activity
20222026
most citedImproved Analytic Solution of Black Hole Superradiance

26 citations · 35 across the 5 of their papers we have counts for

collaborators

6 papers

gr-qc2026

Chaotic signatures in extreme-mass-ratio systems surrounded by bosonic environments

Qi-Xuan Xu, Kyriakos Destounis, Yin-Da Guo +2

Extreme-mass-ratio inspirals are key gravitational-wave sources for testing strong gravity and the environments of massive black holes. While orbital motion in Kerr black hole spac…

gr-qc2026

Revisiting environmental effects on black hole quasibound-state spectra with relativistic perturbation theory

Yin-Da Guo, Qi-Xuan Xu, Richard Brito +1

We present a relativistic framework for computing corrections to the eigenfrequency spectrum of a massive scalar field in perturbed black-hole spacetimes, including first-order shi…

gr-qc2026

Resonances as signatures of scalar clouds in eccentric extreme-mass-ratio inspirals

Qi-Xuan Xu, Richard Brito, Riccardo Della Monica +2

Ultralight scalars arise naturally in many extensions to the Standard Model and are compelling dark matter candidates. Around spinning black holes, dense scalar clouds could form t…

gr-qc2026

Relativistic effects in extreme-mass-ratio inspirals within scalar clouds: Eccentric and inclined orbits

Qi-Xuan Xu, Richard Brito, Riccardo Della Monica +2

We study extreme-mass-ratio inspirals (EMRIs) evolving in a scalar cloud environment that may form through superradiant instabilities, using a fully relativistic perturbative frame…

gr-qc2023★ 9 cited

Next-to-leading-order solution to Kerr-Newman black hole superradiance

Shou-Shan Bao, Qi-Xuan Xu, Hong Zhang

The superradiant instabilities of Kerr-Newman black holes with charged or uncharged massive spin-0 fields are calculated analytically to the next-to-leading order in the limit of $…

gr-qc2022★ 26 cited

Improved Analytic Solution of Black Hole Superradiance

Shou-Shan Bao, Qi-Xuan Xu, Hong Zhang

The approximate solution of the Klein-Gordon equation for a real scalar field of mass in the geometry of a Kerr black hole obtained by Detweiler \cite{Detweiler:1980uk} is wide…