2 citations · 3 across the 5 of their papers we have counts for
6 papers
Detectability of bulk viscosity effects on post-merger gravitational wave signals from binary neutron star mergers
Zhenyu Zhu, Michail Chabanov, Richard O'Shaughnessy
We investigate bulk viscosity (BV) effects on post-merger gravitational wave (PMGW) signals from binary neutron star (BNS) mergers and their detectability using realistic equation…
Constraining the Equation of State of Neutron Stars with third-generation Gravitational Wave detectors
Zhenyu Zhu, Richard O'Shaughnessy
We investigated the impact of the number of binary neutron star merger events and neutron star (NS) mass distributions on constraining the equation of state (EoS), tidal deformabil…
Subgrid Mean-field Dynamo Model with Dynamical Quenching in General Relativistic Magnetohydrodynamic Simulations
Hongzhe Zhou, Yosuke Mizuno, Zhenyu Zhu
Large-scale magnetic fields are relevant for a number of dynamical processes in accretion disks, including driving turbulence, reconnection events, and launching outflows. Numerica…
Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
Zhenyu Zhu, Richard O'Shaughnessy
We investigate the constraints on the neutron star equation of state (EoS) and nuclear properties achievable with third-generation gravitational wave detectors using the Fisher inf…
Three-dimensional equation of state extension of quark matter in Fermi-liquid theory
Zhenyu Zhu, Shuai Zha, Sophia Han
The cold, dense matter equation of state (EoS) determines crucial global properties of neutron stars (NSs), including the mass, radius and tidal deformability. However, a one-dimen…
Equation of State of Decompressed Quark Matter, and Observational Signatures of Quark-Star Mergers
Zhiqiang Miao, Zhenyu Zhu, Dong Lai
Quark stars are challenging to confirm or exclude observationally because they can have similar masses and radii as neutron stars. By performing the first calculation of the non-eq…