CDM/WDM Small Scale Structure - Sub-Halo Counting with Stellar Streams

Explore the latest research on dark matter structure through a 20-minute conference talk focusing on CDM/WDM small scale structure and sub-halo counting with stellar streams. Delivered by Raymond Carlberg from the University of Toronto, this presentation is part of the "Cosmic Signals of Dark Matter Physics: New Synergies" conference held at the Kavli Institute for Theoretical Physics. Gain insights into the ongoing efforts to constrain dark matter physics using cosmic observables, including astrophysical and cosmological probes. Delve into the synthesis of theoretical, computational, and observational approaches aimed at unraveling the nature of dark matter across various cosmic epochs and length scales.

CDM/WDM small scale structure: Sub-Halo counting with Stellar Streams ▸ Raymond Carlberg (U Toronto)