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==Distribution== Let ''Q''(''x'') denote the number of square-free integers between 1 and ''x'' ({{OEIS2C|A013928}} shifting index by 1). For large ''n'', 3/4 of the positive integers less than ''n'' are not divisible by 4, 8/9 of these numbers are not divisible by 9, and so on. Because these ratios satisfy the [[multiplicative function|multiplicative property]] (this follows from [[Chinese remainder theorem]]), we obtain the approximation: :<math>\begin{align}Q(x) &\approx x\prod_{p\ \text{prime}} \left(1-\frac{1}{p^2}\right) = x\prod_{p\ \text{prime}} \frac{1}{(1-\frac{1}{p^2})^{-1}}\\ &=x\prod_{p\ \text{prime}} \frac{1}{1+\frac{1}{p^2}+\frac{1}{p^4}+\cdots} = \frac{x}{\sum_{k=1}^\infty \frac{1}{k^2}} = \frac{x}{\zeta(2)} = \frac{6x}{\pi^2}.\end{align}</math> This argument can be made rigorous for getting the estimate (using [[big O notation]]) :<math>Q(x) = \frac{6x}{\pi^2} + O\left(\sqrt{x}\right).</math> ''Sketch of a proof:'' the above characterization gives :<math>Q(x)=\sum_{n\leq x} \sum_{d^2\mid n} \mu(d)=\sum_{d\leq x} \mu(d)\sum_{n\leq x, d^2\mid n}1=\sum_{d\leq x} \mu(d)\left\lfloor\frac{x}{d^2}\right\rfloor;</math> observing that the last summand is zero for <math>d>\sqrt{x}</math>, it follows that {{NumBlk|:|<math>Q(x) = \sum_{d\leq\sqrt{x}} \mu(d)\left\lfloor\frac{x}{d^2}\right\rfloor</math>|{{EquationRef|1}}}} :<math>\begin{align} \phantom{Q(x)} &= \sum_{d\leq\sqrt{x}} \frac{x\mu(d)}{d^2}+O\left(\sum_{d\leq\sqrt{x}} 1\right) =x\sum_{d\leq\sqrt{x}} \frac{\mu(d)}{d^2}+O(\sqrt{x})\\ &=x\sum_{d} \frac{\mu(d)}{d^2}+O\left(x\sum_{d>\sqrt{x}}\frac{1}{d^2}+\sqrt{x}\right) =\frac{x}{\zeta(2)}+O(\sqrt{x}). \end{align}</math> By exploiting the largest known zero-free region of the Riemann zeta function [[Arnold Walfisz]] improved the approximation to<ref>{{cite book |last1=Walfisz |first1=A. |title=Weylsche Exponentialsummen in der neueren Zahlentheorie |date=1963 |publisher=[[VEB Deutscher Verlag der Wissenschaften]] |location=Berlin}}</ref> :<math>Q(x) = \frac{6x}{\pi^2} + O\left(x^{1/2}\exp\left(-c\frac{(\log x)^{3/5}}{(\log\log x)^{1/5}}\right)\right),</math> for some positive constant {{math|''c''}}. Under the [[Riemann hypothesis]], the error term can be reduced to<ref>Jia, Chao Hua. "The distribution of square-free numbers", ''Science in China Series A: Mathematics'' '''36''':2 (1993), pp. 154β169. Cited in Pappalardi 2003, [http://www.mat.uniroma3.it/users/pappa/papers/allahabad2003.pdf A Survey on ''k''-freeness]; also see Kaneenika Sinha, "[http://www.math.ualberta.ca/~kansinha/maxnrevfinal.pdf Average orders of certain arithmetical functions]", ''Journal of the Ramanujan Mathematical Society'' '''21''':3 (2006), pp. 267β277.</ref> :<math>Q(x) = \frac{x}{\zeta(2)} + O\left(x^{17/54+\varepsilon}\right) = \frac{6}{\pi^2}x + O\left(x^{17/54+\varepsilon}\right).</math> In 2015 the error term was further reduced (assuming also Riemann hypothesis) to<ref>{{cite journal |last1=Liu |first1=H.-Q. |title=On the distribution of squarefree numbers |journal=Journal of Number Theory |date=2016 |volume=159 |pages=202β222|doi=10.1016/j.jnt.2015.07.013 |doi-access=free }}</ref> :<math>Q(x) = \frac{6}{\pi^2}x + O\left(x^{11/35+\varepsilon}\right).