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Illustration of the perfect number status of the number 6

In number theory, a perfect number is a positive integer that is equal to the sum of its positive proper divisors, that is, divisors excluding the number itself.[1] For instance, 6 has proper divisors 1, 2, and 3, and 1 + 2 + 3 = 6, so 6 is a perfect number. The next perfect number is 28, because 1 + 2 + 4 + 7 + 14 = 28.

The first seven perfect numbers are 6, 28, 496, 8128, 33550336, 8589869056, and 137438691328.[2]

The sum of proper divisors of a number is called its aliquot sum, so a perfect number is one that is equal to its aliquot sum. Equivalently, a perfect number is a number that is half the sum of all of its positive divisors; in symbols, where is the sum-of-divisors function.

This definition is ancient, appearing as early as Euclid's Elements (VII.22) where it is called τέλειος ἀριθμός (perfect, ideal, or complete number). Euclid also proved a formation rule (IX.36) whereby is an even perfect number whenever is a prime of the form for positive integer —what is now called a Mersenne prime. Two millennia later, Leonhard Euler proved that all even perfect numbers are of this form.[3] This is known as the Euclid–Euler theorem.

It is not known whether there are any odd perfect numbers, nor whether infinitely many perfect numbers exist.

History

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In about 300 BC Euclid showed that if 2p − 1 is prime then 2p−1(2p − 1) is perfect. The first four perfect numbers were the only ones known to early Greek mathematics, and the mathematician Nicomachus noted 8128 as early as around AD 100.[4] In modern language, Nicomachus states without proof that every perfect number is of the form where is prime.[5][6] He seems to be unaware that n itself has to be prime. He also says (wrongly) that the perfect numbers end in 6 or 8 alternately. (The first 5 perfect numbers end with digits 6, 8, 6, 8, 6; but the sixth also ends in 6.) Philo of Alexandria in his first-century book "On the creation" mentions perfect numbers, claiming that the world was created in 6 days and the moon orbits in 28 days because 6 and 28 are perfect. Philo is followed by Origen,[7] and by Didymus the Blind, who adds the observation that there are only four perfect numbers that are less than 10,000. (Commentary on Genesis 1. 14–19).[8] Augustine of Hippo defines perfect numbers in The City of God (Book XI, Chapter 30) in the early 5th century AD, repeating the claim that God created the world in 6 days because 6 is the smallest perfect number. The Egyptian mathematician Ismail ibn Fallūs (1194–1252) mentioned the next three perfect numbers (33,550,336; 8,589,869,056; and 137,438,691,328) and listed a few more which are now known to be incorrect.[9] The first known European mention of the fifth perfect number is a manuscript written between 1456 and 1461 by an unknown mathematician.[10] In 1588, the Italian mathematician Pietro Cataldi identified the sixth (8,589,869,056) and the seventh (137,438,691,328) perfect numbers, and also proved that every perfect number obtained from Euclid's rule ends with a 6 or an 8.[11][12][13]

Even perfect numbers

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Unsolved problem in mathematics
Are there infinitely many perfect numbers?

Euclid proved that is an even perfect number whenever is prime (Elements, Prop. IX.36).

For example, the first four perfect numbers are generated by the formula with p a prime number, as follows:

Prime numbers of the form are known as Mersenne primes, after the seventeenth-century monk Marin Mersenne, who studied number theory and perfect numbers. For to be prime, it is necessary that p itself be prime. However, not all numbers of the form with a prime p are prime; for example, 211 − 1 = 2047 = 23 × 89 is not a prime number.[a] In fact, Mersenne primes are very rare: of the approximately 4 million primes p up to 68,874,199, is prime for only 48 of them.[14]

While Nicomachus had stated (without proof) that all perfect numbers were of the form where is prime (though he stated this somewhat differently), Ibn al-Haytham (Alhazen) circa AD 1000 was unwilling to go that far, declaring instead (also without proof) that the formula yielded only every even perfect number.[15] It was not until the 18th century that Leonhard Euler proved that the formula indeed yields all the even perfect numbers. Thus, there is a one-to-one correspondence between even perfect numbers and Mersenne primes; each Mersenne prime generates one even perfect number, and vice versa. This result is often referred to as the Euclid–Euler theorem.

