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Robin's Inequality at Colossally Abundant Numbers and Nicolas' Inequality at Their Largest Prime Factor

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Abstract

Robin's criterion states that the Riemann Hypothesis holds if and only if σ(n)<eγ⋅n⋅log⁡log⁡n\sigma(n) < e^{\gamma} \cdot n \cdot \log\log n for every n>5040n > 5040, and Nicolas' criterion states that it holds if and only if c(q)=log⁡(q#/φ(q#))−γ−log⁡log⁡θ(q)>0c(q) = \log(q\#/\varphi(q\#)) - \gamma - \log\log\theta(q) > 0 for every prime qq, where q#q\# is the primorial of qq and θ\theta is the Chebyshev function. Let NN be a colossally abundant number, let ξ(N)\xi(N) be the real number associated with NN by Nicolas, and let qq be the largest prime not exceeding ξ(N)\xi(N). Writing Δ(N)=log⁡(σ(N)/N)−γ−log⁡log⁡log⁡N\Delta(N) = \log(\sigma(N)/N) - \gamma - \log\log\log N, we prove without any hypothesis that, whenever log⁡q≥31\log q \geq 31, 1.353/(qlog⁡2q)≤Δ(N)−c(q)+22/(qlog⁡q)≤3.970/(qlog⁡2q)1.353/(\sqrt{q} \log^{2} q) \leq \Delta(N) - c(q) + 2\sqrt{2}/(\sqrt{q} \log q) \leq 3.970/(\sqrt{q} \log^{2} q). Thus Robin's inequality at NN and Nicolas' inequality at qq differ by 22/(qlog⁡q)2\sqrt{2}/(\sqrt{q} \log q) up to an explicit error of smaller order. As consequences, every colossally abundant counterexample to Robin's inequality yields a prime qq with c(q)>2.70/(qlog⁡q)c(q) > 2.70/(\sqrt{q} \log q); conversely, every prime qq with log⁡q≥31\log q \geq 31 and c(q)>22(1−0.4787/log⁡q)/(qlog⁡q)c(q) > 2\sqrt{2}(1 - 0.4787/\log q)/(\sqrt{q} \log q) yields a colossally abundant counterexample, so that Nicolas' oscillation theorem implies Robin's theorem on colossally abundant counterexamples; and under the Riemann Hypothesis every colossally abundant number with log⁡q≥31\log q \geq 31 satisfies Δ(N)<−0.654/(qlog⁡q)\Delta(N) < -0.654/(\sqrt{q} \log q), in accordance with the constant 2(2−1)2(\sqrt{2}-1) of Ramanujan's bound. For superabundant counterexamples, using the exponent bound of Nazardonyavi and Yakubovich, which gives log⁡n≥ψ(pk)\log n \geq \psi(p_{k}) for the largest prime factor pkp_{k}, we prove c(pk)>0.9991/(pklog⁡pk)c(p_{k}) > 0.9991/(\sqrt{p_{k}} \log p_{k}), and we show that the least colossally abundant number not smaller than the least counterexample nn is itself a counterexample NN with log⁡N−log⁡ξ(N)≤log⁡n\log N - \log\xi(N) \leq \log n.

Introduction

The Riemann Hypothesis (RH) is the conjecture that the Riemann zeta function has its zeros only at the negative even integers and at complex numbers with real part 12\frac{1}{2} [1]. It has been called the “Holy Grail of Mathematics” [2, 3], and numerous equivalent formulations exist [4]. One of particular interest here is Robin’s criterion [5], which asserts that RH is equivalent to the inequality

σ(n)<eγ⋅n⋅log⁡log⁡nfor every integer n>5040.(1)\sigma(n)<e^\gamma\cdot n\cdot\log\log n \qquad\text{for every integer } n>5040. \tag*{(1)}

Here γ≈0.57721\gamma\approx0.57721 is the Euler–Mascheroni constant, σ(n)=∑d∣nd\sigma(n)=\sum_{d\mid n}d is the sum-of-divisors function, and log⁡\log denotes the natural logarithm. Grönwall’s theorem [6] states that lim sup⁡n→∞σ(n)/(nlog⁡log⁡n)=eγ\limsup_{n\to\infty}\sigma(n)/(n\log\log n)=e^\gamma, so (1) asserts that this limiting value is never attained beyond 5040. A closely related elementary reformulation in terms of harmonic numbers is due to Lagarias [7], and the extremal integers relevant to both criteria have been studied computationally by Briggs [8] and structurally by Caveney, Nicolas and Sondow [9].

It is known that (1) holds for many classes of integers: odd integers exceeding 9 and squarefree integers exceeding 30 [10], sums of two squares exceeding 720 [11], and tt-free integers for t=5,7,11t=5,7,11 and 20 [10, 12, 13, 14]. Akbary and Friggstad [15] showed that the least counterexample to (1), should one exist, must be a superabundant number, Nazardonyavi and Yakubovich [16] refined this to the smaller class of extremely abundant numbers, and the author proved that its largest prime factor exceeds e31.018e^{31.018} [17]. Robin [5] proved that if RH is false, then (1) fails for infinitely many colossally abundant numbers.

A second criterion concerns the primorials q#=∏p≤qpq\# = \prod_{p \le q} p. For a real number x≥2x \ge2 put

c(x)=∑p≤xlog⁡pp−1−γ−log⁡log⁡θ(x),c(x) = \sum_{p \le x} \log\frac{p}{p-1} - \gamma- \log\log\theta(x),

where θ(x)=∑p≤xlog⁡p\theta(x) = \sum_{p \le x} \log p is the Chebyshev function, so that c(q)>0c(q) > 0 is the inequality q#φ(q#)>eγ⋅log⁡log⁡(q#)\frac{q\#}{\varphi(q\#)} > e^\gamma\cdot\log\log(q\#), with φ\varphi Euler’s totient function. Nicolas [18] proved that c(x)>0c(x) > 0 for every x≥2x \ge2 if RH is true, and that if RH is false, then c(x)=Ω±(x−b)c(x) = \Omega_{\pm}(x^{-b}) for some 0<b<120 < b < \frac{1}{2}. Under RH, Ramanujan’s asymptotic upper bound for σ(n)/n\sigma(n)/n [19] contains the term −2(2−1)log⁡n-\frac{2(\sqrt{2}-1)}{\sqrt{\log n}}, and Nicolas [20] gave an effective form of this bound, using the structure of colossally abundant numbers and his estimate [21] of c(x)c(x) under RH.

In this paper we compare Robin’s inequality at a colossally abundant number with Nicolas’ inequality at its largest prime factor, without assuming RH. For an integer n≥16n \ge16 put

Δ(n)=log⁡σ(n)n−γ−log⁡log⁡log⁡n,\Delta(n) = \log\frac{\sigma(n)}{n} - \gamma- \log\log\log n,

so that Robin’s inequality holds for n>5040n > 5040 if and only if Δ(n)<0\Delta(n) < 0. To each colossally abundant number NN Nicolas associates a real number ξ(N)\xi(N) [20] Definition 4.3; every prime factor of NN is at most ξ(N)\xi(N) § 3. Our main result is the following.

Theorem 1.1. Let NN be a colossally abundant number, and let qq be the largest prime with q≤ξ(N)q \le\xi(N). If log⁡q≥31\log q \ge31, then

1.353q⋅log⁡2q≤Δ(N)−c(q)+22q⋅log⁡q≤3.970q⋅log⁡2q.\frac{1.353}{\sqrt{q}\cdot\log^2 q} \le\Delta(N)-c(q)+\frac{2\sqrt{2}}{\sqrt{q}\cdot\log q} \le\frac{3.970}{\sqrt{q}\cdot\log^2 q}.

Thus Robin’s function at NN and Nicolas’ function at qq differ by 22qlog⁡q\frac{2\sqrt{2}}{\sqrt{q}\log q}, up to an explicit error that is smaller by a factor log⁡q\log q. Remark 3.5 describes the relation of Theorem 1.1 to the work of Robin and Nicolas, and Remark 3.6 the size of its error term. Theorem 1.1 has the following consequences.

  1. Every colossally abundant counterexample to (1) yields a prime qq with log⁡q>31.03\log q > 31.03 and c(q)>2.70qlog⁡qc(q) > \frac{2.70}{\sqrt{q}\log q} (Corollary 4.2).

  1. Conversely, every prime qq with log⁡q≥31\log q \ge31 and c(q)>22qlog⁡q(1−0.4787log⁡q)c(q) > \frac{2\sqrt{2}}{\sqrt{q}\log q}\left(1-\frac{0.4787}{\log q}\right) yields a colossally abundant counterexample to (1) (Corollary 4.3).

  1. Nicolas’ theorem c(x)=Ω+(x−b)c(x) = \Omega_{+}(x^{-b}) under the failure of RH implies, through (2), Robin’s theorem that (1) then fails for infinitely many colossally abundant numbers (Corollary 4.4).

  1. Under RH, every colossally abundant number NN with log⁡q≥31\log q \ge31 satisfies Δ(N)<−0.654qlog⁡q\Delta(N) < -\frac{0.654}{\sqrt{q}\log q} (Corollary 4.6); the constant 22−2=2(2−1)2\sqrt{2}-2=2(\sqrt{2}-1) obtained from Theorem 1.1 and the main term of c(q)c(q) is the constant of Ramanujan’s bound.

  1. RH holds if and only if c(q)<2.70qlog⁡qc(q) < \frac{2.70}{\sqrt{q}\log q} for every prime q≥109q \ge10^9 (Corollary 4.7). This equivalence also follows from Nicolas’ theorem [18] together with his estimate under RH [21, 20], and holds with 2.70 replaced by any constant greater than 2+τ=2.0461…2+\tau=2.0461\ldots; Corollary 4.7 shows that the primes qq of item (1) violate it.

For superabundant counterexamples, which need not be colossally abundant, we prove the following (§ 5).

  1. Every superabundant number nn with largest prime factor pkp_k satisfies log⁡n≥ψ(pk)\log n \ge\psi(p_k) (Lemma 5.1, following [16]), and every superabundant counterexample satisfies c(pk)>0.9991pklog⁡pkc(p_k) > \frac{0.9991}{\sqrt{p_k}\log p_k} (Theorem 5.4).

If nn is the least counterexample, then the least colossally abundant number N≥nN \ge n is a counterexample, and log⁡N−log⁡ξ(N)≤log⁡n≤log⁡N\log N - \log\xi(N) \le\log n \le\log N (Corollary 5.5).

