Write for the Chebyshev theta function and for the Second Chebyshev function. Throughout, denotes a prime and all logarithms are natural. Each prime divides the central binomial coefficient, so
Apply this at and telescope: . Bounding a general by the next power of two proves . Splitting the prime-counting function at now gives
This is the required Chebyshev estimate from central binomial coefficients, with no use of a prime asymptotic.
The higher prime powers also satisfy
For an integer , the prime factorization of a factorial gives
The Stirling formula, or integral comparison for , says . After division by we obtain . Moreover
Subtract this bounded contribution and replace by . The factorial proof of Mertens first theorem therefore yields
For fixed , apply partial summation to and :
The main contribution is
The bounded error in contributes at the endpoint and in the integral, since . Thus the positive logarithmic moments of reciprocal primes satisfy
First continue the Riemann zeta function into . Summing the integral of the integer-part function gives, initially for ,
The last integral defines a holomorphic function for , so this continuation has only a simple pole at one, of residue one.
For , logarithmic expansion of the Euler product and give
This proves the three-four-one product proof of zeta boundary nonvanishing inequality
If and to order , the middle factor is , the first is , and the last remains bounded. Their product tends to zero, a contradiction. At there is a pole, not a zero. The zeta function has no zero on .
Put , where is the Von Mangoldt function. Logarithmic differentiation of the Euler product gives for . The first integral of the Chebyshev function is consequently
To check its kernel, evaluate the contour integral of by closing to the left for and to the right for . The residues at zero and minus one give in the first case and zero in the second. Multiplication by and substitution therefore produce . On the line , the Dirichlet series and vertical integral have absolute convergence, justifying their interchange; at the kernel is zero on either side.
Here is the smoothing step that establishes the requested asymptotic. Shift the line of this contour integral to the left. The pole of at one has residue ; at each Nontrivial zero of the Riemann zeta function of zero multiplicity its residue is . The denominators also contribute at zero and minus one, and the trivial zeros of the Riemann zeta function occur at . Summing these residues yields the smoothed explicit formula for the Chebyshev function
Zeros are repeated with zero multiplicity. For the limits of the contour integral, choose horizontal heights avoiding zero ordinates, where the logarithmic derivative on each fixed strip is . The factor makes their integrals tend to zero. On left edges chosen a fixed distance from the trivial zeros, the functional equation of the Riemann zeta function controls the logarithmic derivative by ; for fixed the remaining vertical integral vanishes as that edge moves left. This is why the extra integration of is useful.
The Riemann–von Mangoldt formula, stated in Question 3, gives , hence
Indeed each dyadic height block contributes . The zero-free line just proved, the nonvanishing Euler product on its right, and the functional equation of the Riemann zeta function put every Nontrivial zero of the Riemann zeta function in . Therefore each tends to zero, with absolute value at most one for . Divide the explicit formula by and use dominated convergence on the zero terms with absolute convergence. The remaining displayed terms are , and we obtain
Monotonicity of removes the smoothing. For ,
After division by , the limits of the two bounds are and . Let to get . Question 1 gives , so . Partial summation now gives
The integral is , by splitting at and using . Inverting this at , we have and hence . Thus the th prime satisfies
Use the Jacobi theta function , . Its transformation law follows directly from the Gaussian Fourier transform. With the Fourier transform convention ,
For example, differentiating the transform and using integration by parts gives ; its value at zero is the Gaussian integral . Periodize the Gaussian. Its Fourier coefficients are these transforms at integer frequencies, and both series converge absolutely, so evaluating its Fourier series at zero proves the Poisson summation formula here:
For , integrating the exponentially convergent series termwise gives the Mellin representation of the completed Riemann zeta function
Split at one and substitute in the lower part, using the transformation just proved. The contribution of is . We obtain the pole-subtracted theta integral for the completed zeta function
The integral is entire: decays exponentially, uniformly dominating the integrand and all its derivatives on compact sets. Both the rational term and the integral are invariant under . This proves the meromorphic identity
Equivalently the Riemann xi function
is entire and satisfies . The reflection and duplication formulas for the Gamma function turn the same identity into
understood by meromorphic continuation at removable exceptional points. This establishes the functional equation of the Riemann zeta function, rather than assuming it.
