Lecture 3 · Block A — Mathematical + relativistic foundations · 42 min · HOST
General relativity
General relativity: geometry that responds to mass and energy.
About this lecture
Christoffel symbols, geodesics, the Riemann tensor, and Einstein’s field equations Gμν = 8πTμν. The two simplest exact solutions — Schwarzschild and FLRW — read carefully. Closes with the first block-transition beat tying the math to the simplicity-in-nature theme.
Excerpt
Christoffel symbols, geodesics, the Riemann tensor, and Einstein’s field equations Gμν = 8πTμν. The two simplest exact solutions — Schwarzschild and FLRW — read carefully. Closes with the first block-transition beat tying the math to the simplicity-in-nature theme.
Full script + citations available in the SME companion app. Audio narration via Google Cloud Chirp HD; lecture-length runtime ≈ 40–44 minutes.
What you'll learn
Each claim in this lecture is placed on the four-tier disciplinary spine: peer-reviewed-replicated, peer-reviewed-once, patent-attested, or claim-only. By the end of Season 1 listeners can read any new physics claim in this territory and place it correctly.