Why Escaping a Black Hole Is Physically Impossible | Feynman Explained скачать в хорошем качестве

Why Escaping a Black Hole Is Physically Impossible | Feynman Explained

#blackhole, #blackholes, #eventhorizon, #escapeblackhole, #blackholephysics, #physics, #theoreticalphysics, #astrophysics, #cosmology, What really happens beyond the event horizon? In this video, we explore the physics of black holes and why escape becomes impossible according to modern science. What if the reason you can't escape a black hole has nothing to do with speed? Most explanations stop at "the escape velocity exceeds the speed of light." That's technically correct — but it hides something far more disturbing about what space and time actually become inside an event horizon. The real reason is geometric, not mechanical. And once you understand it, you'll never think about space and time the same way again. In this video, we explore the physics of black holes through the lens of Richard Feynman's legendary teaching style — starting with something as simple as throwing a ball, then layering complexity until we arrive somewhere profound. Drawing on the conceptual approach found in Feynman's gravitational physics lectures and the rigorous spacetime geometry of Misner, Thorne, and Wheeler, this lecture builds from escape velocity to the Schwarzschild metric to the information paradox in one continuous arc. 📚 SOURCES: Richard P. Feynman, "Feynman Lectures on Gravitation," Lectures 10–13 (Addison-Wesley, 1995) Charles W. Misner, Kip S. Thorne, John A. Wheeler, "Gravitation," Chapters 31–34 (W.H. Freeman, 1973) Kip Thorne, "Black Holes and Time Warps: Einstein's Outrageous Legacy," Chapters 3, 6, 7 (W.W. Norton, 1994) John Michell, "On the Means of Discovering the Distance, Magnitude, &c. of the Fixed Stars," Philosophical Transactions of the Royal Society of London, Vol. 74 (1784) Karl Schwarzschild, "Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie," Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften (1916) S.W. Hawking, "Particle Creation by Black Holes," Communications in Mathematical Physics, Vol. 43 (1975) David Finkelstein, "Past-Future Asymmetry of the Gravitational Field of a Point Particle," Physical Review, Vol. 110 (1958) 🎙️ CREDITS: Script: AI-generated in the style of Richard Feynman Voice: AI-synthesized narration Visuals: AI-generated imagery Channel: [Your Channel Name] ⏱️ TIMESTAMPS: 00:00 – What happens when you throw a ball? 03:45 – Squeezing the Earth into a marble 08:10 – The country parson who predicted black holes in 1783 13:30 – Why Newton got the right answer for the wrong reason 18:50 – Einstein's revolution: gravity isn't a force 24:15 – Schwarzschild's solution from the trenches 29:40 – Inside the horizon: when space becomes time 36:20 – What you'd actually see falling in 42:00 – The photon sphere and how we photograph the invisible 47:30 – Hawking radiation and the information paradox 53:10 – Why escaping is like walking into yesterday What's more unsettling — that space and time can trade places, or that the boundary where it happens is completely invisible? ⚠️ WARNING: [This video is AI-generated (synthetic voice and visuals). It is an original, fictional lecture inspired by Richard Feynman's teaching style and public ideas, and is not an authentic recording, endorsement, or statement by Richard Feynman or his estate. Any resemblance is for educational/creative purposes #blackhole, #blackholes, #eventhorizon, #escapeblackhole, #blackholephysics, #physics, #theoreticalphysics, #astrophysics, #cosmology,