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General Relativity

General relativity is Einstein's geometric theory of gravitation, published in 1915, which reinterprets gravity not as a force acting between masses but as the curvature of a four-dimensional spacetime continuum caused by the presence of mass and energy.

Type: Concept Domain: Physics Mathematics Philosophy

Overview

Massive objects warp the fabric of spacetime, and other objects and even light follow geodesics — the straightest possible paths — through that curved geometry; the equivalence principle asserts that gravitational acceleration is locally indistinguishable from inertial acceleration, and the theory is expressed through Einstein's field equations, which relate spacetime curvature to the distribution of matter and energy.

Why it matters

General relativity constitutes a foundational revolution in humanity's understanding of space, time, and causality, predicting phenomena Newtonian gravity could not account for — Mercury's perihelion precession, light bending around the Sun, gravitational redshift — and has been confirmed most dramatically by LIGO's direct detection of gravitational waves in 2015 and the first imaging of a black hole event horizon in 2019.

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