The proofs use the description of colossally abundant numbers by Alaoglu and Erdős [22], Robin [5] and Nicolas [20], explicit estimates for the Chebyshev function of Rosser and Schoenfeld [23], Büthe [24] and Dusart [25], the estimate of Axler [26] for the Mertens product, and the numerical verification of (1) for all 5040<n≤1013.114855040<n\le10^{13.11485} due to Morrill and Platt [14]. Section 2 collects these results, Section 3 proves Theorem 1.1, Section 4 derives its consequences, Section 5 treats superabundant counterexamples, and Section 6 describes the computer verification of the numerical constants.

Background

We write I(n)=σ(n)nI(n)=\frac{\sigma(n)}{n} for the abundancy index, and we say that Robin’s inequality holds for nn if I(n)<eγ⋅log⁡log⁡nI(n)<e^\gamma\cdot\log\log n. An integer n>5040n>5040 for which Robin’s inequality does not hold is called a counterexample. We write ψ(x)=∑pj≤xlog⁡p=∑j≥1θ(x1/j)\psi(x)=\sum_{p^j\le x}\log p=\sum_{j\ge1}\theta(x^{1/j}) for the second Chebyshev function, so that ψ(x)=∑q≤x⌊log⁡xlog⁡q⌋log⁡q\psi(x)=\sum_{q\le x}\left\lfloor\frac{\log x}{\log q}\right\rfloor\log q and ψ(x)≥θ(x)+θ(x)\psi(x)\ge\theta(x)+\theta(\sqrt{x}). For a prime pp we write p#=∏q≤pqp\#=\prod_{q\le p}q, so that log⁡(p#)=θ(p)\log(p\#)=\theta(p), and p1=2<p2=3<⋯p_1=2<p_2=3<\cdots denotes the sequence of primes. Since ∑p≤xlog⁡pp−1\sum_{p\le x}\log\frac{p}{p-1} and θ(x)\theta(x) change only at primes, c(x)=c(q)c(x)=c(q) when qq is the largest prime with q≤xq\le x.

Robin’s Criterion and Counterexamples

Proposition 2.1. Robin’s inequality holds for all natural numbers n>5040n>5040 if and only if the Riemann Hypothesis is true [5] [Theorem 1 pp. 188].

Proposition 2.2. For n>1n>1, I(n)<∏q∣nqq−1=n′φ(n′)I(n)<\prod_{q\mid n}\frac{q}{q-1}=\frac{n'}{\varphi(n')}, where n′n' is the product of the distinct primes dividing nn [10] [(2.7) pp. 362].

Proposition 2.3. Robin’s inequality holds for every integer nn with 5040<n≤1013.114855040<n\le10^{13.11485} [14] [Theorem 5].

A natural number nn is superabundant if I(m)<I(n)I(m)<I(n) for every m<nm<n, and colossally abundant if there is ε>0\varepsilon>0 with σ(m)m1+ε≤σ(n)n1+ε\frac{\sigma(m)}{m^{1+\varepsilon}}\le\frac{\sigma(n)}{n^{1+\varepsilon}} for every m≥1m\ge1 [22]; every colossally abundant number is superabundant [22].

Proposition 2.4. If nn is superabundant with largest prime factor pkp_k, then n=∏i=1kpiain=\prod_{i=1}^{k}p_i^{a_i} with a1≥a2≥⋯≥ak≥1a_1\ge a_2\ge\cdots\ge a_k\ge1 [22] [Theorem 1 pp. 450].

Proposition 2.5. If n>5040n>5040 is the smallest integer such that Robin’s inequality does not hold for nn, then nn is superabundant [15] [Theorem 3, p. 273].

Proposition 2.6. If the Riemann Hypothesis is false, then Robin’s inequality fails for infinitely many colossally abundant numbers [5] [Section 4, Proposition 1].

Nicolas’ Criterion

Proposition 2.7. If the Riemann Hypothesis is true, then c(x)>0c(x)>0 for every x≥2x\ge2. If the Riemann Hypothesis is false, then there is bb with 0<b<120<b<\frac{1}{2} such that c(x)=Ω±(x−b)c(x)=\Omega_{\pm}(x^{-b}); more precisely, this holds for every bb with 1−Θ<b<121-\Theta<b<\frac{1}{2}, where Θ\Theta is the supremum of the real parts of the zeros of the Riemann zeta function [18] [Theorem 3 (b), (c)], see also [21].

In [18, 21] the statement is given for log⁡f(x)=−c(x)\log f(x)=-c(x), where f(x)=eγ⋅log⁡θ(x)⋅∏p≤x(1−1p)f(x)=e^\gamma\cdot\log\theta(x)\cdot\prod_{p\le x}\left(1-\frac{1}{p}\right). Put

τ=2+γ−log⁡(4π)=0.0461914…,S1(x)=∑ρxρ−1ρ(1−ρ).\tau=2+\gamma-\log(4\pi)=0.0461914\ldots,\qquad S_1(x)=\sum_{\rho}\frac{x^{\rho-1}}{\rho(1-\rho)}.

where ρ\rho runs over the nontrivial zeros of the Riemann zeta function [20] [(1.3), (1.5)].

Proposition 2.8. Assume the Riemann Hypothesis. Then ∣S1(x)∣≤τx|S_1(x)| \le\frac{\tau}{\sqrt{x}} for x>1x > 1 [20] [(1.4)], and for x≥109x \ge10^9 [21] [(2.16)], [20] [(1.11)],

0.055xlog⁡2x≤−c(x)+2xlog⁡x+S1(x)log⁡x≤2.062xlog⁡2x.\frac{0.055}{\sqrt{x}\log^2 x} \le-c(x) + \frac{2}{\sqrt{x}\log x} + \frac{S_1(x)}{\log x} \le\frac{2.062}{\sqrt{x}\log^2 x}.

Consequently c(x)<2+τxlog⁡x<2.0462xlog⁡xc(x) < \frac{2+\tau}{\sqrt{x}\log x} < \frac{2.0462}{\sqrt{x}\log x} for every x≥109x \ge10^9.

Proof. The left inequality gives c(x)≤2xlog⁡x+S1(x)log⁡x−0.055xlog⁡2x<2+τxlog⁡xc(x) \le\frac{2}{\sqrt{x}\log x} + \frac{S_1(x)}{\log x} - \frac{0.055}{\sqrt{x}\log^2 x} < \frac{2+\tau}{\sqrt{x}\log x}, and 2+τ<2.04622+\tau< 2.0462.

Explicit Estimates for Primes

Proposition 2.9. The following hold.

(a) θ(x)<x\theta(x) < x for 0<x≤10190 < x \le10^{19}, and θ(x)>x−1.94x\theta(x) > x - 1.94\sqrt{x} for 1427<x≤10191427 < x \le10^{19} [24] [Theorem 2], see also [20] [(2.1), (2.2)].

(b) ∣θ(x)−x∣<xlog⁡3x|\theta(x)-x| < \frac{x}{\log^3 x} for x≥89,967,803x \ge89,967,803 [25] [Theorem 4.2].

(c) For every x≥89,693x \ge89,693 there is a prime pp with x<p≤x⋅(1+1log⁡3x)x < p \le x \cdot\left(1+\frac{1}{\log^3 x}\right) [25] [Proposition 5.4].

(d) θ(x)≥0.945⋅x\theta(x) \ge0.945 \cdot x for x≥853x \ge853 [23] [Theorem 10], and π(x)<1.26⋅xlog⁡x\pi(x) < \frac{1.26\cdot x}{\log x} for x>1x > 1 [23] [(3.6)], where π(x)\pi(x) is the number of primes p≤xp \le x.

(e) ∑p≥x1p3≤0.086x2\sum_{p\ge x}\frac{1}{p^3} \le\frac{0.086}{x^2} for x≥1418x \ge1418 [20] [(2.15)].

(f) For x≥46,909,038x \ge46,909,038 [26] [Proposition 6.1],

∏p≤xpp−1<eγ⋅log⁡x⋅(1−ε(log⁡x))−1,ε(P)=120P3+316P4.\prod_{p\le x}\frac{p}{p-1} < e^\gamma\cdot\log x \cdot\left(1-\varepsilon(\log x)\right)^{-1}, \qquad\varepsilon(P)=\frac{1}{20P^3}+\frac{3}{16P^4}.

Lemma 2.10. The following hold.

(a) θ(t)<1.000012⋅t\theta(t) < 1.000012\cdot t for every t>0t>0.

(b) Let λ≥31\lambda\ge31. Then ∣θ(t)−t∣≤0.022λ⋅t|\theta(t)-t| \le\frac{0.022}{\lambda}\cdot t for every t≥1.39838⋅eλ/2t \ge1.39838\cdot e^{\lambda/2}.

Proof. (a) For t≤1019t \le10^{19} this is Proposition 2.9 (a); for t>1019t > 10^{19}, Proposition 2.9 (b) gives θ(t)<t⋅(1+1log⁡3(1019))<1.000012⋅t\theta(t)<t\cdot\left(1+\frac{1}{\log^3(10^{19})}\right)<1.000012\cdot t.

(b) Let t≥1.39838⋅eλ/2t \ge1.39838\cdot e^{\lambda/2}. If t≤1019t \le10^{19}, Proposition 2.9 (a) gives ∣θ(t)−t∣<1.94t⋅t|\theta(t)-t|<\frac{1.94}{\sqrt{t}}\cdot t and t≥1.18253⋅eλ/4\sqrt{t}\ge1.18253\cdot e^{\lambda/4}, so λ⋅∣θ(t)−t∣t<1.94λe−λ/41.18253\lambda\cdot\frac{|\theta(t)-t|}{t}<\frac{1.94\lambda e^{-\lambda/4}}{1.18253}; the right-hand side is decreasing for λ≥4\lambda\ge4, and is less than 0.0220.022 at λ=31\lambda=31. If t>1019t>10^{19}, Proposition 2.9 (b) gives λ⋅∣θ(t)−t∣t<λlog⁡3t\lambda\cdot\frac{|\theta(t)-t|}{t}<\frac{\lambda}{\log^3t} with log⁡t>max⁡(log⁡(1019),λ2)\log t>\max\left(\log(10^{19}),\frac{\lambda}{2}\right). If λ≤2log⁡(1019)\lambda\le2\log(10^{19}), this is at most 2log⁡(1019)log⁡3(1019)<0.022\frac{2\log(10^{19})}{\log^3(10^{19})}<0.022, and otherwise it is at most 8λ2<8312<0.022\frac{8}{\lambda^2}<\frac{8}{31^2}<0.022.

