Abundancy | Count | When last number was discovered | Which was last? | Are all discovered? | Estimated total number |
---|---|---|---|---|---|
1 | 1 | - | - | yes and proved | 1 |
2 | 51 | 2018-12-07 | 18.5560326 | no, there are infinitely many | ∞ |
3 | 6 | <= 1643 | 3.2049844 | yes | 6 |
4 | 36 | <= 1929 | 4.3351682 | yes | 36 |
5 | 65 | <= 1990 | 5.1744360 | yes | 65 |
6 | 245 | 1993-05-?? | 5.6720844 | yes | 245 |
7 | 516 | 1994-01-09 | 5.9403364 | almost surely yes | ~ 515 |
8 | 1136 | 2022-05-22 | 6.5244184 | probably yes | ~ 1140 |
9 | 2164 | 2022-06-05 | 7.1993123 | no | ~ 2200 |
10 | 1710 | 2022-06-11 | 7.8125224 | no | ~ 4500 |
11 | 2 | 2022-09-07 | 8.2948075 | no | ~ 10000 |
Search this database of 5932 MPNs
Each search-pattern matches literally, except the wild-characters *,?,!,$ which mean:
* -- arbitrary, maybe empty, sequence of characters
? -- exactly one character
! -- begin of record
$ -- end of record.
Hint: orient on the field separator | or the comma in each record to get easier what you want.
And a further list of multiply perfect numbers sorted only by their factorizations (built from the 5932 MPNs of the master list and gziped 226 kB).
It has each line cut down to 120 columns and no discovery information or comments are given. Rich's
out-dated indentifier is omitted, but a log10(MPN) is given for traditional reasons.
Finally, here are the (email-extracted and edited to put it syntactically in standard form)
0 claimed new (since the database update) found MPNs which I irregularly append (last change: 2023-01-12).
To verify these numbers, three steps must be taken: 1) verify for each number n
given in its prime factorization that all factors are really prime numbers, 2) compute σ(n) which envolves the factorization of large numbers and then check n's claimed abundancy 3) and lastly test whether n is really new.
A = 19^2.127^1.151^0.911^0 B = 19^4.127^0.151^1.911^1 size(A,B) = 4 , k = 4,5,6,7,8,9 [occurs 257 times for the known MPNs] C = 23^1.37^3.73^1.79^0.137^2 D = 23^2.37^1.73^0.79^1.137^1 size(C,D) = 5 , k = 6,7,8,9 [occurs 21 times for the known MPNs] E = 13^1.31^2.61^1.83^1.97^0.331^1 F = 13^2.31^1.61^2.83^0.97^1.331^0 size(E,F) = 6 , k = 6,7,8 [occurs 31 times for the known MPNs] G = 3^10.107^1.137^0.547^0.1093^0.3851^1 H = 3^6.107^0.137^1.547^1.1093^1.3851^0 size(G,H) = 6 , k = 4,5,6 [occurs 31 times for the known MPNs] I = 5^0 J = 5^1 size(I,J) = 1 , k = 5 [occurs 20 times for the known MPNs] K = 7^5.17^1.37^1.43^1.67^0.307^0.1063^0 L = 7^8.17^2.37^2.43^0.67^1.307^1.1063^1 size(K,L) = 7 , k = 7 [occurs 9 times for the known MPNs] M = 7^4.13^4.31^1.43^1.61^1.79^0.97^0.157^0.631^0.30941^1 N = 7^9.13^5.31^0.43^2.61^2.79^2.97^1.157^1.631^1.30941^0 size(M,N) = 10 , k = 5,6,7,8 [occurs 4 times for the known MPNs] P = 2^38.53^1.59^0.157^0.229^1.8191^1.43331^0.121369^1.3033169^0.715827883^0.2147483647^0 Q = 2^61.53^0.59^1.157^1.229^0.8191^0.43331^1.121369^0.3033169^1.715827883^1.2147483647^1 size(P,Q) = 11 , k = 5,6 [occurs 9 times for the known MPNs] R = 13^14.139^0.157^1.181^1.191^2.199^1.229^1.397^1.827^0.1163^1.4651^1.8269^0.14197^0.28393^0.30941^1.40493^1.161971^1 S = 13^11.139^1.157^2.181^2.191^1.199^0.229^2.397^0.827^1.1163^0.4651^0.8269^1.14197^1.28393^1.30941^0.40493^0.161971^0 size(R,S) = 17 , k = 9,10 [occurs 2 times for the known MPNs] T = 3^4.11^3.13^1 U = 3^5.11^1.13^2 size(T,U) = 3 , k = 6 [occurs 8 times for the known MPNs] V = 5^2.7^2.11^1.31^1.71^0 W = 5^4.7^3.11^2.31^0.71^1 size(V,W) = 5 , k = 6 [occurs 8 times for the known MPNs]They are as more important, as fewer primes are involved in such a substitution. As larger the smallest prime in such a pair is, as more usefull it is, too. On the other hand, as smaller the quotient of the number of different primes in n to the size of the substitution becomes, as more worthless such a substitution becomes for this n. Therefore we demand arbitrarily that the size of a substitution must be less than the number of different primes in each of the two components. Sadly it looks like that substitutions occur only for mpns with small abundancy as the following table of counts for substitutions of size of at most 12 suggests:
