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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…