activity
20182026
most citedPSR J0030+0451, GW170817 and the nuclear data: joint constraints on equation of state and bulk properties of neutron stars

89 citations · 1k across the 60 of their papers we have counts for

collaborators
Showing 2020Show all

9 papers · 1 filter

astro-ph.HE2020★ 6 cited

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…

astro-ph.HE2020★ 53 cited

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…

astro-ph.HE2020★ 2 cited

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…

astro-ph.HE2020★ 32 cited

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…

astro-ph.HE2020★ 32 cited

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)…

astro-ph.HE2020★ 9 cited

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…

astro-ph.HE2020★ 7 cited

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…

astro-ph.HE2020★ 55 cited

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…

astro-ph.HE2020

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…