collaborators

6 papers

astro-ph.GA2026

Strong Stellar Diffusion from Wave DM Cosmological Simulation and Potential Unified Origin for dSphs, UFGs, and UDGs

A. Pozo, T. Broadhurst, J. Zhang +6

Our DM simulations predict that stars diffuse throughout dark matter halos over the Hubble time through a random walk driven by the wave perturbations intrinsic to DM. The…

astro-ph.HE2026

Probing Axions with Relativistic Jet Polarimetry

Dashon Michel Jones, Richard Anantua, Razieh Emami +1

The prospect of identifying axion signals due to axion-photon coupling induced changes to the polarization has now become a reality in view of near-horizon polarimetric observation…

astro-ph.GA2025

A smooth filament origin for distant prolate galaxies seen by JWST and HST

Alvaro Pozo, Tom Broadhurst, Razieh Emami +7

The initial gravitational collapse of Dark Matter and gas forms a universal filamentary network where the first galaxies form, with shapes and sizes that depend on the choice of Da…

astro-ph.CO2025

Infalling ultra-faint dwarfs as emissaries of the Axiverse

A. Pozo, T. Broadhurst, H. N. Luu +8

Recent discoveries of ultra-faint dwarf galaxies (UFDs) infalling onto the Milky Way, namely Leo K \& M at kpc, considerably strengthens the case that UFDs constitute…

astro-ph.CO2025

Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint

Alvaro Pozo, Razieh Emami, Philip Mocz +9

Dark matter-dominated cores have long been claimed for the well-studied local group dwarf galaxies. More recently, extended stellar halos have been uncovered around several of thes…

astro-ph.CO2025

Diverse dark matter haloes in Two-field Fuzzy Dark Matter

Hoang Nhan Luu, Philip Mocz, Mark Vogelsberger +8

Fuzzy dark matter (FDM) is a compelling candidate for dark matter, offering a natural explanation for the structure of diffuse low-mass haloes. However, the canonical FDM model wit…