Date: Wednesday 23-Apr-2025
Time: 11:30-12:30 pm
Location: PSC 1136
Speaker: Nico Garavito-Camargo (University of Arizona)
Title: Galaxies in disequilibrium and the nature of Dark Matter
Abstract: Galaxies in the local universe exhibit signatures of disequilibrium at various scales—for example, disk perturbations such as warps, phase-space spirals, or lopsided stellar distributions. At even larger scales, the distribution of satellite galaxies is highly asymmetric in systems like the Milky Way and Andromeda.
In this talk, I will discuss how the presence of disequilibrium encodes valuable information about the dynamical state of dark matter halos and, consequently, the nature of dark matter itself. I will show how Basis Function Expansions (BFE) are an ideal tool to characterize the interplay between dark matter and baryonic matter in cosmological simulations. As a result, BFE enable the quantification of the dynamical state of galaxies across different dark matter models, allowing for direct comparison with the signatures of disequilibrium observed in the local universe.
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Special accommodations for individuals with disabilities can be made by calling (301) 405-3001. It would be appreciated if we are notified at least one week in advance.