56 citations · 281 across the 15 of their papers we have counts for
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Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
Jin-Ping Zhu, Shichao Wu, Yuan-Pei Yang +8
In the second work of this series, we explore the optimal search strategy for serendipitous and gravitational-wave-triggered target-of-opportunity (ToO) observations of kilonovae a…
Prospects for detecting exoplanets around double white dwarfs with LISA and Taiji
Yacheng Kang, Chang Liu, Lijing Shao
Recently, Tamanini & Danielski (2019) discussed the possibility to detect circumbinary exoplanets (CBPs) orbiting double white dwarfs (DWDs) with the Laser Interferometer Space Ant…
New limits on the Lorentz/CPT symmetry through fifty gravitational-wave events
Ziming Wang, Lijing Shao, Chang Liu
Lorentz invariance plays a fundamental role in modern physics. However, tiny violations of the Lorentz invariance may arise in some candidate quantum gravity theories. Prominent si…
Stringent Tests of Gravity with Highly Relativistic Binary Pulsars in the Era of LISA and SKA
Xueli Miao, Heng Xu, Lijing Shao +2
At present, 19 double neutron star (DNS) systems are detected by radio timing and 2 merging DNS systems are detected by kilo-hertz gravitational waves. Because of selection effects…
Neutron StarNeutron Star and Neutron StarBlack Hole Mergers: Multiband Observations and Early Warnings
Chang Liu, Lijing Shao
The detections of gravitational waves (GWs) from binary neutron star (BNS) systems and neutron star--black hole (NSBH) systems provide new insights into dense matter properties in…
Probing dipole radiation from binary neutron stars with ground-based laser-interferometer and atom-interferometer gravitational-wave observatories
Junjie Zhao, Lijing Shao, Yong Gao +3
Atom-interferometer gravitational-wave (GW) observatory, as a new design of ground-based GW detector for the near future, is sensitive at a relatively low frequency for GW observat…