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
Formation and Astrophysical Evidence

Ripples in Spacetime

5 / 9
Einstein predicted that violent cosmic events would ripple through spacetime itself. LIGO detects these gravitational waves using laser interferometry. When a wave passes, it stretches one arm of the detector while squeezing the other, changing the laser interference pattern by less than the width of a proton.
0:00 / 0:00

Generating Gravitational Waves

General Relativity predicts that accelerating massive objects distort spacetime, sending out ripples called gravitational waves. These waves stretch and squeeze space perpendicular to their direction of travel.

LIGO Detection Principle

LIGO uses laser interferometry to detect these tiny distortions. A passing wave changes the length of the detector's arms by a fraction of a proton width, altering the interference pattern of the lasers.

Previous5 / 9Next

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