Lemma 2.11. Let y>1y>1 and 0≤δ<10\le\delta<1 be such that ∣θ(t)−t∣≤δt|\theta(t)-t|\le\delta t for every t≥yt\ge y. Put Aj=1ylog⁡jyA_j=\frac{1}{y\log^j y}. Then

(1−3δ)⋅A1−A2≤∑p>y1p2≤(1+3δ)⋅A1−(1+δ)⋅A2+2(1+δ)⋅A3.(1-3\delta)\cdot A_1-A_2\le\sum_{p>y}\frac{1}{p^2}\le(1+3\delta)\cdot A_1-(1+\delta)\cdot A_2+2(1+\delta)\cdot A_3.

Proof. Put Jj=∫y∞dtt2log⁡jtJ_j=\int_y^\infty\frac{dt}{t^2\log^j t}. Since ddt(−1tlog⁡jt)=1t2log⁡jt+jt2log⁡j+1t\frac{d}{dt}\left(-\frac{1}{t\log^j t}\right)=\frac{1}{t^2\log^j t}+\frac{j}{t^2\log^{j+1}t}, we have Jj=Aj−jJj+1J_j=A_j-jJ_{j+1}, hence J1=A1−J2J_1=A_1-J_2, J2=A2−2J3J_2=A_2-2J_3, and 0<Jj≤Aj0<J_j\le A_j. By Stieltjes integration,

∑p>y1p2=∫y∞dθ(t)t2log⁡t=−θ(y)y2log⁡y+∫y∞θ(t)⋅2log⁡t+1t3log⁡2t dt.\sum_{p>y}\frac{1}{p^2}=\int_y^\infty\frac{d\theta(t)}{t^2\log t}=-\frac{\theta(y)}{y^2\log y}+\int_y^\infty\theta(t)\cdot\frac{2\log t+1}{t^3\log^2t}\,dt.

and ∫y∞2log⁡t+1t3log⁡2t dt=2J1+J2=2A1−J2\int_y^\infty\frac{2\log t+1}{t^3\log^2t}\,dt=2J_1+J_2=2A_1-J_2. Using (1−δ)t≤θ(t)≤(1+δ)t(1-\delta)t\le\theta(t)\le(1+\delta)t for t≥yt\ge y, the sum is at least −(1+δ)A1+(1−δ)(2A1−A2)≥(1−3δ)A1−A2-(1+\delta)A_1+(1-\delta)(2A_1-A_2)\ge(1-3\delta)A_1-A_2, and at most −(1−δ)A1+(1+δ)(2A1−A2+2A3)-(1-\delta)A_1+(1+\delta)(2A_1-A_2+2A_3), using J2≥A2−2A3J_2\ge A_2-2A_3.

Colossally Abundant Numbers

The Structure of Colossally Abundant Numbers

We recall the description given by Nicolas [20] [Section 4], which goes back to Alaoglu and Erdős [22] and Robin [5]. For real t>1t>1 and an integer j≥1j\ge1 put

F(t,j)=log⁡(1+1t+t2+⋯+tj)log⁡t,F(t,j)=\frac{\log\left(1+\frac{1}{t+t^2+\cdots+t^j}\right)}{\log t},

which is decreasing in tt. Let NN be a colossally abundant number and κ\kappa its largest parameter. Then ξ=ξ(N)>1\xi=\xi(N)>1 is defined by F(ξ,1)=κF(\xi,1)=\kappa, and ξj=ξj(N)\xi_j=\xi_j(N) for j≥2j\ge2 by F(ξj,j)=κF(\xi_j,j)=\kappa, with ξ1=ξ\xi_1=\xi; KK is the largest jj with ξj≥2\xi_j\ge2 [20] [Definition 4.3]. Put Nκ=∏j=1K∏ξj+1<p≤ξjpjN_\kappa=\prod_{j=1}^{K}\prod_{\xi_{j+1}<p\le\xi_j}p^j.

Proposition 3.1. With this notation, the following hold.

(a) NκN_\kappa is colossally abundant with largest parameter κ\kappa, and NN divides NκN_\kappa; every prime dividing NN is at most ξ\xi, and a prime p≤ξp\le\xi has exponent jj in NκN_\kappa if ξj+1<p≤ξj\xi_{j+1}<p\le\xi_j [20] [(4.11), Proposition 4.2, Lemma 4.4], [22] [Theorem 10].

(b) ∑j=1Kθ(ξj)−log⁡ξ≤log⁡N≤∑j=1Kθ(ξj)\sum_{j=1}^{K}\theta(\xi_j)-\log\xi\le\log N\le\sum_{j=1}^{K}\theta(\xi_j), and ξξK+1⋅I(Nκ)≤I(N)≤I(Nκ)\frac{\xi}{\xi_{K+1}}\cdot I(N_\kappa)\le I(N)\le I(N_\kappa), where

I(Nκ)=∏j=1K∏ξj+1<p≤ξj1−p−(j+1)1−p−1.I(N_\kappa)=\prod_{j=1}^{K}\prod_{\xi_{j+1}<p\le\xi_j}\frac{1-p^{-(j+1)}}{1-p^{-1}}.

[20] [Proposition 4.5].

(c) ξ1/j≤ξj≤(jξ)1/j\xi^{1/j}\le\xi_j\le(j\xi)^{1/j} for every j≥2j\ge2 [20] [(4.26)].

(d) 2ξ⋅(1−log⁡22log⁡ξ)≤ξ2\sqrt{2\xi}\cdot\left(1-\frac{\log2}{2\log\xi}\right)\le\xi_2 for ξ≥1530\xi\ge1530 [5] [p. 190], [20] [(4.28)], and ξ2≤2ξ⋅(1−0.323log⁡ξ)\xi_2\le\sqrt{2\xi}\cdot\left(1-\frac{0.323}{\log\xi}\right) for ξ≥109\xi\ge10^9 [20] [(4.29)].

(e) If ξ>109+7\xi>10^9+7, then ∑j=3Kξj≤1.9769⋅ξ1/3\sum_{j=3}^{K}\xi_j\le1.9769\cdot\xi^{1/3} [20] [Lemmas 4.8–4.10].

(f) For every integer m≥2m\ge2 there are two consecutive colossally abundant numbers N′<NN'<N with Nξ(N)≤N′<m≤N\frac{N}{\xi(N)}\le N'<m\le N [20] [Proposition 4.6].

(g) If 3≤N′<N3\le N'<N are consecutive colossally abundant numbers and N′≤m≤NN'\le m\le N, then

I(m)log⁡log⁡m≤max⁡{I(N′)log⁡log⁡N′,I(N)log⁡log⁡N}.\frac{I(m)}{\log\log m}\le\max\left\{\frac{I(N')}{\log\log N'},\frac{I(N)}{\log\log N}\right\}.

[5] [Proposition 1], see also [16].

In (e), Nicolas states [20] [Lemma 4.10] for N≥N(0)N\ge N^{(0)}, where N(0)N^{(0)} is the colossally abundant number with ξ(N(0))=109+7\xi(N^{(0)})=10^9+7. If ξ>109+7\xi>10^9+7, then κ<F(109+7,1)\kappa<F(10^9+7,1), and since the parameters of colossally abundant numbers decrease as the numbers increase [20] [(4.4)], we have N>N(0)N>N^{(0)}, so (e) applies.

Three Estimates

Throughout this subsection, NN is a colossally abundant number with λ=log⁡ξ≥31\lambda=\log\xi\ge31, where ξ=ξ(N)\xi=\xi(N), and we put

Mξ=2ξ⋅λ,L(t)=log⁡log⁡t,S2=∑ξ2<p≤ξ1p2.M_\xi=\frac{\sqrt{2}}{\sqrt{\xi}\cdot\lambda},\qquad L(t)=\log\log t,\qquad S_2=\sum_{\xi_2<p\le\xi}\frac{1}{p^2}.

By Proposition 3.1 (d), and since 1−log⁡22⋅31>0.988821-\frac{\log2}{2\cdot31}>0.98882 and 2⋅0.98882>1.39838\sqrt{2}\cdot0.98882>1.39838,

\underaccent{\bar}{\xi}_2:=\sqrt{2\xi}\cdot\left(1-\frac{\log2}{2\lambda}\right)\le\xi_2\le\underaccent{\bar}{\xi}_2^{+}:=\sqrt{2\xi}\cdot\left(1-\frac{0.323}{\lambda}\right),\qquad\xi_2\ge1.39838\cdot e^{\lambda/2}, \tag*{(2)}

so Lemma 2.10 (b) applies to every t\ge\underaccent{\bar}{\xi}_2 with δ=0.022λ\delta=\frac{0.022}{\lambda}. Moreover \log\underaccent{\bar}{\xi}_2\le\frac{1}{2}(\lambda+\log2), and since −log⁡(1−log⁡22⋅31)<0.011306-\log\left(1-\frac{\log2}{2\cdot31}\right)<0.011306, also \log\underaccent{\bar}{\xi}_2\ge\frac{1}{2}(\lambda+\log2)-0.011306\ge\frac{\lambda}{2}\left(1+\frac{0.670535}{\lambda}\right).

Lemma 3.2. Mξ⋅(1−2.43616λ)≤S2≤Mξ⋅(1−1.920374λ)M_{\xi}\cdot\left(1-\frac{2.43616}{\lambda}\right)\le S_2\le M_{\xi}\cdot\left(1-\frac{1.920374}{\lambda}\right).

Proof. Put ℓ=log⁡ξ2\ell=\log\xi_2 and Aj=1ξ2ℓA_j=\frac{1}{\xi_2^{\ell}}. Since t↦tlog⁡tt\mapsto t\log t is increasing, the bounds on ξ2\xi_2 and ℓ\ell give

A1≥Mξ(1−0.323λ)(1+log⁡2λ)≥Mξ1+0.370148λ≥Mξ⋅(1−0.370148λ).A_1\ge\frac{M_{\xi}}{\left(1-\frac{0.323}{\lambda}\right)\left(1+\frac{\log2}{\lambda}\right)}\ge\frac{M_{\xi}}{1+\frac{0.370148}{\lambda}}\ge M_{\xi}\cdot\left(1-\frac{0.370148}{\lambda}\right).

and, since

(1−log⁡22λ)(1+0.670535λ)≥1+0.316464λ\left(1-\frac{\log2}{2\lambda}\right)\left(1+\frac{0.670535}{\lambda}\right)\ge1+\frac{0.316464}{\lambda}

for λ≥31\lambda\ge31,

A1≤Mξ1+0.316464λ≤Mξ⋅(1−0.316464λ+0.3164642λ2)≤Mξ⋅(1−0.313233λ).A_1\le\frac{M_{\xi}}{1+\frac{0.316464}{\lambda}}\le M_{\xi}\cdot\left(1-\frac{0.316464}{\lambda}+\frac{0.316464^2}{\lambda^2}\right)\le M_{\xi}\cdot\left(1-\frac{0.313233}{\lambda}\right).

