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Spacetime algebra : ウィキペディア英語版
Spacetime algebra
In mathematical physics, spacetime algebra (STA) is a name for the Clifford algebra ''C''ℓ1,3(R), or equivalently the geometric algebra ''G''4 = ''G''(M4), which can be particularly closely associated with the geometry of special relativity and relativistic spacetime.
It is a vector space allowing not just vectors, but also bivectors (directed quantities associated with particular planes, such as areas, or rotations) or multivectors (quantities associated with particular hyper-volumes) to be combined, as well as rotated, reflected, or Lorentz boosted. It is also the natural parent algebra of spinors in special relativity. These properties allow many of the most important equations in physics to be expressed in particularly simple forms, and can be very helpful towards a more geometric understanding of their meanings.
==Structure==
The spacetime algebra is built up from combinations of one time-like basis vector \gamma_0 and three orthogonal space-like vectors, \, under the multiplication rule
: \gamma_\mu \gamma_\nu + \gamma_\nu \gamma_\mu = 2 \eta_
where \eta_ \, is the Minkowski metric with signature (+ − − −)
Thus \gamma_0^2 = , \gamma_1^2 = \gamma_2^2 = \gamma_3^2 = , otherwise \displaystyle \gamma_\mu \gamma_\nu = - \gamma_\nu \gamma_\mu.
The basis vectors \gamma_k share these properties with the Dirac matrices, but no explicit matrix representation is utilized in STA.
This generates a basis of one scalar \, four vectors \, six bivectors \, four pseudovectors \ and one pseudoscalar \, where i=\gamma_0 \gamma_1 \gamma_2 \gamma_3.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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