
14 3 Comparison Between the Real and the Complex Language
Since ai =−ia if a ∈ M, a exp(iβ/2) = (exp(−iβ/2)a, and
a ∈ M ⇒ b = Ra
˜
R ∈ M,ψa
˜
ψ = ρb ∈ M
one can write
ψe
0
˜
ψ = ρv = j,v
2
= 1,ρ>0 (3.2)
The time-like vector j is the probability current.
Three other currents may be defined
ψe
k
˜
ψ = j
k
= ρn
k
, n
2
k
=−1, k = 1, 2, 3 (3.3)
The vectors n
k
play an important role in the theory of the electron, and, associated
with three bosons, in the electroweak theory, also in the presentation that we propose
of the chromodynamics theory.
Note that, in replacement of the Dirac spinor, an expression similar to Eq. 3.1
has been written in [2] by the employment of the Dirac matrices, but carries more
complications in the use of ψ.
We shall call the biquaternion ψ a Hestenes spinor when it is written in the form
of Eq. 3.1 and applied to the study of quantum mechanics.
Given all the applications in Physics of Cl
+
(1, 3), Hestenes has given to this ring
the name of Space–Time Algebra (STA)[3].
In the gauge theories the density ρ does not interverne. Only the vectors n
1
, n
2
in
the U(1) gauge, the three vectors n
k
in the SU(2) one. They play also a role in the
definition of the momentum–energy tensors (see Sects. 5.2 and 8.2.2).
Note on the “angle” β. The role of the Yvon–Takabayasi–Hestenes “angle” β,
which concerns not the vectors but the bivectors of M is obscure.
This “angle” plays no role in the gauge theories but gives an interpretation of the
link electron–positron more satisfactory than the use of the T transform of the CPT
invariance in the passage from the equation of the electron to the one of its associated
positron.
We show in Sect. 7.2 that this interpretation proposed by Takabayasi (see [4],
Eq. 10.3
b
) is in fact a necessity.
The scalar β was introduced in the theory of the electron by Yvon [5], used by
Lochak [2] in its expression of the wave function of the electron, studied in detail by
Takabayasi [4], and independently rediscovered by Hestenes [1].
The presence in a physical theory of this scalar β is “strange” (as said Louis de
Brogie) with respect to ρ (probability) and R (Lorentz rotation) widely used in the
standard presentation of quantum mechanics. But, because it is an indisputable com-
ponent of a biquaternion, element of Cl
+
(1, 3), when this biquaternion is considered
as containing a Lorentz rotation R, its necessity is confirmed by the place played
by the biquaternions in physics. We recall that the biquaternions were introduced by
Sommerfeld (see [6]) in the study of the hydrogenic atoms.
We have shown in [7] that β has a value non null, though small, in the solution of
the hydrogen atom, except in the plane x
3
= 0.