collaborators

5 papers

astro-ph.CO2026

Statistical imprints of wave-like dark matter on multiply-imaged galaxies in strong cluster lenses from JWST

Nino Ephremidze, Daniel Gilman, Cora Dvorkin

Wave-like dark matter (DM) is an elusive dark matter (DM) candidate. The model, often also called fuzzy or ultralight DM, proposes that DM is an extremely light ($m\sim10^{-22}…

astro-ph.GA2026

Role of prompt cusps in driving the core collapse of SIDM halos

Vinh Tran, Daniel Gilman, M. Sten Delos +4

Prompt cusps (PCs) form from the direct collapse of overdensities in the early Universe, reside at the center of every dark matter halo, and have density profiles steeper than $r^{…

astro-ph.CO2026

LSST Strong Lensing Systems Dark Matter Sensitivity Analysis with Neural Ratio Estimators

Andreas Filipp, Yashar Hezaveh, Laurence Perreault-Levasseur +2

Strong gravitational lensing offers a unique probe of dark matter (DM) on sub-galactic scales, where the abundance and distribution of low-mass halos are highly sensitive to the un…

astro-ph.CO2025

Dark Matter Subhalos and Higher Order Catastrophes in Gravitational Wave Lensing

Luka Vujeva, Jose María Ezquiaga, Daniel Gilman +2

Gravitational lensing is an invaluable probe of the nature of dark matter, and the structures it forms. Lensed gravitational waves in particular allow for unparalleled sensitivity…

astro-ph.GA2025

Generating Dark Matter Subhalo Populations Using Normalizing Flows

Jack Lonergan, Andrew Benson, Daniel Gilman

Strong gravitational lensing is a powerful tool for probing the nature of dark matter, as lensing signals are sensitive to the dark matter substructure within the lensing galaxy. W…