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astro-ph.HE2023
Double Neutron Star Mergers: Are Late-time Radio Signals Overestimated?
Shao-Ze Li, Yun-Wei Yu, He Gao +1
The coalescence of binary neutron stars can yield the expulsion of a fast-moving, quasi-isotropic material, which may induce thermal radiation and give rise to kilonova emission. M…
gr-qc2023
On the possibility to detect gravitational waves from post-merger super-massive neutron stars with a kilohertz detector
Yikang Chen, Bin Liu, Shunke Ai +4
The detection of a secular post-merger gravitational wave (GW) signal in a binary neutron star (BNS) merger serves as strong evidence for the formation of a long-lived post-merger…
astro-ph.HE2023
What constraints can one pose on the maximum mass of neutron stars from multi-messenger observations?
Shunke Ai, He Gao, Yong Yuan +2
The maximum mass of neutron stars () plays a crucial role in understanding their equation of state (EoS). Previous studies have used the measurements for the compactne…