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 Wolfram Language
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.,
(7)
|
To compute the continued fraction convergents to , use the usual recurrence
relations
(8)
| |||
(9)
| |||
(10)
| |||
(11)
| |||
(12)
| |||
(13)
| |||
(14)
|
where
is the floor function. For reasons to be explained
shortly, also compute the two additional quantities
and
defined by
(15)
| |||
(16)
| |||
(17)
| |||
(18)
| |||
(19)
| |||
(20)
| |||
(21)
|
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
(33)
| |||
(34)
|
which gives the family of solutions
(35)
| |||
(36)
|
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, ... (OEIS A033313)
and 2, 1, 4, 2, 3, 1, 6, 3, 2, 180, ... (OEIS A033317),
respectively. The values of
having
, 3, ... are 3, 2, 15, 6, 35, 12, 7, 5, 11, 30, ... (OEIS
A033314) and the values of
having
, 2, ... are 3, 2, 7, 5, 23, 10, 47, 17, 79, 26, ... (OEIS
A033318). Values of the incrementally largest
minimal
are 3, 9, 19, 649, 9801, 24335, 66249, ... (OEIS A033315)
which occur at
,
5, 10, 13, 29, 46, 53, 61, 109, 181, ... (OEIS A033316).
Values of the incrementally largest minimal
are 2, 4, 6, 180, 1820, 3588, 9100, 226153980, ... (OEIS A033319), which occur at
, 5, 10, 13, 29, 46, 53, 61, ... (OEIS 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
(41)
| |||
(42)
|
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
(43)
|
has three distinct sets of fundamental solutions, , (13, 4), and (57, 18). Using (42),
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
(44)
|
can be reduced to the one above by multiplying through by ,
(45)
|
finding solutions in ,
and then selecting those for which
is an integer.
According to Dickson (2005, pp. 408 and 411), the equation
(46)
|
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 (46) 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 the Wolfram Language as Reduce[x^2
+ d y^2 == n,
x, y
, Integers].