An exhaustive search by the GIMPS distributed computing project has shown that the first 50 even perfect numbers are for

p = 2, 3, 5, 7, 13, 17, 19, 31, 61, 89, 107, 127, 521, 607, 1279, 2203, 2281, 3217, 4253, 4423, 9689, 9941, 11213, 19937, 21701, 23209, 44497, 86243, 110503, 132049, 216091, 756839, 859433, 1257787, 1398269, 2976221, 3021377, 6972593, 13466917, 20996011, 24036583, 25964951, 30402457, 32582657, 37156667, 42643801, 43112609, 57885161, 74207281, 77232917 OEISA000043.[14]

Two higher perfect numbers have also been discovered, namely those for which p = 82589933 and 136279841. Although it is still possible there may be others within this range, initial but exhaustive tests by GIMPS have revealed no other perfect numbers for p below 138277717. As of October 2024, 52 Mersenne primes are known,[16] and therefore 52 even perfect numbers (the largest of which is 2136279840 × (2136279841 − 1) with 82,048,640 digits). It is not known whether there are infinitely many perfect numbers, nor whether there are infinitely many Mersenne primes.

As well as having the form , each even perfect number is the -th triangular number (and hence equal to the sum of the integers from 1 to ) and the -th hexagonal number. Furthermore, each even perfect number except for 6 is the -th centered nonagonal number and is equal to the sum of the first odd cubes (odd cubes up to the cube of ):

Even perfect numbers (except 6) are of the form

with each resulting triangular number T7 = 28, T31 = 496, T127 = 8128 (after subtracting 1 from the perfect number and dividing the result by 9) ending in 3 or 5, the sequence starting with T2 = 3, T10 = 55, T42 = 903, T2730 = 3727815, ...[17] It follows that by adding the digits of any even perfect number (except 6), then adding the digits of the resulting number, and repeating this process until a single digit (called the digital root) is obtained, always produces the number 1. For example, the digital root of 8128 is 1, because 8 + 1 + 2 + 8 = 19, 1 + 9 = 10, and 1 + 0 = 1. This works with all perfect numbers with odd prime p and, in fact, with all numbers of the form for odd integer (not necessarily prime) m.

Owing to their form, every even perfect number is represented in binary form as p ones followed by p − 1 zeros; for example:

Thus every even perfect number is a pernicious number.

Every even perfect number is also a practical number (cf. Related concepts).

Odd perfect numbers

[edit]
Unsolved problem in mathematics
Are there any odd perfect numbers?

It is unknown whether any odd perfect numbers exist, though various results have been obtained. In 1496, Jacques Lefèvre stated that Euclid's rule gives all perfect numbers,[18] thus implying that no odd perfect number exists, but Euler himself stated: "Whether ... there are any odd perfect numbers is a most difficult question".[19] More recently, Carl Pomerance has presented a heuristic argument suggesting that indeed no odd perfect number should exist.[20] All perfect numbers are also harmonic divisor numbers, and it has been conjectured as well that there are no odd harmonic divisor numbers other than 1.

Any odd perfect number N must satisfy the following conditions:

  • N > 101500.[21]
  • N is not divisible by 105.[22]
  • N is of the form N ≡ 1 (mod 12) or N ≡ 117 (mod 468) or N ≡ 81 (mod 324).[23]
  • The largest prime power pa that divides N is greater than 1062.[21]
  • The largest prime factor of N is greater than 108,[24] and less than [25]
  • The second largest prime factor is greater than 104,[26] and is less than .[27]
  • The third largest prime factor is greater than 100,[28] and less than [29]
  • N has at least 101 prime factors and at least 10 distinct prime factors.[21][30] If 3 does not divide N, then N has at least 12 distinct prime factors.[31]
  • N is of the form
where:
  • qp1, ..., pk are distinct odd primes (Euler).
  • q ≡ α ≡ 1 (mod 4) (Euler).
  • The smallest prime factor of N is at most [32]
  • [33][34]
  • .[32][35][36]
  • .[37]
  • .[38][39]

Furthermore, several minor results are known about the exponents e1, ..., ek.

  • Not all ei ≡ 1 (mod 3).[40]
  • Not all ei ≡ 2 (mod 5).[41]
  • If all ei ≡ 1 (mod 3) or 2 (mod 5), then the smallest prime factor of N must lie between 108 and 101000.[41]
  • More generally, if all 2ei+1 have a prime factor in a given finite set S, then the smallest prime factor of N must be smaller than an effectively computable constant depending only on S.[41]
  • If (e1, ..., ek) =  (1, ..., 1, 2, ..., 2) with t ones and u twos, then .[42]
  • (e1, ..., ek) ≠ (1, ..., 1, 3),[43] (1, ..., 1, 5), (1, ..., 1, 6).[44]
  • If e1 = ... = ek = e, then
    • e cannot be 3,[45] 5, 24,[46] 6, 8, 11, 14 or 18.[44]
    • .[47]

In 1888, Sylvester stated:[48]

... a prolonged meditation on the subject has satisfied me that the existence of any one such [odd perfect number]—its escape, so to say, from the complex web of conditions which hem it in on all sides—would be little short of a miracle.