Abundancy | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 |
---|---|---|---|---|---|---|---|---|---|
# known mpns | 6 | 36 | 65 | 245 | 516 | 1136 | 2164 | 1710 | 2 |
# different subst | 0 | 30 | 37 | 283 | 59 | 6 | 2 | 0 | 0 |
period / year | Antiquity | Middle Ages | < 1910 | < 1915 | < 1930 | < 1955 | < 1980 | < 1990 | 1991 | 1992 | 1993 | 1994 | 1995 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
known MPNs | 5 | 35 | 47 | 235 | 347 | 556 | 596 | 611 | 713 | 1179 | 1821 | 1983 | 2101 |
increament | 5 | 30 | 12 | 188 | 112 | 209 | 40 | 15 | 102 | 466 | 642 | 162 | 118 |
period | 1996 | 1997 | 1998 | 1999 | 2000 | 2001 | 2002 | 2003 | 2004 | 2005 | 2006 | 2007 | 2008 | 2009 | 2010 | 2011 | 2012 | 2013 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
known MPNs | 2335 | 3051 | 3259 | 3464 | 4501 | 4997 | 5040 | 5050 | 5147 | 5189 | 5222 | 5245 | 5271 | 5287 | 5301 | 5303 | 5307 | 5311 |
increament | 234 | 716 | 208 | 205 | 1037 | 496 | 43 | 10 | 97 | 42 | 33 | 23 | 26 | 16 | 14 | 2 | 4 | 4 |
period / year | 2014 | 2015 | 2016 | 2017 | 2018 | 2019 | 2020 | 2021 | 2022 |
---|---|---|---|---|---|---|---|---|---|
known MPNs | 5311 | 5311 | 5312 | 5314 | 5315 | 5315 | 5315 | 5772 | 5932 |
increament | 0 | 0 | 1 | 2 | 1 | 0 | 0 | 457 | 160 |
Now a list of the discoverer names follows according to Rich Schroeppel (report him, if you think you aren't credited sufficiently):
Discoverer | count | period | Discoverer | count | period |
---|---|---|---|---|---|
Armengaud&Woltman&et.al. | 1* | 1996 | Brown | 78 | 1954 |
Cameron&Woltman&Kurowski&et.al. | 1* | 2001 | Carmichael | 98 | 1907-1911 |
Cataldi | 2* | 1588 | Clarkson&Woltman&Kurowski&et.al. | 1* | 1998 |
codex-Lat.-Monac.- | 1* | 1456 | Colquitt&Welsh | 1* | 1988 |
Cooper&Boone&Woltman&Kurowski&et.al. | 2* | 2005-2006 | Cooper&Woltman&Kurowski&et.al. | 1* | 2013 |
Cooper&Woltman&Kurowski&Blosser&et.al. | 1* | 2016 | Cunningham | 3 | 1902 |
Descartes | 9 | 1638-1639 | Dokshitzer&Vasyunin | 1 | 1993 |
Euclid | 4* | -275 | Euler | 1* | 1772 |
Elvenich&Woltman&Kurowski&et.al. | 1* | 2008 | Fermat | 11? | 1636-1643 |
Findley&Woltman&Kurowski&et.al. | 1* | 2004 | Flammenkamp | 137 | 1993-2000 |
Flammenkamp&Woltman | 344 | 2000-2001 | Franqui&Garcia | 135 | 1953-1954 |
Freniclei | 3 | 1638 | Gage&Slowinski | 3* | 1992-1996 |
Gillies | 3* | 1963 | Gretton | 123 | 1990-1993 |
Gretton&Schroeppel | 5 | 1991-1992 | Hajratwala&Woltman&Kurowski&et.al. | 1* | 1999 |
Harrison&Moxham | 3 | 2000 | Helenius | 1261 | 1992-1997 |
Helenius&Schroeppel | 16 | 1993 | Hurwitz&Selfridge | 2* | 1961 |
in-Mersenne-epoch | 4 | 1639-1643 | Jumeau | 1 | 1638 |
Kapek&Moxham | 1 | 2000 | Laroche&Woltman&Blosser&et.al. | 1* | 2018 |
Lehmer | 5 | 1901 | Lucas | 1* | 1876 |
Martinson&Moxham | 1 | 2000 | Mason | 89 | 1911 |
Moxham | 1006 | 1995-2001 | Nelson&Slowinski | 1* | 1979 |
Nickel&Noll | 1* | 1978 | Noll | 1* | 1979 |
Nowak&Woltman&Kurowski&et.al. | 1* | 2005 | Pace&Woltman&Kurowski&Blosser&et.al. | 1* | 2017 |
Perrier&Woltman | 38  | 2000 | Pervouchine | 1* | 1883 |
Poulet | 145 | 1929,1954 | Powers | 2* | 1911-1914 |
Pythagoras | 1* | -500 | Recorde | 1 | 1557 |
