In physics, quantum field theory (QFT) was developed to describe structureless elementary particles (e.g., electrons, quarks, photons, etc.), their interaction with each other and with their environment [1-3]. A graphical technique to account for physical processes in QFT (e.g., scattering) is by using diagrams known as the Feynman diagrams. These consist of points (vertices) connected by lines (propagators) [4-5]. The lines represent free propagation of elementary particles and the points represent the interaction among particles meeting at those points. One way to represent free scalar particles in QFT is to utilize solutions of the Klein-Gordon wave equation in 3+1 dimensional Minkowski space-time that reads
where
m is the rest mass of the scalar particle and we have adopted the relativistic units
. Recently, a formulation of QFT for elementary particles that have internal structure was developed in which the quantum field operator
is written as Fourier expansion over the energy domain consisting of continuous and discrete components:
The integral over
represents the continuous energy spectrum of the particle whereas the sum represents its structure, which is resolved in the energy and of size
. This formulation of QFT is referred to by the acronym SAQFT that stands for “Structural Algebraic QFT” and could be useful in treating elementary particles that are thought to be structureless at low energy scale [
6]. We take
to stand for the single energy interval
and take
. The objects
and
are field operators (the vacuum annihilation operators) that satisfy the conventional commutation relations:
and
. The continuous and discrete Fourier energy components in (2) are written as the following pointwise convergent series
where
,
and
is a complete set of functions, which for scalar particles satisfy the following differential equation
where
are real constants that are independent of
z and such that
for all
n. Using (4) in the free Klein-Gordon wave equation (1) gives the following algebraic relation
for
. This is a symmetric three-term recursion relation that makes
a sequence of polynomials in
z with the two initial values
and
. Favard theorem (a.k.a. the spectral theorem; see Section 2.5 in [
7]) dictates that the polynomial solutions of Eq. (5) satisfy the following general orthogonality relation [
7,
8,
9]
where
is the continuous component of the weight function and
is the discrete component. These weight functions are positive definite and related to the energy functions
and
as
(with
for
) and
.
In conventional QFT, the propagators in the Feynman diagrams are tagged with the energy-momentum four-vector
. However, in SAQFT these propagators are tagged with the spectral parameter
z. For free scalar particles,
making
z positive. However, doing scattering calculation with the Feynman diagrams in closed loops, one should integrate and sum over all possible values of the real energy in
(i.e.,
) making the values of these spectral parameters
z greater than or equal to
. At each vertex in the Feynman diagrams, the energy-momentum 4-vector is conserved. For example, when calculating the first order correction to the three-particle interaction vertex, we encounter loop diagrams similar to that shown in
Figure 1 where the spectral parameters
are indicated on their respective propagators. Choosing a counterclockwise loop, the three energy conservation equations are:
,
, and
, where
. This leads to a special rule for adding and subtracting spectral parameters. For example,
gives
where “sgn” is ±, which is the product of the signs of the two energies
and
. Moreover, the sign of the energy
is the sign of
. Therefore, for the spectral parameters to contain full physical information, they must carry the sign of their corresponding energies. Hence, we associate with each spectral parameter a ± parity, which will be indicated as superscript on the parameter. For example, the parity of
z in (7) is the sign of
where
σ is the sign of the energy
(i.e., parity of
x) and
τ is the sign of the energy
(i.e., parity of
y). Thus, we rewrite (7) properly as follows
where
ρ is the (nonzero) sign of the energy
(i.e., parity of
z). This equation defines the operation of addition of the spectral parameters. Repeating the same for the energy conservation equation
, we obtain the following rule for the subtraction of spectral parameters
where
ρ is the (nonzero) sign of
. The parity of each spectral parameter
in the figure (not shown) is the sign of the corresponding energy.