Ciro Santilli
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Full set of all possible special relativity symmetries:
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In simple and concrete terms. Suppose you observe N particles following different trajectories in Spacetime.
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There are two observers traveling at constant speed relative to each other, and so they see different trajectories for those particles:
  • space and time shifts, because their space origin and time origin (time they consider 0, i.e. when they started their timers) are not synchronized. This can be modelled with a 4-vector addition.
  • their space axes are rotated relative to one another. This can be modelled with a 4x4 matrix multiplication.
  • and they are moving relative to each other, which leads to the usual spacetime interactions of special relativity. Also modelled with a 4x4 matrix multiplication.
Note that the first two types of transformation are exactly the non-relativistic Galilean transformations.
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The Poincare group is the set of all matrices such that such a relationship like this exists between two frames of reference.
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Ancestors

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