</math> The asymptotic/[[natural density]] of square-free numbers is therefore :<math>\lim_{x\to\infty} \frac{Q(x)}{x} = \frac{6}{\pi^2}\approx 0.6079</math> Therefore over 3/5 of the integers are square-free. Likewise, if ''Q''(''x'',''n'') denotes the number of ''n''-free integers (e.g. 3-free integers being cube-free integers) between 1 and ''x'', one can show<ref>{{cite journal | first1 = E. H. | last1 = Linfoot | author-link1 = Edward Linfoot | first2 = C. J. A. | last2 = Evelyn | title = On a Problem in the Additive Theory of Numbers | journal = Mathematische Zeitschrift | date = 1929 | volume = 30 | pages = 443β448 | doi = 10.1007/BF01187781 | s2cid = 120604049 | url = https://gdz.sub.uni-goettingen.de/id/PPN266833020_0030?tify={%22pages%22:[437],%22view%22:%22info%22} }}</ref> :<math>Q(x,n) = \frac{x}{\sum_{k=1}^\infty \frac{1}{k^n}} + O\left(\sqrt[n]{x}\right) = \frac{x}{\zeta(n)} + O\left(\sqrt[n]{x}\right).</math> Since a multiple of 4 must have a square factor 4=2<sup>2</sup>, it cannot occur that four consecutive integers are all square-free. On the other hand, there exist infinitely many integers ''n'' for which 4''n'' +1, 4''n'' +2, 4''n'' +3 are all square-free. Otherwise, observing that 4''n'' and at least one of 4''n'' +1, 4''n'' +2, 4''n'' +3 among four could be non-square-free for sufficiently large ''n'', half of all positive integers minus finitely many must be non-square-free and therefore :<math>Q(x) \leq \frac{x}{2}+C</math> for some constant ''C'', contrary to the above asymptotic estimate for <math>Q(x)</math>. There exist sequences of consecutive non-square-free integers of arbitrary length. Indeed, for every tuple {{math|1=(''p''<sub>1</sub>, ..., ''p''<sub>''l''</sub>)}} of distinct primes, the [[Chinese remainder theorem]] guarantees the existence of an {{mvar|n}} that satisfies the simultaneous congruence :<math>n\equiv -i\pmod{p_i^2} \qquad (i=1, 2, \ldots, l).</math> Each {{math|1=''n'' + ''i''}} is then divisible by {{math|1=''p''{{su|b=''i''|p=2}}}}.<ref>{{cite book | last1= Parent | first1=D. P. |title=Exercises in Number Theory | publisher=[[Springer-Verlag]] New York | isbn=978-1-4757-5194-9 | url=https://www.springer.com/book/9780387960630 | doi=10.1007/978-1-4757-5194-9 | year=1984| series=Problem Books in Mathematics }}</ref> On the other hand, the above-mentioned estimate <math>Q(x) = 6x/\pi^2 + O\left(\sqrt{x}\right)</math> implies that, for some constant ''c'', there always exists a square-free integer between ''x'' and <math>x+c\sqrt{x}</math> for positive ''x''. Moreover, an elementary argument allows us to replace <math>x+c\sqrt{x}</math> by <math>x+cx^{1/5}\log x.</math><ref>{{cite journal | last1 = Filaseta | first1 = Michael | last2 = Trifonov | first2 = Ognian | doi = 10.1112/jlms/s2-45.2.215 | issue = 2 | journal = Journal of the London Mathematical Society | mr = 1171549 | pages = 215β221 | series = Second Series | title = On gaps between squarefree numbers. II | volume = 45 | year = 1992}}</ref> The [[abc conjecture|''abc'' conjecture]] would allow <math>x+x^{o(1)}</math>.