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Four-vector
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====Pure rotations about an arbitrary axis ==== For two frames rotated by a fixed angle {{math|''ΞΈ''}} about an axis defined by the [[unit vector]]: <math display="block">\hat{\mathbf{n}} = \left(\hat{n}_1, \hat{n}_2, \hat{n}_3\right)\,,</math> without any boosts, the matrix '''Ξ''' has components given by:<ref>{{cite book| author=C.B. Parker| title=McGraw Hill Encyclopaedia of Physics| publisher=McGraw Hill| edition=2nd| page=[https://archive.org/details/mcgrawhillencycl1993park/page/1333 1333]| year=1994| isbn=0-07-051400-3| url-access=registration| url=https://archive.org/details/mcgrawhillencycl1993park/page/1333}}</ref> <math display="block">\begin{align} \Lambda_{00} &= 1 \\ \Lambda_{0i} = \Lambda_{i0} &= 0 \\ \Lambda_{ij} &= \left(\delta_{ij} - \hat{n}_i \hat{n}_j\right) \cos\theta - \varepsilon_{ijk} \hat{n}_k \sin\theta + \hat{n}_i \hat{n}_j \end{align}</math> where ''Ξ΄<sub>ij</sub>'' is the [[Kronecker delta]], and ''Ξ΅<sub>ijk</sub>'' is the [[three-dimensional]] [[Levi-Civita symbol]]. The spacelike components of four-vectors are rotated, while the timelike components remain unchanged. For the case of rotations about the ''z''-axis only, the spacelike part of the Lorentz matrix reduces to the [[rotation matrix]] about the ''z''-axis: <math display="block"> \begin{pmatrix} {A'}^0 \\ {A'}^1 \\ {A'}^2 \\ {A'}^3 \end{pmatrix} = \begin{pmatrix} 1 & 0 & 0 & 0 \\ 0 & \cos\theta & -\sin\theta & 0 \\ 0 & \sin\theta & \cos\theta & 0 \\ 0 & 0 & 0 & 1 \\ \end{pmatrix} \begin{pmatrix} A^0 \\ A^1 \\ A^2 \\ A^3 \end{pmatrix}\ . </math>
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