A special case of the quadratic Diophantine
equation having the form
 |
(1)
|
where is a nonsquare natural number (Dickson 2005). The equation
 |
(2)
|
arising in the computation of fundamental units is sometimes also called the Pell equation (Dörrie 1965, Itô
1987), and Dörrie calls the positive form of (2)
the Fermat difference
equation. While Fermat deserves credit for being the first to extensively study
the equation, the erroneous attribution to Pell was perpetrated by none other than
Euler himself (Nagell 1951, p. 197; Burton 1989; Dickson 2005, p. 341).
The Pell equation was also solved by the Indian mathematician Bhaskara. Pell equations
are extremely important in number
theory, and arise in the investigation of numbers which are figurate in more than one way, for example, simultaneously
square and triangular.
The equation has an obvious generalization to the Pell-like equation
 |
(3)
|
as well as the general second-order bivariate Diophantine equation
 |
(4)
|
However, several different techniques are required to solve this equation for arbitrary values of , , and . The Mathematica command Reduce[f[x, y] && Element[x|y,
Integers]] finds solutions to the general equation (4)
when they exist.
Pell equations of the form (1), as
well as certain cases of the analogous equation with a minus sign on the right,
 |
(5)
|
can be solved by finding the continued fraction of . Note that
although the equation (5) is solvable for only
certain values of , the continued fraction technique provides
solutions when they exist, and always in the case of (1), for which a solution always
exists. A necessary condition that (5) be solvable
is that all odd prime factors of be of the form , and that cannot be doubly
even (i.e., divisible by 4). However, these conditions are not sufficient for a solution to exist, as demonstrated by the
equation , which has no solutions in
integers (Nagell 1951, pp. 201 and 204).
In all subsequent discussion, ignore the trivial solution , . Let denote the
th convergent , then we will have solved (1) or
(5) if we can find a convergent which obeys the identity
 |
(6)
|
Amazingly, this turns out to always be possible as a result of the fact that the continued fraction of
a quadratic surd always becomes
periodic at some term , where , i.e.,
![sqrt(D)=[a_0,a_1,...,a_r,2a_0^_].](/images/equations/PellEquation/NumberedEquation7.gif) |
(7)
|
To compute the continued fraction convergents to , use the usual recurrence relations
where is the floor function. For reasons to be explained shortly, also compute
the two additional quantities and defined by
Now, two important identities satisfied by continued
fraction convergents are
 |
(22)
|
 |
(23)
|
(Beiler 1966, p. 262), so both linear
 |
(24)
|
and quadratic
 |
(25)
|
equations are solved simply by finding an appropriate continued fraction.
Let be the term at which the
continued fraction becomes periodic (which will always happen for a quadratic surd).
For the Pell equation
 |
(26)
|
with odd,
is positive
and the solution in terms of smallest integers
is and , where is the th convergent. If is even, then is negative, but
 |
(27)
|
so the solution in smallest integers is , . Summarizing,
 |
(28)
|
The equation
 |
(29)
|
can be solved analogously to the equation with on the right
side iff is even, but has no solution if is odd,
 |
(30)
|
Given one solution (which can be found as above),
a whole family of solutions can be found by taking each side to the th power,
 |
(31)
|
Factoring gives
 |
(32)
|
and
which gives the family of solutions
These solutions also hold for
 |
(37)
|
except that can take on only odd values.
The following table gives the smallest integer solutions to the Pell
equation with constant (Beiler 1966, p. 254).
Square are not included,
since they would result in an equation of
the form
 |
(38)
|
which has no solutions (since the difference of two squares cannot be 1).