<ref>{{cite journal |last1=Granville |first1=Andrew |author-link=Andrew Granville |year=1998 |title=ABC allows us to count squarefrees |journal=Int. Math. Res. Not. |volume=1998 |issue=19 |pages=991β1009 |doi=10.1155/S1073792898000592 |doi-access=<!-- not free-->}}</ref> === Computation of {{Math|''Q''(''x'')}} === The squarefree integers {{Math|≤ ''x''}} can be identified and counted in {{Math|[[big O notation|''Γ'']](''x'')}} time by using a modified [[Sieve of Eratosthenes]]. If only {{Math|''Q''(''x'')}} is desired, and not a list of the numbers that it counts, then ({{EquationNote|1}}) can be used to compute {{Math|''Q''(''x'')}} in {{Math|''Γ''({{radical|''x''}})}} time. The largest known value of {{Math|''Q''(''x'')}}, for {{Math|1=''x'' = 10<sup>36</sup>}}, was computed by Jakub Pawlewicz in 2011 using an algorithm that achieves {{Math|''Γ''(''x''<sup>2/5</sup>)}} time,<ref>{{cite arXiv |eprint=1107.4890 |last1=Pawlewicz |first1=Jakub |title=Counting Square-Free Numbers |date=2011 |class=math.NT }}</ref> and an algorithm taking {{Math|''Γ''(''x''<sup>1/3</sup>)}} time has been outlined but not implemented.{{r|HirschKesslerMendlovic2024|at=§5.5}} ===Table of ''Q''(''x''), {{Sfrac|6|Ο<sup>2</sup>}}''x'', and ''R''(''x'') === The table shows how <math> Q(x)</math> and <math>\frac{6}{\pi^2}x</math> (with the latter rounded to one decimal place) compare at powers of 10. <math> R(x) = Q(x) -\frac{6}{\pi^2}x </math> , also denoted as <math> \Delta(x) </math>. :{| class="wikitable" style="text-align: right" ! <math> x </math> ! <math> Q(x) </math> ! <math> \frac{6}{\pi^2}x</math> !<math> R(x)</math> |- | 10 | 7 | 6.1 | 0.9 |- | 10<sup>2</sup> | 61 | 60.8 | 0.2 |- | 10<sup>3</sup> | 608 | 607.9 | 0.1 |- | 10<sup>4</sup> | 6,083 | 6,079.3 | 3.7 |- | 10<sup>5</sup> | 60,794 | 60,792.7 | 1.3 |- | 10<sup>6</sup> | 607,926 | 607,927.1 | {{font color|red|β1.3}} |- | 10<sup>7</sup> | 6,079,291 | 6,079,271.0 | 20.0 |- | 10<sup>8</sup> | 60,792,694 | 60,792,710.2 | {{font color|red|β16.2}} |- | 10<sup>9</sup> | 607,927,124 | 607,927,101.9 | 22.1 |- | 10<sup>10</sup> | 6,079,270,942 | 6,079,271,018.5 | {{font color|red|β76.5}} |- | 10<sup>11</sup> | 60,792,710,280 | 60,792,710,185.4 | 94.6 |- | 10<sup>12</sup> | 607,927,102,274 | 607,927,101,854.0 | 420.0 |- | 10<sup>13</sup> | 6,079,271,018,294 | 6,079,271,018,540.3 | {{font color|red|β246.3}} |- | 10<sup>14</sup> | 60,792,710,185,947 | 60,792,710,185,402.7 | 544.3 |- | 10<sup>15</sup> | 607,927,101,854,103 | 607,927,101,854,027.0 | 76.0 |- |} <math> R(x) </math> changes its sign infinitely often as <math> x </math> tends to infinity.<ref>{{cite journal |last1=Minoru |first1=Tanaka |title=Experiments concerning the distribution of squarefree numbers |journal=Proceedings of the Japan Academy, Series A, Mathematical Sciences |year=1979 |volume=55 |issue=3 |doi=10.3792/pjaa.55.101 |s2cid=121862978 |url=https://projecteuclid.org/euclid.pja/1195517398|doi-access=free }}</ref> The absolute value of <math> R(x) </math> is astonishingly small compared with <math> x </math>.
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