On the other hand, several odd integers come close to being perfect. René Descartes observed that the number D = 32 ⋅ 72 ⋅ 112 ⋅ 132 ⋅ 22021 = (3⋅1001)2 ⋅ (22⋅1001 − 1) = 198585576189 would be an odd perfect number if only 22021 (= 192 ⋅ 61) were a prime number. The odd numbers with this property (they would be perfect if one of their composite factors were prime) are the Descartes numbers. Many of the properties proven about odd perfect numbers also apply to Descartes numbers, and Pace Nielsen has suggested that sufficient study of these numbers may lead to a proof that no odd perfect numbers exist.[49]

Minor results

[edit]

All even perfect numbers have a very precise form; odd perfect numbers either do not exist or are rare. There are a number of results on perfect numbers that are actually quite easy to prove but nevertheless superficially impressive; some of them also come under Richard Guy's strong law of small numbers:

  • The only even perfect number of the form n3 + 1 is 28 (Makowski 1962).[50]
  • 28 is also the only even perfect number that is a sum of two positive cubes of integers (Gallardo 2010).[51]
  • The reciprocals of the divisors of a perfect number N must add up to 2 (to get this, take the definition of a perfect number, , and divide both sides by n):
    • For 6, we have ;
    • For 28, we have , etc.
  • The number of divisors of a perfect number (whether even or odd) must be even, because N cannot be a perfect square.[52]
  • The even perfect numbers are not trapezoidal numbers; that is, they cannot be represented as the difference of two positive non-consecutive triangular numbers. There are only three types of non-trapezoidal numbers: even perfect numbers, powers of two, and the numbers of the form formed as the product of a Fermat prime with a power of two in a similar way to the construction of even perfect numbers from Mersenne primes.[53]
  • The number of perfect numbers less than n is less than , where c > 0 is a constant.[54] In fact it is , using little-o notation.[55]
  • Every even perfect number ends in 6 or 28 in base ten and, with the only exception of 6, ends in 1 in base 9.[56][57] Therefore, in particular the digital root of every even perfect number other than 6 is 1.
  • The only square-free perfect number is 6.[58]
[edit]
Euler diagram of numbers under 100:
   Weird
   Perfect

The sum of proper divisors gives various other kinds of numbers. Numbers where the sum is less than the number itself are called deficient, and where it is greater than the number, abundant. These terms, together with perfect itself, come from Greek numerology. A pair of numbers which are the sum of each other's proper divisors are called amicable, and larger cycles of numbers are called sociable. A positive integer such that every smaller positive integer is a sum of distinct divisors of it is a practical number.

By definition, a perfect number is a fixed point of the restricted divisor function s(n) = σ(n) − n, and the aliquot sequence associated with a perfect number is a constant sequence. All perfect numbers are also -perfect numbers, or Granville numbers.

A semiperfect number is a natural number that is equal to the sum of all or some of its proper divisors. A semiperfect number that is equal to the sum of all its proper divisors is a perfect number. Most abundant numbers are also semiperfect; abundant numbers which are not semiperfect are called weird numbers.

See also

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Notes

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References

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Further reading

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[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A perfect number is a positive equal to the sum of its proper positive divisors, where proper divisors exclude the number itself. Equivalently, the sum of all positive divisors of such a number nn, denoted σ(n)\sigma(n), satisfies σ(n)=2n\sigma(n) = 2n. The smallest perfect numbers are 6 (with proper divisors 1, 2, 3) and 28 (with proper divisors 1, 2, 4, 7, 14). These examples illustrate the rarity of perfect numbers, a concept originating in mathematics. Around 300 BCE, described in his Elements a construction for even perfect numbers: if 2p12^p - 1 is prime (a ), then 2p1(2p1)2^{p-1}(2^p - 1) is perfect. In the , Leonhard Euler proved the converse—that every even perfect number must take this form—establishing a one-to-one correspondence between even perfect numbers and Mersenne primes. As of November 2025, 52 Mersenne primes are known, yielding exactly 52 known perfect numbers, all even. The largest, corresponding to the Mersenne prime 213627984112^{136279841} - 1 (discovered by Luke Durant on October 12, 2024), is 2136279840(21362798411)2^{136279840} (2^{136279841} - 1), a number with over 41 million digits. No odd perfect numbers are known, and their existence remains an open problem in number theory; if any exist, they must exceed 10150010^{1500} and have at least ten distinct prime factors. Euler further showed that any odd perfect number must be of the form pkm2p^k m^2, where pp is a prime congruent to 1 modulo 4, k1(mod4)k \equiv 1 \pmod{4}, and gcd(p,m)=1\gcd(p, m) = 1. Extensive computational searches and theoretical bounds continue to constrain possible candidates, but the question persists as one of the oldest unsolved problems in mathematics.

