collaborators

6 papers

gr-qc2026

Living on the Edge of Effective Field Theory: Near-Extremal Black Holes in Quadratic Gravity

Kelvin Ka-Ho Lam, Gary T. Horowitz, Nicolás Yunes

Near-extremal black holes can amplify higher-derivative corrections to general relativity, making them sharp probes of the perturbative control of gravitational effective field the…

gr-qc2026

Measuring a Black Hole's Area Immediately after Merger: A Direct-Wave Test of Hawking's Area Law

Adrian Ka-Wai Chung, Kelvin Ka-Ho Lam, Anna Liu +1

Black-hole area is the geometric variable behind horizon thermodynamics. We introduce a gravitational-wave method to infer a Kerr-equivalent horizon area from direct waves in the n…

gr-qc2026

Quadratic gravity corrections to scalar QNMs of rapidly rotating black holes

Stef J. B. Husken, Tom van der Steen, Simon Maenaut +6

In an effective-field-theory framework for gravity, black-hole quasinormal mode spectra acquire corrections in quadratic-curvature, scalar-tensor extensions of general relativity.…

gr-qc2026

Spinning Black Holes in Modified Gravity via Spectral Methods

Kelvin Ka-Ho Lam, Adrian Ka-Wai Chung, Nicolás Yunes

Rapidly-rotating black-hole spacetimes outside general relativity are key to many tests of Einstein's theory. We here develop an efficient spectral method to represent such spaceti…

gr-qc2026

Analytic and accurate approximate metrics for black holes with arbitrary rotation in beyond-Einstein gravity using spectral methods

Kelvin Ka-Ho Lam, Adrian Ka-Wai Chung, Nicolás Yunes

A key obstacle for theory-specific tests of general relativity is the lack of accurate black-hole solutions in beyond-Einstein theories, especially for moderate to high spins. We a…

gr-qc2025

Quasinormal mode frequencies and gravitational perturbations of spinning black holes in modified gravity through METRICS: The dynamical Chern-Simons gravity case

Adrian Ka-Wai Chung, Kelvin Ka-Ho Lam, Nicolas Yunes

We present the first precise calculations of the gravitational quasinormal-mode (QNM) frequencies for spinning black holes with dimensionless angular momenta $J/M^2 := a \lesssim 0…