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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
Hawking Radiation and Quantum Effects

Primordial Black Hole Challenge

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Now it's your turn. Here are five hypothetical black holes formed in the early universe. Remember, lighter ones die younger. Drag each one to either the 'Evaporated' pile or the 'Surviving' pile. Pay close attention to the mass values. A black hole with the mass of a mountain would have evaporated long ago, but one with the mass of the Sun is still here.
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A game-like challenge where the learner must identify which hypothetical black holes would have already evaporated by the present day based on their initial masses.

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