Since λ2≤ℓ≤λ2(1+log⁡2λ)\frac{\lambda}{2}\le\ell\le\frac{\lambda}{2}\left(1+\frac{\log2}{\lambda}\right), we get A2=A1ℓ≤2MξλA_2=\frac{A_1}{\ell}\le\frac{2M_{\xi}}{\lambda}, A3=A2ℓ≤4Mξλ2A_3=\frac{A_2}{\ell}\le\frac{4M_{\xi}}{\lambda^2} and

A2≥2Mξλ⋅1−0.370148λ1+log⁡2λ≥2Mξλ⋅(1−1.06329631)>1.9314⋅Mξλ.A_2\ge\frac{2M_{\xi}}{\lambda}\cdot\frac{1-\frac{0.370148}{\lambda}}{1+\frac{\log2}{\lambda}}\ge\frac{2M_{\xi}}{\lambda}\cdot\left(1-\frac{1.063296}{31}\right)>\frac{1.9314\cdot M_{\xi}}{\lambda}.

By Lemma 2.11 with y=ξ2y=\xi_2 and 3δ=0.066λ3\delta=\frac{0.066}{\lambda},

∑p>ξ21p2≥(1−0.066λ)(1−0.370148λ)Mξ−2Mξλ≥Mξ⋅(1−2.436148λ)\sum_{p>\xi_2}\frac{1}{p^2}\ge\left(1-\frac{0.066}{\lambda}\right)\left(1-\frac{0.370148}{\lambda}\right)M_{\xi}-\frac{2M_{\xi}}{\lambda}\ge M_{\xi}\cdot\left(1-\frac{2.436148}{\lambda}\right)

and

∑p>ξ21p2≤(1+0.066λ)(1−0.313233λ)Mξ−1.9314⋅Mξλ+8.006⋅Mξλ2≤Mξ⋅(1−1.920374λ),\sum_{p>\xi_2}\frac{1}{p^2}\le\left(1+\frac{0.066}{\lambda}\right)\left(1-\frac{0.313233}{\lambda}\right)M_{\xi}-\frac{1.9314\cdot M_{\xi}}{\lambda}+\frac{8.006\cdot M_{\xi}}{\lambda^2}\le M_{\xi}\cdot\left(1-\frac{1.920374}{\lambda}\right),

where we used 2(1+δ)⋅4<8.0062(1+\delta)\cdot4<8.006 and 8.006λ≤8.00631<0.258259\frac{8.006}{\lambda}\le\frac{8.006}{31}<0.258259. By Lemma 2.11 with y=ξy=\xi, using −(1+δ)A2(ξ)+2(1+δ)A3(ξ)≤0-(1+\delta)A_2(\xi)+2(1+\delta)A_3(\xi)\le0,

0≤∑p>ξ1p2≤1.0022ξλ=1.00222⋅ξ⋅Mξ≤1.0022⋅31⋅e−31/22⋅Mξλ<4.08⋅10−6⋅Mξλ,0\le\sum_{p>\xi}\frac{1}{p^2}\le\frac{1.0022}{\xi\lambda}=\frac{1.0022}{\sqrt{2}\cdot\sqrt{\xi}}\cdot M_{\xi}\le\frac{1.0022\cdot31\cdot e^{-31/2}}{\sqrt{2}}\cdot\frac{M_{\xi}}{\lambda}<\frac{4.08\cdot10^{-6}\cdot M_{\xi}}{\lambda},

because λe−λ/2\lambda e^{-\lambda/2} is decreasing for λ≥2\lambda\ge2. Since S2=∑p>ξ21p2−∑p>ξ1p2S_2=\sum_{p>\xi_2}\frac{1}{p^2}-\sum_{p>\xi}\frac{1}{p^2}, the claim follows.

Lemma 3.3. Mξ⋅(1−0.369659λ)≤L(log⁡N)−L(θ(ξ))≤Mξ⋅(1−0.05272λ)M_{\xi}\cdot\left(1-\frac{0.369659}{\lambda}\right)\le L(\log N)-L(\theta(\xi))\le M_{\xi}\cdot\left(1-\frac{0.05272}{\lambda}\right).

Proof. Put D=log⁡N−θ(ξ)D=\log N-\theta(\xi). By Proposition 3.1 (c), ξ3≥ξ1/3≥e31/3>853\xi_3\ge\xi^{1/3}\ge e^{31/3}>853, so K≥3K\ge3, and by Proposition 2.9 (d), θ(ξ3)≥0.945⋅ξ1/3>λ\theta(\xi_3)\ge0.945\cdot\xi^{1/3}>\lambda, because 0.945⋅es/3>s0.945\cdot e^{s/3}>s for s≥31s\ge31. Proposition 3.1 (b) and (e) and Lemma 2.10 then give

θ(ξ2)≤D≤θ(ξ2)+1.000012⋅1.9769⋅ξ1/3.\theta(\xi_2)\le D\le\theta(\xi_2)+1.000012\cdot1.9769\cdot\xi^{1/3}.

By (2) and Lemma 2.10 (b),

θ(ξ2)≥(1−0.022λ)(1−log⁡22λ)2ξ≥(1−0.368574λ)2ξ\theta(\xi_2)\ge\left(1-\frac{0.022}{\lambda}\right)\left(1-\frac{\log2}{2\lambda}\right)\sqrt{2\xi}\ge\left(1-\frac{0.368574}{\lambda}\right)\sqrt{2\xi}

and

θ(ξ2)≤(1+0.022λ)(1−0.323λ)2ξ≤(1−0.301λ)2ξ.\theta(\xi_2)\le\left(1+\frac{0.022}{\lambda}\right)\left(1-\frac{0.323}{\lambda}\right)\sqrt{2\xi}\le\left(1-\frac{0.301}{\lambda}\right)\sqrt{2\xi}.

Moreover

1.000012⋅1.9769⋅ξ1/32ξ≤1.397905⋅e−λ/6≤1.397905⋅31⋅e−31/6λ<0.24717λ.\frac{1.000012\cdot1.9769\cdot\xi^{1/3}}{\sqrt{2\xi}}\le1.397905\cdot e^{-\lambda/6}\le\frac{1.397905\cdot31\cdot e^{-31/6}}{\lambda}<\frac{0.24717}{\lambda}.

because λe−λ/6\lambda e^{-\lambda/6} is decreasing for λ≥6\lambda\ge6. Hence

(1−0.368574λ)2ξ≤D≤(1−0.0538λ)2ξ.\left(1-\frac{0.368574}{\lambda}\right)\sqrt{2\xi}\le D\le\left(1-\frac{0.0538}{\lambda}\right)\sqrt{2\xi}.

By Proposition 2.9 (b), ξ⋅(1−λ−3)<θ(ξ)<ξ⋅(1+λ−3)\xi\cdot(1-\lambda^{-3})<\theta(\xi)<\xi\cdot(1+\lambda^{-3}). Hence log⁡N=θ(ξ)+D≤ξ⋅(1+λ−3+2e−λ/2)≤ξ⋅(1+0.0010488λ)\log N=\theta(\xi)+D\le\xi\cdot(1+\lambda^{-3}+\sqrt{2}e^{-\lambda/2})\le\xi\cdot\left(1+\frac{0.0010488}{\lambda}\right), so that log⁡log⁡N≤λ+0.0010488λ≤λ⋅(1+0.0000339λ)\log\log N\le\lambda+\frac{0.0010488}{\lambda}\le\lambda\cdot\left(1+\frac{0.0000339}{\lambda}\right) and

log⁡N⋅log⁡log⁡N≤ξλ⋅(1+0.001085λ).\log N\cdot\log\log N\le\xi\lambda\cdot\left(1+\frac{0.001085}{\lambda}\right).

Also log⁡θ(ξ)≥λ+log⁡(1−λ−3)≥λ−1.0001λ−3\log\theta(\xi)\ge\lambda+\log(1-\lambda^{-3})\ge\lambda-1.0001\lambda^{-3}, so that

θ(ξ)⋅log⁡θ(ξ)≥ξλ⋅(1−λ−3)(1−1.0001λ−4)≥ξλ⋅(1−0.00108λ).\theta(\xi)\cdot\log\theta(\xi)\ge\xi\lambda\cdot(1-\lambda^{-3})(1-1.0001\lambda^{-4})\ge\xi\lambda\cdot\left(1-\frac{0.00108}{\lambda}\right).

Since L′(t)=1tlog⁡tL'(t)=\frac{1}{t\log t} is decreasing for t>1t>1, the mean value theorem gives

Dlog⁡N⋅log⁡log⁡N≤L(log⁡N)−L(θ(ξ))≤Dθ(ξ)⋅log⁡θ(ξ).\frac{D}{\log N\cdot\log\log N}\le L(\log N)-L(\theta(\xi))\le\frac{D}{\theta(\xi)\cdot\log\theta(\xi)}.

With 2ξξ=Mξ\frac{\sqrt{2\xi}}{\xi} = M_\xi, the lower bound is at least Mξ⋅1−0.368574/λ1+0.001085/λ≥Mξ⋅(1−0.369659λ)M_\xi\cdot\frac{1-0.368574/\lambda}{1+0.001085/\lambda}\ge M_\xi\cdot\left(1-\frac{0.369659}{\lambda}\right), and the upper bound is at most Mξ⋅1−0.0538/λ1−0.00108/λ≤Mξ⋅(1−0.05272λ)M_\xi\cdot\frac{1-0.0538/\lambda}{1-0.00108/\lambda}\le M_\xi\cdot\left(1-\frac{0.05272}{\lambda}\right).

Lemma 3.4. Let qq be the largest prime with q≤ξq\le\xi. Then

∑p≤qlog⁡pp−1−S2−1.0156⋅Mξλ≤log⁡I(N)≤∑p≤qlog⁡pp−1−S2.\sum_{p\le q}\log\frac{p}{p-1}-S_2-\frac{1.0156\cdot M_\xi}{\lambda}\le\log I(N)\le\sum_{p\le q}\log\frac{p}{p-1}-S_2.

