Sum of Divisors of the Primorial and Sum of Squarefree Parts

Total Page:16

File Type:pdf, Size:1020Kb

Sum of Divisors of the Primorial and Sum of Squarefree Parts International Mathematical Forum, Vol. 12, 2017, no. 7, 331 - 338 HIKARI Ltd, www.m-hikari.com https://doi.org/10.12988/imf.2017.7113 Two Topics in Number Theory: Sum of Divisors of the Primorial and Sum of Squarefree Parts Rafael Jakimczuk Divisi´onMatem´atica,Universidad Nacional de Luj´an Buenos Aires, Argentina Copyright c 2017 Rafael Jakimczuk. This article is distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduc- tion in any medium, provided the original work is properly cited. Abstract Let pn be the n-th prime and σ(n) the sum of the positive divisors of n. Let us consider the primorial Pn = p1:p2 : : : pn, the sum of its Qn positive divisors is σ(Pn) = i=1(1 + pi). In the first section we prove the following asymptotic formula n 6 σ(P ) = Y(1 + p ) = eγ P log p + O (P ) : n i π2 n n n i=1 Let a(k) be the squarefree part of k, in the second section we prove the formula π2 X a(k) = x2 + o(x2): 30 1≤k≤x We also study integers with restricted squarefree parts and generalize these results to s-th free parts. Mathematics Subject Classification: 11A99, 11B99 Keywords: Primorial, divisors, squarefree parts, s-th free parts, average of arithmetical functions 332 Rafael Jakimczuk 1 Sum of Divisors of the Primorial In this section p denotes a positive prime and pn denotes the n-th prime. The following Mertens's formulae are well-known (see [5, Chapter VI]) 1 1 ! X = log log x + M + O ; (1) p≤x p log x where M is called Mertens's constant. 1! 1 ! X log 1 − = − log log x − γ + O ; (2) p≤x p log x where γ is the Euler's constant. ! −γ ! Y 1 e 1 1 − = + O 2 ; (3) p≤x p log x log x 0 1 Y 1 γ @ 1 A = e log x + O(1): (4) p≤x 1 − p Note that equation (4) is an immediate consequence of (3) if we use the formula 1 = 1 − x(1 + o(1)) (x ! 0); 1 + x since then 1 1 ! = 1 + O : 1 log x 1 + O log x P 1 Q 1 In this section we examine the sum p≤x log 1 + p and the product p≤x 1 + p . Then, we apply the results to the sum of the divisors of the primorial. Our main theorem is the following. Theorem 1.1 The following asymptotic formulae hold. ! ! X 1 6 1 log 1 + = log log x + γ + log 2 + O ; (5) p≤x p π log x ! Y 1 6 γ 1 + = 2 e log x + O(1): (6) p≤x p π Two topics in number theory: The primorial and squarefree parts 333 Proof. If we consider the formula ex = 1 + x(1 + o(1)) (x ! 0) then equation (6) is an immediate consequence of equation (5). Since we have 1 !! 1 ! exp O = 1 + O : log x log x Therefore we have that to prove equation (5). We have the equation 1 log(1 + x) = x − x2(1 + o(1)) (x ! 0) 2 Consequently ! X 1 X 1 1 X 1 + o(1) log 1 + = − 2 : (7) p≤x p p≤x p 2 p≤x p Now, we have X 1 + o(1) X 1 + o(1) X 1 + o(1) X 1 + o(1) 1 2 = 2 − 2 = 2 + O (8) p≤x p p p p>x p p p x Note that we have used the well-known formula (see [1, Chapter 3]) X 1 1 2 = O ; n>x n x where n denotes a positive integer. Substituting (1) and (8) into (7) we obtain almost (5) 1! 1 ! X log 1 + = log log x + C + O ; p≤x p log x where C is a constant. Therefore we have almost (6) 1! Y 1 + = eC log x + O(1): p≤x p It is well-known the limit (Euler's product formula)(see [1, Chapter 11]) n 1 ! 6 lim Y 1 − = : (9) n!1 2 2 i=1 pi π π2 Note that ζ(2) = 6 , where ζ(s) denotes the Riemann zeta function. Equations C 6 γ (3) and (9) give e = π2 e . The theorem is proved. 