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		<title><![CDATA[MKLab - NUMBER THEORY]]></title>
		<link>https://mklab.gr/</link>
		<description><![CDATA[MKLab - https://mklab.gr]]></description>
		<pubDate>Sun, 13 Sep 2026 13:30:34 +0000</pubDate>
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			<title><![CDATA[The MRDP Theorem]]></title>
			<link>https://mklab.gr/showthread.php?tid=1909</link>
			<pubDate>Tue, 08 Sep 2026 19:14:52 +0300</pubDate>
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			<description><![CDATA[The MRDP Theorem — Peter Smith<br />
<br />
Peter Smith gives an accessible introduction to the <span style="font-weight: bold;" class="mycode_b">MRDP theorem</span>—the Matiyasevich–Robinson–Davis–Putnam theorem—which provides the negative solution to <span style="font-weight: bold;" class="mycode_b">Hilbert’s Tenth Problem</span>. Hilbert asked whether there could be an algorithm which, given an arbitrary Diophantine equation &#36;p(x_1,\ldots,x_n)=0&#36; with integer coefficients, decides in finitely many steps whether it has an integer solution. Smith first explains Diophantine equations and Diophantine sets: a set &#36;K\subseteq\mathbb N&#36; is Diophantine when membership can be expressed as &#36;x\in K\iff \exists y_1\cdots \exists y_k;p(x,y_1,\ldots,y_k)=0&#36;. He then connects this apparently number-theoretic notion with computability. Every Diophantine set is <span style="font-weight: bold;" class="mycode_b">recursively enumerable</span> because possible tuples can simply be searched mechanically. The profound converse, completed by Yuri Matiyasevich following work of Martin Davis, Hilary Putnam and Julia Robinson, states that <span style="font-weight: bold;" class="mycode_b">every recursively enumerable set is Diophantine</span>. Matiyasevich supplied the crucial step by showing how exponential behaviour could itself be represented Diophantinely, using properties of Fibonacci-type sequences.<br />
<br />
Thus, &#36;\boxed{\text{Diophantine sets}=\text{recursively enumerable sets}}&#36;. Since recursively enumerable sets exist whose membership is undecidable, a hypothetical algorithm deciding whether every polynomial equation has a solution would make every recursively enumerable set decidable—a contradiction. Hence the MRDP theorem implies that <span style="font-weight: bold;" class="mycode_b">there is no algorithm which determines for every Diophantine equation whether it has a solution</span>. Smith then develops the striking connection with mathematical logic: recursively enumerable sets correspond to &#36;\Sigma_1&#36;-definable sets, and MRDP allows such statements to be translated into assertions about polynomial equations. Consequently, statements equivalent to “this particular Diophantine equation has no solution” can be <span style="font-weight: bold;" class="mycode_b">true but unprovable in Peano Arithmetic</span>.<br />
<br />
The theorem therefore creates a remarkable bridge between <span style="font-weight: bold;" class="mycode_b">number theory, computability and mathematical logic</span>. In particular, Gödelian incompleteness can appear in a very concrete arithmetic form: there are particular polynomial equations for which the assertion that they have no integer solutions is true but cannot be proved within a given sufficiently strong formal theory.<br />
<br />
<span style="font-weight: bold;" class="mycode_b">Key takeaways</span><ul class="mycode_list"><li><span style="font-weight: bold;" class="mycode_b">Hilbert’s Tenth Problem has a negative answer:</span> there is no universal algorithm deciding whether arbitrary Diophantine equations have integer solutions.<br />
</li>
<li>The central equivalence is &#36;\boxed{K\text{ is Diophantine}\iff K\text{ is recursively enumerable}}&#36;.<br />
</li>
<li>MRDP connects <span style="font-weight: bold;" class="mycode_b">Diophantine equations, computability theory and mathematical logic</span>.<br />
</li>
<li>Some statements of the form “this polynomial equation has no integer solution” can be <span style="font-weight: bold;" class="mycode_b">true but unprovable</span> in a sufficiently strong formal system.<br />
</li>
</ul>
<br />
<a href="https://logicmatters.net/igt/pdfs/MRDP.pdf" target="_blank" rel="noopener" class="mycode_url">ARTICLE [PDF]</a>]]></description>
			<content:encoded><![CDATA[The MRDP Theorem — Peter Smith<br />
<br />
Peter Smith gives an accessible introduction to the <span style="font-weight: bold;" class="mycode_b">MRDP theorem</span>—the Matiyasevich–Robinson–Davis–Putnam theorem—which provides the negative solution to <span style="font-weight: bold;" class="mycode_b">Hilbert’s Tenth Problem</span>. Hilbert asked whether there could be an algorithm which, given an arbitrary Diophantine equation &#36;p(x_1,\ldots,x_n)=0&#36; with integer coefficients, decides in finitely many steps whether it has an integer solution. Smith first explains Diophantine equations and Diophantine sets: a set &#36;K\subseteq\mathbb N&#36; is Diophantine when membership can be expressed as &#36;x\in K\iff \exists y_1\cdots \exists y_k;p(x,y_1,\ldots,y_k)=0&#36;. He then connects this apparently number-theoretic notion with computability. Every Diophantine set is <span style="font-weight: bold;" class="mycode_b">recursively enumerable</span> because possible tuples can simply be searched mechanically. The profound converse, completed by Yuri Matiyasevich following work of Martin Davis, Hilary Putnam and Julia Robinson, states that <span style="font-weight: bold;" class="mycode_b">every recursively enumerable set is Diophantine</span>. Matiyasevich supplied the crucial step by showing how exponential behaviour could itself be represented Diophantinely, using properties of Fibonacci-type sequences.<br />
<br />
Thus, &#36;\boxed{\text{Diophantine sets}=\text{recursively enumerable sets}}&#36;. Since recursively enumerable sets exist whose membership is undecidable, a hypothetical algorithm deciding whether every polynomial equation has a solution would make every recursively enumerable set decidable—a contradiction. Hence the MRDP theorem implies that <span style="font-weight: bold;" class="mycode_b">there is no algorithm which determines for every Diophantine equation whether it has a solution</span>. Smith then develops the striking connection with mathematical logic: recursively enumerable sets correspond to &#36;\Sigma_1&#36;-definable sets, and MRDP allows such statements to be translated into assertions about polynomial equations. Consequently, statements equivalent to “this particular Diophantine equation has no solution” can be <span style="font-weight: bold;" class="mycode_b">true but unprovable in Peano Arithmetic</span>.<br />
<br />
The theorem therefore creates a remarkable bridge between <span style="font-weight: bold;" class="mycode_b">number theory, computability and mathematical logic</span>. In particular, Gödelian incompleteness can appear in a very concrete arithmetic form: there are particular polynomial equations for which the assertion that they have no integer solutions is true but cannot be proved within a given sufficiently strong formal theory.<br />
<br />
<span style="font-weight: bold;" class="mycode_b">Key takeaways</span><ul class="mycode_list"><li><span style="font-weight: bold;" class="mycode_b">Hilbert’s Tenth Problem has a negative answer:</span> there is no universal algorithm deciding whether arbitrary Diophantine equations have integer solutions.<br />
</li>
<li>The central equivalence is &#36;\boxed{K\text{ is Diophantine}\iff K\text{ is recursively enumerable}}&#36;.<br />
</li>
<li>MRDP connects <span style="font-weight: bold;" class="mycode_b">Diophantine equations, computability theory and mathematical logic</span>.<br />
</li>
<li>Some statements of the form “this polynomial equation has no integer solution” can be <span style="font-weight: bold;" class="mycode_b">true but unprovable</span> in a sufficiently strong formal system.<br />
</li>
</ul>
<br />
<a href="https://logicmatters.net/igt/pdfs/MRDP.pdf" target="_blank" rel="noopener" class="mycode_url">ARTICLE [PDF]</a>]]></content:encoded>
		</item>
		<item>
			<title><![CDATA[Strong law of small numbers]]></title>
			<link>https://mklab.gr/showthread.php?tid=1795</link>
