In relativity physics, the shortening of an object along the direction of its motion relative to an observer. Dimensions in other directions are not contracted. This concept was proposed by the Irish physicist George F. FitzGerald (1851–1901) in 1889 and later independently developed by Hendrik Antoon Lorentz. Significant at speeds approaching that of light, the contraction results from the properties of space and time, not from compression, cooling, or any similar physical disturbance. Seealso time dilation.
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It is important to note that this effect is negligible at everyday speeds, and can be ignored for all regular purposes. It is only when an object approaches speeds on the order of 30,000,000 m/s, i.e. one-tenth of the speed of light, that it becomes important. As the magnitude of the velocity approaches the speed of light, the effect becomes dominant, as we can see from the formula:
Note that in this equation it is assumed that the object is parallel with its line of movement. Also note that for the observer in relative movement, the length of the object is measured by subtracting the simultaneously measured distances of both ends of the object. For more general conversions, see the Lorentz transformations.
An observer at rest viewing an object travelling at the speed of light would observe the length of the object in the direction of motion as zero. Among other reasons, this suggests that objects with mass cannot travel at the speed of light.
The origin of length contraction in the special theory of relativity can be traced to the operational definitions of simultaneity and length. According to Milne and Bondi the following operational definitions are assigned to simultaneity and length: an observer moving uniformly along a straight line sends out a light signal at time t0 to a distant point (stationary according to the observer), where it arrives and is immediately reflected at time tr, arriving back at the observer at time ta. We ask: what time does the observer ascribe to the time of reflection tr, or, what event is simultaneous with the reflection? Let ℓ be the distance to the point of reflection. With his definition of c, the observer says it takes time ℓ / c for light to reach the reflector. Because light travels at the same speed c in both directions, it takes the same time both ways, so it returns to the observer at time ta = t0 + 2 ℓ / c, or in other words, the distance to the point of reflection is ℓ = c (ta − t0 ) / 2, and the time at which reflection occurred is simultaneous with the clock registering (t0 + ta ) / 2. With these operational definitions for determining length and simultaneous events, two observers in constant relative motion at velocity v are considered, and their time and length scales compared. The result of the above definitions is that time and length are connected by the Lorentz factor γ: In short, the slowing of time and the contraction of space are consequences of choosing a consistent set of definitions for length and simultaneity, coupled with the postulate that the speed of light is is the same in all directions for all observers. Being a consequence of definitions, these contractions are not a consequence of any underlying dynamical laws.
The Lorentz–FitzGerald contraction hypothesis, the more formal name for length contraction was proposed by George Francis FitzGerald and independently proposed and extended by Hendrik Lorentz to explain the negative result of the Michelson–Morley experiment, which attempted to detect Earth's motion relative to the luminiferous aether.
After reading a paper by Heaviside that showed how electric and magnetic fields are affected by motion, FitzGerald hit on the idea that when a body moves through space its size changes due to its motion, and that this may explain Michelson and Morley's "null result". FitzGerald suggested the contraction in an 1889 letter to Science, but did not himself see the letter in print, and it attracted no notice until many years later. He did, however, describe the idea to his scientific friends, and Oliver Lodge mentioned it in print in 1892. Lorentz had hit on the idea independently in 1891 and in 1892 showed how such an effect might be expected based on electromagnetic theory and the electrical constitution of matter. When a body moves through space its dimension parallel to the line of motion would, he said, become less by an amount that depended on its speed. If the speed of the body is and the speed of light is , then the contraction is in the ratio
For Earth moving in its orbit at about 30 km/s (18.5 mile/s), the contraction would amount to about one part in 200,000,000, which would be about 6 cm (2.5 inches) on the diameter of Earth. This small change accounts for Michelson and Morley's negative result by making the source of light and the mirror draw closer together when the system is moving lengthwise.
The formula itself suggests that it is impossible for the velocity of objects () to surpass the speed of light. Doing so results in a fraction larger than 1; thus a square root of a negative number.
