Fundamentals of Time and Relativity

EM Bivector

  • The electromagnetic field in the STA formalism is a bivector field F with the same components as the anti-symmetric field tensor F μν .
  • In a given inertial frame, the bivector F decomposes into a complex pair of three-vectors E and iB .

As an example of the use of STA, we consider electromagnetism. For each spacetime point x , the standard frame { e μ } as defined in STA, determines a set of ‘rectangular coordinates’ { x μ } given by x μ = e μ x and x= x μ e μ . In terms of these coordinates the derivative with respect to a spacetime point x is the operator := e μ μ , where μ = e μ =( 0 , ) is the coordinate derivative.

Writing the electromagnetic field F μν in terms of the 4-potential A(x)= A μ (x) e μ we have

9.15

A= μ A ν ( e μ e ν )= 1 2 F μν ( e μ e ν )=:F

where F is the so-called electromagnetic field bivector with its six components given by:

9.16

F μν = e μ F e ν =( e ν e μ )F

Like in Minkowski space, in STA a given inertial system is completely characterized by the single future-pointing, timelike unit vector e 0 . The spacetime split of F into an electric (relative vector) part E and a magnetic (relative bivector) part iB in the e 0 -system is achieved by separating F into parts which anti-commute and commute with e 0 . Thus F=E+iB , where

9.17

E:=(F e 0 ) e 0 = 1 2 (F+ F )

is the part of F that anti-commutes with e 0 , and

9.18

iB:=(F e 0 ) e 0 = 1 2 (F F )

is the part that commutes; the quantity F =EiB is called the conjugated field. Importantly, this type of conjugation is not frame-independent, but is relative to the e 0 -frame.

  • The geometric properties of i keep F reference-frame-independent, even though the decomposition into relative fields E and B still implicitly depends upon the chosen time axis.
  • In STA electromagnetic theory, the geometric pseudo-scalar i plays the role of the scalar imaginary unit i . There is no need for the introduction of any additional complex entities.