activity
20242026
most citedQuantum Gravity Corrections to the Scalar Quasi-Normal Modes in Near-Extremal Reissener-Nordström Black Holes

3 citations · 4 across the 9 of their papers we have counts for

collaborators
Showing gr-qcShow all

8 papers · 1 filter

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

Can Oscillatory and Persistent Nonlinearities Be Bridged in Black Hole Ringdown?

Jun-Xi Shi, Zhen-Tao He, Jiageng Jiao +4

Quadratic quasinormal modes (QQNMs) and Christodoulou memory effect are key nonlinear phenomena in gravitational wave physics. QQNMs characterize the near zone nonlinear response o…

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

Internal structure of Hayward black holes

Caiying Shao, Jun-Qi Guo, Yu Tian +1

Regular black holes, free of central singularities, provide an ideal laboratory for probing the geometric structure of spacetime. The global structure of some regular black holes,…

gr-qc2025

Emergence of critical phenomena from the black hole interior

Caiying Shao, Junqi Guo, Yu Tian +1

The emergence of the singularity inside a spherically symmetric charged black hole, is studied numerically within the Einstein-Maxwell-real scalar model. When the scalar fiel…