Fundamentals

Definition

A perfect number is a positive that equals the sum of its proper divisors, where proper divisors are the positive divisors of the number excluding the number itself. For example, the proper divisors of 6 are 1, 2, and 3, and their sum is 1+2+3=61 + 2 + 3 = 6. Similarly, the proper divisors of 28 are 1, 2, 4, 7, and 14, summing to 1+2+4+7+14=281 + 2 + 4 + 7 + 14 = 28. The first few perfect numbers are 6, 28, 496, and 8128. An equivalent formulation uses the divisor sum function σ(n)\sigma(n), which denotes the sum of all positive divisors of nn including nn itself; a number nn is perfect if σ(n)=2n\sigma(n) = 2n, or equivalently, if the sum of its proper divisors equals nn. The term "perfect" originates from the Greek word teleios, meaning complete or finished, reflecting ancient views of these numbers as embodying mathematical harmony; this nomenclature is attributed to early Greek mathematicians such as Euclid and Nicomachus. All known perfect numbers are even.

Divisor Sum Function

The divisor sum function, denoted σ(n), is defined as the sum of all positive divisors of a positive n, including both 1 and n itself. This function is a fundamental in , capturing the total "divisibility measure" of n. The function σ(n) is multiplicative, meaning that if m and n are coprime positive integers (i.e., gcd(m, n) = 1), then σ(mn) = σ(m) σ(n). For a general n with prime n=p1a1p2a2pkakn = p_1^{a_1} p_2^{a_2} \cdots p_k^{a_k}, where each pip_i is a distinct prime and ai1a_i \geq 1, the multiplicativity yields σ(n)=i=1k(1+pi+pi2++piai)=i=1kpiai+11pi1.\sigma(n) = \prod_{i=1}^k \left(1 + p_i + p_i^2 + \cdots + p_i^{a_i}\right) = \prod_{i=1}^k \frac{p_i^{a_i + 1} - 1}{p_i - 1}. This formula allows efficient computation of σ(n) from the prime factors of n. A positive n is perfect σ(n) = 2n. Equivalently, the abundance (or abundancy index) of n, defined as h(n)=σ(n)nh(n) = \frac{\sigma(n)}{n}, equals 2. For example, the smallest perfect number is 6, since its divisors are 1, 2, 3, and 6, so σ(6) = 1 + 2 + 3 + 6 = 12 = 2 × 6. Similarly, for 28, the divisors are 1, 2, 4, 7, 14, and 28, giving σ(28) = 1 + 2 + 4 + 7 + 14 + 28 = 56 = 2 × 28. No p is perfect, as σ(p) = 1 + p < 2p for any prime p > 1. This follows directly from the definition, since the only positive divisors of p are 1 and p. The divisor sum function relates closely to the concept of aliquot parts, where the sum of proper divisors s(n) is defined as s(n) = σ(n) - n (excluding n itself). Thus, n is perfect if s(n) = n.

