Goldston and Yildirim's ``Small gaps between consecutive primes''
Goldston and Yildirim define
We give a (simplified) version of how the error occurred.
Consider the sum:
Now the idea is to move the path of each integral slightly to the left of
the imaginary axis
We move the paths to
If we move the paths of integration one at a time to the left to
Consequently, it was believed that the integral was asymptotic to
The consensus is that the definition of
is the Möbius function,
is the least common multiple of the
for
and
is the greatest common divisor of
and
.
Their main theorems involve the sums
and
.
The asymptotic evaluations of these sums are correct
in the two cases when there is just one
factor but incorrect
for certain
and
when there are two
factors.
. Here the basic parameter is
and
is about
;
the magnitude of the expression is
. Then Goldston and Yildirim
express this as a multiple complex integral:
is the Riemann zeta-function and where all of the paths
are
which stands for the vertical line from
to
, and where things have been simplified so that the dependency
of the sum on
has been suppressed for simplicity of exposition.
and determine all of the residues, employing
Cauchy's residue theorem together with known estimates for the
function.
which is the path
with
for a certain
; it is known that
has no
zeros to the right of this path and that
are
bounded by
on this path.
and collect the residues in order from the poles at
,
, and
then it is easy to see that one has a total
contribution
from these residues.
Moreover, the integrals on the new paths are much smaller, actually of
size
, as can be seen by arguments similar to
what one uses in the proof of the prime number theorem; the point is that
the exponent of
is sufficiently negative on these paths so that the
overall integrals are small.
.
However, notice that if we move the paths for
and
and consider the new integrals (not the residues) then we have a quadruple
integral over
that
must also be estimated. Now we move the
integral and use the residue
term
from the double pole at
and then we move the
term and use the residue
that occurs from the
pole of the zeta-function
in the numerator; the net result is a term
. Moreover, there doesn't seem to be any way to identify
the constant in any reasonable way other than as this numerical integral.
It doesn't seem to simplify.
Note: the integral shown above actually can be evaluated, because
the sum we considered is a bit simpler than that required by
Goldston and Yildirim. The integrals in the general case are somewhat
more complicated and cannot be evaluated exactly.
needs to be changed
so that terms like this one do not appear. However, it is not obvious how
to do this change. Work is continuing by Goldston and Yildirim and others
to rectify the problem. It does seem reasonable to believe that an
improvement on the current world record for small gaps between primes will
be achieved by these methods; however, the more dramatic result
for some
, for infinitely many n, seems less
likely.