Multiply perfect number

In mathematics, a multiply perfect number (also called multiperfect number or pluperfect number) is a generalization of a perfect number.
For a given natural number k, a number n is called Template:Nowrap (or Template:Nowrap perfect) if the sum of all positive divisors of n (the divisor function, σ(n)) is equal to kn; a number is thus perfect if and only if it is Template:Nowrap. A number that is Template:Nowrap for a certain k is called a multiply perfect number. As of 2014, Template:Nowrap numbers are known for each value of k up to 11.[1]
It is unknown whether there are any odd multiply perfect numbers other than 1. The first few multiply perfect numbers are:
- 1, 6, 28, 120, 496, 672, 8128, 30240, 32760, 523776, 2178540, 23569920, 33550336, 45532800, 142990848, 459818240, ... Template:OEIS.
Example
The sum of the divisors of 120 is
- 1 + 2 + 3 + 4 + 5 + 6 + 8 + 10 + 12 + 15 + 20 + 24 + 30 + 40 + 60 + 120 = 360
which is 3 × 120. Therefore 120 is a Template:Nowrap number.
Smallest known k-perfect numbers
The following table gives an overview of the smallest known Template:Nowrap numbers for k ≤ 11 Template:OEIS:
| k | Smallest k-perfect number | Factors | Found by |
|---|---|---|---|
| 1 | 1 | ancient | |
| 2 | 6 | 2 × 3 | ancient |
| 3 | 120 | 23 × 3 × 5 | ancient |
| 4 | 30240 | 25 × 33 × 5 × 7 | René Descartes, circa 1638 |
| 5 | 14182439040 | 27 × 34 × 5 × 7 × 112 × 17 × 19 | René Descartes, circa 1638 |
| 6 | 154345556085770649600 (21 digits) | 215 × 35 × 52 × 72 × 11 × 13 × 17 × 19 × 31 × 43 × 257 | Robert Daniel Carmichael, 1907 |
| 7 | 141310897947438348259849...523264343544818565120000 (57 digits) | 232 × 311 × 54 × 75 × 112 × 132 × 17 × 193 × 23 × 31 × 37 × 43 × 61 × 71 × 73 × 89 × 181 × 2141 × 599479 | TE Mason, 1911 |
| 8 | 826809968707776137289924...057256213348352000000000 (133 digits) | 262 × 315 × 59 × 77 × 113 × 133 × 172 × 19 × 23 × 29 × 312 × 37 × 41 × 43 × 53 × 612 × 712 × 73 × 83 × 89 × 972 × 127 × 193 × 283 × 307 × 317 × 331 × 337 × 487 × 5212 × 601 × 1201 × 1279 × 2557 × 3169 × 5113 × 92737 × 649657 | Stephen F. Gretton, 1990[1] |
| 9 | 561308081837371589999987...415685343739904000000000 (287 digits) | 2104 × 343 × 59 × 712 × 116 × 134 × 17 × 194 × 232 × 29 × 314 × 373 × 412 × 432 × 472 × 53 × 59 × 61 × 67 × 713 × 73 × 792 × 83 × 89 × 97 × 1032 × 107 × 127 × 1312 × 1372 × 1512 × 191 × 211 × 241 × 331 × 337 × 431 × 521 × 547 × 631 × 661 × 683 × 709 × 911 × 1093 × 1301 × 1723 × 2521 × 3067 × 3571 × 3851 × 5501 × 6829 × 6911 × 8647 × 17293 × 17351 × 29191 × 30941 × 45319 × 106681 × 110563 × 122921 × 152041 × 570461 × 16148168401 | Fred Helenius, 1995[1] |
| 10 | 448565429898310924320164...000000000000000000000000 (639 digits) | 2175 × 369 × 529 × 718 × 1119 × 138 × 179 × 197 × 239 × 293 × 318 × 372 × 414 × 434 × 474 × 533 × 59 × 615 × 674 × 714 × 732 × 79 × 83 × 89 × 97 × 1013 × 1032 × 1072 × 109 × 113 × 1272 × 1312 × 139 × 149 × 151 × 163 × 179 × 1812 × 191 × 197 × 199 × 2113 × 223 × 239 × 257 × 271 × 281 × 307 × 331 × 337 × 3532 × 367 × 373 × 397 × 419 × 421 × 521 × 523 × 5472 × 613 × 683 × 761 × 827 × 971 × 991 × 1093 × 1741 × 1801 × 2113 × 2221 × 2237 × 2437 × 2551 × 2851 × 3221 × 3571 × 3637 × 3833 × 4339 × 5101 × 5419 × 6577 × 6709 × 7621 × 7699 × 8269 × 8647 × 11093 × 13421 × 13441 × 14621 × 17293 × 26417 × 26881 × 31723 × 44371 × 81343 × 88741 × 114577 × 160967 × 189799 × 229153 × 292561 × 579281 × 581173 × 583367 × 1609669 × 3500201 × 119782433 × 212601841 × 2664097031 × 2931542417 × 43872038849 × 374857981681 × 4534166740403 | George Woltman, 2013[1] |