 |  |  |  |  |  | | 2 | 3 | 2 | 54 | 485 | 66 | | 3 | 2 | 1 | 55 | 89 | 12 | | 5 | 9 | 4 | 56 | 15 | 2 | | 6 | 5 | 2 | 57 | 151 | 20 | | 7 | 8 | 3 | 58 | 19603 | 2574 | | 8 | 3 | 1 | 59 | 530 | 69 | | 10 | 19 | 6 | 60 | 31 | 4 | | 11 | 10 | 3 | 61 | 1766319049 | 226153980 | | 12 | 7 | 2 | 62 | 63 | 8 | | 13 | 649 | 180 | 63 | 8 | 1 | | 14 | 15 | 4 | 65 | 129 | 16 | | 15 | 4 | 1 | 66 | 65 | 8 | | 17 | 33 | 8 | 67 | 48842 | 5967 | | 18 | 17 | 4 | 68 | 33 | 4 | | 19 | 170 | 39 | 69 | 7775 | 936 | | 20 | 9 | 2 | 70 | 251 | 30 | | 21 | 55 | 12 | 71 | 3480 | 413 | | 22 | 197 | 42 | 72 | 17 | 2 | | 23 | 24 | 5 | 73 | 2281249 | 267000 | | 24 | 5 | 1 | 74 | 3699 | 430 | | 26 | 51 | 10 | 75 | 26 | 3 | | 27 | 26 | 5 | 76 | 57799 | 6630 | | 28 | 127 | 24 | 77 | 351 | 40 | | 29 | 9801 | 1820 | 78 | 53 | 6 | | 30 | 11 | 2 | 79 | 80 | 9 | | 31 | 1520 | 273 | 80 | 9 | 1 | | 32 | 17 | 3 | 82 | 163 | 18 | | 33 | 23 | 4 | 83 | 82 | 9 | | 34 | 35 | 6 | 84 | 55 | 6 | | 35 | 6 | 1 | 85 | 285769 | 30996 | | 37 | 73 | 12 | 86 | 10405 | 1122 | | 38 | 37 | 6 | 87 | 28 | 3 | | 39 | 25 | 4 | 88 | 197 | 21 | | 40 | 19 | 3 | 89 | 500001 | 53000 | | 41 | 2049 | 320 | 90 | 19 | 2 | | 42 | 13 | 2 | 91 | 1574 | 165 | | 43 | 3482 | 531 | 92 | 1151 | 120 | | 44 | 199 | 30 | 93 | 12151 | 1260 | | 45 | 161 | 24 | 94 | 2143295 | 221064 | | 46 | 24335 | 3588 | 95 | 39 | 4 | | 47 | 48 | 7 | 96 | 49 | 5 | | 48 | 7 | 1 | 97 | 62809633 | 6377352 | | 50 | 99 | 14 | 98 | 99 | 10 | | 51 | 50 | 7 | 99 | 10 | 1 | | 52 | 649 | 90 | 101 | 201 | 20 | | 53 | 66249 | 9100 | 102 | 101 | 10 |
The first few minimal values of and for nonsquare are 3, 2, 9, 5, 8, 3, 19, 10, 7, 649, ... (Sloane's
A033313)
and 2, 1, 4, 2, 3, 1, 6, 3, 2, 180, ... (Sloane's A033317), respectively. The values of having , 3, ... are
3, 2, 15, 6, 35, 12, 7, 5, 11, 30, ... (Sloane's A033314) and the values of having , 2, ... are
3, 2, 7, 5, 23, 10, 47, 17, 79, 26, ... (Sloane's A033318). Values of the incrementally largest minimal are 3, 9, 19, 649, 9801, 24335, 66249, ... (Sloane's
A033315)
which occur at , 5, 10, 13, 29, 46, 53, 61, 109, 181,
... (Sloane's A033316).
Values of the incrementally largest minimal are 2, 4, 6, 180,
1820, 3588, 9100, 226153980, ... (Sloane's A033319), which occur at , 5, 10, 13,
29, 46, 53, 61, ... (Sloane's A033316).
The more complicated Pell-like equation
 |
(39)
|
with has solution iff is one of the values
for , 2, ..., computed in the process of finding the convergents
to (where, as above, is
the term at which the continued fraction becomes periodic). If ,
the procedure is significantly more complicated (Beiler 1966, p. 265; Dickson
2005, pp. 387-388) and is discussed by Gérardin (1910) and Chrystal (1961).
Regardless of how it is found, if a single solution , to (39) is known, other solutions can be found. Let and be solutions to
(39), and and solutions to the
"unit" form
 |
(40)
|
Then the identity
allows larger solutions to the equation to be found by using incrementally larger
values of the , which can be easily computed using
the standard technique for the Pell equation. Such a family of solutions does not
necessarily generate all solutions, however. For example, the equation
 |
(44)
|
has three distinct sets of fundamental solutions, , (13,
4), and (57, 18). Using (43), these generate
the solutions shown in the following table, from which the set of all solutions (7,
2), (13, 4), (57, 18), (253, 80), (487, 154), (2163, 684), (9607, 3038), ... can
be generated.
| fundamental | generated solutions | | (7, 2) | (253, 80), (9607, 3038),
(364813, 115364), (13853287, 4380794), ... | | (13,
4) | (487, 154), (18493, 5848), (702247, 222070), (26666893, 8432812),
... | | (57, 18) | (2163,
684), (82137, 25974), (3119043, 986328), (118441497, 37454490), ... |
The case
 |
(45)
|
can be reduced to the one above by multiplying through by ,
 |
(46)
|
finding solutions in , and then selecting those for
which is an integer.
According to Dickson (2005, pp. 408 and 411), the equation
 |
(47)
|
with , which has either no solutions
or a finite number of solutions, was solved by Gauss in 1863 using the method of exclusions and considered by Euler (1773) and Nasimoff
(1885), although Euler's methods were incomplete (Smith 1965; Dickson 2005, p. 378).
According to Itô (1987), this equation can be solved completely using solutions
to Pell's equation. Nasimoff (1885) applied Jacobi elliptic functions to express
the number of solutions of this equation for odd (Dickson 2005, p. 411). Additional discussion including
the connection with elliptic functions is given in Dickson (2005, pp. 387-391).