			<pubDate>Thu, 03 Sep 2026 02:07:16 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1795</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">Summar</span>y<br />
<br />
The <span style="font-weight: bold;" class="mycode_b">Strong Law of Small Numbers</span>, introduced by mathematician <span style="font-weight: bold;" class="mycode_b">Richard K. Guy</span>, is a humorous but useful warning about mathematical patterns: there simply are not enough small integers to avoid them appearing repeatedly in seemingly unrelated situations. As Guy put it, “There aren't enough small numbers to meet the many demands made of them.” Consequently, striking coincidences involving numbers such as &#36;1,2,3,4,\dots&#36; may look profound even when they are simply consequences of the limited supply of small numbers. Guy developed this idea in his influential 1988 paper <span style="font-style: italic;" class="mycode_i">The Strong Law of Small Numbers</span>. <br />
<br />
Guy later proposed a <span style="font-weight: bold;" class="mycode_b">Second Strong Law of Small Numbers</span>: when two numerical patterns appear to agree, they may eventually diverge. Observing only the first few terms of a sequence can therefore lead to false conjectures. One example involves numbers of the form &#36;2^p-1&#36;: for the first prime values &#36;p=2,3,5,7&#36;, the results are prime, which might suggest that &#36;2^p-1&#36; is always prime whenever &#36;p&#36; is prime. But the pattern already fails at &#36;p=11&#36;, since &#36;2^{11}-1=2047=23\times89&#36;. Another famous example is <span style="font-weight: bold;" class="mycode_b">Moser's circle problem</span>, where the maximum number of regions created by joining &#36;n&#36; points on a circle follows &#36;1,2,4,8,16&#36; for the first five cases, tempting one to guess &#36;2^{n-1}&#36;; at &#36;n=6&#36;, however, the correct value is &#36;31&#36;, not &#36;32&#36;. <br />
<br />
The broader lesson is methodological: <span style="font-weight: bold;" class="mycode_b">small numerical examples are excellent for discovering conjectures but weak evidence for proving them</span>. Mathematical patterns can survive surprisingly many initial cases before breaking down, so genuine proof is essential before treating an observed pattern as a general law. <br />
<br />
Key takeaways<ul class="mycode_list"><li>The Strong Law of Small Numbers is a <span style="font-weight: bold;" class="mycode_b">mathematical observation and joke, not a formal theorem</span>.<br />
</li>
<li>Small integers recur so frequently that apparently remarkable coincidences should be treated cautiously.<br />
</li>
<li>A formula fitting the first several cases of a sequence may eventually fail.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Examples suggest conjectures; proofs establish them.</span><br />
</li>
</ul>
<br />
<a href="https://en.wikipedia.org/wiki/Strong_law_of_small_numbers" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">Summar</span>y<br />
<br />
The <span style="font-weight: bold;" class="mycode_b">Strong Law of Small Numbers</span>, introduced by mathematician <span style="font-weight: bold;" class="mycode_b">Richard K. Guy</span>, is a humorous but useful warning about mathematical patterns: there simply are not enough small integers to avoid them appearing repeatedly in seemingly unrelated situations. As Guy put it, “There aren't enough small numbers to meet the many demands made of them.” Consequently, striking coincidences involving numbers such as &#36;1,2,3,4,\dots&#36; may look profound even when they are simply consequences of the limited supply of small numbers. Guy developed this idea in his influential 1988 paper <span style="font-style: italic;" class="mycode_i">The Strong Law of Small Numbers</span>. <br />
<br />
Guy later proposed a <span style="font-weight: bold;" class="mycode_b">Second Strong Law of Small Numbers</span>: when two numerical patterns appear to agree, they may eventually diverge. Observing only the first few terms of a sequence can therefore lead to false conjectures. One example involves numbers of the form &#36;2^p-1&#36;: for the first prime values &#36;p=2,3,5,7&#36;, the results are prime, which might suggest that &#36;2^p-1&#36; is always prime whenever &#36;p&#36; is prime. But the pattern already fails at &#36;p=11&#36;, since &#36;2^{11}-1=2047=23\times89&#36;. Another famous example is <span style="font-weight: bold;" class="mycode_b">Moser's circle problem</span>, where the maximum number of regions created by joining &#36;n&#36; points on a circle follows &#36;1,2,4,8,16&#36; for the first five cases, tempting one to guess &#36;2^{n-1}&#36;; at &#36;n=6&#36;, however, the correct value is &#36;31&#36;, not &#36;32&#36;. <br />
<br />
The broader lesson is methodological: <span style="font-weight: bold;" class="mycode_b">small numerical examples are excellent for discovering conjectures but weak evidence for proving them</span>. Mathematical patterns can survive surprisingly many initial cases before breaking down, so genuine proof is essential before treating an observed pattern as a general law. <br />
<br />
Key takeaways<ul class="mycode_list"><li>The Strong Law of Small Numbers is a <span style="font-weight: bold;" class="mycode_b">mathematical observation and joke, not a formal theorem</span>.<br />
</li>
<li>Small integers recur so frequently that apparently remarkable coincidences should be treated cautiously.<br />
</li>
<li>A formula fitting the first several cases of a sequence may eventually fail.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Examples suggest conjectures; proofs establish them.</span><br />
</li>
</ul>
<br />
<a href="https://en.wikipedia.org/wiki/Strong_law_of_small_numbers" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
		</item>
		<item>
			<title><![CDATA[Bounded gaps between primes]]></title>
			<link>https://mklab.gr/showthread.php?tid=1775</link>
			<pubDate>Tue, 01 Sep 2026 18:54:53 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1775</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">Bounded Gaps Between Primes</span><br />
<span style="font-weight: bold;" class="mycode_b">Author:</span> Julia Stadlmann<br />
<span style="font-weight: bold;" class="mycode_b">Submitted:</span> 31 August 2026<br />
<span style="font-weight: bold;" class="mycode_b">Field:</span> Number Theory<br />
<br />
<br />
Julia Stadlmann improves the best known unconditional bound for gaps between consecutive primes occurring infinitely often. If<br />
&#36;H1=lim inf⁡n→∞(pn+1−pn)&#36;,<br />
then the famous Twin Prime Conjecture predicts &#36;H_1=2&#36;. After Zhang proved in 2013 that &#36;H_1&#36; is finite, successive improvements by Maynard, Tao and the Polymath8 project eventually established &#36;H_1\le246&#36;. Stadlmann's new result lowers this to<br />
&#36;\boxed{H_1\le240}&#36;.<br />
Thus, there are infinitely many pairs of consecutive primes whose difference is at most &#36;240&#36;. The number &#36;240&#36; comes from the shortest known admissible &#36;49&#36;-tuple, whereas the previous value &#36;246&#36; corresponded to an admissible &#36;50&#36;-tuple. <br />
<br />
The main innovation is not merely the six-unit improvement but the way it is obtained. Stadlmann combines the classical <span style="font-weight: bold;" class="mycode_b">Bombieri–Vinogradov theorem</span> with newer Zhang-type equidistribution estimates for moduli possessing large smooth factors. Within the GPY/Maynard–Tao sieve framework, this permits a larger region of support for the sieve functions, producing a stronger optimization problem. The proof also develops relaxed equidistribution estimates suited to these more general moduli and uses ideas from <span style="font-weight: bold;" class="mycode_b">Harman's sieve</span>. <br />
<br />
The resulting optimization is transformed into a large matrix/eigenvalue problem. Remarkably, the new &#36;240&#36; bound is obtained using symmetric polynomials only up to degree &#36;21&#36;, whereas Polymath needed degree up to &#36;27&#36; for the weaker &#36;246&#36; bound. Direct integration in &#36;49&#36; variables would be computationally impractical, so Stadlmann develops recursive formulas that reduce the required integrals to matrix multiplication. For &#36;k=49&#36;, the final matrices satisfy the key ratio &#36;&gt;1&#36;, which proves &#36;H_1\le240&#36;. The author presents the result largely as a <span style="font-weight: bold;" class="mycode_b">proof of concept</span>, noting that greater computational resources and higher-degree polynomial bases could potentially push the bound below &#36;240&#36;. <br />
