Brun's theorem

{{Short description|Theorem that the sum of the reciprocals of the twin primes converges}}

File:Bruns-constant.svg

In number theory, Brun's theorem states that the sum of the reciprocals of the twin primes (pairs of prime numbers which differ by 2) converges to a finite value known as Brun's constant, usually denoted by B2 {{OEIS|id=A065421}}. Brun's theorem was proved by Viggo Brun in 1919, and it has historical importance in the introduction of sieve methods.

Asymptotic bounds on twin primes

The convergence of the sum of reciprocals of twin primes follows from bounds on the density of the sequence of twin primes.

Let \pi_2(x) denote the number of primes px for which p + 2 is also prime (i.e. \pi_2(x) is the number of twin primes with the smaller at most x). Then, we have

:\pi_2(x) = O\!\left(\frac {x(\log\log x)^2}{(\log x)^2} \right)\!.

That is, twin primes are less frequent than prime numbers by nearly a logarithmic factor.

This bound gives the intuition that the sum of the reciprocals of the twin primes converges, or stated in other words, the twin primes form a small set. In explicit terms, the sum

:\sum\limits_{ p \, : \, p + 2 \in \mathbb{P} } {\left( {\frac{1}{p} + \frac{1}{{p + 2}}} \right)} = \left( {\frac{1}{3} + \frac{1}{5}} \right) + \left( {\frac{1}{5} + \frac{1}{7}} \right) + \left( {\frac{1}{{11}} + \frac{1}{{13}}} \right) + \cdots

either has finitely many terms or has infinitely many terms but is convergent: its value is known as Brun's constant.

If it were the case that the sum diverged, then that fact would imply that there are infinitely many twin primes. Because the sum of the reciprocals of the twin primes instead converges, it is not possible to conclude from this result that there are finitely many or infinitely many twin primes. Brun's constant could be an irrational number only if there are infinitely many twin primes.

Numerical estimates

The series converges extremely slowly. Thomas Nicely remarks that after summing the first billion (109) terms, the relative error is still more than 5%.{{cite web |url=http://www.trnicely.net/twins/twins2.html |last=Nicely |first=Thomas R. |title=Enumeration to 1.6*10^15 of the twin primes and Brun's constant |access-date=16 February 2010 |work=Some Results of Computational Research in Prime Numbers (Computational Number Theory) |date=18 January 2010 |archive-url=https://web.archive.org/web/20131208192242/http://trnicely.net/twins/twins2.html |archive-date=8 December 2013 |url-status=dead }}

By calculating the twin primes up to 1014 (and discovering the Pentium FDIV bug along the way), Nicely heuristically estimated Brun's constant to be 1.902160578. Nicely has extended his computation to 1.6{{e|15}} as of 18 January 2010 but this is not the largest computation of its type.

In 2002, Pascal Sebah and Patrick Demichel used all twin primes up to 1016 to give the estimate{{cite CiteSeerX | last1=Sebah | first1=Pascal | last2=Gourdon | first2=Xavier | title=Introduction to twin primes and Brun's constant computation |citeseerx = 10.1.1.464.1118}} that B2 ≈ 1.902160583104. Hence,

class="wikitable" style="text-align:left"

!Year!! B2!! set of twin
primes below #!! by

19761.9021605401 × 1011Brent
19961.9021605781 × 1014Nicely
20021.9021605831041 × 1016Sebah and Demichel

The last is based on extrapolation from the sum 1.830484424658... for the twin primes below 1016. Dominic Klyve showed conditionally (in an unpublished thesis) that B2 < 2.1754 (assuming the extended Riemann hypothesis). Then in 2025, Lachlan Dunn showed B2 < 2.1609, assuming the generalised Riemann hypothesis.{{cite arXiv |eprint=2504.15658 |last1=Dunn |first1=Lachlan |title=Improved Upper Bound on Brun's Constant Under GRH |date=2025 |class=math.NT }} It has been shown unconditionally that B2 < 2.347.{{cite web |url=https://collections.dartmouth.edu/archive/object/dcdis/dcdis-klyve2007?ctx=dcdis#?length=12&start=0&view=list&rdat_only_u=no&rdat_u=yes&col=dcdis&oc_0=main-title&od_0=a&sv=Brun%27s+constant |last=Klyve |first=Dominic |title=Explicit bounds on twin primes and Brun's Constant |access-date=24 May 2021}}

