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In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between space and time.In Albert Einstein's 1905 paper, On the Electrodynamics of Moving Bodies, the theory is presented as being based on just two postulates: [p 1] [1] [2]
The late-medieval author Chaucer (c. 1343 –1400) observed "The lyf so short, the craft so long to lerne" ("The life so short, the craft so long to learn", the first line of the Parlement of Foules). [6] The first-century CE rabbi Tarfon is quoted as saying "The day is short, the labor vast, the workers are lazy, the reward great, the Master ...
According to Paul Virilio, time-space compression is an essential facet of capitalist life, saying that "we are entering a space which is speed-space ... This new other time is that of electronic transmission, of high-tech machines, and therefore, man is present in this sort of time, not via his physical presence, but via programming" (qtd. in ...
The laws of physics are the same for all observers in any inertial frame of reference relative to one another (principle of relativity). The speed of light in vacuum is the same for all observers, regardless of their relative motion or of the motion of the light source. The resultant theory copes with experiment better than classical mechanics.
The magnitude of this scale factor (nearly 300,000 kilometres or 190,000 miles in space being equivalent to one second in time), along with the fact that spacetime is a manifold, implies that at ordinary, non-relativistic speeds and at ordinary, human-scale distances, there is little that humans might observe that is noticeably different from ...
One set of tests focuses on effects predicted by general relativity for the behavior of gyroscopes travelling through space. One of these effects, geodetic precession, has been tested with the Lunar Laser Ranging Experiment (high-precision measurements of the orbit of the Moon). Another, which is related to rotating masses, is called frame-dragging
This is done in "3+1" formulations, where spacetime is split into three space dimensions and one time dimension. The best-known example is the ADM formalism . [ 174 ] These decompositions show that the spacetime evolution equations of general relativity are well-behaved: solutions always exist , and are uniquely defined, once suitable initial ...
Time is a scalar which is the same in all space E 3 and is denoted as t. The ordered set { t } is called a time axis. Motion (also path or trajectory ) is a function r : Δ → R 3 that maps a point in the interval Δ from the time axis to a position (radius vector) in R 3 .