Proof. For p≤ξp\le\xi let vpv_p be the exponent of pp in NκN_\kappa. By Proposition 3.1 (a) and (b), the primes p≤ξp\le\xi are the primes p≤qp\le q, and

log⁡I(Nκ)=∑p≤qlog⁡pp−1+∑p≤qlog⁡(1−p−(vp+1)).\log I(N_\kappa)=\sum_{p\le q}\log\frac{p}{p-1}+\sum_{p\le q}\log(1-p^{-(v_p+1)}).

Every term of the second sum is negative, and vp=1v_p=1 for ξ2<p≤ξ\xi^2<p\le\xi; since log⁡(1−u)≤−u\log(1-u)\le-u, the second sum is at most −S2-S_2, and the upper bound follows from I(N)≤I(Nκ)I(N)\le I(N_\kappa).

For the lower bound we split the second sum into three parts. For ξ2<p≤ξ\xi^2<p\le\xi, −log⁡(1−p−2)≤p−21−ξ−2-\log(1-p^{-2})\le\frac{p^{-2}}{1-\xi^{-2}}, so this part is at least −S2−2ξ2−2S2-S_2-2\xi_2^{-2}S_2. For ξ3<p≤ξ2\xi^3<p\le\xi^2, vp=2v_p=2, and by Proposition 2.9 (e), since ξ3>1418\xi^3>1418, this part is at least −11−ξ−3⋅0.086ξ2/3≥−0.0861⋅ξ−2/3-\frac{1}{1-\xi^{-3}}\cdot\frac{0.086}{\xi^{2/3}}\ge-0.0861\cdot\xi^{-2/3}. For p≤ξ3p\le\xi^3, if ξj+1<p≤ξj\xi^{j+1}<p\le\xi^j with j≥3j\ge3, then pj+1>ξj+1≥ξp^{j+1}>\xi^{j+1}\ge\xi by Proposition 3.1 (c), so −log⁡(1−p−(j+1))≤1ξj+1-\log(1-p^{-(j+1)})\le\frac{1}{\xi^{j+1}}; by Proposition 2.9 (d) and Proposition 3.1 (c), the number of such primes is at most π((3ξ)1/3)<3⋅1.26⋅31/35.4518ξ1/3\pi((3\xi)^{1/3})<\frac{3\cdot1.26\cdot3^{1/3}}{5.4518}\xi^{1/3}, so this part is at least −5.451831⋅ξ1/3ξ−1≥−0.17587⋅ξ−2/3-\frac{5.4518}{31}\cdot\frac{\xi^{1/3}}{\xi-1}\ge-0.17587\cdot\xi^{-2/3}. Together with I(N)≥ξξ+1I(Nκ)I(N)\ge\frac{\xi}{\xi+1}I(N_\kappa) and log⁡(1+1ξ)≤1ξ≤e−31/3⋅ξ−2/3\log(1+\frac{1}{\xi})\le\frac{1}{\xi}\le e^{-31/3}\cdot\xi^{-2/3},

log⁡I(N)≥∑p≤qlog⁡pp−1−S2−2ξ2−2S2−0.26201⋅ξ−2/3.\log I(N)\ge\sum_{p\le q}\log\frac{p}{p-1}-S_2-2\xi_2^{-2}S_2-0.26201\cdot\xi^{-2/3}.

Finally ξ−2/3=λ2e−λ/62⋅Mξλ\xi^{-2/3}=\frac{\lambda^2e^{-\lambda/6}}{\sqrt{2}}\cdot\frac{M_\xi}{\lambda}, and λ2e−λ/6\lambda^2e^{-\lambda/6} is decreasing for λ≥12\lambda\ge12, so 0.26201⋅ξ−2/3≤0.26201⋅312⋅e−31/62⋅Mξλ<1.0155Mξλ0.26201\cdot\xi^{-2/3}\le\frac{0.26201\cdot3^{12}\cdot e^{-31/6}}{\sqrt{2}}\cdot\frac{M_\xi}{\lambda}<\frac{1.0155M_\xi}{\lambda}, while 2ξ2−2S2≤2ξ2−2Mξ<10−4⋅Mξλ2\xi_2^{-2}S_2\le2\xi_2^{-2}M_\xi<\frac{10^{-4}\cdot M_\xi}{\lambda} by Lemma 3.2 and (2).

Proof of Theorem 1.1

Proof of Theorem 1.1. Put ξ=ξ(N)\xi=\xi(N), λ=log⁡ξ\lambda=\log\xi and u=log⁡q≥31u=\log q\ge31, so that λ≥u≥31\lambda\ge u\ge31. Since q≤ξq\le\xi and the primes p≤ξp\le\xi are the primes p≤qp\le q, we have θ(ξ)=θ(q)\theta(\xi)=\theta(q) and

Δ(N)−c(q)=(log⁡I(N)−∑p≤qlog⁡pp−1)−(L(log⁡N)−L(θ(ξ))).\Delta(N)-c(q)=\left(\log I(N)-\sum_{p\le q}\log\frac{p}{p-1}\right)-(L(\log N)-L(\theta(\xi))).

By Lemmas 3.2, 3.3 and 3.4,

−Mξ⋅(2−1.973094−1.0156λ)≤Δ(N)−c(q)≤−Mξ⋅(2−0.369659+2.43616λ),-M_{\xi}\cdot\left(2-\frac{1.973094-1.0156}{\lambda}\right)\le\Delta(N)-c(q)\le-M_{\xi}\cdot\left(2-\frac{0.369659+2.43616}{\lambda}\right),

that is,

−Mξ⋅(2−0.957494u)≤Δ(N)−c(q)≤−Mξ⋅(2−2.805819u).-M_{\xi}\cdot\left(2-\frac{0.957494}{u}\right)\le\Delta(N)-c(q)\le-M_{\xi}\cdot\left(2-\frac{2.805819}{u}\right).

Put Mq=2q uM_q=\frac{\sqrt{2}}{\sqrt{q}\,u}. The prime following qq exceeds ξ\xi, so by Proposition 2.9 (c), ξ<q⋅(1+u−3)\xi<q\cdot(1+u^{-3}) and λ<u+u−3\lambda<u+u^{-3}. Hence Mξ≤MqM_{\xi}\le M_q, 1λ≥1−u−4u\frac{1}{\lambda}\ge\frac{1-u^{-4}}{u}, and

MξMq≥1(1+u−3)1/2(1+u−4)≥1−u−2/2+u−3u≥1−0.000554u.\frac{M_{\xi}}{M_q}\ge\frac{1}{(1+u^{-3})^{1/2}(1+u^{-4})}\ge1-\frac{u^{-2}/2+u^{-3}}{u}\ge1-\frac{0.000554}{u}.

Therefore

Δ(N)−c(q)≥−Mq⋅(2−0.957494⋅(1−31−4)u)≥−Mq⋅(2−0.9574u)\Delta(N)-c(q)\ge-M_q\cdot\left(2-\frac{0.957494\cdot(1-31^{-4})}{u}\right)\ge-M_q\cdot\left(2-\frac{0.9574}{u}\right)

and

Δ(N)−c(q)≤−Mq⋅(1−0.000554u)(2−2.805819u)≤−Mq⋅(2−2.8070u).\Delta(N)-c(q)\le-M_q\cdot\left(1-\frac{0.000554}{u}\right)\left(2-\frac{2.805819}{u}\right)\le-M_q\cdot\left(2-\frac{2.8070}{u}\right).

Since 2Mq=22qlog⁡q2M_q=\frac{2\sqrt{2}}{\sqrt{q}\log q}, 0.9574⋅2>1.3530.9574\cdot\sqrt{2}>1.353 and 2.8070⋅2<3.9702.8070\cdot\sqrt{2}<3.970, the theorem follows.

In the notation of the proof, Theorem 1.1 is the pair of inequalities

c(q)−22qlog⁡q(1−0.4787log⁡q)≤Δ(N)≤c(q)−22qlog⁡q(1−1.4035log⁡q).(3)c(q)-\frac{2\sqrt{2}}{\sqrt{q}\log q}\left(1-\frac{0.4787}{\log q}\right)\le\Delta(N)\le c(q)-\frac{2\sqrt{2}}{\sqrt{q}\log q}\left(1-\frac{1.4035}{\log q}\right). \tag*{(3)}

Remark 3.5. The decomposition of Δ(N)−c(q)\Delta(N)-c(q) used in the proof of Theorem 1.1 follows Nicolas’ proof of [20] Proposition 5.1, in which log⁡(σ(N)/N)\log(\sigma(N)/N) is written as U=U1+U2+U3−U4−U5U=U_1+U_2+U_3-U_4-U_5 [20] [(5.4)], with −U5=∑p≤ξlog⁡pp−1-U_5=\sum_{p\le\xi}\log\frac{p}{p-1} the Mertens product; a comparison of σ(N)/N\sigma(N)/N with this product for colossally abundant numbers NN also underlies Robin’s proof of Proposition 2.6 [5] [Section 4]. In [20] Proposition 5.1 the Mertens product is evaluated under RH by [21] [(2.16)], that is, by Proposition 2.8. In Theorem 1.1 it is kept in the form c(q)+γ+log⁡log⁡θ(q)c(q)+\gamma+\log\log\theta(q), so that no hypothesis on the zeros of the Riemann zeta function is used, and the remaining terms are bounded from above and from below with explicit constants for every colossally abundant number with log⁡q≥31\log q\ge31.

Remark 3.6. The two bounds of Theorem 1.1 differ by 3.970−1.353qlog⁡2q\frac{3.970-1.353}{\sqrt{q}\log^2q}. Consequently, Corollaries 4.2 and 4.3 below do not decide whether Robin’s inequality holds at a colossally abundant number NN when c(q)qlog⁡q\frac{c(q)}{\sqrt{q}\log q} lies between 22qlog⁡q(1−1.4035log⁡q)\frac{2\sqrt{2}}{\sqrt{q}\log q}\left(1-\frac{1.4035}{\log q}\right) and 22qlog⁡q(1−0.4787log⁡q)\frac{2\sqrt{2}}{\sqrt{q}\log q}\left(1-\frac{0.4787}{\log q}\right). In the proof, the two sides differ by (2.805819−0.957494)⋅Mξλ=1.848325⋅Mξλ(2.805819-0.957494)\cdot\frac{M_{\xi}}{\lambda}=1.848325\cdot\frac{M_{\xi}}{\lambda}; of this, 1.01561.0156 comes from Lemma 3.4 (the primes p≤ξ2p\le\xi_2, which have exponent at least 2), 2.43616−1.920374=0.5157862.43616-1.920374=0.515786 from Lemma 3.2, and 0.369659−0.05272=0.3169390.369659-0.05272=0.316939 from Lemma 3.3.

