107 citations · 172 across the 7 of their papers we have counts for
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Equation of state and hybrid star properties with the weakly interacting light U-boson in relativistic models
Dong-Rui Zhang, Wei-Zhou Jiang, Si-Na Wei +2
It has been a puzzle whether quarks may exist in the interior of massive neutron stars, since the hadron-quark phase transition softens the equation of state (EOS) and reduce the n…
Novel halos in light kaonic nuclei as an indicator of nuclear equation of state at supra-normal densities
Yang Rong-Yao, Jiang Wei-Zhou, Wei Si-Na +1
The sensitive correlations between the low-density halo structure and the high-density properties of the nuclear equation of state (EOS) are constructed in light kaonic nuclei with…
Symmetry energy and neutron star properties in the saturated Nambu-Jona-Lasinio model
Si-Na Wei, Wei-Zhou Jiang, Rong-Yao Yang +1
In this work, we adopt the Nambu-Jona-Lasinio (NJL) model that ensures the nuclear matter saturation properties to study the density dependence of the symmetry energy. With the int…
Relativistic symmetry breaking in light kaonic nuclei
Rong-Yao Yang, Wei-Zhou Jiang, Qian-Fei Xiang +2
As the experimental data from kaonic atoms and scatterings imply that the -nucleon interaction is strongly attractive at saturation density, there is a possibility…
Symmetry energy softening in nuclear matter with non-nucleonic constituents
Wei-Zhou Jiang, Rong-Yao Yang, Dong-Rui Zhang
We study the trend of the nuclear symmetry energy in relativistic mean-field models with appearance of the hyperon and quark degrees of freedom at high densities. On the pure hadro…
Effects of a weakly interacting light U boson on the nuclear equation of state and properties of neutron stars in relativistic models
Dong-Rui Zhang, Ping-Liang Yin, Wei Wang +2
We investigate the effects of the light vector U-boson that couples weakly to nucleons in relativistic mean-field models on the equation of state and subsequently the consequence i…