REVIEW 4 minor 8 references
A weaker but simpler sieve inequality
T0 review · 0 major / 4 minor · reviewed 2026-07-11 · grok-4.5
Pith's one-line read A simpler identity for sieve weights yields the same short-interval cancellation with less work.
desk verdict Clean expository note that publicizes Selberg's 1981 identity for the weaker sum U, shows it already covers the short-interval applications, and fixes the Opera lemma gap Matomäki flagged. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The identity (2.3) that rewrites U as product_p (1-1/p) times sum_delta theta_delta^2 / phi(delta), where theta_m = sum_{d|m} lambda_d; a trivial bound theta^2 <= tau |theta| (or tau_2 theta) then reduces the problem to a standard sieve estimate of dimension 2.
What would settle it
Compute the sum of theta_delta^2 / phi(delta) explicitly for beta-sieve weights with beta < 8 and check whether it remains bounded independently of the sifting range; if it grows, the final O(1) claim fails for those smaller beta.
Extended reading notes
Core claim
For beta-sieve weights (or suitable Lambda-squared weights) the sum U = sum_d phi(d) (sum_{m: d|m} lambda_m/m)^2 is << product_p (1-1/p). This is the same order of magnitude previously obtained for the larger sum W, and is precisely the quantity needed for the short-interval applications.
Load-bearing premise
The argument needs the sieve level parameter beta to be at least 8 so that a standard two-dimensional sieve inequality can absorb the extra divisor growth introduced by the crude bound on the squares of the weight sums.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proves that for beta-sieve weights (or suitable Selberg Lambda-squared weights) the sum U = sum_{d|P} phi(d) (sum_{m: d|m} lambda_m/m)^2 satisfies U << product_{p|P} (1-1/p). An elementary identity (2.3) reduces U to a sum of theta_delta^2/phi(delta), which is then bounded by the same dimension-kappa=2 sieve estimates used for the larger sum W in Opera de Cribro. The bound is sufficient for the short-interval applications that motivate the work; an appendix supplies a corrected proof of the original Opera Lemma 6.18 (addressing a coprimality gap noted by Matomaki) and related identities for general density functions are recorded.
Significance. The result supplies a cleaner, more natural route to the estimate actually needed for upper bounds on primes and lower bounds on almost-primes in almost all intervals of length g(x) log x (g->infty arbitrarily slowly). The identity (2.3) is transparent and self-contained; the appendix correction of Lemma 6.18 is a useful service to the literature. The historical framing via Selberg's 1981 letter adds context without affecting the mathematics. The argument relies only on standard beta-sieve machinery already in wide use, so the contribution is incremental but cleanly executed and immediately applicable.
minor comments (4)
- [Appendix] Appendix, line after (4.3): 'Propostion 6.7' is misspelled; correct to 'Proposition'.
- [Appendix] Appendix, paragraph containing (4.3): the hyphenation 'dimen- sion kappa=2' should be repaired for readability.
- [Section 2] Section 2, after (2.5): the text says the proof of (2.2) 'can be taken to run along the very same lines as does that for (1.3) in Section 4'; a one-sentence reminder that the same conditions beta >= 8 and s >= beta+1 are in force would make the dependence fully explicit without forcing the reader to the appendix.
- [References] References: the arXiv identifier of the present paper appears as 2607.05707; if this is a placeholder it should be updated on final submission.
Circularity Check
No significant circularity; elementary identity (2.3) is self-contained and the bound follows standard sieve estimates without definitional reduction.
full rationale
The paper's central contribution is the elementary identity (2.3) obtained by direct interchange of summation and complementary divisors, reducing the bound for U to an estimate of sum theta_delta^2 / phi(delta). That estimate proceeds via the crude majorant (2.4) (or (2.8)) and then the same lines as the corrected proof of the stronger bound for W given in the appendix, which invokes only the classical beta-sieve estimates of dimension kappa=2 under the usual level condition s >= beta+1 (beta >= 8). These estimates are standard results of sieve theory (appearing in the authors' prior book and used by many subsequent authors); they do not presuppose the target inequality for U, nor is there any definitional loop, fitted parameter renamed as a prediction, uniqueness theorem imported from the authors, or ansatz smuggled via citation. The appendix itself supplies an independent correction of a minor gap previously noted by Matomaki. Self-citations to Opera de Cribro and earlier papers of the author are present but supply established machinery rather than forcing the conclusion by construction. The derivation is therefore free of the circular patterns listed.
Assumptions & free parameters
assumptions (3)
- domain assumption Beta-sieve weights of level D with beta >= 8 satisfy the dimension-kappa=2 estimates of Opera Proposition 6.7 (upper and lower bounds for sum lambda_c g(c)).
- domain assumption For beta-sieve weights one has |lambda_d| <= 1, hence theta_m = sum_{d|m} lambda_d satisfies |theta_m| <= tau(m); for Lambda^2 weights |lambda_d| <= 3^{nu(d)} and theta_m <= tau_2(m).
- standard math The elementary identity relating sum phi(d) (sum_{d|m} lambda_m/m)^2 to product (1-1/p) times sum theta_delta^2 / phi(delta) holds for any real coefficients lambda.
Cite this review
Pith. "Pith review of A weaker but simpler sieve inequality." pith.science (2026). https://pith.science/paper/AMTWLOOI
@misc{pith2026260705707,
author = {Pith},
title = {Pith review of: A weaker but simpler sieve inequality},
year = {2026},
howpublished = {\url{https://pith.science/paper/AMTWLOOI}},
note = {Machine review of arXiv:2607.05707}
}
read the original abstract
We discuss a cancellation property of sieve weights, one that is applicable to the distribution of primes and almost-primes in very short intervals.
Reference graph
Works this paper leans on
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[1]
Friedlander, Sifting short intervals, Math
J.B. Friedlander, Sifting short intervals, Math. Proc. Cambridge Philos. Soc. 91(1982), 9–15
work page 1982
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[2]
Friedlander, Sifting short intervals II, Math
J.B. Friedlander, Sifting short intervals II, Math. Proc. Cambridge Philos. Soc.92(1982), 381–384
work page 1982
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[3]
J.B. Friedlander and H. Iwaniec, Opera de Cribro,Colloquium Publications, 57, (xx plus 527 pages), Amer. Math. Soc. (Providence) 2010
work page 2010
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[4]
Iwaniec, Rosser’s sieve, Acta Arith.36, (1980) 171–202
H. Iwaniec, Rosser’s sieve, Acta Arith.36, (1980) 171–202
work page 1980
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[5]
Matom¨ aki, e-mail to JF and HI, Oct
K. Matom¨ aki, e-mail to JF and HI, Oct. 5, 2020. 10 FRIEDLANDER
work page 2020
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[6]
Matom¨ aki, Almost primes in almost all very short intervals
K. Matom¨ aki, Almost primes in almost all very short intervals. J. Lond. Math. Soc. (2) 106 (2022), no. 2, 1061–1097
work page 2022
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[7]
Selberg, personal communication, Nov
A. Selberg, personal communication, Nov. 13, 1981
work page 1981
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[8]
A. Selberg, Lectures on sieves, appearing in Collected Papers II, pp 65–247, Springer Verlag (Berlin) 1991. Department of Mathematics, University of Toronto Toronto, Ontario M5S 2E4, Canada (frdlndr@math.utoronto.ca)
work page 1991
Reviewed July 11, 2026 · model on record in the stance chip above.
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