SuperFast Guide to General Relativity
Quick and easy summaries of relativity and related subjects
General Relativity, also known as the General Theory of Relativity, is the theory of
gravitation published by Albert Einstein in 1915. It is the current description of gravity in
modern physics, one of the fundamental forces in the universe.
General Relativity refines Newton’s Law of Universal Gravitation, providing a unified
description of gravity as a property of space and time, called four-dimensional
spacetime. In particular, the curvature of spacetime is directly related to the energy
and momentum of whatever matter and radiation are present.
The relation is specified by the Einstein field equations. These are complex, requiring
much computation, and the effects are only significant at very high masses (such as
found near stars, for example). For this reason the paths of space probes are still
usually calculated using Newtonian gravitation. Any difference in the calculated results
of the two systems will almost always be so small as to be negligible.
Some predictions of General Relativity, however, are beyond Newton’s Law of
Universal Gravitation in classical physics. Examples include:
The passage of time: Time slows down near large masses. The larger the mass
the more time slows down.
The geometry of space, meaning light can bend around large masses such as
stars. A phenomena known as gravitational lensing.
Black holes: Regions of space from which even light cannot escape.
All tests of General Relativity have so far been shown to be in agreement with the
theory and have provided the modern framework for the history of the universe and
cosmology, thus leading to the discovery of the Big Bang. Despite the introduction of a
number of alternative theories, General Relativity is generally accepted by scientists to
be the simplest theory consistent with experimental data.
However, combining General Relativity with the laws of quantum physics remains a
problem and it is not yet known how gravity can be unified with the three non-
gravitational forces: strong, weak, and electromagnetic.
In summary: General Relativity is Albert Einstein’s theory of gravity, published in 1915,
which describes gravity as a curvature of space and time caused by mass and energy.
It predicts phenomena like gravitational time dilation and the existence of black holes.
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SuperFast Guide to
General Relativity