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Under the condition, that
the free-space vacuum energy vanishes, we obtain the angular
integrated form of the canonical
vacuum energy density
as
Thereby, jl denotes the spherical Bessel function,
and the subscripts n, ,
and
stand for
the radial quantum number, the Dirac
quantum number, and the angular momentum projection, respectively.
The radial quantum number
labels the mode energy closest to
,
and
is a normalization constant (see Ref. [21]).
In Eq. (1) the integral over k corresponds to
the free-space subtraction.
Hard fluctuations are excluded by
distinguishing two cases: 1) hard fluctuations with
or
,
are omitted by
truncation of the mode sum, and 2) hard fluctuations with
,
are discarded
by restriction of the z-integration.
The canonical vacuum energy E is given by
.
Next: The fermionic bag constant
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Marc Schumann
2000-10-16