In the level- convention used here, the Selberg upper-bound sieve states that a nonnegative sequence with sieve distribution satisfiesIt follows by minimizing the quadratic form with the Selberg sieve weights and using the Selberg least-common-multiple weights bound .
Sieve the interval by two and by the primes congruent to three modulo four, up to . The interval divisor counts giveThus , , and uniformly in the location of the interval. Take and .
To bound , let and form the Euler product over the forbidden primes at most . The given reciprocal-prime sum in residue class one modulo four, subtracted from the Mertens second theorem, yieldsMoreover, the Mertens first theorem bounds the logarithmic mean by for large . The truncated Euler-product lower bound gives .
The full-range summatory bound for three to the prime omega bounds the error by , which is . Every integer whose prime factors are all congruent to one modulo four survives this finite sieve. Therefore the half-dimensional interval sieve givesThe constants are independent of . Enlarging them covers the bounded range of before the asymptotic product estimates apply, so the result holds throughout .
Finite rearrangement and the Von Mangoldt divisor identity giveFor , integral comparison of the increasing logarithm gives . Moving to real changes the main term by . Thus the integrated Chebyshev sum hasFor , chooseThese are logarithmic Möbius function weights; they need not be upper-bound sieve weights. For , the Möbius inversion identities and giveHence the expression suggested in the question isWe will use the elementary Möbius harmonic logarithmic moments, , for whichHere is a proof of the needed estimates. From , replacing floors by gives . Also , because . Substituting the permitted harmonic number estimate gives , so .
For , the weighted Dirichlet hyperbola method gives the harmonic divisor sum expansionExplicitly, for , . Substitute the harmonic estimate and , obtained by unit-interval integral comparison. This proves the expansion without a prime-distribution theorem. Since , we have , and thereforeThe summed error is bounded by , by integral comparison. Thus .
Finally substitute the asymptotic for into . The main term isThe error sum is : partition the integers into ; each interval contributes , and the resulting series converges. Using the moment estimates proves the Selberg symmetry formula:In particular, the factor two comes from the quadratic logarithmic moment, rather than from an assumption of the Prime number theorem.
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