| 11 | 251850413483992918774837...000000000000000000000000 (1907 digits) | 2468 × 3140 × 566 × 749 × 1140 × 1331 × 1711 × 1912 × 239 × 297 × 3111 × 378 × 415 × 433 × 473 × 534 × 593 × 612 × 674 × 714 × 733 × 79 × 832 × 89 × 974 × 1014 × 1033 × 1093 × 1132 × 1273 × 1313 × 1372 × 1392 × 1492 × 151 × 1572 × 163 × 167 × 173 × 181 × 191 × 1932 × 197 × 199 × 2113 × 223 × 227 × 2292 × 239 × 251 × 257 × 263 × 2693 × 271 × 2812 × 293 × 3073 × 313 × 317 × 331 × 347 × 349 × 367 × 373 × 397 × 401 × 419 × 421 × 431 × 4432 × 449 × 457 × 461 × 467 × 491 × 4992 × 541 × 547 × 569 × 571 × 599 × 607 × 613 × 647 × 691 × 701 × 719 × 727 × 761 × 827 × 853 × 937 × 967 × 991 × 997 × 1013 × 1061 × 1087 × 1171 × 1213 × 1223 × 1231 × 1279 × 1381 × 1399 × 1433 × 1609 × 1613 × 1619 × 1723 × 1741 × 1783 × 1873 × 1933 × 1979 × 2081 × 2089 × 2221 × 2357 × 2551 × 2657 × 2671 × 2749 × 2791 × 2801 × 2803 × 3331 × 3433 × 4051 × 4177 × 4231 × 5581 × 5653 × 5839 × 6661 × 7237 × 7699 × 8081 × 8101 × 8269 × 8581 × 8941 × 10501 × 11833 × 12583 × 12941 × 13441 × 14281 × 15053 × 17929 × 19181 × 20809 × 21997 × 23063 × 23971 × 26399 × 26881 × 27061 × 28099 × 29251 × 32051 × 32059 × 32323 × 33347 × 33637 × 36373 × 38197 × 41617 × 51853 × 62011 × 67927 × 73547 × 77081 × 83233 × 92251 × 93253 × 124021 × 133387 × 141311 × 175433 × 248041 × 256471 × 262321 × 292561 × 338753 × 353641 × 441281 × 449653 × 509221 × 511801 × 540079 × 639083 × 696607 × 746023 × 922561 × 1095551 × 1401943 × 1412753 × 1428127 × 1984327 × 2556331 × 5112661 × 5714803 × 7450297 × 8334721 × 10715147 × 14091139 × 14092193 × 18739907 × 19270249 × 29866451 × 96656723 × 133338869 × 193707721 × 283763713 × 407865361 × 700116563 × 795217607 × 3035864933 × 3336809191 × 35061928679 × 143881112839 × 161969595577 × 287762225677 × 761838257287 × 840139875599 × 2031161085853 × 2454335007529 × 2765759031089 × 31280679788951 × 75364676329903 × 901563572369231 × 2169378653672701 × 4764764439424783 × 70321958644800017 × 79787519018560501 × 702022478271339803 × 1839633098314450447 × 165301473942399079669 × 604088623657497125653141 × 160014034995323841360748039 × 25922273669242462300441182317 × 15428152323948966909689390436420781 × 420391294797275951862132367930818883361 × 23735410086474640244277823338130677687887 × 628683935022908831926019116410056880219316806841500141982334538232031397827230330241 | George Woltman, 2001[1] |
Properties
It can be proven that:
- For a given prime number p, if n is Template:Nowrap and p does not divide n, then pn is Template:Nowrap. This implies that an integer n is a Template:Nowrap number divisible by 2 but not by 4, if and only if n/2 is an odd perfect number, of which none are known.
