Editing Invariant (physics) (section)

==Examples==
{{See also|Lorentz scalar}}
In classical and quantum mechanics, invariance of space under translation results in momentum being an invariant and the [[conservation of momentum]], whereas invariance of the origin of time, i.e. translation in time, results in energy being an invariant and the [[conservation of energy]]. In general, by [[Noether's theorem]], any invariance of a physical system under a [[continuous symmetry]] leads to a fundamental [[Conservation law (physics)|conservation law]]. 

In [[Crystal|crystals]], the [[Electronic density|electron density]] is periodic and invariant with respect to discrete translations by unit cell vectors. In very few materials, this symmetry can be broken due to enhanced [[Electronic correlation|electron correlations]].

Another examples of physical invariants are the [[speed of light]], and [[Electric charge|charge]] and [[Invariant mass|mass]] of a particle observed from two [[Frame of reference|reference frames]] moving with respect to one another (invariance under a spacetime [[Lorentz transformation]]<ref>{{cite book|last=French|first=A.P.|title=Special Relativity|publisher=W. W. Norton & Company|year=1968|isbn=0-393-09793-5}}</ref>), and invariance of [[time]] and [[acceleration]] under a [[Galilean transformation]] between two such frames moving at low velocities. 

Quantities can be invariant under some common transformations but not under others. For example, the velocity of a particle is invariant when switching coordinate representations from rectangular to curvilinear coordinates, but is not invariant when transforming between frames of reference that are moving with respect to each other. Other quantities, like the speed of light, are always invariant.

Physical laws are said to be invariant under transformations when their predictions remain unchanged. This generally means that the form of the law (e.g. the type of differential equations used to describe the law) is unchanged in transformations so that no additional or different solutions are obtained.

{{Quotation|For example the rule describing Newton's force of gravity between two chunks of matter is the same whether they are in this galaxy or another ([[translational invariance]] in space). It is also the same today as it was a million years ago (translational invariance in time). The law does not work differently depending on whether one chunk is east or north of the other one ([[rotational invariance]]). Nor does the law have to be changed depending on whether you measure the force between the two chunks in a railroad station, or do the same experiment with the two chunks on a uniformly moving train ([[principle of relativity]]).|[[David Mermin]]<ref name=Mermin-2009>{{Cite book |last=Mermin |first=N. David |title=It's about time: understanding Einstein's relativity |date=2009 |publisher=Princeton University Press |isbn=978-0-691-14127-5 |edition=Sixth printing, and first paperback printing |location=Princeton, NJ and Oxford}}</ref>{{rp|2}}}}

[[Covariance and contravariance of vectors|Covariance and contravariance]] generalize the mathematical properties of [[Invariant (mathematics)|invariance]] in [[tensor|tensor mathematics]], and are frequently used in [[electromagnetism]], [[special relativity]], and [[general relativity]].