Historical Development

Ancient and Medieval Contributions

The concept of perfect numbers emerged in as numbers equal to the sum of their proper divisors. , in his Elements (c. 300 BCE), provided the earliest systematic characterization in Book IX, Proposition 36, stating that if 2p12^p - 1 is prime, then 2p1(2p1)2^{p-1}(2^p - 1) is a perfect number. This formulation implicitly generates the first two known perfect numbers, 6 and 28, through the cases p=2p=2 and p=3p=3, respectively, where 3 and 7 are Mersenne primes. Around 100 CE, of Gerasa expanded on these ideas in his Introduction to Arithmetic, listing the first four perfect numbers—6, 28, 496, and 8128—as exemplars of numerical harmony between abundance and deficiency. He emphasized their rarity, noting that they occur infrequently and always even, a pattern observed empirically from Euclid's construction. Nicomachus's work influenced subsequent generations by framing perfect numbers within Pythagorean classifications of numerical properties, portraying them as balanced and self-sufficient. of (c. 245–325 CE), drawing from , further elaborated on perfect numbers in his Theology of Arithmetic, associating them with cosmic and completeness. He described the perfect numbers within the decad (1 through 10) as embodying proportional equality, linking 6 to the synthesis of unity and multiplicity in a balanced whole, and viewing their structure as reflective of divine order and musical concords like the fourth and . Ancient thinkers also imbued perfect numbers with mystical significance, connecting 6 to the six days of creation in and Pythagorean cosmogonies, symbolizing the world's perfected formation before rest. Similarly, 28 was tied to the lunar cycle of approximately 28 days, representing celestial completeness and rhythmic harmony in the natural order. These associations underscored the Pythagorean view of numbers as archetypal principles underlying reality. In the medieval Islamic world, scholars built upon Greek foundations; Thābit ibn Qurra (c. 836–901 CE) generalized Euclid's form for perfect numbers to derive amicable pairs, where two distinct numbers are each the sum of the proper divisors of the other, using expressions like 32n113 \cdot 2^{n-1} - 1 for prime factors when n>2n > 2. This extension, detailed in his astronomical and mathematical treatises, highlighted interconnections between perfect, amicable, and deficient numbers within divisor sum theory. European medieval mathematics revived interest through Leonardo of (Fibonacci, c. 1170–1250 CE), who referenced perfect numbers in his (1202), illustrating their generation via Euclid's method and including 496 as an example to demonstrate computational techniques with Hindu-Arabic numerals. Fibonacci's inclusion helped disseminate ancient Greek arithmetic to the Latin West, integrating perfect numbers into practical and theoretical instruction.

Modern Formulations

In the 18th century, Leonhard Euler advanced the understanding of even perfect numbers through his correspondence with , proving that every even perfect number must be of the form 2p1(2p1)2^{p-1}(2^p - 1), where 2p12^p - 1 is a . This result, published posthumously in Euler's Opera Omnia (Volume 3, 1921), provided a complete characterization of even perfect numbers, building on Euclid's earlier generation method and confirming that no other forms exist for even cases. Euler's proof relied on analyzing the sum function for numbers with exactly two distinct prime factors, one of which is 2, demonstrating that deviations from this structure lead to abundance or deficiency. Advancements continued into the with computational efforts verifying and corresponding perfect numbers. In 1726, French mathematician Pierre de Lagny computed and confirmed the perfect number 230(2311)=2,305,843,008,139,952,1282^{30}(2^{31} - 1) = 2,305,843,008,139,952,128, associated with the 23112^{31} - 1, extending the known list beyond Cataldi's earlier claims. By the , manual calculations yielded further discoveries, such as the perfect number 288(2891)2^{88}(2^{89} - 1) found by American mathematician R. E. Powers in 1911, highlighting the growing reliance on systematic prime testing despite the labor-intensive nature of the work. The marked a shift toward mechanized in searches, directly impacting perfect number verification. In , American mathematician Derrick Henry Lehmer used desk calculators to confirm the compositeness of 225712^{257} - 1 (one of Mersenne's conjectured primes) and verify even perfect numbers up to exponents around 100, establishing early computational benchmarks that ruled out smaller undiscovered cases. These efforts linked perfect number theory to broader primality ing, with the Lucas-Lehmer —refined by Lehmer in —enabling efficient checks for Mersenne primality. As of November 2025, 52 even perfect numbers are known, all generated from s discovered primarily through the (GIMPS), with the largest corresponding to the Mersenne prime 213627984112^{136279841} - 1 found in 2024. Theoretical progress on odd perfect numbers includes Touchard's 1953 result that any such number, if it exists, must be congruent to 1 modulo 12 or 9 modulo 36, severely restricting possible forms and implying a sparse distribution among odd integers. Recent constraints, such as those by Pascal Ochem and , establish that an odd perfect number must exceed 10150010^{1500}, based on exhaustive checks and structural inequalities involving prime factors.

