55 citations · 212 across the 9 of their papers we have counts for
18 papers
Mass and effective spin distributions of binary black hole events: Evidence for a population of hierarchical black hole mergers in active galactic nuclei disks
Yuan-Zhu Wang, Yi-Zhong Fan, Shao-Peng Tang +2
The origins of the coalescing binary black holes (BBHs) detected by the advanced LIGO/Virgo are still in debate and clues may present in the mass and effective spin ()…
GRB 200716C: Evidence for a Short Burst Being Lensed
Yun Wang, Lu-Yao Jiang, Cheng-Kui Li +5
A tiny fraction of observed gamma-ray bursts (GRBs) may be lensed. The time delays induced by the gravitational lensing are milliseconds to seconds if the point lenses are intermed…
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…
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…