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Lorentz covariance
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{{Use American English|date = March 2019}} {{Short description|Concept in relativistic physics}} In [[relativistic mechanics|relativistic physics]], '''Lorentz symmetry''' or '''Lorentz invariance''', named after the Dutch physicist [[Hendrik Lorentz]], is an equivalence of observation or observational symmetry due to [[special relativity]] implying that the laws of physics stay the same for all observers that are moving with respect to one another within an [[inertial frame]]. It has also been described as "the feature of nature that says experimental results are independent of the orientation or the boost velocity of the laboratory through space".<ref>{{cite web|first=Neil| last=Russell |url= https://cerncourier.com/a/framing-lorentz-symmetry/ |title=Framing Lorentz symmetry |publisher=CERN Courier |date=2004-11-24 |access-date=2019-11-08}}</ref> '''Lorentz covariance''', a related concept, is a property of the underlying [[spacetime]] manifold. Lorentz covariance has two distinct, but closely related meanings: # A [[physical quantity]] is said to be Lorentz covariant if it transforms under a given [[group representation|representation]] of the [[Lorentz group]]. According to the [[representation theory of the Lorentz group]], these quantities are built out of [[scalar (physics)|scalar]]s, [[four-vector]]s, [[four-tensor]]s, and [[spinor]]s. In particular, a [[Lorentz scalar|Lorentz covariant scalar]] (e.g., the [[space-time interval]]) remains the same under [[Lorentz transformation]]s and is said to be a ''Lorentz invariant'' (i.e., they transform under the [[trivial representation]]). # An [[equation]] is said to be Lorentz covariant if it can be written in terms of Lorentz covariant quantities (confusingly, some use the term ''invariant'' here). The key property of such equations is that if they hold in one inertial frame, then they hold in any inertial frame; this follows from the result that if all the components of a tensor vanish in one frame, they vanish in every frame. This condition is a requirement according to the [[principle of relativity]]; i.e., all non-[[gravitation]]al laws must make the same predictions for identical experiments taking place at the same spacetime event in two different [[inertial frames of reference]]. On [[manifold]]s, the words [[covariance and contravariance of vectors|''covariant'' and ''contravariant'']] refer to how objects transform under general coordinate transformations. Both covariant and contravariant four-vectors can be Lorentz covariant quantities. '''Local Lorentz covariance''', which follows from [[general relativity]], refers to Lorentz covariance applying only [[local symmetry|''locally'']] in an infinitesimal region of spacetime at every point. There is a generalization of this concept to cover [[Poincare covariance|Poincaré covariance]] and Poincaré invariance.
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