In order to place our previous discussion in the right perspective and
partly to justify the more technical approach in the following subsections,
let us consider the inflationary idea that the early phase of the exponential
expansion of the universe inflated a microscopic volume of space
to a size much larger that the presently observable part of the universe;
this idea can be formulated
within the framework of General Relativity as a special case of ``Classical
Bubble Dynamics'' (CBD), i.e., the study of the evolution of a vacuum
bubble in the presence of gravity [10]. In our own formulation of CBD,
inflation is driven by a gauge field
which is equivalent to a cosmological constant [11], and the
boundary effects in CBD, completely similar to those discussed in the
previous section, constitute the precise mechanism which extracts dark
matter from the self-energy of
.
In short, how does that process take place? The following properties of
constitute the crux of the boundary mechanism in the
inflation-axion scenario:
a) When massless,
represents `` dark stuff '' by definition, since in
(3+1)-dimensions
does not possess radiative degrees of
freedom. In fact, the field strength
, as a solution of the
classical field equation, is simply a constant disguised as a
gauge field. This property, even though peculiar, is not new in
field theory: it is shared by all -potential forms in
-spacetime dimensions.
For instance in two dimensions,
while in
four dimensions,
,
and
represents a constant background field in both cases by virtue of the field
equations. What is then the meaning of ``''?
As a gauge field,
is
endowed with an energy momentum tensor and thus it couples to gravity
[15]: the resulting equations are Einstein's equations with the
cosmological term
.
For this reason we call
the ``cosmological field''.
This alternative interpretation of the cosmological constant can be traced
back to Ref. [15] and its application to the inflationary scenario
in Ref. [11]; it will be discussed in more detail in the following
subsection.
b) If the cosmological field acquires a mass, then it describes massive pseudoscalar particles, in contrast with the usual Higgs
mechanism. Indeed, in the massive case the free field equation for