334 Rafael Jakimczuk Theorem 1.2 Let us consider the primorial Pn = p1:p2 : : : pn, the sum of Qn its positive divisors is σ(Pn) = i=1(1 + pi). We have the following asymptotic formula n Y 6 γ σ(Pn) = (1 + pi) = 2 e (p1:p2 : : : pn) log pn + O ((p1:p2 : : : pn)) i=1 π 6 = eγP log p + O(P ) (10) π2 n n n Note that the primorial Pn = p1:p2 : : : pn is its greatest divisor. Proof. Put x = pn in equation (6). The theorem is proved. It is well-known (see [2, Chapter XVIII]) that σ(n) lim sup = eγ: n log log n We have Theorem 1.3 The following limit holds σ(P ) 6 lim n = eγ: (11) n!1 2 Pn log log Pn π (1+o(1))pn Proof. It is well-known that Pn = e , therefore log log Pn ∼ log pn. Now, limit (11) is an immediate consequence of (10). The theorem is proved. 2 Sum of Squarefree Parts and Generalization Every positive integer k can be written in the form k = q:n2 where q is a squarefree or quadratfrei number and n2 is the greatest square that divides k. The positive integer q is called the squarefree part of k and it is denoted a(k) (see [6]). Therefore if k is a square we have a(k) = 1, in contrary case a(k) is the product of primes which have odd exponent in the prime factorization of k. For exampe, if k = 24:53:112:235 then a(k) = 5:23. If q is relatively prime with n in the decomposition k = q:n2, that is (q; n2) = 1, we shall call q the relatively prime squarefree part of k and will be denoted a0(k), besides we shall say that k has a relatively prime squarefree part. The average of the arithmetic function a(k) is studied in the following theorem. Two topics in number theory: The primorial and squarefree parts 335 Theorem 2.1 The following formula holds π2 X a(k) = x2 + o(x2): (12) 1≤k≤x 30 Proof. The number of squarefree integers q not exceeding x (denoted Q(x)) is well-known (see either [2, Chapter XVIII] or [4]). We have 1 Q(x) = X 1 = x + o(x); (13) q≤x ζ(2) where ζ(s) denotes the Riemann zeta function. From here, we can obtain easily (see [2, Chapter XXII]) that X 1 2 2 Q1(x) = q = x + o(x ): (14) q≤x 2ζ(2) Let us consider the set Sn such that x S = q : q ≤ (15) n n2 Let us consider > 0. We choose the positive integer N such that 1 1 < (16) ζ(2) (N + 1)2 and 1 X 1 4 < (17) 2ζ(2) n≥N+1 n Besides, for sake of simplicity, we put 0 1 B(x) = X B X qC : (18) p @ A N+1≤n≤ x q≤ x n2 Now, we have (see (14), (15) and (18)) 0 1 0 1 0 1 N X X X X B X C X B X C a(k) = @ qA = @ qA = @ qA + B(x) p x x 1≤k≤x n2≤x qSn n≤ x q≤ n=1 q≤ n2 n2 N N ! X x 1 2 X 1 2 = Q1 2 + B(x) = x 4 + o(x ) + B(x) n=1 n 2ζ(2) n=1 n 2 ζ(4) 2 x X 1 2 = x − 4 + o(1)x + B(x) 2ζ(2) 2ζ(2) n≥N+1 n 336 Rafael Jakimczuk That is P 1≤k≤x a(k) ζ(4) 1 X 1 B(x) 2 − = − 4 + o(1) + 2 (19) x 2ζ(2) 2ζ(2) n≥N+1 n x n x o 2 Note that SN+1 [ SN [ SN−1 [ · · · ⊆ q : q ≤ (N+1)2 . Besides, since qn ≤ x, the number of sets Si such that qSi is less than or equal to the number of j x k multiples of q not exceeding x, namely q , where b:c denotes the integer part function. Hence (see (13) and (16)) 0 1 $x% X B X C X X 0 ≤ B(x) = @ qA ≤ q ≤ x 1 p x x q x N+1≤n≤ x q≤ q≤ q≤ n2 (N+1)2 (N+1)2 x ! 1 1 ! = xQ = + o(1) x2 ≤ 2x2 (N + 1)2 ζ(2) (N + 1)2 That is, B(x) 0 ≤ ≤ 2. (20) x2 Therefore (see (19), (17) and (20)) we have P a(k) ζ(4) 1≤k≤x − ≤ 4. (21) x2 2ζ(2) Consequently equation (12) is proved, since can be arbitrarily small, ζ(2) = π2 π4 6 and ζ(4) = 90 (see [2, Chapter XVII]). The theorem is proved. In the following theorem we examine the sum X a0(k); k≤x where the sum run on the k that have a relatively prime squarefree part. Suppose that the prime factorization of n2 is 2 h1 h2 hs n = p1 p2 ··· ps ; where p1; p2; : : : ; ps are the different primes in the prime factorization and h1; h2; : : : ; hs are the even exponents. We put 0 n = p1p2 ··· ps 00 n = (p1 + 1)(p2 + 1) ··· (ps + 1) Two topics in number theory: The primorial and squarefree parts 337 If n2 = 1 then we put n0 = n00 = 1.