Even Perfect Numbers

Euclid-Euler Theorem

The states that an even positive is perfect it is of the form 2p1(2p1)2^{p-1}(2^p - 1), where pp is a and 2p12^p - 1 is a . In Book IX, 36 of the Elements, established the forward implication: if 2p12^p - 1 is prime for prime pp, then n=2p1(2p1)n = 2^{p-1}(2^p - 1) is perfect. To see this, note that the divisor sum function σ\sigma is multiplicative, so σ(n)=σ(2p1)σ(2p1)=(2p1)((2p1)+1)=(2p1)2p=22p1(2p1)=2n,\sigma(n) = \sigma(2^{p-1}) \cdot \sigma(2^p - 1) = (2^p - 1) \cdot ( (2^p - 1) + 1 ) = (2^p - 1) \cdot 2^p = 2 \cdot 2^{p-1}(2^p - 1) = 2n, as required for perfection. Euler completed the characterization in 1747 by proving the converse: every even perfect number has Euclid's form. To outline the proof, suppose nn is an even perfect number, so σ(n)=2n\sigma(n) = 2n. Write n=2amn = 2^a m with m>1m > 1 odd. Multiplicativity of σ\sigma yields σ(2a)σ(m)=2a+1m,\sigma(2^a) \cdot \sigma(m) = 2^{a+1} m, and since σ(2a)=2a+11\sigma(2^a) = 2^{a+1} - 1, (2a+11)σ(m)=2a+1m    σ(m)=2a+1m2a+11.(2^{a+1} - 1) \sigma(m) = 2^{a+1} m \implies \sigma(m) = \frac{2^{a+1} m}{2^{a+1} - 1}. Let r=a+1r = a + 1, so 2r12^r - 1 divides mm (as it is coprime to 2a+12^{a+1} and divides the right side). Thus, m=(2r1)km = (2^r - 1) k for some odd integer k1k \geq 1. Substituting gives σ(2r1)σ(k)=2rk    σ(2r1)σ(k)k=2r.\sigma(2^r - 1) \cdot \sigma(k) = 2^r k \implies \sigma(2^r - 1) \cdot \frac{\sigma(k)}{k} = 2^r. Here, σ(k)/k1\sigma(k)/k \geq 1 with equality if and only if k=1k = 1, so σ(2r1)2r\sigma(2^r - 1) \leq 2^r. But σ(2r1)1+(2r1)=2r\sigma(2^r - 1) \geq 1 + (2^r - 1) = 2^r, forcing equality: k=1k = 1 and σ(2r1)=2r\sigma(2^r - 1) = 2^r. The latter holds if and only if 2r12^r - 1 is prime (for if composite, it has at least four divisors, yielding σ(2r1)>2r\sigma(2^r - 1) > 2^r). Finally, rr must be prime, as composite exponents yield composite Mersenne numbers. Thus, m=2r1m = 2^r - 1 is a Mersenne prime, a=r1a = r - 1, and n=2r1(2r1)n = 2^{r-1}(2^r - 1) with rr prime.

Properties and Generation

Even perfect numbers are generated using Mersenne primes q=2p1q = 2^p - 1, where pp is a , via the formula Np=2p1qN_p = 2^{p-1} q. This pairing, established by the Euclid-Euler theorem, produces all known even perfect numbers. As of November 2025, 52 such Mersenne primes are known, yielding 52 even perfect numbers, with the largest corresponding to p=136,279,841p = 136{,}279{,}841. The number of digits in NpN_p is approximately plog104p \log_{10} 4, or roughly 0.60206p0.60206 p; for the largest known, this exceeds 82 million digits. All even perfect numbers possess several distinctive properties. They are triangular numbers, expressible as Np=T2p1N_p = T_{2^p - 1}, where the kk-th triangular number is given by Tk=k(k+1)2.T_k = \frac{k(k+1)}{2}. Additionally, due to their form, even perfect numbers are hexagonal numbers, satisfying the equation for the mm-th hexagonal number Hm=m(2m1)H_m = m(2m - 1) with m=2p1m = 2^{p-1}. Each even perfect number is even and has exactly two distinct prime factors: 2 (with multiplicity p1p-1) and the qq. They end in either 6 or 8 in base 10; for example, 6 ends in 6, 28 in 8, 496 in 6, and 8128 in 8. The sum of the digits of even perfect numbers lacks a general closed-form formula. Representative examples include N2=6N_2 = 6 (digit sum 6) and N3=28N_3 = 28 (digit sum 10). No three even perfect numbers can be consecutive integers, as they are all even; the gaps between successive even perfect numbers grow exponentially with increasing pp.