Consequences

Lemma 4.1. Let nn be a counterexample with largest prime factor pkp_k. Then log⁡pk>31.0319\log p_k>31.0319 and log⁡log⁡n<1.000002⋅log⁡pk\log\log n<1.000002\cdot\log p_k.

Proof. Put L=log⁡log⁡nL=\log\log n and P=log⁡pkP=\log p_k. By Proposition 2.3, n>101013.11485n>10^{10^{13.11485}}, so L>13.11485⋅log⁡10+log⁡log⁡10>31.032L>13.11485\cdot\log10+\log\log10>31.032. By Proposition 2.2, eγL≤I(n)<∏p≤pkpp−1e^{\gamma L}\le I(n)<\prod_{p\le p_k}\frac{p}{p-1}. If pk<46,909,038p_k<46,909,038, then by Proposition 2.9 (f) at x=46,909,038x=46,909,038, this product is less than eγ⋅17.6638⋅1.000011<eγ⋅31.032e^\gamma\cdot17.6638\cdot1.000011<e^\gamma\cdot31.032, a contradiction. Hence pk≥46,909,038p_k\ge46,909,038, and Proposition 2.9 (f) gives L<P⋅(1−ε(P))−1L<P\cdot(1-\varepsilon(P))^{-1}. Since ε\varepsilon is decreasing and P≥log⁡(46,909,038)P\ge\log(46,909,038), (1−ε(P))−1<1.000011(1-\varepsilon(P))^{-1}<1.000011, so P>31.0321.000011>31.0316P>\frac{31.032}{1.000011}>31.0316; then (1−ε(P))−1≤(1−ε(31.0316))−1<1.000002(1-\varepsilon(P))^{-1}\le(1-\varepsilon(31.0316))^{-1}<1.000002, so L<1.000002⋅PL<1.000002\cdot P and P>31.0321.000002>31.0319P>\frac{31.032}{1.000002}>31.0319. □

For the least counterexample, the author proved log⁡pk>31.018\log p_k>31.018 [17] [Theorem 4.2]; Lemma 4.1 applies to every counterexample.

Corollary 4.2. Let NN be a colossally abundant counterexample, and qq the largest prime with q≤ξ(N)q\le\xi(N). Then log⁡q>31.0319\log q>31.0319 and

c(q)>22qlog⁡q(1−1.4035log⁡q)>2.70qlog⁡q,that is,q#φ(q#)>eγ⋅log⁡θ(q)⋅exp⁡(2.70qlog⁡q).c(q)>\frac{2\sqrt{2}}{\sqrt{q}\log q}\left(1-\frac{1.4035}{\log q}\right)>\frac{2.70}{\sqrt{q}\log q},\qquad\text{that is,}\qquad\frac{q^\#}{\varphi(q^\#)}>e^\gamma\cdot\log\theta(q)\cdot\exp\left(\frac{2.70}{\sqrt{q}\log q}\right).

Proof. The largest prime factor pkp_k of NN is at most ξ(N)\xi(N) by Proposition 3.1 (a), so pk≤qp_k\le q and log⁡q>31.0319\log q>31.0319 by Lemma 4.1. Since Robin’s inequality fails for NN, Δ(N)≥0\Delta(N)\ge0, and the upper bound in (3) gives the first inequality. The function u↦22(1−1.4035u)u\mapsto2\sqrt{2}\left(1-\frac{1.4035}{u}\right) is increasing, and its value at u=31.0319u=31.0319 exceeds 2.702.70. □

Corollary 4.3. Let qq be a prime with log⁡q≥31\log q\ge31 and

c(q)>22qlog⁡q(1−0.4787log⁡q).c(q)>\frac{2\sqrt{2}}{\sqrt{q}\log q}\left(1-\frac{0.4787}{\log q}\right).

Then every colossally abundant number NN such that qq is the largest prime with q≤ξ(N)q\le\xi(N) is a counterexample. In particular, the colossally abundant number NF(q,1)N_{F(q,1)} of Proposition 3.1 (a), for which ξ=q\xi=q, is a counterexample.

Proof. The lower bound in (3) gives Δ(N)>0\Delta(N)>0, that is, I(N)>eγlog⁡log⁡NI(N)>e^\gamma\log\log N, and N>5040N>5040 because qq divides NκN_\kappa and log⁡N≥θ(q)−log⁡q\log N\ge\theta(q)-\log q by Proposition 3.1 (b). For κ=F(q,1)\kappa=F(q,1), the number NκN_\kappa is colossally abundant with largest parameter κ\kappa by Proposition 3.1 (a), and ξ(Nκ)=q\xi(N_\kappa)=q because F(⋅,1)F(\cdot,1) is decreasing. □

By Corollaries 4.2 and 4.3, for colossally abundant numbers NN with log⁡q≥31\log q\ge31, Robin’s inequality fails at NN when c(q)qlog⁡q>22(1−0.4787log⁡q)c(q)\sqrt{q}\log q>2\sqrt{2}\left(1-\frac{0.4787}{\log q}\right) and holds at NN when c(q)qlog⁡q<22(1−1.4035log⁡q)c(q)\sqrt{q}\log q<2\sqrt{2}\left(1-\frac{1.4035}{\log q}\right).

Corollary 4.4. Proposition 2.7 and Corollary 4.3 imply Proposition 2.6: if the Riemann Hypothesis is false, then Robin’s inequality fails for infinitely many colossally abundant numbers.

Proof. If RH is false, Proposition 2.7 gives b<12b<\frac12 and C>0C>0 such that c(x)>Cx−bc(x)>Cx^{-b} for arbitrarily large xx. Let qq be the largest prime with q≤xq\le x; then c(q)=c(x)c(q)=c(x) and q>x2q>\frac{x}{2}, so c(q)>Cx−b>4xlog⁡(x/2)>22qlog⁡qc(q)>Cx^{-b}>\frac{4}{\sqrt{x\log(x/2)}}>\frac{2\sqrt{2}}{\sqrt{q}\log q} for all sufficiently large such xx. Corollary 4.3 gives a colossally abundant counterexample NF(q,1)N_{F(q,1)} for each such qq with log⁡q≥31\log q\ge31, and these numbers are distinct because ξ(NF(q,1))=q\xi(N_{F(q,1)})=q. □

Remark 4.5. Corollary 4.4 recovers Proposition 2.6 of Robin [5], here obtained from Proposition 2.7. Corollary 4.6 below is an explicit inequality, for colossally abundant numbers with log⁡q≥31\log q\ge31, of the type of Ramanujan’s upper bound for σ(n)/n\sigma(n)/n under RH, of which [20] [Theorem 1.1] gives an effective form for every n≥2n\ge2.

Corollary 4.6. Assume the Riemann Hypothesis. Let NN be a colossally abundant number, and qq the largest prime with q≤ξ(N)q\le\xi(N). If log⁡q≥31\log q\ge31, then

Δ(N)<−0.654qlog⁡q,that is,σ(N)N<eγ⋅log⁡log⁡N⋅exp⁡(−0.654qlog⁡q).\Delta(N)<-\frac{0.654}{\sqrt{q}\log q},\qquad\text{that is,}\qquad\frac{\sigma(N)}{N}<e^\gamma\cdot\log\log N\cdot\exp\left(-\frac{0.654}{\sqrt{q}\log q}\right).

Proof. By (3) and Proposition 2.8, since q>109q > 10^{9},

Δ(N)qlog⁡q<2+τ−22+22⋅1.4035log⁡q≤2+τ−22+22⋅1.403531<−0.654.\Delta(N)\sqrt{q}\log q < 2+\tau-2\sqrt{2}+\frac{2\sqrt{2}\cdot1.4035}{\log q}\le2+\tau-2\sqrt{2}+\frac{2\sqrt{2}\cdot1.4035}{31}<-0.654.

The number 22−2−τ=2(2−1)−τ=0.7822…2\sqrt{2}-2-\tau=2(\sqrt{2}-1)-\tau=0.7822\ldots appearing in the proof is the constant obtained from Ramanujan’s bound [19] together with ∣S1(x)∣≤τx|S_1(x)|\le\frac{\tau}{\sqrt{x}}, as in [20] [(1.8)]; here qlog⁡q\sqrt{q}\log q plays the role of log⁡N⋅log⁡log⁡N\sqrt{\log N\cdot\log\log N}, since log⁡N=q⋅(1+o(1))\log N=q\cdot(1+o(1)) by the proof of Lemma 3.3 and Proposition 2.9 (c).

Corollary 4.7. The Riemann Hypothesis is true if and only if

q#φ(q#)<eγ⋅log⁡ϑ(q)⋅exp⁡(2.70qlog⁡q)\frac{q\#}{\varphi(q\#)}<e^\gamma\cdot\log\vartheta(q)\cdot\exp\left(\frac{2.70}{\sqrt{q}\log q}\right)

for every prime q≥109q\ge10^{9}.

Proof. The inequality is c(q)<2.70qlog⁡qc(q)<\frac{2.70}{\sqrt{q}\log q}. If RH is true, it holds for every prime q≥109q\ge10^{9} by Proposition 2.8. If RH is false, Proposition 2.6 gives a colossally abundant counterexample, and Corollary 4.2 gives a prime qq with log⁡q>31.0319\log q>31.0319, so q>109q>10^{9}, and c(q)>2.70qlog⁡qc(q)>\frac{2.70}{\sqrt{q}\log q}.

By Propositions 2.7 and 2.8, the equivalence of Corollary 4.7 also holds with 2.70 replaced by any constant greater than 2+τ2+\tau. Corollary 4.2 identifies primes that violate it: the primes qq attached to colossally abundant counterexamples.

Superabundant Counterexamples

Lemma 5.1. Let n=∏i=1kpiain=\prod_{i=1}^{k}p_i^{a_i} be a superabundant number with largest prime factor pkp_k. Then ai≥⌈log⁡pklog⁡pi⌉a_i\ge\left\lceil\frac{\log p_k}{\log p_i}\right\rceil for every 1≤i≤k1\le i\le k, and consequently log⁡n≥ψ(pk)\log n\ge\psi(p_k).

