Put and . For any positive integer shift , translating the interval changes its sum by at most . Averaging the shifts gives the bilinear shift averaging for a logarithmic phase identitySince , the alternating Taylor expansion of the logarithm has remainder at most . ThusFor , we have , hence the error is at most . The exponential function on an imaginary argument changes by at most the change in that argument. ThereforeUse and . Taking absolute values provesThe boundary error comes from integer shifts, so this argument also covers intervals shorter than a shift. Here range over positive integers; no zero term is needed.
The Vinogradov mean value isBy orthogonality of integer Fourier modes, it counts the ordered integer solutions of for , with every coordinate between one and . The diagonal solutions give .
Put . The moment vector has at most possible values. If counts the tuples with vector , then and . The Cauchy-Schwarz inequality gives . Combining the two lower bounds, with one common positive constant for large , yields
Here is an explicit way that upper bounds enter the Vinogradov mean-value method for a bilinear exponential sum. Write and . Two applications of the Holder inequality, followed by grouping equal differences of moment vectors, giveAt integer the minimum is defined as ; means distance to the nearest integer. To explain the mean-value factor, let count pairs of -tuples with prescribed moment difference. It is an autocorrelation of , so by Cauchy-Schwarz inequality. The first Holder inequality groups the tuples, and the second groups the tuples, providing the two factors . The remaining sums over moment differences are bounded by the displayed finite geometric series estimates. Good Vinogradov mean value upper bounds, together with rational approximation or spacing bounds for , therefore give cancellation in . The mean-value estimate alone does not force cancellation for arbitrary coefficients: when all are integers, . For the paper take and the specified .
Set and . By the Hardy-Littlewood approximation to the Riemann zeta function at , it is enough to bound : the integral term has size because .
On a dyadic interval with , the assumed estimate holds for every initial subinterval. Abel summation with therefore givesIndeed the weighted endpoint and integral of the term proportional to the subinterval length are , and those of the constant term are . The constants can be uniform in .
For the first term, write and complete the square:The sum of a shifted Gaussian function on a fixed-spaced lattice is , uniformly in the shift. Thus these dyadic contributions are . This is the Gaussian dyadic summation bound.
For the second term, if its dyadic sum is bounded. If , a crude bound is . The positive exponent obeys , and can be absorbed into uniformly on by increasing the fixed constant . The finitely many initial terms cause no problem. We conclude, with one fixed sufficiently large ,In particular the endpoint gives under the assumed exponential-sum hypothesis. This conditional conclusion uses that hypothesis, not an unconditional improvement of the stated Richert bound for the Riemann zeta function.
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