General relativity, also known as the
general theory of relativity, and as
Einstein's theory of gravity, is the
geometric theory of
gravitation published by
Albert Einstein in May 1916 and is the accepted description of the gravitation of macroscopic objects in
modern physics. General
relativity generalizes
special relativity and refines
Isaac Newton's
law of universal gravitation, providing a unified description of gravity as a geometric property of
space and
time, or four-dimensional
spacetime. In particular, the
curvature of spacetime is directly related to the
energy,
momentum and
stress of whatever is present, including
matter and
radiation. The relation is specified by the
Einstein field equations, a system of second-order
partial differential equations.
John Archibald Wheeler summarized it: "Space-time tells matter how to move; matter tells space-time how to curve."
Newton's law of universal gravitation, which describes gravity in classical mechanics, can be seen as a prediction of general relativity for the almost flat spacetime geometry around stationary mass distributions. Some predictions of general relativity, however, are beyond Newton's law of universal gravitation in
classical physics. These predictions concern the passage of time, the
geometry of space, the motion of bodies in
free fall, and the propagation of light, and include
gravitational time dilation,
gravitational lensing, the
gravitational redshift of light, the
Shapiro time delay and
singularities/
black holes. So far, all
tests of general relativity have been in agreement with the theory. The time-dependent solutions of general relativity enable us to extrapolate the history of the universe into the past and future, and have provided the modern framework for
cosmology, thus leading to the discovery of the
Big Bang and
cosmic microwave background radiation. Despite the introduction of a number of
alternative theories, general relativity continues to be the simplest theory consistent with
experimental data. (
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