Proof. The first claim is due to Nazardonyavi and Yakubovich [16]; we give the proof for completeness. For a prime pp and an integer b≥0b\ge0 put g(p,b)=∑j=0bp−jg(p,b)=\sum_{j=0}^{b}p^{-j}. For i=ki=k the claim is ak≥1a_k\ge1. Let i<ki<k, write q=piq=p_i and a=ai≥1a=a_i\ge1, and suppose that a≤⌊log⁡pklog⁡q⌋−1a\le\left\lfloor\frac{\log p_k}{\log q}\right\rfloor-1. Then qa+1≤pkq^{a+1}\le p_k, and since qa+1≠pkq^{a+1}\ne p_k, we have qa+1<pkq^{a+1}<p_k. Put m=nqapkm=\frac{nq^a}{p_k}, which is an integer with m<nm<n, and write b=ak≥1b=a_k\ge1. Since II is multiplicative,

I(n)I(m)=g(q,a)g(q,2a+1)⋅g(pk,b)g(pk,b−1)=1+pk−b/g(pk,b−1)1+q−(a+1)≤1+1pk1+1qa+1<1.\frac{I(n)}{I(m)}=\frac{g(q,a)}{g(q,2a+1)}\cdot\frac{g(p_k,b)}{g(p_k,b-1)} =\frac{1+p_k^{-b}/g(p_k,b-1)}{1+q^{-(a+1)}}\le\frac{1+\frac{1}{p_k}}{1+\frac{1}{q^{a+1}}}<1.

where we used g(q,2a+1)=g(q,a)⋅(1+q−(a+1))g(q,2a+1)=g(q,a)\cdot(1+q^{-(a+1)}), g(pk,b−1)≥1g(p_k,b-1)\ge1 and qa+1<pkq^{a+1}<p_k. Thus I(m)>I(n)I(m)>I(n) with m<nm<n, which contradicts the superabundance of nn. Finally, by Proposition 2.4 the primes dividing nn are exactly the primes q≤pkq\le p_k, so

log⁡n=∑q≤pkaqlog⁡q≥∑q≤pk⌈log⁡pklog⁡q⌉log⁡q=ψ(pk),\log n=\sum_{q\le p_k}a_q\log q\ge\sum_{q\le p_k}\left\lceil\frac{\log p_k}{\log q}\right\rceil\log q=\psi(p_k),

where aqa_q denotes the exponent of qq in nn.

Lemma 5.2. Let nn be a counterexample, and n′n' the product of the distinct primes dividing nn. Then n′>15n'>15 and

log⁡n′φ(n′)−γ−log⁡log⁡log⁡n′>log⁡log⁡log⁡n−log⁡log⁡log⁡n′≥0.\log\frac{n'}{\varphi(n')}-\gamma-\log\log\log n'>\log\log\log n-\log\log\log n'\ge0.

Proof. By Proposition 2.2, and since Robin’s inequality fails for nn, n′φ(n′)>I(n)≥eγ⋅log⁡log⁡n\frac{n'}{\varphi(n')}>I(n)\ge e^\gamma\cdot\log\log n. By Proposition 2.3, log⁡log⁡n>31.032\log\log n>31.032, so n′φ(n′)>55\frac{n'}{\varphi(n')}>55. Since mφ(m)≤3\frac{m}{\varphi(m)}\le3 for every m≤15m\le15, we get n′>15n'>15, hence log⁡log⁡n′>0\log\log n'>0. Taking logarithms gives log⁡n′φ(n′)≥γ+log⁡log⁡log⁡n\log\frac{n'}{\varphi(n')}\ge\gamma+\log\log\log n, and subtracting log⁡log⁡log⁡n′\log\log\log n' gives the first inequality. The second follows from n≥n′n\ge n'.

For a superabundant counterexample with largest prime factor pkp_k, Proposition 2.4 gives n′=pk#n'=p_k\#, so Lemma 5.2 gives

c(pk)>log⁡log⁡log⁡n−log⁡log⁡θ(pk)≥0.(4)c(p_k)>\log\log\log n-\log\log\theta(p_k)\ge0. \tag*{(4)}

Lemma 5.3. Let nn be a superabundant counterexample with largest prime factor pkp_k. Then log⁡log⁡n<log⁡pk+0.0562log⁡2pk\log\log n<\log p_k+\frac{0.0562}{\log^2 p_k} and log⁡n⋅log⁡log⁡n<1.0000603⋅pk⋅log⁡pk\log n\cdot\log\log n<1.0000603\cdot p_k\cdot\log p_k.

Proof. Put P=log⁡pkP=\log p_k and L=log⁡log⁡nL=\log\log n. By Lemma 4.1, P>31.0319P>31.0319, and by Propositions 2.2 and 2.9 (f), eγL≤I(n)<eγP⋅(1−ε(P))−1e^\gamma L\le I(n)<e^{\gamma}P\cdot(1-\varepsilon(P))^{-1}. Hence

L−P<P⋅ε(P)1−ε(P)=1P2⋅120+316P1−ε(P)≤1P2⋅120+316⋅31.03191−ε(31.0319)<0.0562P2.L-P<\frac{P\cdot\varepsilon(P)}{1-\varepsilon(P)} =\frac{1}{P^2}\cdot\frac{\frac{1}{20}+\frac{3}{16P}}{1-\varepsilon(P)} \le\frac{1}{P^2}\cdot\frac{\frac{1}{20}+\frac{3}{16\cdot31.0319}}{1-\varepsilon(31.0319)} <\frac{0.0562}{P^2}.

Therefore log⁡n<pk⋅e0.0562/P2\log n<p_k\cdot e^{0.0562/P^2} and L<P⋅(1+0.0562P3)L<P\cdot\left(1+\frac{0.0562}{P^3}\right), so that

log⁡n⋅log⁡log⁡n<pk⋅P⋅e0.056231.032⋅(1+0.056231.033)<1.0000603⋅pk⋅P.\log n\cdot\log\log n<p_k\cdot P\cdot e^{\frac{0.0562}{31.032}}\cdot\left(1+\frac{0.0562}{31.033}\right)<1.0000603\cdot p_k\cdot P.

Theorem 5.4. Let nn be a superabundant counterexample with largest prime factor pkp_k. Then

c(pk)>log⁡log⁡ψ(pk)−log⁡log⁡θ(pk)>0.9991pk⋅log⁡pk.c(p_k)>\log\log\psi(p_k)-\log\log\theta(p_k)>\frac{0.9991}{\sqrt{p_k}\cdot\log p_k}.

Proof. By (4) and Lemma 5.1, c(pk)>log⁡log⁡log⁡n−log⁡log⁡θ(pk)≥log⁡log⁡ψ(pk)−log⁡log⁡θ(pk)c(p_k)>\log\log\log n-\log\log\theta(p_k)\ge\log\log\psi(p_k)-\log\log\theta(p_k). The function t↦log⁡log⁡tt\mapsto\log\log t has the decreasing derivative 1tlog⁡t\frac{1}{t\log t} for t>1t>1, and θ(pk)<θ(pk)+θ(pk)≤ψ(pk)≤log⁡n\theta(p_k)<\theta(p_k)+\theta(\sqrt{p_k})\le\psi(p_k)\le\log n. By the mean value theorem and Lemma 5.3,

log⁡log⁡ψ(pk)−log⁡log⁡θ(pk)≥ψ(pk)−θ(pk)ψ(pk)⋅log⁡ψ(pk)≥θ(pk)log⁡n⋅log⁡log⁡n>θ(pk)1.0000603⋅pk⋅log⁡pk.\log\log\psi(p_k)-\log\log\theta(p_k)\ge\frac{\psi(p_k)-\theta(p_k)}{\psi(p_k)\cdot\log\psi(p_k)}\ge\frac{\theta(\sqrt{p_k})}{\log n\cdot\log\log n}>\frac{\theta(\sqrt{p_k})}{1.0000603\cdot p_k\cdot\log p_k}.

By Lemma 4.1, pk>e15.515>5.47⋅106\sqrt{p_k}>e^{15.515}>5.47\cdot10^6, so Proposition 2.9 (a) gives θ(pk)>(1−1.945.47⋅106)pk>0.99917⋅pk\theta(\sqrt{p_k})>\left(1-\frac{1.94}{\sqrt{5.47\cdot10^6}}\right)\sqrt{p_k}>0.99917\cdot\sqrt{p_k} if pk≤1019\sqrt{p_k}\le10^{19}, and Proposition 2.9 (b) gives θ(pk)>(1−0.000012)pk\theta(\sqrt{p_k})>(1-0.000012)\sqrt{p_k} otherwise. Since 0.999171.0000603>0.9991\frac{0.99917}{1.0000603}>0.9991, the second inequality follows.

Corollary 5.5. Suppose that the Riemann Hypothesis is false, and let nn be the least counterexample. Let N′<NN'<N be the consecutive colossally abundant numbers with N′<n≤NN'<n\le N. Then NN is a counterexample,

log⁡N−log⁡ξ(N)≤log⁡N′<log⁡n≤log⁡N,\log N-\log\xi(N)\le\log N'<\log n\le\log N,

and the largest prime q≤ξ(N)q\le\xi(N) satisfies c(q)>2.70qlog⁡qc(q)>\frac{2.70}{\sqrt{q}\log q}.

Proof. By Proposition 3.1 (f) applied to m=nm=n, the consecutive colossally abundant numbers N′<n≤NN'<n\le N satisfy Nξ(N)≤N′\frac{N}{\xi(N)}\le N', which gives the displayed inequalities. The number 55440 is colossally abundant [20] [Figure 1], and 55440 <n<n by Proposition 2.3, so N′≥55440>5040N'\ge55440>5040. Since N′<nN'<n, Robin’s inequality holds for N′N', that is, I(N′)log⁡log⁡N′<eγ\frac{I(N')}{\log\log N'}<e^\gamma, whereas I(n)log⁡log⁡n≥eγ\frac{I(n)}{\log\log n}\ge e^\gamma. By Proposition 3.1 (g), I(N)log⁡log⁡N≥I(n)log⁡log⁡n≥eγ\frac{I(N)}{\log\log N}\ge\frac{I(n)}{\log\log n}\ge e^\gamma, and N≥n>5040N\ge n>5040, so NN is a counterexample. The last claim is Corollary 4.2.

