Dong-Sheng Shao

activity

20182023

M_{TOV} = 2.2 5_{- 0.07}^{+ 0.08} M_{⊙}

inferred at about

3%

precision with multimessenger data of neutron stars

77 citations · 231 across the 5 of their papers we have counts for

collaborators

Showing 2019Show all

2 papers · 1 filter

astro-ph.HE2019★ 51 cited

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…

astro-ph.HE2019★ 25 cited

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 ${p^_{1}, p^_{2}, p^_{3}, p^_{4}}$ and then set…