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Theory of relativity

 
WordNet: theory of relativity
 
Note: click on a word meaning below to see its connections and related words.

The noun has one meaning:

Meaning #1: (physics) the theory that space and time are relative concepts rather than absolute concepts
  Synonyms: relativity, relativity theory, Einstein's theory of relativity


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Wikipedia: Theory of relativity
 
Two-dimensional projection of a three-dimensional analogy of space-time curvature described in General Relativity.
This page is about the scientific concept of relativity, for philosophical or sociological theories about relativity see Relativism.

The theory of relativity, or simply relativity, generally refers specifically to two theories of Albert Einstein: special relativity and general relativity. However, the word "relativity" is sometimes used in reference to Galilean invariance.

The term "theory of relativity" was coined by Max Planck in 1908 to emphasize how special relativity (and later, general relativity) uses the principle of relativity.

Contents

Special relativity

E = mc2

Special relativity is a theory of the structure of spacetime. It was introduced in Albert Einstein's 1905 paper "On the Electrodynamics of Moving Bodies"; however, the term was first used by Galileo Galilei in 1632 in his Dialogue concerning the World's Two Chief Systems. But Galileo's version was flawed: for example, he thought the spin of the Earth caused the tides[1]. Special relativity is based on two postulates which are contradictory in classical mechanics:

  1. The laws of physics are the same for all observers in uniform motion relative to one another (Galileo's principle of relativity),
  2. The speed of light in a vacuum is the same for all observers, regardless of their relative motion or of the motion of the source of the light.

The resultant theory has many surprising consequences. Some of these are:

  • Relativity of simultaneity: Two events, simultaneous for some observer, may not be simultaneous for another observer if the observers are in relative motion.
  • Time dilation: Moving clocks are measured to tick more slowly than an observer's "stationary" clock. To illustrate this further, imagine an observer sitting beside an oval race track, with a motorcycle driver traveling close to the speed of light for several years around the track.The sitting observer will age faster because time for the motorcycle driver will elapse relatively slower.
  • Length contraction: Objects are measured to be shortened in the direction that they are moving with respect to the observer.
  • Mass-energy equivalence: E = mc2, energy and mass are equivalent and transmutable.

The defining feature of special relativity is the replacement of the Galilean transformations of classical mechanics by the Lorentz transformations. (See Maxwell's equations of electromagnetism and introduction to special relativity).

General relativity

General relativity is a theory of gravitation developed by Einstein in the years 1907–1915. The development of general relativity began with the equivalence principle, under which the states of accelerated motion and being at rest in a gravitational field (for example when standing on the surface of the Earth) are physically identical. The upshot of this is that free fall is inertial motion: In other words an object in free fall is falling because that is how objects move when there is no force being exerted on them, instead of this being due to the force of gravity as is the case in classical mechanics. This is incompatible with classical mechanics and special relativity because in those theories inertially moving objects cannot accelerate with respect to each other, but objects in free fall do so. To resolve this difficulty Einstein first proposed that spacetime is curved. In 1915, he devised the Einstein field equations which relate the curvature of spacetime with the mass, energy, and momentum within it.

Some of the consequences of general relativity are:

Technically, general relativity is a metric theory of gravitation whose defining feature is its use of the Einstein field equations. The solutions of the field equations are metric tensors which define the topology of the spacetime and how objects move inertially.

References and links

See the special relativity references and the general relativity references.

For information on the silent film produced on this subject, see The Einstein Theory of Relativity.

References

External links

Wikisource
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Wikipedia. This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Theory of relativity" Read more

 

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