<br />
<span style="font-weight: bold;" class="mycode_b">Key takeaways:</span><ul class="mycode_list"><li>The best published bound in this preprint improves from &#36;H_1\le246&#36; to <span style="font-weight: bold;" class="mycode_b">&#36;H_1\le240&#36;</span>.<br />
</li>
<li>It proves that infinitely many consecutive prime pairs are separated by no more than <span style="font-weight: bold;" class="mycode_b">240 integers</span>.<br />
</li>
<li>The important advance is the hybrid use of <span style="font-weight: bold;" class="mycode_b">Bombieri–Vinogradov + newer smooth-moduli equidistribution estimates</span> inside the Maynard–Tao sieve.<br />
</li>
<li>The method appears to contain room for further numerical improvement; &#36;240&#36; is presented as a first demonstration rather than an apparent theoretical limit. <br />
</li>
</ul>
<br />
<a href="https://arxiv.org/abs/2608.31126" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">Bounded Gaps Between Primes</span><br />
<span style="font-weight: bold;" class="mycode_b">Author:</span> Julia Stadlmann<br />
<span style="font-weight: bold;" class="mycode_b">Submitted:</span> 31 August 2026<br />
<span style="font-weight: bold;" class="mycode_b">Field:</span> Number Theory<br />
<br />
<br />
Julia Stadlmann improves the best known unconditional bound for gaps between consecutive primes occurring infinitely often. If<br />
&#36;H1=lim inf⁡n→∞(pn+1−pn)&#36;,<br />
then the famous Twin Prime Conjecture predicts &#36;H_1=2&#36;. After Zhang proved in 2013 that &#36;H_1&#36; is finite, successive improvements by Maynard, Tao and the Polymath8 project eventually established &#36;H_1\le246&#36;. Stadlmann's new result lowers this to<br />
&#36;\boxed{H_1\le240}&#36;.<br />
Thus, there are infinitely many pairs of consecutive primes whose difference is at most &#36;240&#36;. The number &#36;240&#36; comes from the shortest known admissible &#36;49&#36;-tuple, whereas the previous value &#36;246&#36; corresponded to an admissible &#36;50&#36;-tuple. <br />
<br />
The main innovation is not merely the six-unit improvement but the way it is obtained. Stadlmann combines the classical <span style="font-weight: bold;" class="mycode_b">Bombieri–Vinogradov theorem</span> with newer Zhang-type equidistribution estimates for moduli possessing large smooth factors. Within the GPY/Maynard–Tao sieve framework, this permits a larger region of support for the sieve functions, producing a stronger optimization problem. The proof also develops relaxed equidistribution estimates suited to these more general moduli and uses ideas from <span style="font-weight: bold;" class="mycode_b">Harman's sieve</span>. <br />
<br />
The resulting optimization is transformed into a large matrix/eigenvalue problem. Remarkably, the new &#36;240&#36; bound is obtained using symmetric polynomials only up to degree &#36;21&#36;, whereas Polymath needed degree up to &#36;27&#36; for the weaker &#36;246&#36; bound. Direct integration in &#36;49&#36; variables would be computationally impractical, so Stadlmann develops recursive formulas that reduce the required integrals to matrix multiplication. For &#36;k=49&#36;, the final matrices satisfy the key ratio &#36;&gt;1&#36;, which proves &#36;H_1\le240&#36;. The author presents the result largely as a <span style="font-weight: bold;" class="mycode_b">proof of concept</span>, noting that greater computational resources and higher-degree polynomial bases could potentially push the bound below &#36;240&#36;. <br />
<br />
<span style="font-weight: bold;" class="mycode_b">Key takeaways:</span><ul class="mycode_list"><li>The best published bound in this preprint improves from &#36;H_1\le246&#36; to <span style="font-weight: bold;" class="mycode_b">&#36;H_1\le240&#36;</span>.<br />
</li>
<li>It proves that infinitely many consecutive prime pairs are separated by no more than <span style="font-weight: bold;" class="mycode_b">240 integers</span>.<br />
</li>
<li>The important advance is the hybrid use of <span style="font-weight: bold;" class="mycode_b">Bombieri–Vinogradov + newer smooth-moduli equidistribution estimates</span> inside the Maynard–Tao sieve.<br />
</li>
<li>The method appears to contain room for further numerical improvement; &#36;240&#36; is presented as a first demonstration rather than an apparent theoretical limit. <br />
</li>
</ul>
<br />
<a href="https://arxiv.org/abs/2608.31126" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
		</item>
		<item>
			<title><![CDATA[Cuban prime]]></title>
			<link>https://mklab.gr/showthread.php?tid=1691</link>
			<pubDate>Wed, 19 Aug 2026 17:53:21 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1691</guid>
			<description><![CDATA[Cuban Prime<br />
<br />
A <span style="font-weight: bold;" class="mycode_b">Cuban prime</span> is a prime number obtained from particular expressions involving the difference of two cubes. The name has nothing to do with Cuba; it comes from the word <span style="font-weight: bold;" class="mycode_b">cube</span>, because the defining expressions involve third powers. The Wikipedia article describes two main families. In the first, one considers consecutive integers, &#36;x=y+1&#36;, and forms<br />
&#36;<br />
p=\frac{x^3-y^3}{x-y}.<br />
&#36;<br />
<br />
Since &#36;\frac{x^3-y^3}{x-y}=x^2+xy+y^2&#36;, substituting &#36;x=y+1&#36; gives &#36;p=3y^2+3y+1&#36;. Whenever this number is prime, it is called a Cuban prime of the first kind. The sequence begins &#36;7,19,37,61,127,271,\ldots&#36;. Interestingly, numbers of the form &#36;3y^2+3y+1&#36; are exactly the <span style="font-weight: bold;" class="mycode_b">centered hexagonal numbers</span>, giving these primes a geometric interpretation as well. <br />
<br />
The second family arises when the two integers differ by two, so &#36;x=y+2&#36;. The same quotient becomes &#36;p=3y^2+6y+4&#36;. Making the substitution &#36;y=n-1&#36; gives the particularly simple expression &#36;p=3n^2+1&#36;, with &#36;n&gt;1&#36;. Prime values of this polynomial form the second Cuban-prime sequence, beginning &#36;13,109,193,433,769,1201,\ldots&#36;. Thus Cuban primes provide an elementary example of an important theme in number theory: studying when polynomial expressions take prime values. Although the formulas are simple, determining which inputs actually produce primes becomes increasingly difficult as the numbers grow. <br />
<br />
The first family also produces extraordinarily large primes. Wikipedia reports that, <span style="font-weight: bold;" class="mycode_b">as of July 2023</span>, the largest known Cuban prime had <span style="font-weight: bold;" class="mycode_b">3,153,105 decimal digits</span>, obtained using &#36;y=3^{3304301}-1&#36;. This statement is explicitly dated in the article, so it should not necessarily be interpreted as the current 2026 record. The subject connects elementary algebra—the factorization &#36;x^3-y^3=(x-y)(x^2+xy+y^2)&#36;—with prime-number theory, polynomial prime generation, and figurate numbers. <br />
<br />
Key Takeaways<ul class="mycode_list"><li><span style="font-weight: bold;" class="mycode_b">Definition:</span> Cuban primes are primes generated from quotients of differences of cubes, especially when &#36;x-y=1&#36; or &#36;x-y=2&#36;.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Two principal forms:</span> the families reduce to &#36;3y^2+3y+1&#36; and &#36;3n^2+1&#36;.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Geometric connection:</span> Cuban primes of the first kind are prime <span style="font-weight: bold;" class="mycode_b">centered hexagonal numbers</span>.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Significance:</span> They illustrate how very simple polynomial formulas can generate primes while making the question of <span style="font-style: italic;" class="mycode_i">when</span> they are prime a nontrivial number-theoretic problem. <br />
</li>
</ul>
<br />
