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Detecting the Beaming Effect of Gravitational Waves
Alejandro Torres-Orjuela, Xian Chen, Zhoujian Cao +2
The models currently used in the detection of gravitational waves (GWs) either do not consider a relative motion between the center-of-mass of the source and the observer, or usual…
Dark matter: an efficient catalyst for intermediate-mass-ratio-inspiral events
Xiao-Jun Yue, Wen-Biao Han, Xian Chen
Gravitational waves (GWs) can be produced if a stellar compact object, such as a black hole (BH) or neutron star, inspirals into an intermediate-massive black hole (IMBH) of $(10^3…
A New Type of Extreme-mass-ratio Inspirals Produced by Tidal Capture of Binary Black Holes
Xian Chen, Wen-Biao Han
Extreme-mass-ratio inspiral (EMRI) is an important gravitational-wave (GW) source and it normally consists of one stellar-mass black hole (BH) whirling closely around a supermassiv…
Testing general relativity using binary extreme-mass-ratio inspirals
Wen-Biao Han, Xian Chen
It is known that massive black holes (MBHs) of could capture small compact objects to form extreme-mass-ratio inspirals (EMRIs). Such systems emit gravitational…