A guided tour from Euclidean intuition to general relativity, exploring how curvature, density, and global topology shape the universe. We’ll unpack the cosmic microwave background clues, the omega parameter, and bold ideas like a finite, wrapped cosmos—and why these questions matter for the fate of everything we see.
Note: This podcast was AI-generated, and sometimes AI can make mistakes. Please double-check any critical information.
Sponsored by Embersilk LLC