In the previous section we saw that a combination of a scalar and a vector, a
paravector, A=a0+a, has an amplitude-squared with the same
metric as that of spacetime and yet can be rotated like a normal vector such
that the scalar part is unchanged, while the vector part rotates in space, as
RAR, where the rotor R is itself comprised of a
scalar and a bivector, R=e−xy2θ.
We also saw that we can define a normalised paravector as B=e−b2ϕ, so that BB=1. In this section we will
consider rotating the paravector A by a normalized paravector and
see that the result, BAB, is equivalent to the standard
Lorentz transformation.
A hyperbolic rotation
Similar to the spatial rotation, we can see that A′=BAB
is some type of rotation of A, as even though we are not using the
Clifford conjugation of the rotor for the left-hand multilication, the amplitude
squared is still unchanged:
If we first look at the case where the vector being rotated is in the same
direction as the rotation itself, ie. ab=ba=∣a∣
and since b2=1, then a=∣a∣b, we can further simplify the rotation: