210 citations · 1k across the 19 of their papers we have counts for
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The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy
Nai-Bo Zhang, Bin Qi, Shou-Yu Wang
The constraints on tidal deformability of neutron stars are first extracted from GW170817 by LIGO and Virgo Collaborations but the relation between radius and tidal deforma…
Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
Bao-An Li, Plamen G. Krastev, De-Hua Wen +1
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared goal of both nuclear physics and astrophysics. Except possible phase transitions, the densi…
Implications of the mass M of PSR~J0740+6620 on the Equation of State of Super-Dense Neutron-Rich Nuclear Matter
Nai-Bo Zhang, Bao-An Li
We study implications of the very recently reported mass M of PSR~J0740+6620 on the Equation of State (EOS) of super-dense neutron-rich nuclear matt…
Relation between gravitational mass and baryonic mass for non-rotating and rapidly rotating neutron stars
He Gao, Shun-Ke Ai, Zhou-Jian Cao +5
With a selected sample of neutron star (NS) equation-of-states (EOSs) that are consistent with the current observations and have a range of maximum masses, we investigate the relat…