Euclid–Euler theorem
Template:Short description Template:About Template:Good article The Euclid–Euler theorem is a theorem in number theory that relates perfect numbers to Mersenne primes. It states that an even number is perfect if and only if it has the form Template:Math, where Template:Math is a prime number. The theorem is named after mathematicians Euclid and Leonhard Euler, who respectively proved the "if" and "only if" aspects of the theorem.
It has been conjectured that there are infinitely many Mersenne primes. Although the truth of this conjecture remains unknown, it is equivalent, by the Euclid–Euler theorem, to the conjecture that there are infinitely many even perfect numbers. However, it is also unknown whether there exists even a single odd perfect number.[1]
Statement and examples
A perfect number is a natural number that equals the sum of its proper divisors, the numbers that are less than it and divide it evenly (with remainder zero). For instance, the proper divisors of 6 are 1, 2, and 3, which sum to 6, so 6 is perfect.
A Mersenne prime is a prime number of the form Template:Math, one less than a power of two. For a number of this form to be prime, Template:Mvar itself must also be prime, but not all primes give rise to Mersenne primes in this way. For instance, Template:Nowrap is a Mersenne prime, but Template:Nowrap is not.
The Euclid–Euler theorem states that an even natural number is perfect if and only if it has the form Template:Math, where Template:Math is a Mersenne prime.[1] The perfect number 6 comes from Template:Math in this way, as Template:Nowrap, and the Mersenne prime 7 corresponds in the same way to the perfect number 28.
History
Euclid proved that Template:Math is an even perfect number whenever Template:Math is prime. This is the final result on number theory in Euclid's Elements; the later books in the Elements instead concern irrational numbers, solid geometry, and the golden ratio. Euclid expresses the result by stating that if a finite geometric series beginning at 1 with ratio 2 has a prime sum Template:Mvar, then this sum multiplied by the last term Template:Mvar in the series is perfect. Expressed in these terms, the sum Template:Mvar of the finite series is the Mersenne prime Template:Math and the last term Template:Mvar in the series is the power of two Template:Math. Euclid proves that Template:Math is perfect by observing that the geometric series with ratio 2 starting at Template:Mvar, with the same number of terms, is proportional to the original series; therefore, since the original series sums to Template:Math, the second series sums to Template:Math, and both series together add to Template:Math, two times the supposed perfect number. However, these two series are disjoint from each other and (by the primality of Template:Mvar) exhaust all the divisors of Template:Math, so Template:Math has divisors that sum to Template:Math, showing that it is perfect.[2]
Over a millennium after Euclid, Alhazen Template:Circa conjectured that Template:Em even perfect number is of the form Template:Math where Template:Math is prime, but he was not able to prove this result.[3] It was not until the 18th century, over 2000 years after Euclid,[4] that Leonhard Euler proved that the formula Template:Math will yield all the even perfect numbers.[1][5] Thus, there is a one-to-one relationship between even perfect numbers and Mersenne primes; each Mersenne prime generates one even perfect number, and vice versa. After Euler's proof of the Euclid–Euler theorem, other mathematicians have published different proofs, including Victor-Amédée Lebesgue, Robert Daniel Carmichael, Leonard Eugene Dickson, John Knopfmacher, and Wayne L. McDaniel. Dickson's proof, in particular, has been commonly used in textbooks.[6]
This theorem was included in a web listing of the "top 100 mathematical theorems", dating from 1999, which later became used by Freek Wiedijk as a benchmark set to test the power of different proof assistants. By 2024, the proof of the Euclid–Euler theorem had been formalized in 7 of the 12 proof assistants recorded by Wiedijk.[7]
Proof
Euler's proof is short[1] and depends on the fact that the sum of divisors function Template:Mvar is multiplicative; that is, if Template:Mvar and Template:Mvar are any two relatively prime integers, then Template:Math. For this formula to be valid, the sum of divisors of a number must include the number itself, not just the proper divisors. A number is perfect if and only if its sum of divisors is twice its value.
Sufficiency
One direction of the theorem (the part already proved by Euclid) immediately follows from the multiplicative property: every Mersenne prime gives rise to an even perfect number. When Template:Math is prime, The divisors of Template:Math are Template:Math. The sum of these divisors is a geometric series whose sum is Template:Math. Next, since Template:Math is prime, its only divisors are Template:Math and itself, so the sum of its divisors is Template:Math.
Combining these, Therefore, Template:Math is perfect.[8][9][10]
Necessity
In the other direction, suppose that an even perfect number has been given, and partially factor it as Template:Math, where Template:Mvar is odd. For Template:Math to be perfect, the sum of its divisors must be twice its value: Template:NumBlk The odd factor Template:Math on the right side of (∗) is at least 3, and it must divide Template:Mvar, the only odd factor on the left side, so Template:Math is a proper divisor of Template:Mvar. Dividing both sides of (∗) by the common factor Template:Math and taking into account the known divisors Template:Mvar and Template:Mvar of Template:Mvar gives Template:Block indent For this equality to be true, there can be no other divisors. Therefore, Template:Mvar must be Template:Math, and Template:Mvar must be a prime of the form Template:Math.[8][9][10]
References
- ↑ 1.0 1.1 1.2 1.3 Template:Citation.
- ↑ Template:Citation. See in particular Prop. IX.36.
- ↑ Template:MacTutor Biography
- ↑ Template:Citation
- ↑ Template:Citation. Originally read to the Berlin Academy on February 23, 1747, and published posthumously. See in particular section 8, p. 88.
- ↑ Template:Citation
- ↑ Template:Citation
- ↑ 8.0 8.1 Template:Citation.
- ↑ 9.0 9.1 Template:Citation.
- ↑ 10.0 10.1 Template:Citation.