In number theory, Waring's problem, proposed in 1770 by Edward Waring, asks whether for every natural number k there exists an associated positive integer s such that every natural number is the sum of at most s kth powers of natural numbers (for example, every number is the sum of at most 4 squares, or 9 cubes, or 19 fourth powers, etc.). The affirmative answer, known as the Hilbert–Waring theorem, was provided by Hilbert in 1909.[1] Waring's problem has its own Mathematics Subject Classification, 11P05, "Waring's problem and variants."
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For every k, we denote by g(k) the minimum number s of kth powers needed to represent all integers. Note we have g(1) = 1. Some simple computations show that 7 requires 4 squares, 23 requires 9 cubes, and 79 requires 19 fourth-powers; these examples show that g(2) ≥ 4, g(3) ≥ 9, and g(4) ≥ 19. Waring conjectured that these values were in fact the best possible.
Lagrange's four-square theorem of 1770 states that every natural number is the sum of at most four squares; since three squares are not enough, this theorem establishes g(2) = 4. Lagrange's four-square theorem was conjectured in Bachet's 1621 edition of Diophantus; Fermat claimed to have a proof, but did not publish it.[2]
Over the years various bounds were established, using increasingly sophisticated and complex proof techniques. For example, Liouville showed that g(4) is at most 53. Hardy and Littlewood showed that all sufficiently large numbers are the sum of at most 19 fourth powers.
That g(3) = 9 was established from 1909 to 1912 by Wieferich[3] and A. J. Kempner,[4] g(4) = 19 in 1986 by R. Balasubramanian, F. Dress, and J.-M. Deshouillers,[5][6] g(5) = 37 in 1964 by Chen Jingrun, and g(6) = 73 in 1940 by Pillai.[7]
Let [x] and {x} denote the integral and fractional part of x respectively. Since 2k[(3/2)k]-1<3k only 2k and 1k can be used to represent this number and the most economical representation requires [(3/2)k]-1 2ks and 2k-1 1ks it follows that g(k) is at least as large as 2k + [(3/2)k] − 2. J. A. Euler, the son of Leonard Euler, conjectured about 1772 that, in fact, g(k) = 2k + [(3/2)k] − 2.[8] Later work by Dickson, Pillai, Rubugunday, Niven[9] and many others have proved that
No values of k are known for which 2k{(3/2)k} + [(3/2)k] > 2k, Mahler[10] has proved there can only be a finite number of such k and Kubina and Wunderlich [11] have shown that any such k must satisfy k > 471,600,000. Thus it is conjectured that this never happens, i.e. that g(k) = 2k + [(3/2)k] − 2 for each positive integer k.
The first few values of g(k) are 1, 4, 9, 19, 37, 73, 143, 279, 548, 1079, 2132, 4223, 8384, 16673, 33203, 66190, 132055 ... (sequence A002804 in OEIS).
From the work of Hardy and Littlewood, more fundamental than g(k) turned out to be G(k), which is defined to be the least positive integer s such that every sufficiently large integer (i.e. every integer greater than some constant) can be represented as a sum of at most s kth powers of positive integers. Since squares are congruent to 0, 1, or 4 (mod 8), no integer congruent to 7 (mod 8) can be represented as a sum of three squares, implying that G(2) ≥ 4. Since G(k) ≤ g(k) for all k, this shows that G(2) = 4. Davenport showed that G(4) = 16 in 1939, by demonstrating that any sufficiently large number congruent to 1 through 14 mod 16 could be written as a sum of 14 fourth powers (Vaughan in 1985 and 1989 reduced the 14 successively to 13 and 12). The exact value of G(k) is unknown for any other k, but there exist bounds.
Bounds |
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4 ≤ G(2) ≤ 4 |
4 ≤ G(3) ≤ 7 |
16 ≤ G(4) ≤ 16 |
6 ≤ G(5) ≤ 17 |
9 ≤ G(6) ≤ 24 |
8 ≤ G(7) ≤ 33 |
32 ≤ G(8) ≤ 42 |
13 ≤ G(9) ≤ 50 |
12 ≤ G(10) ≤ 59 |
12 ≤ G(11) ≤ 67 |
16 ≤ G(12) ≤ 76 |
14 ≤ G(13) ≤ 84 |
15 ≤ G(14) ≤ 92 |
16 ≤ G(15) ≤ 100 |
64 ≤ G(16) ≤ 109 |
18 ≤ G(17) ≤ 117 |
27 ≤ G(18) ≤ 125 |
20 ≤ G(19) ≤ 134 |
25 ≤ G(20) ≤ 142 |
The number G(k) is greater than or equal to
In the absence of congruence restrictions, a density argument suggests that G(k) should equal k + 1.
G(3) is at least four (since cubes are congruent to 0, 1 or −1 mod 9); for numbers less than 1.3×109, 1290740 is the last to require six cubes, and the number of numbers between N and 2N requiring five cubes drops off with increasing N at sufficient speed to have people believe G(3)=4; the largest number now known not to be a sum of four cubes is 7373170279850,[12] and the authors give reasonable arguments there that this may be the largest possible.
13792 is the largest number to require seventeen fourth powers (Deshouillers, Hennecart and Landreau showed in 2000 [13] that every number between 13793 and 10245 required at most sixteen, and Kawada, Wooley and Deshouillers extended Davenport's 1939 result to show that every number above 10220 required no more than sixteen). Sixteen fourth powers are always needed to write a number of the form 31·16n.
617597724 is the last number less than 1.3×109 which requires ten fifth powers, and 51033617 the last number less than 1.3×109 which requires eleven.
The upper bounds on the right with k=5,...,20 are due to Vaughan and Wooley [1993], [1994], [1995], [2000] (see Vaughan and Wooley [2002]).
Using his improved Hardy-Littlewood method, I. M. Vinogradov published numerous refinements leading to
in 1947 and, ultimately,
for an unspecified constant C and sufficiently large k in 1959.
Applying his -adic form of the Hardy-Littlewood-Ramanujan-Vinogradov method to estimating trigonometric sums, in which the summation is taken over numbers with small prime divisors, Anatolii Alexeevitch Karatsuba obtained[14] (1985) a new estimate of the Hardy function (for ):
Further in his investigation of the Waring problem Karatsuba obtained[15][16] the following two-dimensional generalization of that problem:
Consider the system of equations
where are given positive integers with the same order or growth, , and are unknowns, which are also positive integers. This system has solutions, if , and if , then there exist such , that the system has no solutions.
Further minor refinements were obtained by Vaughan [1989].
Wooley then established that for some constant C
Vaughan and Wooley have written a comprehensive survey article [2002].