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20242026
most citedThe Science of the Einstein Telescope

97 citations · 132 across the 12 of their papers we have counts for

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6 papers · 1 filter

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

Stochastic gravitational-wave background from self-interacting superradiant clouds

Yin-Da Guo, Richard Brito, Chen Yuan

Gravitational-wave (GW) observations offer a powerful probe of new fundamental fields. One well-motivated source is black hole (BH)--boson cloud systems, in which an ultralight sca…

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

Extreme mass-ratio inspirals into Newtonian Proca stars

João Bernardo Silva, Richard Brito

Massive bosonic fields can form self-gravitating solitonic structures, which for vector fields are known as Proca stars. For ultralight fields, these structures can describe the co…

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…