Recommended publications
  • On the First Occurrences of Gaps Between Primes in a Residue Class
    On the First Occurrences of Gaps Between Primes in a Residue Class Alexei Kourbatov JavaScripter.net Redmond, WA 98052 USA [email protected] Marek Wolf Faculty of Mathematics and Natural Sciences Cardinal Stefan Wyszy´nski University Warsaw, PL-01-938 Poland [email protected] To the memory of Professor Thomas R. Nicely (1943–2019) Abstract We study the first occurrences of gaps between primes in the arithmetic progression (P): r, r + q, r + 2q, r + 3q,..., where q and r are coprime integers, q > r 1. ≥ The growth trend and distribution of the first-occurrence gap sizes are similar to those arXiv:2002.02115v4 [math.NT] 20 Oct 2020 of maximal gaps between primes in (P). The histograms of first-occurrence gap sizes, after appropriate rescaling, are well approximated by the Gumbel extreme value dis- tribution. Computations suggest that first-occurrence gaps are much more numerous than maximal gaps: there are O(log2 x) first-occurrence gaps between primes in (P) below x, while the number of maximal gaps is only O(log x). We explore the con- nection between the asymptotic density of gaps of a given size and the corresponding generalization of Brun’s constant. For the first occurrence of gap d in (P), we expect the end-of-gap prime p √d exp( d/ϕ(q)) infinitely often. Finally, we study the gap ≍ size as a function of its index in thep sequence of first-occurrence gaps. 1 1 Introduction Let pn be the n-th prime number, and consider the difference between successive primes, called a prime gap: pn+1 pn.
    [Show full text]
  • Ramanujan, Robin, Highly Composite Numbers, and the Riemann Hypothesis
    Contemporary Mathematics Volume 627, 2014 http://dx.doi.org/10.1090/conm/627/12539 Ramanujan, Robin, highly composite numbers, and the Riemann Hypothesis Jean-Louis Nicolas and Jonathan Sondow Abstract. We provide an historical account of equivalent conditions for the Riemann Hypothesis arising from the work of Ramanujan and, later, Guy Robin on generalized highly composite numbers. The first part of the paper is on the mathematical background of our subject. The second part is on its history, which includes several surprises. 1. Mathematical Background Definition. The sum-of-divisors function σ is defined by 1 σ(n):= d = n . d d|n d|n In 1913, Gr¨onwall found the maximal order of σ. Gr¨onwall’s Theorem [8]. The function σ(n) G(n):= (n>1) n log log n satisfies lim sup G(n)=eγ =1.78107 ... , n→∞ where 1 1 γ := lim 1+ + ···+ − log n =0.57721 ... n→∞ 2 n is the Euler-Mascheroni constant. Gr¨onwall’s proof uses: Mertens’s Theorem [10]. If p denotes a prime, then − 1 1 1 lim 1 − = eγ . x→∞ log x p p≤x 2010 Mathematics Subject Classification. Primary 01A60, 11M26, 11A25. Key words and phrases. Riemann Hypothesis, Ramanujan’s Theorem, Robin’s Theorem, sum-of-divisors function, highly composite number, superabundant, colossally abundant, Euler phi function. ©2014 American Mathematical Society 145 This is a free offprint provided to the author by the publisher. Copyright restrictions may apply. 146 JEAN-LOUIS NICOLAS AND JONATHAN SONDOW Figure 1. Thomas Hakon GRONWALL¨ (1877–1932) Figure 2. Franz MERTENS (1840–1927) Nowwecometo: Ramanujan’s Theorem [2, 15, 16].
