59 citations · 78 across the 3 of their papers we have counts for
4 papers
Constraining the nuclear symmetry energy and properties of neutron star from GW170817 by Bayesian analysis
Yuxi Li, Houyuan Chen, Dehua Wen +1
Based on the distribution of tidal deformabilities and component masses of binary neutron star merger GW170817, the parametric equation of states (EOS) are employed to probe the nu…
Universal behavior of compact star based upon gravitational binding energy
Rongrong Jiang, Dehua Wen, Houyuan Chen
Similar to the compactness parameter (), the gravitational binding energy (GBE) is also a characteristic parameter which can reflect the internal structure of a neutron star…
Suitable resolution for EOS tables in neutron star investigation
Houyuan Chen, Dehua Wen, Na Zhang
Inasmuch as the hydrostatic structure of interior neutron stars uniquely depends on the equation of state (EOS), the inverse constraints on EOS from astrophysical observation have…
GW170817 implications on the frequency and damping time of f-mode oscillations of neutron stars
De-Hua Wen, Bao-An Li, Hou-Yuan Chen +1
Within a minimum model for neutron stars consisting of nucleons, electrons and muons at -equilibrium using about a dozen Equation of States (EOSs) from microscopic nuclear many-…