DarkLight: The Impact of Reionization on the Stellar-Mass-Halo-Mass Relation for Dwarf Galaxies

Explore a 23-minute conference talk on the impact of reionization on the stellar-mass-halo-mass relation for dwarf galaxies. Delivered by Stacy Kim from Carnegie Observatories, this presentation is part of the "Cosmic Signals of Dark Matter Physics: New Synergies" conference held at the Kavli Institute for Theoretical Physics. Delve into the latest research on dark matter physics, focusing on how reionization affects the relationship between stellar mass and halo mass in dwarf galaxies. Gain insights into the ongoing efforts to extract dark matter physics from cosmic observables and understand the constraints on dark matter models through astrophysical and cosmological probes. Discover new synergies between particle physics, cosmology, and astronomy in the quest to unravel the nature of dark matter.