Mersenne prime



         


In mathematics, a Mersenne prime is a prime number that is one less than a power of two. For example, 3 = 4 − 1 = 22 − 1 is a Mersenne prime; so is 7 = 8 − 1 = 23 − 1. On the other hand, 15 = 16 − 1 = 24 − 1, for example, is not a prime.

More generally, Mersenne numbers (not necessarily primes, but candidates for primes) are numbers that are one less than a power of two; hence,

Mn = 2n − 1.

Mersenne primes have a close connection to perfect numbers, which are numbers that are equal to the sum of their proper divisors. Historically, the study of Mersenne primes was motivated by this connection; in the 4th century BC Euclid demonstrated that if M is a Mersenne prime then M(M+1)/2 is a perfect number. Two millennia later, in the 18th century, Euler proved that all even perfect numbers have this form. No odd perfect numbers are known, and it is suspected that none exist.

It is currently unknown whether there is an infinite number of Mersenne primes.

The calculation

<math>(2^a-1)\cdot (1+2^a+2^{2a}+2^{3a}+\dots+2^{(b-1)a})=2^{ab}-1<math>

shows that Mn can be prime only if n itself is prime, which simplifies the search for Mersenne primes considerably. But the converse is not true; Mn may be composite even though n is prime. For example, 211 − 1 = 23 · 89.

Fast algorithms for finding Mersenne primes are available, and this is why the largest known prime numbers today are Mersenne primes.

The first four Mersenne primes M2, M3, M5, M7 were known in antiquity. The fifth, M13, was discovered anonymously before 1461; the next two (M17 and M19) were found by Cataldi in 1588. After more than a century M31 was verified to be prime by Euler in 1750. The next (in historical, not numerical order) was M127, found by Lucas in 1876, then M61 by Pervushin in 1883. Two more - M89 and M107 - were found early in the 20th century, by Powers in 1911 and 1914, respectively.

The numbers are named after 17th century French mathematician Marin Mersenne, who provided a list of Mersenne primes with exponents up to 257; unfortunately, his list was not correct, though, as he mistakenly included M67 and M257, and omitted M61, M89 and M107.

The best method presently known for testing the primality of Mersenne numbers is based on the computation of a recurring sequence, as developed originally by Lucas in 1878 and improved by Lehmer in the 1930s, now known as the Lucas-Lehmer test. Specifically, it can be shown that Mn = 2n − 1 is prime if and only if Mn evenly divides Sn-2, where S0 = 4 and for k > 0, Sk = Sk − 12 − 2.

The search for Mersenne primes was revolutionized by the introduction of the electronic digital computer. The first successful identification of a Mersenne prime, M521, by this means was achieved at 10:00 P.M. on January 30, 1952 using the U.S. National Bureau of Standards Western Automatic Computer (SWAC) at the Institute for Numerical Analysis at the University of California, Los Angeles, under the direction of Lehmer, with a computer search program written and run by Prof. R.M. Robinson. It was the first Mersenne prime to be identified in thirty-eight years; the next one, M607, was found by the computer a little less than two hours later. Three more - M1279, M2203, M2281 - were found by the same program in the next several months.

As of May 2004, only 41 Mersenne primes were known; the largest known prime number (224,036,583 − 1) is a Mersenne prime. Like several previous Mersenne primes, it was discovered by a distributed computing project on the Internet, known as the Great Internet Mersenne Prime Search (GIMPS). The table below lists all known Mersenne primes (sequence in OEIS):

#nMnDigits in MnDate of discoveryDiscoverer
1231ancientancient
2371ancientancient
35312ancientancient
471273ancientancient
513819141456anonymous
61713107161588Cataldi
71952428761588Cataldi
8312147483647101772Euler
9612305843009213693951191883Pervushin
1089618970019…449562111271911Powers
11107162259276…010288127331914Powers
12127170141183…884105727391876Lucas
13521686479766…115057151157January 30 1952Robinson
14607531137992…031728127183January 30 1952Robinson
151,279104079321…168729087386June 25 1952Robinson
162,203147597991…697771007664October 7 1952Robinson
172,281446087557…132836351687October 9 1952Robinson
183,217259117086…9093150719691957Riesel
194,253190797007…3504849911,2811961Hurwitz
204,423285542542…6085806071,3321961Hurwitz
219,689478220278…2257541112,9171963Gillies
229,941346088282…7894635512,993May 16 1963Gillies
2311,213281411201…6963921913,376June 2 1963Gillies
2419,937431542479…9680414716,002March 4 1971Tuckerman
2521,701448679166…5118827516,533October 30 1978Noll & Nickel
2623,209402874115…7792645116,987February 9 1979Noll
2744,497854509824…01122867113,395April 8 1979Nelson & Slowinski
2886,243536927995…43343820725,962September 25 1982Slowinski
29110,503521928313…46551500733,2651988Colquitt & Welsh
30132,049512740276…73006131139,751September 20 1983Slowinski
31216,091746093103…81552844765,050September 6 1985Slowinski
32756,839174135906…544677887227,832February 19 1992Slowinski & Gage
33859,433129498125…500142591258,716January 10 1994Slowinski & Gage
341,257,787412245773…089366527378,632September 3 1996Slowinski & Gage
351,398,269814717564…451315711420,921November 13 1996GIMPS / Joel Armengaud
362,976,221623340076…729201151895,932August 24 1997GIMPS / Gordon Spence
373,021,377127411683…024694271909,526January 27 1998GIMPS / Roland Clarkson
386,972,593437075744…9241937912,098,960June 1 1999GIMPS / Nayan Hajratwala
39*13,466,917924947738…2562590714,053,946November 14 2001GIMPS / Michael Cameron (Canada)
40*20,996,011125976895…8556820476,320,430November 17 2003GIMPS / Michael Shafer
41*24,036,583299410429…7339694077,235,733May 15 2004GIMPS / Josh Findley



*It is not known whether any undiscovered Mersenne primes exist between the 38th (M6972593) and the 41st (M24036583) on this chart; the ranking is therefore provisional.

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