The special case of and prime was solved
by Cornacchia (Cornacchia 1908, Cox 1989, Wagon 1990). A deterministic algorithm
for finding all primitive solutions to (47)
for fixed relatively prime integers,
, and was given
by Hardy et al. (1990). This algorithm generalizes those of Hermite (1848),
Serret (1848), Brillhart (1972), Cornacchia (1908), and Wilker (1980). It requires
factorization of , and has worst case running time of , independent of
and . An algorithmic
method for finding all solutions is implemented in Mathematica as Reduce[x^2 + d y^2 == n, x, y , Integers].
Beiler, A. H. "The Pellian." Ch. 22 in Recreations in the Theory of Numbers: The Queen of Mathematics
Entertains. New York: Dover, pp. 248-268, 1966.
Brillhart, J. "Note on Representing a Prime as a Sum of Two Squares." Math.
Comput. 26, 1011-1013, 1972.
Burton, D. M. Elementary Number Theory, 4th ed. Boston, MA: Allyn and
Bacon, pp. 379-382 and 392, 1989.
Chrystal, G. Textbook of Algebra, 2nd ed., Vol. 2. New York: Chelsea,
pp. 478-486, 1961.
Cipolla, M. "Un metodo per la risoluzione della congruenza di secondo grado."
Rend. Accad. Sci. Fis. Mat. Napoli 9, 154-163, 1903.
Cohn, H. "Pell's Equation." §6.9 in Advanced Number Theory. New York: Dover, pp. 110-111,
1980.
Cornacchia, G. "Su di un metodo per la risoluzione in numeri unteri dell' equazione ." Giornale di
Matematiche di Battaglini 46, 33-90, 1908.
Cox, D. A. Primes of the form . New York: Wiley, 1989.
Degan, C. F. Canon Pellianus. Copenhagen, Denmark, 1817.
Dickson, L. E. "Pell Equation: Made Square."
Ch. 12 in History of the Theory of Numbers, Vol. 2: Diophantine Analysis.
New York: Dover, pp. 341-400, 2005.
Dörrie, H. 100 Great Problems of Elementary Mathematics: Their History and
Solutions. New York: Dover, 1965.
Euler, L. Novi Comm. Acad. Petrop. 18, 218, 1773. Reprinted in Opera
Omnia, Series Prima, Vol. 3, p. 310.
Euler, L. Comm. Arith. 570. Reprinted in Opera Omnia, Series Prima, Vol. 3,
p. 310.
Gérardin, A. "Formules de récurrence." Sphinx-Oedipe 5,
17-29, 1910.
Hardy, K.; Muskat, J. B.; and Williams, K. S. "A Deterministic Algorithm for Solving in Coprime Integers and ." Math.
Comput. 55, 327-343, 1990.
Havil, J. Gamma: Exploring Euler's Constant. Princeton, NJ: Princeton
University Press, pp. 91-92, 2003.
Hermite, C. "Note au sujet de l'article précédent." J.
Math. Pures Appl. 13, 15, 1848.
Itô, K. (Ed.). Encyclopedic Dictionary of Mathematics, 2nd ed, Vol. 1.
Cambridge, MA: MIT Press, p. 450, 1987.
Lagarias, J. C. "On the Computational Complexity of Determining the Solvability or Unsolvability of the Equation ."
Trans. Amer. Math. Soc. 260, 485-508, 1980.
Lenstra, H. W. Jr. "Solving the Pell Equation." Not. Amer. Math.
Soc. 49, 182-192, 2002.
Nagell, T. "The Diophantine Equation ,"
"The Diophantine Equation ,"
and "The Diophantine Equation ."
§56-58 in Introduction to Number Theory. New York: Wiley, pp. 195-212,
1951.
Nasimoff, P. S. Ch. 1 in Application of Elliptic Functions to the Theory of Numbers. Moscow, 1885. French summary in Ann. sci. de l'École normale
supér. 5, 23-31, 1888.
Robertson, J. "Home Page for John Robertson." http://hometown.aol.com/jpr2718/.
Serret, J. A. "Sur un théorème rélatif aux nombres
enti'eres." J. Math. Pures Appl. 13, 12-14, 1848.
Sloane, N. J. A. Sequences A033313, A033314, A033315, A033316, A033317, A033318, and A033319 in "The On-Line Encyclopedia of Integer Sequences."
Smith, H. J. S. Collected Mathematical Papers I. New York: Chelsea,
pp. 195-202, 1965.
Smarandache, F. "Un metodo de resolucion de la ecuacion diofantica." Gaz.
Math. 1, 151-157, 1988.
Smarandache, F. "Method to Solve the Diophantine Equation ."
In Collected Papers, Vol. 1. Lupton, AZ: Erhus University Press, 1996.
Stillwell, J. C. Mathematics and Its History. New York: Springer-Verlag,
1989.
Wagon, S. "The Euclidean Algorithm Strikes Again." Amer. Math. Monthly 97,
124-125, 1990.
Whitford, E. E. Pell Equation. New York: Columbia University Press, 1912.
Wilker, P. "An efficient Algorithmic Solution of the Diophantine Equation ." Math. Comput. 35,
1347-1352, 1980.
|