    [Show full text]
  • ON the PRIMALITY of N! ± 1 and 2 × 3 × 5 ×···× P
    MATHEMATICS OF COMPUTATION Volume 71, Number 237, Pages 441{448 S 0025-5718(01)01315-1 Article electronically published on May 11, 2001 ON THE PRIMALITY OF n! 1 AND 2 × 3 × 5 ×···×p 1 CHRIS K. CALDWELL AND YVES GALLOT Abstract. For each prime p,letp# be the product of the primes less than or equal to p. We have greatly extended the range for which the primality of n! 1andp# 1 are known and have found two new primes of the first form (6380! + 1; 6917! − 1) and one of the second (42209# + 1). We supply heuristic estimates on the expected number of such primes and compare these estimates to the number actually found. 1. Introduction For each prime p,letp# be the product of the primes less than or equal to p. About 350 BC Euclid proved that there are infinitely many primes by first assuming they are only finitely many, say 2; 3;:::;p, and then considering the factorization of p#+1: Since then amateurs have expected many (if not all) of the values of p# 1 and n! 1 to be prime. Careful checks over the last half-century have turned up relatively few such primes [5, 7, 13, 14, 19, 25, 32, 33]. Using a program written by the second author, we greatly extended the previous search limits [8] from n ≤ 4580 for n! 1ton ≤ 10000, and from p ≤ 35000 for p# 1top ≤ 120000. This search took over a year of CPU time and has yielded three new primes: 6380!+1, 6917!−1 and 42209# + 1.
    [Show full text]
  • Various Arithmetic Functions and Their Applications
    University of New Mexico UNM Digital Repository Mathematics and Statistics Faculty and Staff Publications Academic Department Resources 2016 Various Arithmetic Functions and their Applications Florentin Smarandache University of New Mexico, [email protected] Octavian Cira Follow this and additional works at: https://digitalrepository.unm.edu/math_fsp Part of the Algebra Commons, Applied Mathematics Commons, Logic and Foundations Commons, Number Theory Commons, and the Set Theory Commons Recommended Citation Smarandache, Florentin and Octavian Cira. "Various Arithmetic Functions and their Applications." (2016). https://digitalrepository.unm.edu/math_fsp/256 This Book is brought to you for free and open access by the Academic Department Resources at UNM Digital Repository. It has been accepted for inclusion in Mathematics and Statistics Faculty and Staff Publications by an authorized administrator of UNM Digital Repository. For more information, please contact [email protected], [email protected], [email protected]. Octavian Cira Florentin Smarandache Octavian Cira and Florentin Smarandache Various Arithmetic Functions and their Applications Peer reviewers: Nassim Abbas, Youcef Chibani, Bilal Hadjadji and Zayen Azzouz Omar Communicating and Intelligent System Engineering Laboratory, Faculty of Electronics and Computer Science University of Science and Technology Houari Boumediene 32, El Alia, Bab Ezzouar, 16111, Algiers, Algeria Octavian Cira Florentin Smarandache Various Arithmetic Functions and their Applications PONS asbl Bruxelles, 2016 © 2016 Octavian Cira, Florentin Smarandache & Pons. All rights reserved. This book is protected by copyright. No part of this book may be reproduced in any form or by any means, including photocopying or using any information storage and retrieval system without written permission from the copyright owners Pons asbl Quai du Batelage no.
