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20242026
most citedNumerical computation of electromagnetically sourced nonlinear tails

1 citations · 1 across the 5 of their papers we have counts for

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gr-qc2026

Vanishing Love Numbers of Kerr-Newman Black Holes

Sumanta Chakraborty, Takuya Katagiri, Paolo Pani +1

Tidal Love numbers characterize the conservative response of compact objects to external perturbations and provide a powerful probe of their nature. While the static Love numbers o…

gr-qc2026

Astrophysically Realistic Secondary Spins Trigger Chaos in Schwarzschild Spacetime and Discernible Gravitational Wave Signatures

Dan-Dan Yuan, Jia-Geng Jiao, Yu-Qi Lei +4

Chaos in extreme-mass-ratio inspirals is often thought to require unrealistically large secondary spins, making its astrophysical relevance uncertain. However, we find that chaos p…

gr-qc2026

Nonlinear tails of massive scalar fields around a black hole

Caiying Shao, Zhen-Tao He, Jiageng Jiao +5

Nonlinear effects play a fundamental role in the late-time ringdown of black holes, with direct implications for gravitational-wave observations. For massive fields, these dynamics…

gr-qc2025

Reconstruction of Black Hole Ringdown Signals with Data Gaps using a Deep-Learning Framework

Jing-Qi Lai, Jia-Geng Jiao, Cai-Ying Shao +2

We introduce DenoiseGapFiller (DGF), a deep-learning framework specifically designed to reconstruct gravitational-wave ringdown signals corrupted by data gaps and instrumental nois…

gr-qc2025★ 1 cited

Numerical computation of electromagnetically sourced nonlinear tails

Zhen-Tao He, Jia Du, Jiageng Jiao +4

Amazingly, recent studies indicate that nonlinear effects are of great significance for modelling black hole ringdown. Transient electromagnetic events in the astrophysical environ…

gr-qc2024

The effects of data gaps on ringdown signals with space-based joint observation

Junxi Shi, Jiageng Jiao, Jingqi Lai +3

In space-based gravitational wave observatories such as Taiji, LISA, and TianQin, data gaps are inevitable due to mission design, implementation, and the long duration of observati…