Dwarkesh Podcast

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Adam Brown – A deep but accessible introduction to general relativity

Explore episode Jul 10, 2026
History
Eddington's 1919 Eclipse and Einstein's Near Miss

Adam Brown – A deep but accessible introduction to general … · Jul 10, 2026 History

Two eclipse expeditions failed before 1919 — Argentina got clouded out, and a German team was arrested when WWI broke out. That was lucky: Einstein's pre-GR prediction was wrong, predicting only the Newtonian bending. He corrected it to double the Newtonian value during the quiet of the war, just in time for Eddington's successful 1919 expedition.

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The three ways we know black holes are real

At 1:21:40 · chapter starts 1:18:51

The distant observer sees something strange: as the infaller approaches the event horizon, gravitational time dilation makes them appear to move slower and slower, their light redshifts from visible to infrared to radio, and eventually they just fade — the last photon arrives, and then silence. The observer never crosses, as seen from outside. But from the infaller's own perspective, their clock ticks normally, the horizon is unremarkable, and for a galactic-mass black hole the tidal forces at the horizon are too weak to feel. Brown emphasises that the event horizon is 'teleological' — it is not a locally measurable feature but a fact about your future. For a large enough black hole you could have descendants born inside the event horizon, live out a normal life, and only die at the singularity.

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