- If 3n is Template:Nowrap and 3 does not divide n, then n is Template:Nowrap.
Odd multiply perfect numbers
It is unknown whether there are any odd multiply perfect numbers other than 1. However if an odd Template:Nowrap number n exists where k > 2, then it must satisfy the following conditions:[2]
- The largest prime factor is ≥ 100129
- The second largest prime factor is ≥ 1009
- The third largest prime factor is ≥ 101
Bounds
In little-o notation, the number of multiply perfect numbers less than x is for all ε > 0.[2]
The number of k-perfect numbers n for n ≤ x is less than , where c and c' are constants independent of k.[2]
Under the assumption of the Riemann hypothesis, the following inequality is true for all Template:Nowrap numbers n, where k > 3
where is Euler's gamma constant. This can be proven using Robin's theorem.
The number of divisors τ(n) of a Template:Nowrap number n satisfies the inequality[3]
The number of distinct prime factors ω(n) of n satisfies[4]
If the distinct prime factors of n are , then:[4]
Specific values of k
Perfect numbers
Template:Main A number n with σ(n) = 2n is perfect.
Triperfect numbers
A number n with σ(n) = 3n is triperfect. There are only six known triperfect numbers and these are believed to comprise all such numbers:
- 120, 672, 523776, 459818240, 1476304896, 51001180160 Template:OEIS
If there exists an odd perfect number m (a famous open problem) then 2m would be Template:Nowrap, since σ(2m) = σ(2) σ(m) = 3×2m. An odd triperfect number must be a square number exceeding 1070 and have at least 12 distinct prime factors, the largest exceeding 105.[5]
Variations
Unitary multiply perfect numbers
A similar extension can be made for unitary perfect numbers. A positive integer n is called a unitary multi Template:Nowrap number if σ*(n) = kn where σ*(n) is the sum of its unitary divisors. (A divisor d of a number n is a unitary divisor if d and n/d share no common factors.).
A unitary multiply perfect number is simply a unitary multi Template:Nowrap number for some positive integer k. Equivalently, unitary multiply perfect numbers are those n for which n divides σ*(n). A unitary multi Template:Nowrap number is naturally called a unitary perfect number. In the case k > 2, no example of a unitary multi Template:Nowrap number is yet known. It is known that if such a number exists, it must be even and greater than 10102 and must have more than forty four odd prime factors. This problem is probably very difficult to settle. The concept of unitary divisor was originally due to R. Vaidyanathaswamy (1931) who called such a divisor as block factor. The present terminology is due to E. Cohen (1960).
The first few unitary multiply perfect numbers are:
- 1, 6, 60, 90, 87360 Template:OEIS
Bi-unitary multiply perfect numbers
A positive integer n is called a bi-unitary multi Template:Nowrap number if σ**(n) = kn where σ**(n) is the sum of its bi-unitary divisors. This concept is due to Peter Hagis (1987). A bi-unitary multiply perfect number is simply a bi-unitary multi Template:Nowrap number for some positive integer k. Equivalently, bi-unitary multiply perfect numbers are those n for which n divides σ**(n). A bi-unitary multi Template:Nowrap number is naturally called a bi-unitary perfect number, and a bi-unitary multi Template:Nowrap number is called a bi-unitary triperfect number.
A divisor d of a positive integer n is called a bi-unitary divisor of n if the greatest common unitary divisor (gcud) of d and n/d equals 1. This concept is due to D. Surynarayana (1972). The sum of the (positive) bi-unitary divisors of n is denoted by σ**(n).
Peter Hagis (1987) proved that there are no odd bi-unitary multiperfect numbers other than 1. Haukkanen and Sitaramaiah (2020) found all bi-unitary triperfect numbers of the form 2au where 1 ≤ a ≤ 6 and u is odd,[6][7][8] and partially the case where a = 7.[9] [10] Further, they fixed completely the case a = 8.[11]
The first few bi-unitary multiply perfect numbers are:
- 1, 6, 60, 90, 120, 672, 2160, 10080, 22848, 30240 Template:OEIS
References
Sources
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See also
External links
Template:Divisor classes Template:Classes of natural numbers