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We now consider the constraints which arise from demanding that
and
be non-negative (2). We begin with the necessary condition that their moments
and
be non-negative. If the starting distributions are positive it is easy to show that
(eqs. (5), (6)), but one must consider two possibilities for
.

If the starting distributions are positive, this holds for
, and since
it continues to hold for
. For
, however, it will eventually fail.
Eq. (3) shows that
is non-negative as
or
since it is dominated by the positive terms
or
in these limits, but it has one minimum at

The validity of eq. (8) at
implies that
. Hence
decreases between
and
but
is positive throughout this region. For
, however,
may become negative, depending on the starting distributions.
We have now shown that the moments of the (anti)quark and gluon distributions remain positive for
if they are positive at
. In order that the distributions themselves remain positive, their moments must satisfy eq. (7) for all
. For the large class of starting distributions whose moments behave like inverse powers of
for large
, the asymptotic freedom formulae predict that their moments continue to behave like inverse powers of
for
(apart from
factors which will not affect our argument). In this case
and
will be positive for large
since
for
(where
is the
th-order finite difference operator defined in eq. (7)). A detailed numerical investigation of
and
with a wide variety of positive starting distributions suggests that in all cases they indeed remain positive for
for all
.
We showed above that for
some of the moments inevitably become negative. This is also true of their finite differences. For ``reasonable'' starting distributions, however, we find (sect. 5) that the
conditions only very rarely fail before the
conditions as
is decreased below
. This is to be expected since for a large class of distributions (including all those which decrease monotonically with
) the finite differences of the moments cannot be negative unless the moments themselves are negative.