If counts zeros in the critical strip with , including zero multiplicity, the Riemann–von Mangoldt formula is
At a zero ordinate one may instead use the conventional half-weight boundary count; that only alters the stated error. In particular .
To invert without assuming simple zeros, fix and set . Then , so
For large , , and hence . Let . The asymptotic inversion of the zeta zero count gives
As in the zero-counting formula, the sequence lists ordinates with zero multiplicity; “increasing” means nondecreasing here. The argument does not require the Riemann hypothesis or simplicity of zeros.
The Selberg upper-bound sieve replaces an exact but long inclusion-exclusion expansion by a short nonnegative square, and then minimizes its main term. For an interval , the count of multiples of every integer is
Crucially the remainder bound is independent of .
Let and take real weights , supported on squarefree , with . If , the sum of these weights over divisors of is just one; for all other its square is nonnegative. Thus
Expanding and counting common multiples gives
This separates the local density from a uniform interval error. The weights will be chosen to minimize .
The Euler totient function identity yields the Selberg sieve diagonalization
Only squarefree occur. Inverting this finite triangular sum by Möbius inversion gives
Write . The Cauchy-Schwarz inequality gives , with equality at . The inverse formula then produces the optimal Selberg sieve weights
The constraints are satisfied, since the diagonal transformation is invertible and .
We need the leading constant, not just . Here is an elementary proof of the Selberg sieve denominator asymptotic. For define the multiplicative arithmetic function by
Checking the prime-local factors shows . Also : the local factors for absolute values differ from one by , and their logarithmic first moments sum . The signed local sums are all one, so absolute convergence gives . Using the harmonic number estimate,
For the last equality, is bounded and is bounded too.
The optimal Selberg weights have modulus at most one. To prove this here, for squarefree use . The product is the sum of over , , , with squarefree. All are distinct squarefree integers at most , and so these are a subset of the terms of . The displayed weight formula now gives . Consequently
Every prime in the interval exceeding survives the sieve; at most smaller primes must be restored. Choose . Then
and the uniform interval bound from optimal Selberg weights follows:
All constants are independent of . Given , make the absolute error in the coefficient smaller than by choosing large enough. Uniformly for every and ,
Fix a modulus and a residue class with . The Dirichlet characters modulo are the one-dimensional characters of a representation of , extended by zero on nonunits. Let be the principal Dirichlet character.
For every nonprincipal Dirichlet character the partial sums are bounded: the sum over a full period is zero, and a remaining incomplete period has bounded length. Partial summation therefore continues its Dirichlet L-function holomorphically to by
This shows in particular that it has no pole at one. By contrast
has a simple pole there. We use the stipulated nonvanishing for every real nonprincipal Dirichlet character, and establish the remaining nonvanishing as follows.
For real , take the product over all Dirichlet characters. The Euler product logarithms and Orthogonality of Dirichlet characters give
Thus this product is real and at least one. If a nonreal Dirichlet character had , complex conjugation would also give . These are distinct factors. Two zeros and only one possible simple pole force the whole product to tend to zero as , contradicting the lower bound. Hence all nonprincipal Dirichlet characters have , under the given real-character assumption.
For , absolute convergence of each Euler product gives
with bounded remainder as : the terms of prime-power exponent at least two have total modulus at most . Since a nonprincipal defines a holomorphic function that is nonzero near one, its Euler-product logarithm differs from a local holomorphic logarithm by a fixed integer multiple of on a short real interval. It is therefore bounded there. For the principal Dirichlet character the pole instead gives
Apply the Dirichlet character orthogonality relation at each prime. The prime-character sum near one yields
This tends to infinity. A finite set of primes would have a bounded sum as , so every coprime residue class contains infinitely many primes. This proves the Dirichlet theorem on primes in arithmetic progressions from the specified assumption. In fact it proves divergence of the corresponding reciprocal-prime series and gives Dirichlet density .
Finally, for real each prime satisfies
The integrands are nonnegative, so Tonelli theorem permits summation inside the integral. At a fixed , exactly primes from the residue class have entered. Therefore
Both sides are finite, since they are bounded respectively by and . The values of a counting function at its isolated jump endpoints do not change this integral.

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