<a href="https://en.wikipedia.org/wiki/Cuban_prime" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[Cuban Prime<br />
<br />
A <span style="font-weight: bold;" class="mycode_b">Cuban prime</span> is a prime number obtained from particular expressions involving the difference of two cubes. The name has nothing to do with Cuba; it comes from the word <span style="font-weight: bold;" class="mycode_b">cube</span>, because the defining expressions involve third powers. The Wikipedia article describes two main families. In the first, one considers consecutive integers, &#36;x=y+1&#36;, and forms<br />
&#36;<br />
p=\frac{x^3-y^3}{x-y}.<br />
&#36;<br />
<br />
Since &#36;\frac{x^3-y^3}{x-y}=x^2+xy+y^2&#36;, substituting &#36;x=y+1&#36; gives &#36;p=3y^2+3y+1&#36;. Whenever this number is prime, it is called a Cuban prime of the first kind. The sequence begins &#36;7,19,37,61,127,271,\ldots&#36;. Interestingly, numbers of the form &#36;3y^2+3y+1&#36; are exactly the <span style="font-weight: bold;" class="mycode_b">centered hexagonal numbers</span>, giving these primes a geometric interpretation as well. <br />
<br />
The second family arises when the two integers differ by two, so &#36;x=y+2&#36;. The same quotient becomes &#36;p=3y^2+6y+4&#36;. Making the substitution &#36;y=n-1&#36; gives the particularly simple expression &#36;p=3n^2+1&#36;, with &#36;n&gt;1&#36;. Prime values of this polynomial form the second Cuban-prime sequence, beginning &#36;13,109,193,433,769,1201,\ldots&#36;. Thus Cuban primes provide an elementary example of an important theme in number theory: studying when polynomial expressions take prime values. Although the formulas are simple, determining which inputs actually produce primes becomes increasingly difficult as the numbers grow. <br />
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The first family also produces extraordinarily large primes. Wikipedia reports that, <span style="font-weight: bold;" class="mycode_b">as of July 2023</span>, the largest known Cuban prime had <span style="font-weight: bold;" class="mycode_b">3,153,105 decimal digits</span>, obtained using &#36;y=3^{3304301}-1&#36;. This statement is explicitly dated in the article, so it should not necessarily be interpreted as the current 2026 record. The subject connects elementary algebra—the factorization &#36;x^3-y^3=(x-y)(x^2+xy+y^2)&#36;—with prime-number theory, polynomial prime generation, and figurate numbers. <br />
<br />
Key Takeaways<ul class="mycode_list"><li><span style="font-weight: bold;" class="mycode_b">Definition:</span> Cuban primes are primes generated from quotients of differences of cubes, especially when &#36;x-y=1&#36; or &#36;x-y=2&#36;.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Two principal forms:</span> the families reduce to &#36;3y^2+3y+1&#36; and &#36;3n^2+1&#36;.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Geometric connection:</span> Cuban primes of the first kind are prime <span style="font-weight: bold;" class="mycode_b">centered hexagonal numbers</span>.<br />
</li>
<li><span style="font-weight: bold;" class="mycode_b">Significance:</span> They illustrate how very simple polynomial formulas can generate primes while making the question of <span style="font-style: italic;" class="mycode_i">when</span> they are prime a nontrivial number-theoretic problem. <br />
</li>
</ul>
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<a href="https://en.wikipedia.org/wiki/Cuban_prime" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
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			<title><![CDATA[Chicken McNugget Theorem explained]]></title>
			<link>https://mklab.gr/showthread.php?tid=1543</link>
			<pubDate>Mon, 10 Aug 2026 14:33:51 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1543</guid>
			<description><![CDATA[Chicken McNugget Theorem explained<br />
<br />
Summary<br />
<br />
The Codeforces article explains the <span style="font-weight: bold;" class="mycode_b">Chicken McNugget Theorem</span>, a useful result in number theory for determining which integers can be expressed as nonnegative combinations of two relatively prime positive integers &#36;m&#36; and &#36;n&#36;. It states that the <span style="font-weight: bold;" class="mycode_b">largest integer that cannot be written as &#36;am+bn&#36;</span> is &#36;mn-m-n=(m-1)(n-1)-1&#36;, where &#36;a,b\ge0&#36;, and that every larger integer can be represented in this way. It also gives the number of positive integers that cannot be represented as exactly &#36;\frac{(m-1)(n-1)}{2}&#36;. <br />
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For example, using &#36;m=2&#36; and &#36;n=5&#36;, the impossible values are &#36;1&#36; and &#36;3&#36;, while every integer greater than &#36;3&#36; can be formed. The theorem is particularly useful in competitive programming problems such as Codeforces <span style="font-weight: bold;" class="mycode_b">1526B – I Hate 1111</span>, where recognizing this mathematical structure can replace a more complicated approach. <br />
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<a href="https://codeforces.com/blog/entry/118246" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[Chicken McNugget Theorem explained<br />
<br />
Summary<br />
<br />
The Codeforces article explains the <span style="font-weight: bold;" class="mycode_b">Chicken McNugget Theorem</span>, a useful result in number theory for determining which integers can be expressed as nonnegative combinations of two relatively prime positive integers &#36;m&#36; and &#36;n&#36;. It states that the <span style="font-weight: bold;" class="mycode_b">largest integer that cannot be written as &#36;am+bn&#36;</span> is &#36;mn-m-n=(m-1)(n-1)-1&#36;, where &#36;a,b\ge0&#36;, and that every larger integer can be represented in this way. It also gives the number of positive integers that cannot be represented as exactly &#36;\frac{(m-1)(n-1)}{2}&#36;. <br />
<br />
For example, using &#36;m=2&#36; and &#36;n=5&#36;, the impossible values are &#36;1&#36; and &#36;3&#36;, while every integer greater than &#36;3&#36; can be formed. The theorem is particularly useful in competitive programming problems such as Codeforces <span style="font-weight: bold;" class="mycode_b">1526B – I Hate 1111</span>, where recognizing this mathematical structure can replace a more complicated approach. <br />
<br />
<a href="https://codeforces.com/blog/entry/118246" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
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			<title><![CDATA[Hyperperfect number]]></title>
			<link>https://mklab.gr/showthread.php?tid=1529</link>
			<pubDate>Wed, 05 Aug 2026 04:14:30 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1529</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">Hyperperfect number</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
A <span style="font-weight: bold;" class="mycode_b">hyperperfect number</span> is a concept in number theory that generalizes the idea of a perfect number. A natural number &#36;n&#36; is called <span style="font-weight: bold;" class="mycode_b">&#36;k&#36;-hyperperfect</span> if it satisfies the equation &#36;n = 1 + k(\sigma(n)-n-1)&#36;, where &#36;\sigma(n)&#36; is the sum of all positive divisors of &#36;n&#36;. <br />
<br />
In this formula, &#36;k&#36; is a positive integer, and when &#36;k=1&#36;, the definition reduces to that of a <span style="font-weight: bold;" class="mycode_b">perfect number</span>, meaning that the number equals the sum of its proper divisors. Hyperperfect numbers include all perfect numbers but also many additional examples; for instance, the first non-perfect hyperperfect numbers include &#36;21&#36;, &#36;2133&#36;, and &#36;19521&#36;. <br />
<br />
Mathematicians study these numbers to understand deeper relationships between divisors, divisor sums, and special structures in integers, although many questions about their distribution and properties remain open.<br />
<br />
<a href="https://en.wikipedia.org/wiki/Hyperperfect_number" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">Hyperperfect number</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
