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Black Holes: Physics, Structure, and Theory

1Introduction to Black Holes and Historical Context2Foundations of General Relativity3The Schwarzschild Solution4Geometry of Spacetime and Tidal Forces5Rotating Black Holes: The Kerr Metric6Black Hole Thermodynamics7Hawking Radiation and Quantum Effects8The Information Paradox9Formation and Astrophysical Evidence10Direct Imaging and Future Horizons
Formation and Astrophysical Evidence

Simulating a Black Hole Merger

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This simulation shows the final moments of two black holes. As they orbit, they emit gravitational waves, losing energy and spiraling closer. They eventually merge into one, followed by a 'ringdown' phase where the new black hole settles into a stable shape. Notice how the frequency and amplitude of the waves increase until the merger.
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Interactive visualization of two black holes spiraling inward and merging, emitting gravitational waves.

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