{{anchor|Prime quadruplets}}There is also a Brun's constant for prime quadruplets. A prime quadruplet is a pair of two twin prime pairs, separated by a distance of 4 (the smallest possible distance). The first prime quadruplets are (5, 7, 11, 13), (11, 13, 17, 19), (101, 103, 107, 109). Brun's constant for prime quadruplets, denoted by B4, is the sum of the reciprocals of all prime quadruplets:

:B_4 = \left(\frac{1}{5} + \frac{1}{7} + \frac{1}{11} + \frac{1}{13}\right)

+ \left(\frac{1}{11} + \frac{1}{13} + \frac{1}{17} + \frac{1}{19}\right)

+ \left(\frac{1}{101} + \frac{1}{103} + \frac{1}{107} + \frac{1}{109}\right) + \cdots

with value:

:B4 = 0.87058 83800 ± 0.00000 00005, the error range having a 99% confidence level according to Nicely.

This constant should not be confused with the Brun's constant for cousin primes, as prime pairs of the form (pp + 4), which is also written as B4. Wolf derived an estimate for the Brun-type sums Bn of 4/n.

Further results

Let C_2=0.6601\ldots {{OEIS|A005597}} be the twin prime constant. Then it is conjectured that

:\pi_2(x) \sim 2C_2\frac{x}{(\log x)^2}.

In particular,

:\pi_2(x) < (2C_2+\varepsilon)\frac{x}{(\log x)^2}

for every \varepsilon>0 and all sufficiently large x.

Many special cases of the above have been proved. Jie Wu proved that for sufficiently large x,

:\pi_2(x) \le 3.3996\cdot2C_2\,\frac{x}{(\log x)^2} < 4.5\,\frac{x}{(\log x)^2}.

See also

Notes

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References

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  • {{cite journal | first=Viggo|last= Brun | author-link=Viggo Brun | title=Über das Goldbachsche Gesetz und die Anzahl der Primzahlpaare | journal=Archiv for Mathematik og Naturvidenskab | volume=B34 | issue=8 | year=1915 }}
  • {{cite journal|language=fr| first=Viggo|last= Brun | author-link=Viggo Brun | title=La série 1/5+1/7+1/11+1/13+1/17+1/19+1/29+1/31+1/41+1/43+1/59+1/61+..., où les dénominateurs sont nombres premiers jumeaux est convergente ou finie | url=http://gallica.bnf.fr/ark:/12148/bpt6k486270d |journal=Bulletin des Sciences Mathématiques | year=1919 | volume=43 | pages=100–104, 124–128 }}
  • {{cite book | first1=Alina Carmen|last1= Cojocaru|author1-link= Alina Carmen Cojocaru | first2=M. Ram|last2= Murty |author2-link=M. Ram Murty| title=An introduction to sieve methods and their applications | series=London Mathematical Society Student Texts | volume=66 | publisher=Cambridge University Press | isbn=0-521-61275-6 | pages=73–74 | year=2005 }}
  • {{cite book | first=E.|last=Landau | author-link=Edmund Landau | title=Elementare Zahlentheorie | location=Leipzig, Germany | publisher=Hirzel | year=1927}} Reprinted Providence, RI: Amer. Math. Soc., 1990.
  • {{cite book | first=William Judson|last= LeVeque |author-link=William J. LeVeque| title=Fundamentals of Number Theory | location=New York City| publisher=Dover Publishing | year=1996 | pages=1–288 | isbn=0-486-68906-9}} Contains a more modern proof.
  • {{cite journal |first=J. |last= Wu |title=Chen's double sieve, Goldbach's conjecture and the twin prime problem |journal= Acta Arithmetica |volume=114 |pages=215–273 |year=2004 |orig-year=24 Sep 2007 |issue=3 |doi= 10.4064/aa114-3-2 |arxiv= 0705.1652|bibcode=2004AcAri.114..215W }}

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