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-mode Stability of GW190814's Secondary Component as a Supermassive and Superfast Pulsar
Xia Zhou, Ang Li, Bao-An Li
The nature of GW190814's secondary component of mass in the mass gap between the currently known maximum mass of neutron stars and the minimum…
GW190814's secondary component with mass M as a super-fast pulsar
Nai-Bo Zhang, Bao-An Li
Using Stergioulas's RNS code for investigating fast pulsars with Equation of States (EOSs) on the causality surface (where the speed of sound equals that of light) of the high-dens…
Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars
Wen-Jie Xie, Bao-An Li
Using an explicitly isospin-dependent parametric Equation of State (EOS) for the core of neutron stars (NSs) within the Bayesian statistical approach, we infer the EOS parameters o…
Constraints on the muon fraction and density profile in neutron stars
Nai-Bo Zhang, Bao-An Li
Muons in neutron stars (NSs) play especially important roles in addressing several interesting new physics questions associated with detecting as well as understanding interactions…
Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars
Wen-Jie Xie, Bao-An Li
The radius of neutron stars (NSs) with a mass of 1.4 M has been extracted consistently in many recent studies in the literature. Using representative …
Deep crustal heating by neutrinos from the surface of accreting neutron stars
F. J. Fattoyev, Edward F. Brown, Andrew Cumming +4
We present a new mechanism for deep crustal heating in accreting neutron stars. Charged pions () are produced in nuclear collisions on the neutron star surface during active a…