$\Lambda,~\Xi^0\$ hypernuclei and neutron stars},
  author={Xueyong Xing and Jinniu Hu and Hong Shen},
  journal={Physical Review C},
  year={2017},
  volume={95},
  pages={054310}
}
Properties of $\Lambda,~\Xi^0$ hypernuclei and neutron stars are investigated in quark mean field model with pion and gluon corrections. Firstly, $u, ~d$, and $s$ quarks are confined by relativistic harmonic oscillator potentials to generate the baryons, like nucleon, $\Lambda, ~\Sigma$, and $\Xi$ hyperons. The effects of pion-quark coupling and one-gluon exchange are considered perturbatively. Then, the baryons interact with each other through exchanging $\sigma, ~\omega,$ and $\rho$ mesons… 
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