    [Show full text]
  • Prime Harmonics and Twin Prime Distribution
    Prime Harmonics and Twin Prime Distribution Serge Dolgikh National Aviation University, Kyiv 02000 Ukraine, [email protected] Abstract: Distribution of twin primes is a long stand- in the form: 0; p−1;:::;2;1 with the value of 0 the highest ing problem in the number theory. As of present, it is in the cycle of length p. Trivially, the positions with the not known if the set of twin primes is finite, the problem same value of the modulo p are separated by the minimum known as the twin primes conjecture. An analysis of prime of p odd steps. modulo cycles, or prime harmonics in this work allowed For a prime p, the prime harmonic function hp(x) can be to define approaches in estimation of twin prime distri- defined on IN1 as the modulo of x by p in the above format: butions with good accuracy of approximation and estab- lish constraints on gaps between consecutive twin prime Definition 1. A single prime harmonic hp(x) is defined for pairs. With technical effort, the approach and the bounds an odd integer x ≥ 1 as: obtained in this work can prove sufficient to establish that hp(1) := (p − 1)=2 the next twin prime exists within the estimated distance, hp(n + 1) := hp(n) - 1, hp(n) > 0 leading to the conclusion that the set of twin primes is un- hp(n + 1) := p − 1, hp(n) = 0 limited and reducing the infinitely repeating distance be- Clearly, h (x) = 0 ≡ p j x. tween consecutive primes to two.
    [Show full text]
  • Multiplication Modulo N Along the Primorials with Its Differences And
    Multiplication Modulo n Along The Primorials With Its Differences And Variations Applied To The Study Of The Distributions Of Prime Number Gaps A.K.A. Introduction To The S Model Russell Letkeman r. letkeman@ gmail. com Dedicated to my son Panha May 19, 2013 Abstract The sequence of sets of Zn on multiplication where n is a primorial gives us a surprisingly simple and elegant tool to investigate many properties of the prime numbers and their distributions through analysis of their gaps. A natural reason to study multiplication on these boundaries is a construction exists which evolves these sets from one primorial boundary to the next, via the sieve of Eratosthenes, giving us Just In Time prime sieving. To this we add a parallel study of gap sets of various lengths and their evolution all of which together informs what we call the S model. We show by construction there exists for each prime number P a local finite probability distribution and it is surprisingly well behaved. That is we show the vacuum; ie the gaps, has deep structure. We use this framework to prove conjectured distributional properties of the prime numbers by Legendre, Hardy and Littlewood and others. We also demonstrate a novel proof of the Green-Tao theorem. Furthermore we prove the Riemann hypoth- esis and show the results are perhaps surprising. We go on to use the S model to predict novel structure within the prime gaps which leads to a new Chebyshev type bias we honorifically name the Chebyshev gap bias. We also probe deeper behavior of the distribution of prime numbers via ultra long scale oscillations about the scale of numbers known as Skewes numbers∗.
    [Show full text]
  • On Prime Numbers and Related Applications
    International Journal of Innovative Technology and Exploring Engineering (IJITEE) ISSN: 2278-3075, Volume-8 Issue-12, October 2019 On Prime Numbers and Related Applications V Yegnanarayanan, Veena Narayanan, R Srikanth Abstract: In this paper we probed some interesting aspects of Our motivating factor for this work stems from the classic primorial and factorial primes. We did some numerical analysis result of called Prime Number Theorem which beautifully about the distribution of prime numbers and tabulated our models the statistical behavioral pattern of huge primes viz., findings. Also, we pointed out certain interesting facts about the utility value of the study of prime numbers and their distributions chance for an arbitrarily picked 푛휖푁 to be a prime number is in control engineering and Brain networks. inverse in proportion to log(푛). Keywords: Factorial primes, Primorial primes, Prime numbers. II. RESULTS AND DISCUSSIONS I. INTRODUCTION A. Discussion on Primorial and Factorial Primes The irregular distribution of prime numbers makes it Our journey is driven by fascinating characteristics of difficult for us to presume and discover. Euclid about 2300 primordial primes and factorial primes. A primordial years before established that primes are infinitely many. Till function denoted 푃# is the product of all primes till P and date we are not aware of a formula for finding the nth 푛 includes P. The factorial function is 푛! = 푖=1 푖. A natural prime. It appears as if they are randomly embedded in N and curiosity pushes us to probe large primes. In order to do this, may be because of this that sequences of primes do not tend we need to get an idea by analyzing numbers such as to emanate from naturally happening processes.