Odd Perfect Numbers

Existence and Impossibility Attempts

The existence of odd perfect numbers remains one of the most enduring open problems in , with a prevailing that none exist, though this has neither been proven nor disproven. In the , Leonhard Euler made significant progress by demonstrating that if an odd perfect number exists, it must take the form N=pkm2N = p^k m^2, where pp is a prime congruent to 1 modulo 4, k1(mod4)k \equiv 1 \pmod{4}, and mm is a positive not divisible by pp. This structural constraint, known as the Eulerian form, has guided subsequent research by imposing necessary conditions on any potential odd perfect number. Early efforts to construct or refute odd perfect numbers included René Descartes' 1638 example of a "spoof" odd perfect number, 3272112132220213^2 \cdot 7^2 \cdot 11^2 \cdot 13^2 \cdot 22021, which would be perfect if the composite factor 22021 (equal to 6119261 \cdot 19^2) were prime, highlighting the challenges in verifying such forms. In the 20th century, Jacques Touchard advanced the impossibility side by proving in 1953 that any odd perfect number must be congruent to 1 modulo 12 or 9 modulo 36, a result that underscores their rarity compared to even perfect numbers. Further heuristic arguments against existence emerged in the 1970s from Carl Pomerance, who developed a probabilistic model suggesting that no odd perfect number exists below 1030010^{300}, based on the expected distribution of the divisor sum function. Partial impossibility proofs have ruled out specific forms, such as Rudolf Steuerwald's 1937 demonstration that no odd perfect number can have all even exponents equal to 2 in its prime factorization. More recent theoretical work includes Pascal Ochem and Carl Pomerance's 2012 analysis, which established that any odd perfect number must have at least eight distinct prime factors, tightening constraints through sieve methods and bounds on the abundancy index. This was later improved to at least 10 distinct prime factors by Pace Nielsen in 2015. Additional attempts have explored implications from broader conjectures, such as connections to the , which could impose further restrictions on the prime factors and growth of the divisor sum, though these remain conditional. Heuristically, if odd perfect numbers exist, results like Leonard Eugene Dickson's 1913 theorem imply there would be only finitely many with a fixed number of distinct prime factors, suggesting infinitely many overall but with zero in the natural numbers. Computational searches have verified the absence of odd perfect numbers in ranges up to extremely large values, supporting these theoretical improbabilities.

Computational Bounds and Constraints

Extensive computational efforts have established stringent lower bounds on the magnitude of any odd perfect number. As of November 2025, no odd perfect number exists below 10220010^{2200}, with ongoing efforts targeting 10230010^{2300}, improving upon earlier bounds such as 10150010^{1500} established by Ochem and Rao in through systematic sieving and branching algorithms that rule out candidates by their prime factorizations. Structural constraints further limit the possible forms of odd perfect numbers, assuming Euler's form N=pkm2N = p^k m^2 where pp is a prime congruent to 1 4 and k1(mod4)k \equiv 1 \pmod{4}. Odd perfect numbers cannot be prime powers, as the abundancy index σ(N)/N=2\sigma(N)/N = 2 would require incompatible divisor sums for powers of a single prime. Moreover, they must have at least 115 prime factors counting multiplicity (Ω(N)115\Omega(N) \geq 115) and at least 10 distinct prime factors (ω(N)10\omega(N) \geq 10), with these bounds derived from inequalities on the abundancy via the multiplicativity of the σ\sigma; if not divisible by 3, the number of distinct primes rises to at least 12. Additionally, any odd perfect number must include a prime factor exceeding 10810^8, ensuring significant sparsity in small factors. Computational searches have exhaustively verified the absence of odd perfect numbers up to extraordinarily large limits using the multiplicativity of σ\sigma to test candidates by decomposing them into potential Euler components and checking divisor sums. In the 1990s, Brent, Cohen, and te Riele pushed the bound beyond 1030010^{300} via tree-search algorithms that enumerate and eliminate forms incompatible with perfection. More recent distributed computing efforts, including the ongoing work documented on the LIRMM Odd Perfect Numbers page, have extended verifications to beyond 10100010^{1000}, with targets reaching 10230010^{2300} by November 2025 through parallel sieving of composite factors and abundancy bounds. Specific modular and divisibility constraints provide additional computational filters. Odd perfect numbers cannot be divisible by 105 (3×5×73 \times 5 \times 7), a result stemming from exhaustive case analysis on small prime combinations that force the abundancy to deviate from 2. Recent advances, including 2023 preprints and unpublished extensions, have tightened unconditional bounds to over 10200010^{2000} in some sieving frameworks and conditional bounds approaching 10300010^{3000} assuming restrictions on the Euler prime, while confirming at least 10 distinct primes as a baseline. These results rely on optimized implementations of σ\sigma's multiplicativity to search spaces efficiently.

