activity
20242026
collaborators

6 papers

astro-ph.HE2026

A Collapsar-Disk Origin for GW190814

Vishal Baibhav, Brian D. Metzger, Lam Hui

GW190814 was a remarkable gravitational-wave (GW) event: a merger between a 23 solar-mass black hole (BH) and a 2.6 solar-mass compact object, with an extreme mass ratio that is di…

hep-ph2026

An ultra-broadband axion dark matter experiment

Angelo Esposito, Kin Chung Fong, Lam Hui

We propose a novel broadband strategy to search for axions by leveraging observables controlled by the axion field squared. We present a practical implementation of this concept fo…

astro-ph.CO2025

Caustic fringes for wave dark matter

Andrew Eberhardt, Lam Hui

Wave dark matter is composed of particles sufficiently light that their de Broglie wavelength exceeds the average inter-particle separation. A typical wave dark matter halo exhibit…

astro-ph.CO2025

Heating and scattering of stellar distributions by ultralight dark matter

Andrew Eberhardt, Mateja Gosenca, Lam Hui

Due to wave interference, an ultralight light dark matter halo has stochastic, granular substructures which can scatter stars, leading to the heating of stellar distributions. Stud…

gr-qc2024

Black hole spectroscopy with nonlinear quasi-normal modes

Macarena Lagos, Tomás Andrade, Jordi Rafecas-Ventosa +1

The future detection of quasi-normal modes (QNMs) from black hole ringdown will allow for consistency and independent tests of general relativity (GR) in the strong-field regime. I…

gr-qc2024

The impact of initial conditions on quasi-normal modes

Ameya Chavda, Macarena Lagos, Lam Hui

This study investigates the influence of initial conditions on the evolution and properties of linear quasi-normal modes (QNMs). Using a toy model in which the quasi-normal mode ca…