    [Show full text]
  • An Amazing Prime Heuristic
    AN AMAZING PRIME HEURISTIC CHRIS K. CALDWELL 1. Introduction The record for the largest known twin prime is constantly changing. For example, in October of 2000, David Underbakke found the record primes: 83475759 · 264955 ± 1: The very next day Giovanni La Barbera found the new record primes: 1693965 · 266443 ± 1: The fact that the size of these records are close is no coincidence! Before we seek a record like this, we usually try to estimate how long the search might take, and use this information to determine our search parameters. To do this we need to know how common twin primes are. It has been conjectured that the number of twin primes less than or equal to N is asymptotic to Z N dx 2C2N 2C2 2 ∼ 2 2 (log x) (log N) where C2, called the twin prime constant, is approximately 0:6601618. Using this we can estimate how many numbers we will need to try before we find a prime. In the case of Underbakke and La Barbera, they were both using the same sieving software (NewPGen1 by Paul Jobling) and the same primality proving software (Proth.exe2 by Yves Gallot) on similar hardware{so of course they choose similar ranges to search. But where does this conjecture come from? In this chapter we will discuss a general method to form conjectures similar to the twin prime conjecture above. We will then apply it to a number of different forms of primes such as Sophie Germain primes, primes in arithmetic progressions, primorial primes and even the Goldbach conjecture.
    [Show full text]
  • Prime Numbers and the (Double) Primorial Sieve
    Prime numbers and the (double) primorial sieve. 1. The quest. This research into the distribution of prime numbers started by placing a prime number on the short leg of a Pythagorean triangle. The properties of the Pythagorean triples imply that prime numbers > p4 (with p4 = 7) are not divisible by pi ∈ {2, 3, 5, 7}. These divisors have a combined repeating pattern based on the primorial p4#, the product of the first four prime numbers. This pattern defines the fourth (double) primorial sieve. The P4#−sieve is the first sieve with all the properties of the infinite set of primorial sieves. It also gives an explanation for the higher occurrence of the (9, 1) last digit gap among prime numbers. The (double) primorial sieve has two main functions. The primorial sieve is a method to generate a consecutive list of prime numbers, since the base of the n-th primorial sieve contains all prime numbers < pn# . The double primorial sieve offers preliminary filtering of natural numbers when they are sequential stacked above the base of the sieve. Possible prime numbers are only found in the columns supported by the φ(pn#) struts. Each strut is relative prime to pn# and is like a support beam under a column. Fig. 1: Examples of imaginary struts to support a specific column. Hans Dicker \ _Primorial_sieve En.doc pag 1 / 11 2. The principal of the (double) primorial sieve. The width of the primorial sieve Pn#−sieve is determined by the primorial pn#, the product of the first n prime numbers. All natural numbers g > pn# form a matrix of infinite height when stacked sequential on top of the base of the sieve (Fig.
    [Show full text]
  • A Dedekind Psi Function Inequality N
    A Dedekind Psi Function Inequality N. A. Carella, December, 2011. Abstract: This note shows that the arithmetic function !(N) / N = ! p | N (1+1/ p) , called the Dedekind psi v1 v2 vk function, achieves its extreme values on the subset of primorial integers N = 2 ⋅3 pk , where pi is the kth −2 γ prime, and vi ≥ 1. In particular, the inequality ψ (N)/ N > 6π e loglog N holds for all large squarefree primorial integers N = 2⋅3⋅5⋅⋅⋅pk unconditionally. Mathematics Subject Classifications: 11A25, 11A41, 11Y35. Keywords: Psi function, Divisor function, Totient function, Squarefree Integers, Prime numbers, Riemann hypothesis. 1 Introduction The psi function !(N) = N! p | N (1+1/ p) and its normalized counterpart !(N) / N = ! p | N (1+1/ p) arise in various mathematic, and physic problems. Moreover, this function is entangled with other arithmetic functions. The values of the normalized psi function coincide with the squarefree kernel µ 2 (d) ! (1) d|N d of the sum of divisor function ! (N) = !d | N d . In particular, !(N) / N = ! p | N (1+1/ p) = " (N) / N on the subset of square-free integers. This note proposes a new lower estimate of the Dedekind function. 2 Theorem 1. Let N ∈ ℕ be an integer, then ψ (N)/ N > 6π − eγ loglog N holds unconditionally for all sufficiently large primorial integer N = 2⋅3⋅5⋅⋅⋅pk, where pk is the kth prime. An intuitive and clear-cut relationship between the Riemann hypothesis and the Dedekind psi function is established in Theorem 4 by means of the prime number theorem.