A <span style="font-weight: bold;" class="mycode_b">hyperperfect number</span> is a concept in number theory that generalizes the idea of a perfect number. A natural number &#36;n&#36; is called <span style="font-weight: bold;" class="mycode_b">&#36;k&#36;-hyperperfect</span> if it satisfies the equation &#36;n = 1 + k(\sigma(n)-n-1)&#36;, where &#36;\sigma(n)&#36; is the sum of all positive divisors of &#36;n&#36;. <br />
<br />
In this formula, &#36;k&#36; is a positive integer, and when &#36;k=1&#36;, the definition reduces to that of a <span style="font-weight: bold;" class="mycode_b">perfect number</span>, meaning that the number equals the sum of its proper divisors. Hyperperfect numbers include all perfect numbers but also many additional examples; for instance, the first non-perfect hyperperfect numbers include &#36;21&#36;, &#36;2133&#36;, and &#36;19521&#36;. <br />
<br />
Mathematicians study these numbers to understand deeper relationships between divisors, divisor sums, and special structures in integers, although many questions about their distribution and properties remain open.<br />
<br />
<a href="https://en.wikipedia.org/wiki/Hyperperfect_number" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
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			<title><![CDATA[An Interesting Number]]></title>
			<link>https://mklab.gr/showthread.php?tid=1407</link>
			<pubDate>Wed, 29 Jul 2026 04:16:07 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
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			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">An Interesting Number</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">This Stack Exchange discussion seeks a natural number &#36;m&#36; whose four-digit square (&#36;m^2 = ABCD&#36;) and six-digit cube (&#36;m^3 = EFGHIJ&#36;) together contain all ten digits from &#36;0&#36; to &#36;9&#36; exactly once without repetition. By establishing size bounds (&#36;47 \le m \le 98&#36;), eliminating terminal digits that repeat upon exponentiation, and using modular arithmetic (noting that the sum of the digits &#36;0&#36; through &#36;9&#36; is &#36;45&#36;, meaning &#36;m^2 + m^3&#36; must be divisible by &#36;9&#36;), the post narrows the search down to a handful of candidate numbers. Testing these candidates reveals that the unique solution is <span style="font-weight: bold;" class="mycode_b">&#36;m = 69&#36;</span>, whose square &#36;69^2 = 4761&#36; and cube &#36;69^3 = 328509&#36; combine to span every digit from &#36;0&#36; to &#36;9&#36;.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://math.stackexchange.com/questions/5003319/an-interesting-number-its-square-and-cubes-span-0-9" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">An Interesting Number</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">This Stack Exchange discussion seeks a natural number &#36;m&#36; whose four-digit square (&#36;m^2 = ABCD&#36;) and six-digit cube (&#36;m^3 = EFGHIJ&#36;) together contain all ten digits from &#36;0&#36; to &#36;9&#36; exactly once without repetition. By establishing size bounds (&#36;47 \le m \le 98&#36;), eliminating terminal digits that repeat upon exponentiation, and using modular arithmetic (noting that the sum of the digits &#36;0&#36; through &#36;9&#36; is &#36;45&#36;, meaning &#36;m^2 + m^3&#36; must be divisible by &#36;9&#36;), the post narrows the search down to a handful of candidate numbers. Testing these candidates reveals that the unique solution is <span style="font-weight: bold;" class="mycode_b">&#36;m = 69&#36;</span>, whose square &#36;69^2 = 4761&#36; and cube &#36;69^3 = 328509&#36; combine to span every digit from &#36;0&#36; to &#36;9&#36;.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://math.stackexchange.com/questions/5003319/an-interesting-number-its-square-and-cubes-span-0-9" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></content:encoded>
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			<title><![CDATA[Waring’s problem]]></title>
			<link>https://mklab.gr/showthread.php?tid=1393</link>
			<pubDate>Wed, 29 Jul 2026 00:16:43 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1393</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">Waring’s problem</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
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<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">Proposed by English mathematician Edward Waring in 1770, <span style="font-weight: bold;" class="mycode_b">Waring's problem</span> is a fundamental question in number theory asking whether, for every positive integer &#36;k&#36;, there exists a corresponding minimum integer &#36;g(k)&#36; such that every natural number can be expressed as the sum of at most &#36;g(k)&#36; natural numbers raised to the &#36;k&#36;-th power. For example, every natural number is the sum of at most 4 squares (&#36;g(2) = 4&#36;), 9 cubes (&#36;g(3) = 9&#36;), or 19 fourth powers (&#36;g(4) = 19&#36;). </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">David Hilbert affirmatively proved the existence of such a finite limit for every power &#36;k&#36; in 1909—a result known as the Hilbert–Waring theorem—and modern research continues to explore exact formulas for &#36;g(k)&#36; as well as &#36;G(k)&#36;, which measures the maximum number of &#36;k&#36;-th powers required to express all <span style="font-style: italic;" class="mycode_i">sufficiently large</span> integers.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Waring%27s_problem" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">Waring’s problem</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">Proposed by English mathematician Edward Waring in 1770, <span style="font-weight: bold;" class="mycode_b">Waring's problem</span> is a fundamental question in number theory asking whether, for every positive integer &#36;k&#36;, there exists a corresponding minimum integer &#36;g(k)&#36; such that every natural number can be expressed as the sum of at most &#36;g(k)&#36; natural numbers raised to the &#36;k&#36;-th power. For example, every natural number is the sum of at most 4 squares (&#36;g(2) = 4&#36;), 9 cubes (&#36;g(3) = 9&#36;), or 19 fourth powers (&#36;g(4) = 19&#36;). </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">David Hilbert affirmatively proved the existence of such a finite limit for every power &#36;k&#36; in 1909—a result known as the Hilbert–Waring theorem—and modern research continues to explore exact formulas for &#36;g(k)&#36; as well as &#36;G(k)&#36;, which measures the maximum number of &#36;k&#36;-th powers required to express all <span style="font-style: italic;" class="mycode_i">sufficiently large</span> integers.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Waring%27s_problem" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></content:encoded>
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			<title><![CDATA[Wilson's theorem]]></title>
			<link>https://mklab.gr/showthread.php?tid=1391</link>
			<pubDate>Wed, 29 Jul 2026 00:10:19 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1391</guid>
			<description><![CDATA[Wilson's theorem<br />
<br />
Summary<br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><span style="font-weight: bold;" class="mycode_b">Wilson's theorem</span> is a fundamental result in number theory stating that a natural number &#36;n &gt; 1&#36; is a prime number if and only if the product of all positive integers less than &#36;n&#36; is one less than a multiple of &#36;n&#36;—expressed in modular arithmetic as &#36;(n-1)! \equiv -1 \pmod n&#36;. </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">First stated by Persian mathematician Ibn al-Haytham around 1000 AD and later named after John Wilson (with its first published proof by Joseph-Louis Lagrange in 1771), the theorem provides a theoretical condition for primality, though it is practically useless for testing large prime numbers due to the steep computational complexity of calculating large factorials.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Wilson%27s_theorem" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></description>
			<content:encoded><![CDATA[Wilson's theorem<br />
<br />
