44 citations · 126 across the 7 of their papers we have counts for
23 papers
Amplification of gravitational wave by a Kerr black hole
Yi Gong, Zhoujian Cao, Xian Chen
Binary black hole may form near a supermassive black hole. The background black hole (BH) will affect the gravitational wave (GW) generated by the binary black hole. It is well kno…
The missing link in gravitational-wave astronomy: A summary of discoveries waiting in the decihertz range
Manuel Arca Sedda, Christopher P L Berry, Karan Jani +25
Since 2015 the gravitational-wave observations of LIGO and Virgo have transformed our understanding of compact-object binaries. In the years to come, ground-based gravitational-wav…
The last migration trap of compact objects in AGN accretion disc
Peng Peng, Xian Chen
Many black holes (BHs) detected by the Laser Interferometer Gravitational-wave Observatory (LIGO) and the Virgo detectors are multiple times more massive than those in X-ray binari…
Stellar rotation as a new observable to test general relativity in the Galactic Center
Yun Fang, Xian Chen
S-stars in the Galactic Center are excellent testbeds of various general relativistic effects. While previous works focus on modeling their orbital motion around Sgr A*--the superm…
Degeneracy between mass and peculiar acceleration for the double white dwarfs in the LISA band
Zeyuan Xuan, Peng Peng, Xian Chen
Mass and distance are fundamental quantities to measure in gravitational-wave (GW) astronomy. However, recent studies suggest that the measurement may be biased due to the accelera…
Exciting modes due to the aberration of gravitational waves: Measurability for extreme-mass-ratio inspirals
Alejandro Torres-Orjuela, Pau Amaro Seoane, Zeyuan Xuan +3
Gravitational waves from a source moving relative to us can suffer from special-relativistic effects such as aberration. The required velocities for these to be significant are on…