Worked solution: Maynard's multidimensional sieve: bounded gaps between primes (2013)
The GPY weight only cared about divisors of the whole product , treating the shifted numbers as one indivisible block. Maynard's key new idea is to instead let the coefficient depend on a whole tuple of divisors , one for each shifted number separately.
This sounds like a small change, but it is like upgrading from a one-dimensional dial to a -dimensional control panel: it gives vastly more freedom to design weights that favor 's where many of the look prime simultaneously, rather than just where the product as a whole looks favorable.
Maynard's new weight is , summed over all -tuples of divisors with for every (Maynard 2013, §2, eq. 2.4). Unlike GPY's , which was a single-variable coefficient, the new coefficient is a genuinely -dimensional array — hence 'multidimensional sieve'.
Maynard notes this idea was not entirely without precedent (Selberg had suggested something similar for twin primes, and Goldston–Yıldırım had tried a restricted version), but earlier attempts capped each at , a restriction so severe it erased the benefit. Maynard's choice instead lets the coefficients roughly factor as for a smooth function of real variables, with individually allowed to range up to (Maynard 2013, §2, eq. 2.5).
This multidimensional freedom is precisely what removes the earlier barrier: the counting sums built from these weights can now be evaluated (Proposition 4.1 below) in terms of an arbitrary smooth function of variables, turning sieve design into a calculus-of-variations problem the next steps will exploit.
- Multidimensional sieve weight
- A sieve coefficient indexed by a -tuple of divisors, one per shift , rather than by a single divisor of the whole product — the extra degrees of freedom are what make Maynard's method more powerful than GPY's.