Length contraction as a physical effect on bodies composed of atoms held together by electromagnetic forces was proposed independently by George FitzGerald and by Hendrik Lorentz . The following quote from Joseph Larmor is indicative of the pre-relativity view of the effect as a consequence of James Clerk Maxwell's electromagnetic theory:
The extension of this specific result to a general result was (and is) considered "ad hoc" by many who prefer Einstein's deduction of it from the Principle of Relativity without reference to any physics. In other words, length contraction is an inevitable consequence of the postulates of special relativity. To gain a little physical insight on why length contractions occur, consider what those postulates involve: by requiring the speed of light (a quantity dependent on the fundamental properties of space and time) to be invariant in all frames of reference (including ones in motion) one can appreciate that it would require the "distortion" of the measures of length and time. Apparently Lorentz did not agree to the criticism that his proposal was "ad hoc".
The Trouton–Rankine experiment in 1908 showed that length contraction of an object according to one frame, did not cause changes in the resistance of the object in its rest frame. This is in agreement with some current theories at the time (Special Relativity and Lorentz ether theory) but in disagreement with FitzGerald's ideas on length contraction.
Henri Poincaré was not at first entirely satisfied with the contraction hypothesis. In Science and hypothesis he commented on the contraction:
The Lorentz–FitzGerald contraction effect is described by Lorentz in paragraph 8 of his 1904 paper "Electromagnetic phenomena in a system moving with any velocity smaller than that of light." The hypothesis was directed specifically towards electrons with the final intent of explaining the unexpected result of the Trouton–Noble experiment and the Michelson–Morley experiment. Lorentz does this in paragraph 10 of the same paper. Albert Einstein derived the Lorentz contraction directly from the Principle of relativity. According to Einstein, early explanation attempts including the Lorentz–Fitzgerald contraction hypothesis had been "ad-hoc".
Lorentz did not agree as can be seen from his draft letter of 1915 to Einstein:
Lorentz later believed that relativity had introduced some doubt about whether the length contraction was apparent or real. In his view "... there can be no question about the reality of the change of length ... [rod II] will be shorter than [rod I], just as it would be if it were kept at a lower temperature ...
The modern view according to L.P.Hughston and to Michael Janssen is that the so-called "Lorentz contraction" is not of kinetic, but kinematic origin. In fact, it is a trigonometric phenomenon, with analogy to parallel slices through a cuboid before and after a rotation in E3 (see left half figure at the right). This is the Euclidean analog of boosting a cuboid in E1,2. In the latter case, however, we can interpret the boosted cuboid as the world slab of a moving plate.
Special relativity concerns relativistic kinematics. Poincaré transformations are a class of affine transformations which can be characterized as the transformations between alternative Cartesian coordinate charts on Minkowski spacetime corresponding to alternative states of inertial motion (and different choices of an origin). Lorentz transformations are Poincaré transformations which are linear transformations (preserve the origin).
Lorentz transformations play the same role in Minkowski geometry (the Lorentz group forms the isotropy group of the self-isometries of the spacetime) which are played by rotations in euclidean geometry. Indeed, special relativity largely comes down to studying a kind of noneuclidean trigonometry in Minkowski spacetime, as suggested by the following table:
|Kleinian Geometry||euclidean plane||Galilean plane||Minkowski plane|
|Quadratic form||positive definite||degenerate||non-degenerate but indefinite|
|type of isotropy||rotations||shears||boosts|
|Cayley algebra||complex numbers||dual numbers||Minkowski numbers|
|Spacetime interpretation||none||Newtonian spacetime||Minkowski spacetime|
|slope||tan φ = m||tanp φ = u||tanh φ = v|
|"cosine"||cos φ = (1+m2)-1/2||cosp φ = 1||cosh φ = (1-v2)-1/2|
|"sine"||sin φ = m (1+m2)-1/2||sinp φ = u||sinh φ = v (1-v2)-1/2|
|"secant"||sec φ = (1+m2)1/2||secp φ = 1||sech φ = (1-v2)1/2|
|"cosecant"||csc φ = m-1 (1+m2)1/2||cscp φ = u-1||csch φ = v-1 (1-v2)1/2|