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20242026
most citedHushing black holes: tails in dynamical spacetimes

26 citations · 39 across the 7 of their papers we have counts for

collaborators

7 papers

hep-ph2026

Dynamics and Frequency Conversion of Accreting Axion Clouds

Ximeng Li, Zhen Zhong, Yifan Chen +3

Axion fields can form exponentially growing gravitational clouds around compact objects through self-interaction-driven relaxation of ambient axion waves. As the field amplitude ap…

astro-ph.HE2026

Black Hole Ringdown Seen in Photon Polarization Swings

Jiewei Huang, Yehui Hou, Zhen Zhong +2

Light propagating through a perturbed spacetime could imprint the underlying gravitational waveform directly onto electromagnetic observables. In this Letter, we develop a covarian…

gr-qc2025

Ultralight Boson Ionization from Comparable-Mass Binaries

Yuhao Guo, Zhen Zhong, Yifan Chen +3

Detection of gravitational waves enables probes of environmental effects around compact binaries. Ultralight bosons, well motivated in particle physics and capable of forming core-…

astro-ph.CO2025

Whispers from the Early Universe: The Ringdown of Primordial Black Holes

Chen Yuan, Zhen Zhong, Qing-Guo Huang

We investigate the stochastic gravitational wave background (SGWB) generated by the ringdown phase of primordial black holes (PBHs) formed in the early universe. As the ringdown si…

gr-qc2024★ 9 cited

Forward Ray Tracing and Hot Spots in Kerr Spacetime

Lihang Zhou, Zhen Zhong, Yifan Chen +1

Hotspots, often characterized as pointlike emissions, frequently appear near black holes with significantly enhanced luminosity compared to the surrounding accretion flow. Notably,…

gr-qc2024★ 4 cited

Dynamical Lensing Tomography of Black Hole Ringdown

Zhen Zhong, Vitor Cardoso, Yifan Chen

Strong gravitational lensing occurs when photons pass through the vicinity of a black hole. We investigate this phenomenon in the context of a gravitational-wave event, specificall…

gr-qc2024★ 26 cited

Hushing black holes: tails in dynamical spacetimes

Vitor Cardoso, Gregorio Carullo, Marina De Amicis +6

Stationary, asymptotically flat, black hole solutions of the vacuum field equations of General Relativity belong to the Kerr family. But how does one approach this state, dynamical…