activity
20242026
collaborators

6 papers

gr-qc2026

Topologically equivalent yet radiatively distinct orbits in EMRI system

Chao-Hui Wang, Shao-Wen Wei, Tao Zhu +1

Multiple potential wells for massive test particles, allowing distinct families of bound orbits to coexist, are a characteristic feature of certain exotic compact objects beyond ge…

gr-qc2026

Magnetic field effects on spherical orbit in Kerr-Bertotti-Robinson spacetime: constraints from jet precession of M87*

Chao-Hui Wang, Xiang-Cheng Meng, Shao-Wen Wei

The recently reported precession period of about years of the M87* jet provides a sensitive probe of strong field gravity and the electromagnetic environment in the immedia…

gr-qc2026

Gravitational equal-area law and critical phenomena of cuspy black hole shadow

Shao-Wen Wei, Chao-Hui Wang, Yu-Peng Zhang +2

The formation of a cusp on a black hole shadow is a striking signature of physics beyond the Kerr paradigm. We demonstrate that this morphological change fundamentally alters the s…

gr-qc2025

Equatorial periodic orbits and gravitational waveforms in a black hole free of Cauchy horizon

Chao-Hui Wang, Xiang-Cheng Meng, Yu-Peng Zhang +2

In this paper, we study the periodic orbits and gravitational wave radiation in an extreme mass ratio inspiral system, where a stellar-mass object orbits a supermassive black hole…

gr-qc2025

A new type of multi-branch periodic orbits in dyonic black holes

Chao-Hui Wang, Yu-Peng Zhang, Tao Zhu +1

We investigate bound timelike periodic orbits in dyonic black hole spacetimes arising from quasi-topological electromagnetism. By varying the coupling parameter , we show that…

gr-qc2024

Imprints of black hole charge on the precessing jet nozzle of M87*

Xiang-Cheng Meng, Chao-Hui Wang, Shao-Wen Wei

The observed jet precession period of approximately 11 years for M87* strongly suggests the presence of a supermassive rotating black hole with a tilted accretion disk at the cente…