    [Show full text]
  • Superabundant Numbers, Their Subsequences and the Riemann
    Superabundant numbers, their subsequences and the Riemann hypothesis Sadegh Nazardonyavi, Semyon Yakubovich Departamento de Matem´atica, Faculdade de Ciˆencias, Universidade do Porto, 4169-007 Porto, Portugal Abstract Let σ(n) be the sum of divisors of a positive integer n. Robin’s theorem states that the Riemann hypothesis is equivalent to the inequality σ(n) < eγ n log log n for all n > 5040 (γ is Euler’s constant). It is a natural question in this direction to find a first integer, if exists, which violates this inequality. Following this process, we introduce a new sequence of numbers and call it as extremely abundant numbers. Then we show that the Riemann hypothesis is true, if and only if, there are infinitely many of these numbers. Moreover, we investigate some of their properties together with superabundant and colossally abundant numbers. 1 Introduction There are several equivalent statements to the famous Riemann hypothesis( Introduction). Some § of them are related to the asymptotic behavior of arithmetic functions. In particular, the known Robin’s criterion (theorem, inequality, etc.) deals with the upper bound of σ(n). Namely, Theorem. (Robin) The Riemann hypothesis is true, if and only if, σ(n) n 5041, <eγ, (1.1) ∀ ≥ n log log n where σ(n)= d and γ is Euler’s constant ([26], Th. 1). arXiv:1211.2147v3 [math.NT] 26 Feb 2013 Xd|n Throughout this paper, as Robin used in [26], we let σ(n) f(n)= . (1.2) n log log n In 1913, Gronwall [13] in his study of asymptotic maximal size for the sum of divisors of n, found that the order of σ(n) is always ”very nearly n” ([14], Th.
    [Show full text]
  • Turbulent Candidates” That Note the Term 4290 Shown in Light Face Above Is in A(N), but Must Be Tested Via the Regular Counting Function to See If the Not in A244052
    Working Second Draft TurbulentMichael Thomas Candidates De Vlieger Abstract paper involve numbers whose factors have multiplicities that never approach 9, we will simply concatenate the digits, thus rendering This paper describes several conditions that pertain to the 75 = {0, 1, 2} as “012”. appearance of terms in oeis a244052, “Highly regular numbers a(n) defined as positions of records in a010846.” The sequence In multiplicity notation, a zero represents a prime totative q < is arranged in “tiers” T wherein each member n has equal values gpf(n) = a006530(n), the greatest prime factor of n. Indeed the multiplicity notation a054841(n) of any number n does not ex- ω(n) = oeis a001221(n). These tiers have primorials pT# = oeis a002110(T) as their smallest member. Each tier is divided into press the infinite series of prime totatives q > gpf(n). We could also write a054841(75) = 01200000…, with an infinite number of “levels” associated with integer multiples kpT# with 1 ≤ k < p(T + zeroes following the 2. Because it is understood that the notation 1). Thus all the terms of oeis a060735 are also in a244052. Mem- bers of a244052 that are not in a060735 are referred to as “turbu- “012” implies all the multiplicities “after” the 2 are 0. lent terms.” This paper focuses primarily on the nature of these Regulars. Consider two positive nonzero integers m and n. The terms. We give parameters for their likely appearance in tier T as number m is said to be “regular to” or “a regular of” n if and only if well as methods of efficiently constructing them.
    [Show full text]