Skip to content
Learn Motion
ExploreHow it worksMembership
Log in
Learn Motion

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
Black Hole Thermodynamics

Hawking's Area Theorem

1 / 6
Hawking's Area Theorem tells us that the total surface area of event horizons can never decrease. Imagine two black holes spiraling inward and merging. The resulting single black hole has a larger horizon area than the sum of the two original areas. This irreversible increase in area strongly resembles the Second Law of Thermodynamics, where entropy always increases. This led physicists to suspect that black hole area is actually a form of entropy.
0:00 / 0:00

Introduction to Hawking's Area Theorem, stating that the total surface area of event horizons cannot decrease over time in classical general relativity.

Previous1 / 6Next

Learn Motion

Generate a course. Learn it properly.

Operated by Wuhan Daoyin Technology Co., Ltd.

Contact: [email protected]
Privacy PolicyTerms of Service

© 2026 Learn Motion