Broader Concepts

Classification of Numbers by Divisor Sums

Positive integers are classified according to the relationship between the sum of their , denoted σ(n), and twice the number itself, 2n. A number n is deficient if σ(n) < 2n, perfect if σ(n) = 2n, and abundant if σ(n) > 2n. This classification positions perfect numbers as the boundary case in the spectrum of divisor sum abundance. For example, all prime numbers p are deficient since σ(p) = p + 1 < 2p, while 12 is the smallest abundant number with σ(12) = 28 > 24, and 6 and 496 are even perfect numbers satisfying σ(6) = 12 = 2×6 and σ(496) = 992 = 2×496. The abundance index, defined as h(n) = σ(n)/n, provides a normalized measure of this relationship, where deficient numbers have h(n) < 2, perfect numbers have h(n) = 2, and have h(n) > 2. Among abundant numbers, a primitive abundant number is one whose proper are all deficient. The smallest primitive abundant number is 20. For instance, 18 is abundant with σ(18) = 39 > 36 but not primitive, as it has the perfect proper divisor 6. A related concept is the primitive pseudoperfect number, which belongs to the subset of abundant numbers known as pseudoperfect: those expressible as the sum of some (but not all) of their proper divisors. A primitive pseudoperfect number is pseudoperfect but has no proper divisors that are themselves pseudoperfect. The smallest such number is 6. Regarding distribution, nearly all positive integers are deficient, while the set of abundant numbers has a positive bounded between 0.2474 and 0.2480, implying a density of approximately 0.2476. This density underscores that abundant numbers, including multiples of perfect numbers, form a substantial but minority portion of the integers.

Generalizations and Extensions

Multiperfect numbers generalize perfect numbers by requiring the sum of divisors function σ(n) to equal k n for some integer k > 1, where k=2 recovers the perfect case. For k=3, these are called triperfect numbers; the smallest is 120, with σ(120) = 360 = 3 × 120. As of 2023, exactly six triperfect numbers are known: 120, 672, 523776, 459818240, 1476304896, and 51001180160, all even and discovered through exhaustive up to bounds exceeding 10^{18}. For k=4, known as quadruperfect numbers, 36 are known, with the smallest being 30240, where σ(30240) = 120960 = 4 × 30240; these were fully enumerated by 1929. Higher k yield more examples: 65 quintuplerfect (k=5) numbers are known, starting at 14182439040, and the counts increase rapidly, with over 2000 for k=9, reflecting computational searches that have identified thousands across k up to 11. Hyperperfect numbers extend the divisor sum concept iteratively, defining a k-hyperperfect number n as one satisfying n = 1 + k (σ(n) - n - 1), which for k=1 reduces to the perfect number condition σ(n) = 2n. Unlike multiperfect numbers, which scale the total sum linearly, hyperperfect numbers involve a specific adjustment for proper divisors excluding 1 and n. All even perfect numbers are 1-hyperperfect, but hyperperfect numbers are more abundant; for example, 21 is 2-hyperperfect since σ(21) = 32 and 21 = 1 + 2(32 - 21 - 1). Infinite families exist, such as for odd k where n = p^{k} (p prime) or products of primes, and computations have identified millions below 10^{12}. Harmonic divisor numbers, also known as numbers, generalize perfect numbers through the of divisors: a number n is harmonic divisor if the d(n) n / σ(n) is an , where d(n) is the number of divisors. For perfect numbers, this mean equals d(n)/2, which is since even perfect numbers have an even number of divisors. The smallest non-trivial examples include 6 and 28 (perfect), but also 140, where the is 6; over 10,000 such numbers are known below 10^6, often sharing properties with abundant or deficient numbers but unified by this mean condition. Weird numbers provide a contrasting extension, defined as abundant numbers (σ(n) > 2n) that are not pseudoperfect, meaning no of their proper divisors sums exactly to n. The smallest is 70, with proper divisors summing to 74 > 70 but no combination equaling 70; unlike pseudoperfect numbers (which include all perfect and some abundant), numbers resist subset sums to their value. Only even numbers are known, with 29 primitive weird numbers below 10^8, and it remains open whether odd ones exist. Sociable numbers extend amicable pairs (2-cycles in aliquot sequences, where σ(a) - a = b and σ(b) - b = a) to longer cycles of length greater than 2, where the aliquot parts cycle through a sequence returning to the start. The smallest sociable cycle of length 4 is 1264460 → 1547860 → 1727636 → 1305184 → 1264460; longer cycles, up to length 28, have been discovered computationally, with all known examples even and abundant on average. No odd multiperfect numbers greater than 1 are known, and partial results establish stringent lower bounds: any odd perfect number (k=2) must exceed 10^{1500} and have at least 9 distinct prime factors if it exists. These bounds arise from constraints on the Euler prime factor and overall abundancy, with no odd examples found despite extensive computational searches.

References

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