Riesel | 1* | 1957 | Roberts&Moxham | 2 | 1997 |
Robinson | 5* | 1952 | Schroeppel | 7 | 1983-1991 |
Shafer&Woltman&Kurowski&et.al. | 1* | 2003 | Slowinski | 3* | 1982-1985 |
Smith&Woltman&Kurowski&et.al. | 1* | 2008 | Sorli&Moxham | 27 | 1997-1998 |
Sorli&Woltman | 9 | 2000-2001 | Spence&Woltman&et.al. | 1* | 1997 |
Strindmo&Woltman&Kurowski&et.al. | 1* | 2009 | Toshihiro | 1 | 2017 |
Tuckerman | 1* | 1971 | Whiteside&Moxham | 2 | 1999 |
Woltman | 2416 | 1997-2013,2021-2022 | Yoshitake | 17 | 1974-1993 |
Abundancy | First discovered MPN | Is it smallest? | Date | Discoverer |
---|---|---|---|---|
1 | 1 | yes | ancient | - |
2 | 6 | yes | ancient | - |
3 | 120 | yes | ancient | - |
4 | 30240 | yes | ~ 1638 | R. Descartes |
5 | 14182439040 | yes | ~ 1638 | R. Descartes |
6 | 34111227434420791224041472000 | no | 1643 | P. Fermat |
7 | 6.9545266398342727... *10^70 | no | 1902 | A. J. C. Cunningham |
8 | 2.34111439263306338... *10^161 | no | 1929 | P. Poulet |
9 | 7.9842491755534198... *10^465 | no | 1992-04-15 | F. W. Helenius |
10 | 2.86879876441793479... *10^923 | no | 1997-05-13 | R. M. Sorli |
11 | 2.51850413483992918... *10^1906 | no | 2001-03-13 | G. F. Woltman |
Abund | Smallest value | Largest value | Lowest 2-power | Highest 2-power | Largest eff. expo. | Fewest factors * | Most factors * |
---|---|---|---|---|---|---|---|
2 | 6 (0.5831981) | 10^49724093.6 (18.5560326) | 1 (0.5831981) | 82589932 (18.5560326) | 0 (0.5831981) | 2 (0.5831981) | 82589933 (18.5560326) |
3 | 120 (1.5660066) | 10^10.469 (3.2049844) | 3 (1.5660066) | 14 (3.2049844) | 7 (3.2049844) | 5 (1.5660066) | 19 (3.2049844) |
4 | 30240 (2.3337853) | 10^45.204 (4.6452114) | 2 (2.6806218) | 37 (4.5312242) | 17 (4.5312242) | 8 (2.3415138) | 57 (4.6365489) |
5 | 10^10.148 (3.1516786) | 10^100.276 (5.4419551) | 7 (3.1516786) | 61 (5.0442101) | 45 (5.1777077) | 17 (3.1516786) | 103 (5.3046236) |
6 | 10^20.189 (3.8391453) | 10^192.162 (6.0923690) | 15 (4.0050961) | 92 (6.0923690) | 79 (6.0362173) | 31 (3.8391453) | 164 (6.0923690) |
7 | 10^56.150 (4.8620623) | 10^312.074 (6.5772722) | 29 (5.2987825) | 177 (6.5408889) | 108 (6.4271649) | 71 (4.8620623) | 307 (6.5528603) |
8 | 10^132.917 (5.7237604) | 10^613.291 (7.2528723) | 47 (5.7578915) | 253 (7.1699823) | 156 (7.2528723) | 137 (5.7237604) | 466 (7.1485402) |
9 | 10^286.749 (6.4926404) | 10^1165.883 (7.8952666) | 99 (6.6259527) | 380 (7.8522986) | 283 (7.7478296) | 257 (6.4926404) | 747 (7.8522986) |
10 | 10^638.652 (7.2933919) | 10^1877.645 (8.3718042) | 175 (7.2933919) | 534 (8.3718042) | 434 (8.2500454) | 492 (7.2933919) | 1172 (8.3718042) |
11 | 10^1738.495 (8.2948075) | 10^1906.401 (8.3870050) | 413 (8.2948075) | 468 (8.3870050) | 469 (8.3870050) | 1088 (8.2948075) | 1139 (8.3870050) |
Discovery dates of proper Multiply Perfect Numbers
Abund | First MPN | Smallest MPN | Largest MPN | Latest MPN |
---|---|---|---|---|
3 | ancient (1.5660066) | ancient (1.5660066) | 1643 (3.2049844) | 1643 (3.2049844) |
4 | 1638 (2.3337853) | 1638 (2.3337853) | 1911 (4.6452114) | 1929 (4.3351682) |
5 | 1638 (3.1516786) | 1638 (3.1516786) | 1911 (5.4419551) | 1990 (5.1744360) |
6 | 1643 (4.1850902) | 1907 (3.8391453) | 1992 (6.0923690) | 1993-05-?? (5.6720844) |
7 | 1902 (5.0944883) | 1911 (4.8620623) | 1993 (6.5772722) | 1994-01-09 (5.9403364) |
8 | 1929 (5.9177287) | 1990 (5.7237604) | 1996-04-23 (7.2528723) | 2022-05-22 (6.5244184) |
9 | 1992-04-15 (6.9780083) | 1995-12-06 (6.4926404) | 2001-01-11 (7.8952666) | 2022-06-05 (7.1993123) |
10 | 1997-05-13 (7.6621574) | 2013-01-03 (7.2933919) | 2001-01-28 (8.3718042) | 2022-06-11 (7.8125224) |
11 | 2001-03-13 (8.3870050) | 2022-09-07 (8.2948075) | 2001-03-13 (8.3870050) | 2022-09-07 (8.2948075) |
