A Lorentz transformation is a linear transformation that maintains the length of paravectors. Lorentz transformations include rotations and boosts as proper Lorentz transformations and reflections and non-orthochronous transformations among the improper Lorentz transformations.
A proper Lorentz transformation can be written in spinorial form as

where the spinor
is subject to the condition of unimodularity

In
, the spinor
can be written as the
exponential of a biparavector

If the biparavector
contains only a bivector (complex vector in
), the Lorentz transformations is a rotation in the plane of the bivector

for example, the following expression represents a rotor that applies a rotation angle
around the direction
according to the right hand rule

applying this rotor to the unit vector along
gives the expected result

The rotor
has two fundamental properties. It is said to be unimodular and
unitary, such that
- Unimodular:

- Unitary:

In the case of rotors, the bar conjugation and the reversion have the same effect

If the biparavector
contains only a real vector, the Lorentz transformation is a boost along the direction of the respective vector

for example, the following expression represents a boost along the
direction

where the real scalar parameter
is the rapidity.
The boost
is seen to be:
- Unimodular:

- Real:

In general, the spinor of the proper Lorentz transformation can be written
as the product of a boost and a rotor

The boost factor can be extracted as

and the rotor is obtained from the even grades of

The proper velocity of a particle at rest is equal to one

Any proper velocity, at least instantaneously, can be obtained from an active Lorentz transformation from the particle at rest, such that

that can be written as

so that

where the explicit formula of the square root for a unit length paravector was used.
The proper velocity is the square of the boost

so that

rewriting the rapidity in terms of the product of its magnitude and respective
unit vector

the exponential can be expanded as

so that

and

where we see that in the non-relativistic limit the rapidity becomes the velocity divided by the speed of light

The Lorentz transformation applied to biparavector has a different form from the Lorentz transformation applied to paravectors. Considering a general biparavector written in terms of paravectors

applying the Lorentz transformation to the component paravectors

so that if
is a biparavector, the Lorentz transformations is given
by
