202 citations · 839 across the 30 of their papers we have counts for
30 papers
Implications of supermassive neutron stars for the form of the equation of state of hybrid stars
Hongyi Sun, Dehua Wen
The observations of PSR J0952-0607 and the second object in GW190814 event indicate the possible existence of supermassive neutron stars. In this work, by using the Constant-Sound-…
New quasi-universal relations for static and rapid rotating neutron stars
Wenjie Sun, Dehua Wen, Jue Wang
In the last few decades, lots of universal relations between different global physical quantities of neutron stars have been proposed to constrain the unobservable or hard to be ob…
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…
Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
Bao-An Li, Plamen G. Krastev, De-Hua Wen +1
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared goal of both nuclear physics and astrophysics. Except possible phase transitions, the densi…
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…