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Brown closes by surveying why physicists came to accept black holes: Penrose’s theoretical theorems showed black-hole formation is generic in collapse, and multiple observational pillars followed — decades of stellar orbits around Sagittarius A* indicate a very massive, compact dark object; the LIGO gravitational-wave detections (starting with the late-2015 binary black-hole merger ~1.6 billion light years away) directly measured spacetime dynamics from colliding black holes; and the Event Horizon Telescope imaged the compact accretion shadows consistent with horizons. He contrasts this empirical success with more speculative fronts (quantum gravity, string theory): thought alone can go far (Einstein’s example) but often experiment is essential to break theoretical branching. He ends by reflecting on pedagogy — how a 10-week course can distill Einstein’s core insight for non-specialists — and on broader implications for theory-building in the age of AI, noting both the potential of machine discovery and the enduring necessity of experiments.
Adam Brown (currently at Blue Shift / Google DeepMind, formerly a Stanford physicist) traces GR from Newton (1680s) and Einstein’s 1905 special relativity to his “most beautiful thought” in 1907 and the finished field equations in 1915.
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