SuperFast Guide to General Relativity

Fact box… Time passes a tiny amount more slowly at the bottom of buildings than it does at the top. This is due to the bottom of the building being closer to the center of the Earth and therefore nearer to the center of its mass.
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.
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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. Suggested further reading:
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SuperFast Guide to
General Relativity
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Quick and easy summaries of relativity and related subjects

SuperFast Guide to General Relativity

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. Suggested further reading:
Energy from nuclear fusion - From stars to black holes Isn’t it just a theory? - The word theory has a different meaning in science