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<record version="14" id="6860">
 <title>prime harmonic series</title>
 <name>PrimeHarmonicSeries</name>
 <created>2005-03-09 14:32:33</created>
 <modified>2006-10-14 15:06:51</modified>
 <type>Theorem</type>
 <creator id="8605" name="Cosmin"/>
 <author id="8605" name="Cosmin"/>
 <classification>
	<category scheme="msc" code="11A41"/>
	<category scheme="msc" code="40A05"/>
 </classification>
 <synonyms>
	<synonym concept="prime harmonic series" alias="series of reciprocals of primes"/>
 </synonyms>
 <related>
	<object name="Prime"/>
	<object name="HarmonicSeries"/>
	<object name="HarmonicNumber"/>
	<object name="Series"/>
	<object name="EulersConstant"/>
	<object name="HarmonicSeriesOfPrimes"/>
 </related>
 <keywords>
	<term>prime series</term>
	<term>prime sum</term>
	<term>reciprocal prime</term>
	<term>prime harmonic</term>
 </keywords>
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 <content>\PMlinkescapeword{infinite}
\PMlinkescapeword{constant}
\PMlinkescapeword{bound}
\PMlinkescapephrase{square-free part}
\PMlinkescapephrase{set of primes}
\PMlinkescapephrase{harmonic series}

The prime\footnote{\(\bbP\) denotes the set of 
primes.} harmonic series (also known as series of reciprocals of primes) is the infinite sum \(\sum_{p\in\bbP}\frac{1}{p}\). The following result was originally proved by Euler (using the Euler product of the Riemann Zeta function) but the following extremely elegant proof is due to Paul Erd\H{o}s \cite{Er}.

\begin{thm}
The series \( \sum_{p\in\bbP}\frac{1}{p} \) diverges.
\end{thm}
\begin{proof}
Assume that this series is convergent. If so, then, for a certain \( 
k\in\bbN \), we have:
\[ \sum_{i &gt; k}\frac{1}{p_i} &lt; \frac{1}{2}, \]
where \(p_i\) is the \(i^{\mathrm{th}}\) prime. Now, we define \( 
\lambda_k(n) := \#\{ m\leq n : p_i \div m \Rightarrow i \leq k \} \), the 
number of integers less than \(n\) divisible only by the first \(k\) 
primes. Any of these numbers can be expressed as 
\(m = p_1^{\omega_1} \dotsm p_k^{\omega_k} \cdot s^2,\; 
\omega_i\in\{0,1\} \) (i.e. a square multiplied by a square-free number). There are \(2^k\) ways to chose the square-free part and clearly \(s\leq 
\sqrt{n}\), so \( \lambda_k(n) \leq 2^k \sqrt{n}\). Now, the number of integers divisible by \(p_i\) less than \(n\) is \(\bigl\lfloor\frac{n}{p_i}\bigr\rfloor\), so the number of integers less than \(n\) divisible by primes bigger than \(p_k\) (which we shall denote by \( \Lambda_k(n) \)) is bounded above as follows:
\[\Lambda_k(n) \leq \sum_{i&gt;k}\left\lfloor\frac{n}{p_i}\right\rfloor \leq \sum_{i&gt;k}\frac{n}{p_i} &lt; \frac{n}{2}.\]
However, by their definitions, \(\lambda_k(n)+\Lambda_k(n) = n\) for all \(n\in\bbN\) and so it is sufficient to find an \(n\) such that \(\lambda_k(n)\leq\frac{n}{2}\) for a contradiction and, using the previous bound for \( \lambda_k(n) \), which is \( \lambda_k(n) \leq 2^k \sqrt{n}\), we see that \( n = 2^{2k+2} \) works.
\end{proof}

The series is in some ways similar to the \PMlinkname{Harmonic series}{HarmonicSeries} \(H_n := \sum_{k = 1}^n \frac{1}{n}\). In fact, it is well known that \(H_n = \log n + \gamma + o(1) \), where \(\gamma = 0.577215664905\dots\) is Euler's constant, and this series obeys the similar asymptotic relation \(\sum_{k=1}^n\frac{1}{p_k}= \log\log n + C + o(1)\), where \(C = 0.26149721\dots\) and is sometimes called the Mertens constant. Its divergence, however, is extremely slow: for example, taking \(n\) as the biggest currently known prime, the \( 42^{\mathrm{nd}} \) Mersenne prime \(M_{25964951}\), we get \(\log\log(2^{25964951} - 1) + C \approx 16.9672\) (while \(H_{M_{25964951}}\approx 1.79975\cdot 10^{17} \) which is enormous considering \(H_n\)'s also slow divergence).

\begin{thebibliography}{2}
\bibitem{AZ} \textsc{M.~Aigner \&amp; G.~M.~Ziegler}: \emph{Proofs from THE BOOK}, 3\(^\mathrm{rd}\) edition (2004), Springer-Verlag, 5--6.
\bibitem{Er} \textsc{P.~Erd\H{o}s}: \emph{\"Uber die Reihe \(\sum\frac{1}{p}\)}, Mathematica, Zutphen B 7 (1938).
\end{thebibliography}</content>
</record>