Summary<br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><span style="font-weight: bold;" class="mycode_b">Wilson's theorem</span> is a fundamental result in number theory stating that a natural number &#36;n &gt; 1&#36; is a prime number if and only if the product of all positive integers less than &#36;n&#36; is one less than a multiple of &#36;n&#36;—expressed in modular arithmetic as &#36;(n-1)! \equiv -1 \pmod n&#36;. </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">First stated by Persian mathematician Ibn al-Haytham around 1000 AD and later named after John Wilson (with its first published proof by Joseph-Louis Lagrange in 1771), the theorem provides a theoretical condition for primality, though it is practically useless for testing large prime numbers due to the steep computational complexity of calculating large factorials.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Wilson%27s_theorem" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></content:encoded>
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			<title><![CDATA[Euler's criterion]]></title>
			<link>https://mklab.gr/showthread.php?tid=1388</link>
			<pubDate>Tue, 28 Jul 2026 23:59:49 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1388</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">Euler's criterion</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">In number theory, <span style="font-weight: bold;" class="mycode_b">Euler's criterion</span> (formulated by Leonhard Euler in 1748) provides a direct method to determine whether an integer &#36;a&#36; coprime to an odd prime &#36;p&#36; is a quadratic residue—meaning whether the congruence &#36;x^2 \equiv a \pmod p&#36; has a integer solution. The criterion states that &#36;a^{(p-1)/2} \equiv 1 \pmod p&#36; if &#36;a&#36; is a quadratic residue, and &#36;a^{(p-1)/2} \equiv -1 \pmod p&#36; if it is a nonresidue, which can be concisely expressed using the Legendre symbol as &#36;\left(\frac{a}{p}\right) \equiv a^{\frac{p-1}{2}} \pmod p&#36;. </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">Derived from Fermat's Little Theorem and Lagrange's Theorem on polynomial roots, this fundamental result plays a crucial role in modular arithmetic, connects to the law of quadratic reciprocity, and serves as the theoretical backbone for probabilistic primality tests such as the Solovay–Strassen test.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Euler%27s_criterion" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">Euler's criterion</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">In number theory, <span style="font-weight: bold;" class="mycode_b">Euler's criterion</span> (formulated by Leonhard Euler in 1748) provides a direct method to determine whether an integer &#36;a&#36; coprime to an odd prime &#36;p&#36; is a quadratic residue—meaning whether the congruence &#36;x^2 \equiv a \pmod p&#36; has a integer solution. The criterion states that &#36;a^{(p-1)/2} \equiv 1 \pmod p&#36; if &#36;a&#36; is a quadratic residue, and &#36;a^{(p-1)/2} \equiv -1 \pmod p&#36; if it is a nonresidue, which can be concisely expressed using the Legendre symbol as &#36;\left(\frac{a}{p}\right) \equiv a^{\frac{p-1}{2}} \pmod p&#36;. </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">Derived from Fermat's Little Theorem and Lagrange's Theorem on polynomial roots, this fundamental result plays a crucial role in modular arithmetic, connects to the law of quadratic reciprocity, and serves as the theoretical backbone for probabilistic primality tests such as the Solovay–Strassen test.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Euler%27s_criterion" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></content:encoded>
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			<title><![CDATA[Historical Overview of Pi]]></title>
			<link>https://mklab.gr/showthread.php?tid=1382</link>
			<pubDate>Tue, 28 Jul 2026 23:31:04 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1382</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">Historical Overview of Pi</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
This overview explains that <span style="font-weight: bold;" class="mycode_b">π (pi)</span> is one of the most fundamental mathematical constants, defined as the ratio of a circle’s circumference to its diameter. It discusses how mathematicians have sought increasingly accurate approximations of π for thousands of years, beginning with ancient civilizations and continuing through modern computer calculations. The page highlights the historical progression of π computations, from simple geometric methods to sophisticated algorithms capable of producing billions and even trillions of digits.<br />
<br />
 It also emphasizes that π is an <span style="font-weight: bold;" class="mycode_b">irrational</span> and <span style="font-weight: bold;" class="mycode_b">transcendental</span> number, meaning its decimal expansion never ends or repeats and it cannot be expressed as the root of any polynomial with rational coefficients. Although only a relatively small number of digits are needed for nearly all practical scientific and engineering applications, calculating additional digits has become an important benchmark for testing mathematical algorithms and the power of modern computers. <br />
<br />
<a href="http://www.geom.uiuc.edu/~huberty/math5337/groupe/overview.html" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">Historical Overview of Pi</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
This overview explains that <span style="font-weight: bold;" class="mycode_b">π (pi)</span> is one of the most fundamental mathematical constants, defined as the ratio of a circle’s circumference to its diameter. It discusses how mathematicians have sought increasingly accurate approximations of π for thousands of years, beginning with ancient civilizations and continuing through modern computer calculations. The page highlights the historical progression of π computations, from simple geometric methods to sophisticated algorithms capable of producing billions and even trillions of digits.<br />
<br />
 It also emphasizes that π is an <span style="font-weight: bold;" class="mycode_b">irrational</span> and <span style="font-weight: bold;" class="mycode_b">transcendental</span> number, meaning its decimal expansion never ends or repeats and it cannot be expressed as the root of any polynomial with rational coefficients. Although only a relatively small number of digits are needed for nearly all practical scientific and engineering applications, calculating additional digits has become an important benchmark for testing mathematical algorithms and the power of modern computers. <br />
<br />
<a href="http://www.geom.uiuc.edu/~huberty/math5337/groupe/overview.html" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
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			<title><![CDATA[Ramanujan–Nagell equation]]></title>
			<link>https://mklab.gr/showthread.php?tid=1361</link>
			<pubDate>Sun, 26 Jul 2026 07:52:53 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1361</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b">Ramanujan–Nagell equation</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">The <span style="font-weight: bold;" class="mycode_b">Ramanujan–Nagell equation</span> is an exponential Diophantine equation given by &#36;2^n - 7 = x^2&#36;, which asks for integer solutions where a power of two minus seven equals a perfect square. First conjectured in 1913 by Indian mathematician Srinivasa Ramanujan and definitively proved in 1948 by Norwegian mathematician Trygve Nagell, </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">The equation is famous for having only five solutions for &#36;n&#36; (&#36;n = 3, 4, 5, 7,&#36; and &#36;15&#36;). Beyond its interest in number theory—where it is equivalent to finding Mersenne numbers that are also triangular—the equation plays a crucial role in coding theory by proving the non-existence of certain perfect binary error-correcting codes.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Ramanujan%E2%80%93Nagell_equation" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b">Ramanujan–Nagell equation</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">The <span style="font-weight: bold;" class="mycode_b">Ramanujan–Nagell equation</span> is an exponential Diophantine equation given by &#36;2^n - 7 = x^2&#36;, which asks for integer solutions where a power of two minus seven equals a perfect square. First conjectured in 1913 by Indian mathematician Srinivasa Ramanujan and definitively proved in 1948 by Norwegian mathematician Trygve Nagell, </span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font">The equation is famous for having only five solutions for &#36;n&#36; (&#36;n = 3, 4, 5, 7,&#36; and &#36;15&#36;). Beyond its interest in number theory—where it is equivalent to finding Mersenne numbers that are also triangular—the equation plays a crucial role in coding theory by proving the non-existence of certain perfect binary error-correcting codes.</span></span><br />
