Learning

Evidence for Dark Matter and Detection Methods

Observational Foundations of Galaxies → Synthesis and Open Questions

This advanced graduate-level path systematically builds the observational evidence for dark matter, from galactic rotation curves to cosmological probes, and then explores the leading particle candidates and detection strategies. It integrates necessary foundations in galactic dynamics, general relativity, particle physics, and cosmology, culminating in a critical assessment of current and future detection methods.