Experimental Verification

Every numerical inequality between explicit constants used in this paper was checked by a self-contained Python 3.12 script, verify_robin_nicolas.py, written with the help of Claude Opus 5.5 (Anthropic) and run by the author, as in the earlier version of this work. The script uses the arbitrary-precision library mpmath with 60 significant decimal digits, and exact rational arithmetic (Python’s fractions module) for the inequalities that involve only decimal constants, some of which hold with equality. For each inequality it prints the computed value of its left-hand side. The script has three parts, and all 69 checks performed by the script passed: 14 in Part 1, 50 in Part 2 and 5 in Part 3. We now describe the output.

Part 1: Counterexamples

Part 1 checks the constants of Lemmas 4.1, 5.2 and 5.3 and of Theorem 5.4. The computed values are listed in Table 1.

QuantityComputed valueBound used
log⁡log⁡(101013.11485)\log\log(10^{10^{13.11485}})31.0320905521…>31.032> 31.032
log⁡(46,909,038)\log(46{,}909{,}038)17.6637209227…<17.6638< 17.6638
(1−ε(log⁡46,909,038))−1(1-\varepsilon(\log46{,}909{,}038))^{-1}1.0000109986…<1.000011< 1.000011
31.032/1.00001131.032/1.00001131.0316586518…>31.0316> 31.0316
(1−ε(31.0316))−1(1-\varepsilon(31.0316))^{-1}1.0000018754…<1.000002< 1.000002
31.032/1.00000231.032/1.00000231.0319379361…>31.0319> 31.0319
(120+16⋅31.031920)/(1−ε(31.0319))\left(\frac{1}{20}+\frac{16\cdot31.0319}{20}\right)/(1-\varepsilon(31.0319))0.0560422746…<0.0562< 0.0562
e0.0562/31.032(1+0.056231.032)e^{0.0562/31.032}\left(1+\frac{0.0562}{31.03^2}\right)1.0000602505…<1.0000603< 1.0000603
e15.515e^{15.515}5471153.3376…>5.47⋅106> 5.47\cdot10^6
1−1.94/5.47⋅1061-1.94/\sqrt{5.47\cdot10^6}0.9991705159…>0.99917> 0.99917
0.99917/1.00006030.99917/1.00006030.9991097537…>0.9991> 0.9991
eγ⋅31.032e^\gamma\cdot31.03255.2702392751…>55> 55
max⁡m≤15m/φ(m)\max_{m\le15}m/\varphi(m)3=3=3

Table 1. Values computed in Part 1 of the script.

The starting point is log⁡log⁡(101013.11485)=31.0320905…\log\log(10^{10^{13.11485}}) = 31.0320905\ldots, the bound for log⁡log⁡n\log\log n coming from Proposition 2.3. At x=46,909,038x = 46{,}909{,}038, where Proposition 2.9 (f) begins to apply, log⁡x=17.6637…\log x = 17.6637\ldots and (1−ε(log⁡x))−1=1.0000109986…(1-\varepsilon(\log x))^{-1} = 1.0000109986\ldots, which lies below 1.000011 by 1.4⋅10−91.4 \cdot10^{-9}; this is the smallest margin in Part 1. The two steps of Lemma 4.1 give 31.0321.000011=31.03165…\frac{31.032}{1.000011} = 31.03165\ldots and 31.0321.000002=31.031937…\frac{31.032}{1.000002} = 31.031937\ldots. In Lemma 5.3, the constant 0.0562 exceeds the computed value 0.0560422…, and the factor 1.0000603 exceeds the computed value 1.0000602505… by 4.9⋅10−84.9 \cdot10^{-8}.

Part 2: The Proof of Theorem 1.1

Part 2 checks the constants of Lemmas 2.10, 3.2, 3.3 and 3.4 and of the proof of Theorem 1.1, all at the threshold λ=31\lambda= 31, where e31=29048849665247.4…e^{31} = 29048849665247.4\ldots; each quantity checked at λ=31\lambda= 31 is monotone in λ\lambda in the direction stated in the proofs. Table 2 lists the main values. In Lemma 2.10 (b), the relative error 0.022λ\frac{0.022}{\lambda} for θ(t)\theta(t) on t≥ξ2t\ge\xi_2 comes from Büthe’s bound, with computed value 0.0219063… at λ=31\lambda=31, whereas Dusart’s bound contributes at most 0.00105. In Lemma 3.3, the contribution 1.397905⋅31⋅e−31/6=0.2471636…1.397905\cdot31\cdot e^{-31/6}=0.2471636\ldots of the primes with exponent at least 3 reduces the coefficient 0.301 coming from ξ2\xi_2 to 0.0538. In Lemma 3.4, the primes with exponent 2 and those with exponent at least 3 contribute 0.262002530…⋅ξ−2/30.262002530\ldots\cdot\xi^{-2/3}, which is 1.0154801…⋅Mξλ1.0154801\ldots\cdot\frac{M_\xi}{\lambda} at λ=31\lambda=31. Twelve of the checks in Part 2 are identities or inequalities between the decimal constants of the proofs, such as 0.066+0.370148+2=2.4361480.066+0.370148+2=2.436148 and 0.313233−0.066+1.9314−0.258259=1.9203740.313233-0.066+1.9314-0.258259=1.920374; they are verified in exact rational arithmetic. The smallest positive margins in Part 2 are those of 1312+1313=0.000553858…<0.000554\frac{1}{31^2}+\frac{1}{31^3}=0.000553858\ldots<0.000554, of 2(log⁡22−0.011306)=0.6705351805…≥0.6705352\left(\frac{\log2}{2}-0.011306\right)=0.6705351805\ldots\ge0.670535, and of 2(1−0.370148+18312)=1.9314003…>1.93142\left(1-\frac{0.370148+18}{31^2}\right)=1.9314003\ldots>1.9314, with differences 1.4⋅10−71.4\cdot10^{-7}, 1.8⋅10−71.8\cdot10^{-7} and 3.1⋅10−73.1\cdot10^{-7}. The final constants of Theorem 1.1 are 0.9574⋅2=1.3539680…>1.3530.9574\cdot\sqrt{2}=1.3539680\ldots>1.353 and 2.8070⋅2=3.9696974…<3.9702.8070\cdot\sqrt{2}=3.9696974\ldots<3.970.

QuantityComputed valueBound used
1−log⁡2621-\frac{\log2}{62}0.9888202067 . . .>0.98882>0.98882
1.94⋅31⋅e−31/4/1.182531.94\cdot31\cdot e^{-31/4}/1.182530.0219062995 . . .<0.022<0.022
−log⁡(1−log⁡262)-\log\left(1-\frac{\log2}{62}\right)0.0112427568 . . .<0.011306<0.011306
0.670535−log⁡22−log⁡262⋅0.670535310.670535-\frac{\log2}{2}-\frac{\log2}{62}\cdot\frac{0.670535}{31}0.3164649670 . . .>0.316464>0.316464
0.316464−0.3164642310.316464-\frac{0.316464^2}{31}0.3132333721 . . .>0.313233>0.313233
2(1−0.370148+log⁡231)2\left(1-\frac{0.370148+\log2}{31}\right)1.9314003109 . . .>1.9314>1.9314
1.0022⋅31⋅e−31/2/21.0022\cdot31\cdot e^{-31/2}/\sqrt{2}4.0760229901…⋅10−64.0760229901\ldots\cdot10^{-6}<4.08⋅10−6<4.08\cdot10^{-6}
1.397905⋅31⋅e−31/61.397905\cdot31\cdot e^{-31/6}0.2471636095 . . .<0.24717<0.24717
1312+2⋅31⋅e−31/2\frac{1}{31^2}+\sqrt{2}\cdot31\cdot e^{-31/2}0.0010487169 . . .<0.0010488<0.0010488
0.0861+0.17587+e−31/30.0861+0.17587+e^{-31/3}0.2620025305 . . .<0.26201<0.26201
0.26201⋅312⋅e−31/6/20.26201\cdot31^2\cdot e^{-31/6}/\sqrt{2}1.0154801390 . . .<1.0155<1.0155
12⋅312+1313\frac{1}{2\cdot31^2}+\frac{1}{31^3}0.0005538585 . . .<0.000554<0.000554
0.957494⋅(1−31−4)0.957494\cdot(1-31^{-4})0.9574929632 . . .>0.9574>0.9574
0.9574⋅20.9574\cdot\sqrt{2}1.3539680646 . . .>1.353>1.353
2.8070⋅22.8070\cdot\sqrt{2}3.9696974696 . . .<3.970<3.970

Table 2. Values computed in Part 2 of the script, at λ=31\lambda=31.

Part 3: The Corollaries

Part 3 checks the constants of Proposition 2.8 and Corollaries 4.2, 4.6 and 4.7. The script computes τ=2+γ−log⁡(4π)=0.0461914179…\tau=2+\gamma-\log(4\pi)=0.0461914179\ldots, so that 2+τ=2.0461914179…<2.04622+\tau=2.0461914179\ldots<2.0462, and 22−2−τ=0.7822357068…2\sqrt{2}-2-\tau=0.7822357068\ldots, the constant discussed after Corollary 4.6. The constant of Corollary 4.2 is 22(1−1.403531.0319)=2.7005040047…>2.702\sqrt{2}\left(1-\frac{1.4035}{31.0319}\right)=2.7005040047\ldots>2.70, and the constant of Corollary 4.6 is 2+τ−22+22⋅1.403531=−0.654180497…<−0.6542+\tau-2\sqrt{2}+\frac{2\sqrt{2}\cdot1.4035}{31}=-0.654180497\ldots<-0.654. The constant 2.70 of Corollary 4.7 exceeds the bound 2.0462 of Proposition 2.8 by 0.6538. Finally, e31.0319=2.999…⋅1013>109e^{31.0319}=2.999\ldots\cdot10^{13}>10^9, so the primes qq of Corollary 4.2 lie in the range of Proposition 2.8.

Statements and Declarations

Declaration of interests

The author declares no competing interests.

Funding sources

This research did not receive any specific grant from funding agencies in the public, commercial, or not-for-profit sectors.

Declaration of generative AI in scientific writing

The author used Claude Opus 5.5 to write the verification script verify_robin_nicolas.py of § 6 and to generate parts of the text of this manuscript. The experiments were run by the author. After using this tool, the author reviewed and edited the code and the content as needed and takes full responsibility for the content of the publication.

Data availability

The Python script verify_robin_nicolas.py used in § 6 is available in the preprint.

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