<br />
<span style="color: #1f1f1f;" class="mycode_color"><span style="font-family: 'Google Sans Text', sans-serif;" class="mycode_font"><a href="https://en.wikipedia.org/wiki/Ramanujan%E2%80%93Nagell_equation" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a></span></span>]]></content:encoded>
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			<title><![CDATA[Kissing number]]></title>
			<link>https://mklab.gr/showthread.php?tid=1297</link>
			<pubDate>Sat, 25 Jul 2026 05:33:56 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1297</guid>
			<description><![CDATA[<div style="text-align: center;" class="mycode_align"><span style="font-weight: bold;" class="mycode_b"><img src="https://mathworld.wolfram.com/images/eps-svg/KissingNumber12_1000.svg" loading="lazy"  width="250" height="250" alt="[Image: KissingNumber12_1000.svg]" class="mycode_img" /></span></div>
<br />
<br />
<span style="font-weight: bold;" class="mycode_b">Kissing number</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
The <span style="font-weight: bold;" class="mycode_b">kissing number</span> is a classic problem in geometry that asks for the maximum number of identical, non-overlapping spheres that can simultaneously touch a single sphere of the same size. Although the idea is easy to visualize, finding the exact kissing number becomes increasingly difficult as the number of dimensions grows. The problem originated in a famous 1694 debate between Isaac Newton and David Gregory over whether 12 or 13 spheres could touch one central sphere in three dimensions; Newton was correct, but a rigorous proof was not discovered until 1953. <br />
<br />
The exact kissing numbers are known only for a few dimensions, including 1 (2), 2 (6), 3 (12), 4 (24), 8 (240), and 24 (196,560), while for most higher dimensions mathematicians have established only upper and lower bounds. The kissing number problem is closely related to sphere packing, coding theory, lattice geometry, and optimisation, making it important in both pure and applied mathematics. Research continues to improve bounds and discover new methods, including semidefinite programming and modern AI-assisted techniques, highlighting the problem as one of the most fascinating and enduring challenges in discrete geometry.<br />
<br />
<br />
<a href="https://en.wikipedia.org/wiki/Kissing_number" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[<div style="text-align: center;" class="mycode_align"><span style="font-weight: bold;" class="mycode_b"><img src="https://mathworld.wolfram.com/images/eps-svg/KissingNumber12_1000.svg" loading="lazy"  width="250" height="250" alt="[Image: KissingNumber12_1000.svg]" class="mycode_img" /></span></div>
<br />
<br />
<span style="font-weight: bold;" class="mycode_b">Kissing number</span><br />
<br />
<span style="font-weight: bold;" class="mycode_b">Summary</span><br />
<br />
The <span style="font-weight: bold;" class="mycode_b">kissing number</span> is a classic problem in geometry that asks for the maximum number of identical, non-overlapping spheres that can simultaneously touch a single sphere of the same size. Although the idea is easy to visualize, finding the exact kissing number becomes increasingly difficult as the number of dimensions grows. The problem originated in a famous 1694 debate between Isaac Newton and David Gregory over whether 12 or 13 spheres could touch one central sphere in three dimensions; Newton was correct, but a rigorous proof was not discovered until 1953. <br />
<br />
The exact kissing numbers are known only for a few dimensions, including 1 (2), 2 (6), 3 (12), 4 (24), 8 (240), and 24 (196,560), while for most higher dimensions mathematicians have established only upper and lower bounds. The kissing number problem is closely related to sphere packing, coding theory, lattice geometry, and optimisation, making it important in both pure and applied mathematics. Research continues to improve bounds and discover new methods, including semidefinite programming and modern AI-assisted techniques, highlighting the problem as one of the most fascinating and enduring challenges in discrete geometry.<br />
<br />
<br />
<a href="https://en.wikipedia.org/wiki/Kissing_number" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
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			<title><![CDATA[Graham's number]]></title>
			<link>https://mklab.gr/showthread.php?tid=1280</link>
			<pubDate>Fri, 24 Jul 2026 01:43:23 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1280</guid>
			<description><![CDATA[<span style="font-weight: bold;" class="mycode_b"><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham's number</span></span></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font"><span style="font-weight: bold;" class="mycode_b">Summary</span></span></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham's number is one of the largest numbers ever used in a serious mathematical proof, introduced by mathematician Ronald Graham in the 1970s while studying a problem in Ramsey theory, a branch of combinatorics that explores unavoidable patterns in large structures. The number emerged from a question about how many dimensions are needed in a particular geometric coloring problem, and although the final answer was unimaginably large, Graham proved that it served as an upper bound for the solution. </span></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham’s number is far beyond ordinary large numbers such as a googol or even a googolplex; it is defined through repeated applications of Knuth’s up-arrow notation, a system designed to describe extremely fast-growing operations. Even the number of digits in Graham’s number is itself vastly larger than anything that could be physically represented in the observable universe. Despite its enormous size, the number is finite and mathematically well-defined, showing how abstract mathematics can deal with quantities that have no practical physical interpretation. Its importance lies not in the number itself, but in demonstrating the power of mathematical language to describe structures and relationships far beyond human intuition.</span></span><br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font"><br />
<span style="font-weight: bold;" class="mycode_b">Key takeaways:</span></span></span><ul class="mycode_list"><li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham’s number is a famous extremely large finite number from Ramsey theory.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">It was used as an upper bound in a mathematical proof involving high-dimensional geometry.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Its definition relies on Knuth’s up-arrow notation and repeated exponential growth operations.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">The number of digits in Graham’s number is unimaginably larger than physical scales in the universe.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Its significance is conceptual: it highlights the ability of mathematics to handle abstract extremes.</span></span><br />
</li>
</ul>
<span style="color: #101418;" class="mycode_color"><span style="font-weight: bold;" class="mycode_b">Conclusion: </span>Graham’s number is a remarkable example of how mathematics can create and study quantities that exceed human imagination while remaining precisely defined.</span><br />
<br />
<span style="color: #101418;" class="mycode_color"><a href="https://en.wikipedia.org/wiki/Graham%27s_number" target="_blank" rel="noopener" class="mycode_url"><span style="font-weight: bold;" class="mycode_b">ARTICLE</span></a></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><a href="https://mathworld.wolfram.com/GrahamsNumber.html" target="_blank" rel="noopener" class="mycode_url">ARTICLE (WOFLRAM)</a><br />
