89 citations · 749 across the 24 of their papers we have counts for
24 papers
Long-term impact of the magnetic-field strength on the evolution and electromagnetic emission by neutron-star merger remnants
Jin-Liang Jiang, Harry Ho-Yin Ng, Michail Chabanov +1
Numerical simulations are essential to understand the complex physics accompanying the merger of binary systems of neutron stars. However, these simulations become computationally…
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…
The Bulk Properties of Isolated Neutron Stars Inferred from the Gravitational Redshift Measurements
Chuan-Ning Luo, Shao-Peng Tang, Jing-Liang Jiang +2
The measurements of the bulk properties of most isolated neutron stars (INSs) are challenging tasks. Tang et al. (2020) have developed a new method, based on the equation of state…
A hybrid approach to long-term binary neutron-star simulations
Harry Ho-Yin Ng, Jin-Liang Jiang, Carlo Musolino +3
One of the main challenges in the numerical modeling of binary neutron-star (BNS) mergers is long-term simulations of the post-merger remnant over timescales of the order of second…
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…
Bayesian analysis of neutron-star properties with parameterized equations of state: the role of the likelihood functions
Jin-Liang Jiang, Christian Ecker, Luciano Rezzolla
We have investigated the systematic differences introduced when performing a Bayesian-inference analysis of the equation of state of neutron stars employing either variable- or con…
Magnetic attractive interaction induced superconductivity in metals
Jinhuan Jiang
The BCS theory has described the conventional superconductors successfully.However,it is still not clear when the superconductivity occurs and why the resistance is zero.Also,there…
Bayesian inference of strange star equation of state using the GW170817 and GW190425 data
Zhiqiang Miao, Jin-Liang Jiang, Ang Li +1
The observations of compact star inspirals from LIGO/Virgo provide a valuable tool to study the highly uncertain equation of state (EOS) of dense matter at the densities in which t…
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…
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…
Maximum mass cutoff in the neutron star mass distribution and the prospect of forming supramassive objects in the double neutron star mergers
Dong-Sheng Shao, Shao-Peng Tang, Jin-Liang Jiang +1
The sample of neutron stars with a measured mass is growing quickly. With the latest sample, we adopt both a flexible Gaussian mixture model and a Gaussian plus Cauchy-Lorentz comp…
Bayesian inference of quark star equation of state using the NICER PSR J0030+0451 data
Ang Li, Zhi-Qiang Miao, Jin-Liang Jiang +2
We constrain the equation of state of quark stars within the Bayesian statistical approach using the mass and radius measurements of PSR J0030+0451 from NICER. Three types of bag m…
Constraint on phase transition with the multimessenger data of neutron stars
Shao-Peng Tang, Jin-Liang Jiang, Wei-Hong Gao +2
The equation of state (EoS) of the neutron star (NS) matter remains an enigma. In this work we perform the Bayesian parameter inference with the gravitational wave data (GW170817)…
Strong post-merger gravitational radiation of GW170817-like events
Yi-Zhong Fan, Jin-Liang Jiang, Shao-Peng Tang +2
The post-merger gravitational wave (GW) radiation of the remnant formed in the binary neutron star (BNS) coalescence has not been directly measured, yet. We show in this work that…
Constrains on the electric charges of the binary black holes with GWTC-1 events
Hai-Tian Wang, Peng-Cheng Li, Jin-Liang Jiang +3
Testing black hole's charged property is a fascinating topic in modified gravity and black hole astrophysics. In the first Gravitational-Wave Transient Catalog (GWTC-1), ten binary…
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…
Estimating the maximum gravitational mass of nonrotating neutron stars from the GW170817/GRB 170817A/AT2017gfo observation
Dong-Sheng Shao, Shao-Peng Tang, Xin Sheng +5
Assuming that the differential rotation of the massive neutron star (NS) formed in the double NS (DNS) mergers has been effectively terminated by the magnetic braking and a uniform…
PSR J0030+0451, GW170817 and the nuclear data: joint constraints on equation of state and bulk properties of neutron stars
Jin-Liang Jiang, Shao-Peng Tang, Yuan-Zhu Wang +2
Very recently the NICER collaboration has published the first-ever accurate measurement of mass and radius together for PSR J0030+0451, a nearby isolated quickly-rotating neutron s…
The Masses of Isolated Neutron Stars Inferred from the Gravitational Redshift Measurements
Shao-Peng Tang, Jin-Liang Jiang, Wei-Hong Gao +2
For some neutron stars (NSs) in the binary systems, the masses have been accurately measured. While for the isolated neutron stars (INSs), no mass measurement has been reported yet…
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…
GW170817: The energy extraction process of the off-axis relativistic outflow and the constraint on the equation of state of neutron stars
Yuan-Zhu Wang, Dong-Sheng Shao, Jin-Liang Jiang +6
As revealed recently by the modeling of the multi-wavelength data of the emission following GW170817/GRB 170817A, there was an off-axis energetic relativistic outflow component lau…
Total gravitational mass of the Galactic Double Neutron Star systems: evidence for a bimodal distribution
Yong-Jia Huang, Jin-Liang Jiang, Xiang Li +3
So far, in total 15 double neutron star systems (DNSs) with a reliable measurement of the total gravitational mass () have been detected in the Galaxy. In this work we s…
GW170817 and the prospect of forming supramassive remnants in neutron star mergers
Peng-Xiong Ma, Jin-Liang Jiang, Hao Wang +3
The gravitational wave data of GW170817 favor the equation of state (EoS) models that predict compact neutron stars (NSs), consistent with the radius constraints from X-ray observa…