77 citations · 412 across the 19 of their papers we have counts for
19 papers
SACRA-K: A Performance-Portable Numerical Relativity Code with Kokkos
Ming-Zhe Han, Kenta Kiuchi, Masaru Shibata
We present SACRA-K (SimulAtor for Compact objects in Relativistic Astrophysics with Kokkos), a performance-portable numerical relativity code ported from the Fortran code SACRA-MPI…
Subsolar-mass binary mergers of strange stars and neutron stars: gravitational waves and ejecta
Yong Gao, Ming-Zhe Han, Kenta Kiuchi +3
We present the first numerical-relativity simulations of subsolar-mass binary strange star (SS) mergers and compare with binary neutron star (NS) mergers across equations of state,…
Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers
Ming-Zhe Han, Yong Gao, Kenta Kiuchi +1
We systematically perform numerical-relativity simulations for equal-mass binary neutron star mergers for the models varying the thermal index with three different equ…
Bulk properties of PSR J0030+0451 inferred with the compactness measurement of NICER
Chuan-Ning Luo, Shao-Peng Tang, Ming-Zhe Han +3
In 2019, Neutron star Interior Composition ExploreR (NICER) mission released its findings on the mass and radius of the isolated neutron star (INS) PSR J0030+0451, revealing a mass…
Upper Limit of Sound Speed in Nuclear Matter: A Harmonious Interplay of Transport Calculation and Perturbative Quantum Chromodynamic Constraint
Shao-Peng Tang, Yong-Jia Huang, Ming-Zhe Han +1
Very recently, it has been shown that there is an upper bound on the squared sound speed of nuclear matter from the transport, which reads . In this work, w…
Mass and radius of the most massive neutron star: The probe of the equation of state and perturbative QCD
Shao-Peng Tang, Ming-Zhe Han, Yong-Jia Huang +2
Recently, an association of GW190425 and FRB 20190425A had been claimed and a highly magnetized neutron star (NS) remnant was speculated. Given the -h delay of the occurr…
Maximum gravitational mass inferred at about precision with multimessenger data of neutron stars
Yi-Zhong Fan, Ming-Zhe Han, Jin-Liang Jiang +2
The maximal gravitational mass of nonrotating neutron stars () is one of the key parameters of compact objects and only loose bounds can be set based on the first prin…
Plausible presence of new state in neutron stars with masses above
Ming-Zhe Han, Yong-Jia Huang, Shao-Peng Tang +1
We investigate the neutron star (NS) equation of state (EOS) by incorporating multi-messenger data of GW170817, PSR J0030+0451, PSR J0740+6620, and state-of-the-art theoretical pro…
Nonparametric Representation of Neutron Star Equation of State Using Variational Autoencoder
Ming-Zhe Han, Shao-Peng Tang, Yi-Zhong Fan
We introduce a new nonparametric representation of the neutron star (NS) equation of state (EoS) by using the variational autoencoder (VAE). As a deep neural network, the VAE is fr…
Constraints on the phase transition and nuclear symmetry parameters from PSR and multimessenger data of other neutron stars
Shao-Peng Tang, Jin-Liang Jiang, Ming-Zhe Han +2
Recently, the radius of neutron star (NS) PSR J0740+6620 was measured by Neutron Star Interior Composition Explorer (NICER) and an updated measurement of neutron skin thickness of…
Black Hole Mass Function of Coalescing Binary Black Hole Systems: Is There a Pulsational Pair Instability Mass Cutoff?
Yuan-Zhu Wang, Shao-Peng Tang, Yun-Feng Liang +5
We analyze the LIGO/Virgo GWTC-2 catalog to study the primary mass distribution of the merging black holes. We perform hierarchical Bayesian analysis, and examine whether the mass…
Tight constraints on Einstein-dilation-Gauss-Bonnet gravity from GW190412 and GW190814
Hai-Tian Wang, Shao-Peng Tang, Peng-Cheng Li +2
Gravitational-wave (GW) data can be used to test general relativity in the highly nonlinear and strong field regime. Modified gravity theories such as Einstein-dilation-Gauss-Bonne…
Bayesian nonparametric inference of neutron star equation of state via neural network
Ming-Zhe Han, Jin-Liang Jiang, Shao-Peng Tang +1
We develop a new nonparametric method to reconstruct the Equation of State (EoS) of Neutron Star with multimessenger data. As an universal function approximator, the Feed-Forward N…
GW190426_152155: a merger of neutron star-black hole or low mass binary black holes?
Yin-Jie Li, Ming-Zhe Han, Shao-Peng Tang +5
GW190426_152155 was recently reported as one of the 39 candidate gravitational wave (GW) events in \citet{2020arXiv201014527A}, which has an unusual source-frame chirp mass $\sim 2…
GW190521 and the GWTC-1 Events: Implication on the Black Hole Mass Function of Coalescing Binary Black Hole Systems
Yuan-Zhu Wang, Shao-Peng Tang, Yun-Feng Liang +5
With the black hole mass function (BHMF; assuming an exponential cutoff at a mass of ) of coalescing binary black hole systems constructed with the events detecte…
Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
Shao-Peng Tang, Hao Wang, Yuan-Zhu Wang +3
The discovery of gravitational waves from compact objects coalescence opens a brand-new window to observe the universe. With more events being detected in the future, statistical e…
Is GW190425 consistent with being a neutron starblack hole merger?
Ming-Zhe Han, Shao-Peng Tang, Yi-Ming Hu +5
GW190425 is the second neutron star merger event detected by the Advanced LIGO/Virgo detectors. If interpreted as a double neutron star merger, the total gravitational mass is subs…
The roles of individual advanced LIGO detectors on revealing the neutron star properties
Ming-zhe Han, Jin-liang Jiang, Shao-peng Tang +2
In this work we re-analyze the data of GW170817, the first binary neutron star (BNS) merger event, in two ways, including the parameterized equation of state (EoS) method and gravi…
The equation of state and some key parameters of neutron stars: constraints from GW170817, the nuclear data and the low mass X-ray binary data
Jin-Liang Jiang, Shao-Peng Tang, Dong-Sheng Shao +6
In this work we parameterize the Equation of State of dense neutron star (NS) matter with four pressure parameters of and then set…