</span>]]></description>
			<content:encoded><![CDATA[<span style="font-weight: bold;" class="mycode_b"><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham's number</span></span></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font"><span style="font-weight: bold;" class="mycode_b">Summary</span></span></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham's number is one of the largest numbers ever used in a serious mathematical proof, introduced by mathematician Ronald Graham in the 1970s while studying a problem in Ramsey theory, a branch of combinatorics that explores unavoidable patterns in large structures. The number emerged from a question about how many dimensions are needed in a particular geometric coloring problem, and although the final answer was unimaginably large, Graham proved that it served as an upper bound for the solution. </span></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham’s number is far beyond ordinary large numbers such as a googol or even a googolplex; it is defined through repeated applications of Knuth’s up-arrow notation, a system designed to describe extremely fast-growing operations. Even the number of digits in Graham’s number is itself vastly larger than anything that could be physically represented in the observable universe. Despite its enormous size, the number is finite and mathematically well-defined, showing how abstract mathematics can deal with quantities that have no practical physical interpretation. Its importance lies not in the number itself, but in demonstrating the power of mathematical language to describe structures and relationships far beyond human intuition.</span></span><br />
<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font"><br />
<span style="font-weight: bold;" class="mycode_b">Key takeaways:</span></span></span><ul class="mycode_list"><li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Graham’s number is a famous extremely large finite number from Ramsey theory.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">It was used as an upper bound in a mathematical proof involving high-dimensional geometry.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Its definition relies on Knuth’s up-arrow notation and repeated exponential growth operations.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">The number of digits in Graham’s number is unimaginably larger than physical scales in the universe.</span></span><br />
</li>
<li><span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Its significance is conceptual: it highlights the ability of mathematics to handle abstract extremes.</span></span><br />
</li>
</ul>
<span style="color: #101418;" class="mycode_color"><span style="font-weight: bold;" class="mycode_b">Conclusion: </span>Graham’s number is a remarkable example of how mathematics can create and study quantities that exceed human imagination while remaining precisely defined.</span><br />
<br />
<span style="color: #101418;" class="mycode_color"><a href="https://en.wikipedia.org/wiki/Graham%27s_number" target="_blank" rel="noopener" class="mycode_url"><span style="font-weight: bold;" class="mycode_b">ARTICLE</span></a></span><br />
<br />
<span style="color: #101418;" class="mycode_color"><a href="https://mathworld.wolfram.com/GrahamsNumber.html" target="_blank" rel="noopener" class="mycode_url">ARTICLE (WOFLRAM)</a><br />
</span>]]></content:encoded>
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			<title><![CDATA[Extravagant number]]></title>
			<link>https://mklab.gr/showthread.php?tid=1278</link>
			<pubDate>Fri, 24 Jul 2026 01:30:23 +0300</pubDate>
			<dc:creator><![CDATA[<a href="https://mklab.gr/member.php?action=profile&uid=1">mklabgr</a>]]></dc:creator>
			<guid isPermaLink="false">https://mklab.gr/showthread.php?tid=1278</guid>
			<description><![CDATA[<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Extravagant number</span></span><br />
<br />
Summary<br />
<br />
An <span style="font-weight: bold;" class="mycode_b">extravagant number</span> (also called a <span style="font-style: italic;" class="mycode_i">wasteful number</span>) is a concept from number theory that describes numbers whose prime factorization requires more digits to write down than the number itself in a given numerical base. In base 10, for example, numbers such as 4, 6, 8, and 9 are extravagant because their factorizations (&#36;4 = 2²&#36;, &#36;6 = 2 × 3&#36;, &#36;8 = 2³&#36;, &#36;9 = 3²&#36;) use more written symbols when prime factors and exponents are counted than the original number. <br />
<br />
This idea belongs to the broader study of “economical” representations of numbers, where mathematicians compare the efficiency of expressing a number directly versus describing it through its prime components. Extravagant numbers can be defined in any base, not only decimal, and there are infinitely many examples in every base.<br />
<br />
The topic is interesting because it reveals hidden patterns in the structure of integers and shows how the way we write numbers influences mathematical properties. It connects arithmetic, prime factorization, and information efficiency, offering a different perspective on the simplicity or complexity of numbers.<br />
<br />
 <span style="font-weight: bold;" class="mycode_b">Key takeaways:</span> extravagant numbers are numbers whose prime factorizations are “longer” than the numbers themselves; they depend on the numerical base used; and they demonstrate that even ordinary integers can have surprising structural properties. <br />
<br />
<span style="font-weight: bold;" class="mycode_b">In conclusion</span>, extravagant numbers provide a fascinating example of how mathematics explores not only what numbers are, but also how efficiently we represent them.<br />
<br />
<a href="https://en.wikipedia.org/wiki/Extravagant_number" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></description>
			<content:encoded><![CDATA[<span style="color: #101418;" class="mycode_color"><span style="font-family: 'Linux Libertine', Georgia, Times, 'Source Serif 4', serif;" class="mycode_font">Extravagant number</span></span><br />
<br />
Summary<br />
<br />
An <span style="font-weight: bold;" class="mycode_b">extravagant number</span> (also called a <span style="font-style: italic;" class="mycode_i">wasteful number</span>) is a concept from number theory that describes numbers whose prime factorization requires more digits to write down than the number itself in a given numerical base. In base 10, for example, numbers such as 4, 6, 8, and 9 are extravagant because their factorizations (&#36;4 = 2²&#36;, &#36;6 = 2 × 3&#36;, &#36;8 = 2³&#36;, &#36;9 = 3²&#36;) use more written symbols when prime factors and exponents are counted than the original number. <br />
<br />
This idea belongs to the broader study of “economical” representations of numbers, where mathematicians compare the efficiency of expressing a number directly versus describing it through its prime components. Extravagant numbers can be defined in any base, not only decimal, and there are infinitely many examples in every base.<br />
<br />
The topic is interesting because it reveals hidden patterns in the structure of integers and shows how the way we write numbers influences mathematical properties. It connects arithmetic, prime factorization, and information efficiency, offering a different perspective on the simplicity or complexity of numbers.<br />
<br />
 <span style="font-weight: bold;" class="mycode_b">Key takeaways:</span> extravagant numbers are numbers whose prime factorizations are “longer” than the numbers themselves; they depend on the numerical base used; and they demonstrate that even ordinary integers can have surprising structural properties. <br />
<br />
<span style="font-weight: bold;" class="mycode_b">In conclusion</span>, extravagant numbers provide a fascinating example of how mathematics explores not only what numbers are, but also how efficiently we represent them.<br />
<br />
<a href="https://en.wikipedia.org/wiki/Extravagant_number" target="_blank" rel="noopener" class="mycode_url">ARTICLE</a>]]></content:encoded>
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