If the number of MPNs up to a given limit x is proportional to ln(x), then the density of the MPNs should be proportional to 1/x.
And a further picture to visualize the density of the known MPNs.
In first approximation it may be a Poisson-distribution.
You guess that surely there are missing MPNs at last at the currently known 4000th MPN, but also highly probable earlier.
Finally a best linear fit for the smallest 3600 known MPNs except the first 100 MPNs to avoid 'start-effects' was done on a logarithmic scale. For these 3500 numbers this least-quadratic error approximation results a correlation coefficient of 0.99815 with # MPN ~ 2.2328ln(x)-48.3655.
Richard Schroeppel stated
that he constructed all MPNs < 1070 in the eighties of the twenty-century (but probably only 1990),
i.e. he proved that there exist exactly 258 MPNs smaller than 1070 -- and besides showed that there are no odd MPNs < 1090 except 1.
In March 2008 Achim Flammenkamp finally constructed all MPNs < e350 by an exhaustive tree-search, i.e. proved that there are no further but the 730 known MPNs.
Here is a small paper presenting the theoretical and practical background to this computation.
Let us introduce Fred Helenius' notion of the effective exponent.
The prime p=2 is special compared to other primes, because
p-1 has only the trivial divisor 1.
A consequence of this fact is, only if p equals 2, then numbers of the form pn-1 could be prime.
Assume a fixed MPN m has in its prime factorization the two-power exponent k.
This means that σ(m) has a factor 2k+1-1.
Depending on k this factor may have
some prime divisors of the form 2n-1. Because we are
considering a MPN, σ(2n-1) = 2n must be also a factor of this MPN itself, if 2n-1 occurs exactly onetime!
Hence the original prime-power 2k may produce immediately further two-powers.
Or put it in other words: only the `remainder' of this exponent k must be
produced by other prime-powers. So, the exponent is effectively reduced in
consideration to the to-be-generated two-power factors by other prime-powers.
Primes of the form 2n-1 are called Mersenne Primes and are known up to high
values of n. Thus we have to check which Mersenne Prime 2n-1 divide
a given 2k+1-1 exactly onetimes. Subtracting k+1 by such Mersenne Prime exponents n
gives the effective exponent of k.
There is a small blemish in this model: small primes of the form q=2n-1 may
as well be produced by other prime-powers (than two-powers) of a MPN, such that the exponent of q is not 1 in the factorization of the MPN, but larger.
Hence we have probably overestimated the correction of the two-power exponent a bit.
The two-power exponent k of a (2-fold) perfect number has always an effective exponent of 0.
For such an effective exponent of 0, there seems to exist only the corresponding (2-fold) MPN except in the case k equals 2.
If k = in-1 with n the exponent of a Mersenne Prime and i a
small number, the effective exponent is at most n(i-1), roughly 1-1/i of
the given exponent k. Such exponents k
are typically the largest two-power exponents for which a MPN for a fixed proper abundancy exists: 61=2*31-1, 92=3*31-1, 177=2*89-1, 253=2*127-1, 320=3*107-1,380=3*127-1.
Finally, for a given two-power exponent k the effort to compute a MPN
with an even factor of 2k seems more related to its effective exponent than to k --- this
is heuristically convincing and seems likely to be the reason this quantity was invented --- and lastly the distribution of the prime-exponents of
a `typical' MPN seems proportional to the effective exponent than to the
two-power exponent.
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