With and analogous notation for , Vaughan identity is
Thus, when ,
The first term is short, the next two are Type I sums, and the last becomes a Type II bilinear sum after grouping variables and applying a dyadic decomposition.
Write , where . Split the -interval into consecutive blocks of length at most . If distinct integers lie in one block, then . Since ,
whereas . Hence .
The points in one block are therefore -separated modulo one. Order them by distance from the nearest integer. Apart from a bounded number of endpoints, the th closest point has distance , and consequently
Multiplying by gives
This is the reciprocal fractional-part sum near a rational estimate.
Let
Applying the Cauchy-Schwarz inequality in gives
Take absolute values and apply Cauchy-Schwarz to . Since , expanding the remaining square gives
Taking fourth roots proves the claimed bilinear quadratic exponential sum fourth-moment bound.
In the fourth moment from part c, put
Then the phase is . The contribution with is , because ; the contribution with is . Their fourth roots are respectively and .
Off the diagonals, fix . The variable ranges over an interval of length , subject only to harmless parity and range restrictions. The exponential geometric sum bound gives
Put . We have , and the number of representations of a fixed by the three factors, including signs and range restrictions, is . Hence the fourth moment is
Using in part c proves
This is the factorized fourth moment for a bilinear quadratic exponential sum.
Write and split the last sum in part d according as or . For the first part, the reciprocal fractional-part sum near a rational gives
For the second part, use the supplied second-moment estimate and truncation of a divisor weight by its second moment:
Substitute , take fourth roots, and factor out . The four terms from the bounded-weight estimate become, after harmless enlargement by ,
with the smaller term absorbed by . The large-weight part contributes . Finally, the two diagonal terms from part d contribute and ; since , the first is absorbed by . Therefore
Assume . To beat the trivial bound by , it is enough to make every term in the parentheses of part e smaller than a sufficiently larger negative power of , allowing for the prefactor .
Choose the splitting parameter with large in terms of . It then suffices, for a still larger constant , that
Indeed, these four conditions control respectively the last, third, second, and fourth terms, while the choice of controls the first. Equivalently, away from polylogarithmic neighborhoods of the endpoints, the estimate gives a logarithmic saving whenever
are all sufficiently large powers of , with also larger than the chosen divisor cutoff by such a power. This is the Type II range used after Vaughan identity.

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