Difference Equations with Hypergeometric Coefficients
Manuel Bronstein
Café Project, INRIA Sophia-Antipolis
Algorithms Seminar
March 3, 2000
[summary by Anne Fredet]
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Abstract
Let k be a difference field with automorphism s. Let b be
an element of k, and L be a linear ordinary difference operator
with coefficients in k. A classical problem in the theory of
difference equations is to compute all the solutions in k of the
equation L(y)=b. If C denotes a constant field and if k=C(n)
and s n =n+1 or s n =qn, there are known algorithms (see
[2] for example). Manuel Bronstein presents here a
generalization to monomial extensions of C(n) (see
[5] for details and generalization).
1 Historical Context
The rational solutions of linear differential equations (equations of
the form åi=0n ai y(i)) have been first studied a long
time ago, for example by Beke and Schlesinger at the end of the last
century. In the middle of this century, R. H. Risch gave an
algorithm to compute elementary integrals (see
[11, 12, 13]). In [8], M. Karr considered
difference equations (equations of the form åi=0n ai
y(x+i)). The link between the linear differential equations and the
linear difference equations is now clear, and in [1], an
algorithm to compute the rational solutions of this two types of
equations with coefficients in C(x) is given. In [2],
the author extends the previous algorithm to q-linear difference
equations (equations of the form åi=0n ai y(qi x)).
Algorithms to compute the rational solutions of linear differential,
difference and q-difference equations with coefficients in C(x)
are now available, and extensions of C(x) have been considered.
In [14], M. F. Singer gives an algorithm to compute the
rational solutions of linear differential equations with coefficients
in almost all the Liouvillian extensions of C(x), i.e., the
extensions built up using integral, exponential of integral, and
algebraic functions. In [7], the authors improve
the algorithm for the rational solutions of linear differential
equations with coefficients in an exponential extension of C(x). In
[6], M. Bronstein adapts the algorithm given in
[1] to monomial extensions, and in [5],
the author uses the methods given in [2, 6] to
find the solutions of linear difference equations in their coefficient
field.
2 Introduction
In [6], the author introduced the splitting
factorization: he decomposed a polynomial in two factors, the
normal part where every irreducible factor is coprime with
its derivative, and the special part where every irreducible
factor divides its derivative. He then gave an algorithm to compute
the normal part of the denominator of rational solutions of a linear
differential equation with coefficients in a monomial extension. In
[2], S. Abramov proposed an algorithm to compute a
polynomial which is divisible by the denominator of any rational
solution of a linear difference equation with coefficients in C(n),
where s n =n+1 or s n = qn. In
[7], a method to compute the numerator of the
rational solution of a linear differential equation with coefficients
in an exponential extension of C(x) is given. Manuel Bronstein now
considers difference equations with hypergeometric terms in the
coefficients (a term h(n) is hypergeometric if h(n+1)/h(n) is in
C(n)). He adapts the previous methods to difference equations with
coefficients in an hypergeometric extension of C(n), and this gives
an efficient algorithm to compute the rational solutions of such
equations. Remark that an algorithm to compute the hypergeometric
solutions of linear difference equation with coefficients in C(n) is
given in [10] and in [4] for
q-hypergeometric solutions of q-difference equations.
3 Difference Equations and Hypergeometric Extensions
Let R be a commutative ring of characteristic 0.
Let s be an automorphism of R.
Define
-
Rs = { x Î R such that s x = x } (the
set of invariant elements of R);
- Rs * = { x Î R such that s n x
= x for some n>0 } (the set of periodic elements);
- Rs = { x Î R such that s x = ux
for some u Î R* } (the set of semi-invariant elements);
- Rs * = { x Î R such that s n x
= ux for some n>0, u Î R* } (the set of
semi-periodic elements).
It is clear that we have the inclusion Rs Í
Rs Í Rs *. If R is a unique
factorization domain then R s * is closed under
taking factors, i.e., for any polynomial q in Rs *,
each factor p of q is in Rs *. This property is
false for Rs and Rs, as shown by the example
R=Q[t] and s(t) = 1-t: s (1-t) = t and s (t -
t2) = t - t2 is in Rs (and then in Rs and in
Rs *), whereas t and 1-t are in Rs
*, but neither in Rs nor in Rs.
3.1 Monomial extensions
Let k be a difference field with automorphism s.
Let (K,s) be an extension of (k,s).
Definition 1
t in K is a monomial over k if t is transcendental
over k with s t in k[t].
Let s be an automorphism of K such that s(t) is in
k[t]. Then s induces an automorphism of k(t), an
automorphism of k[t], and thus s(t) = a t + b for some a
in k* and b in k
Proposition 1 [[9]]
If for all w in k* we have s w ¹ aw +b, then t
is transcendental over k and the following equalities hold: k(t)
s = ks and k[t] s = k[t] s* =
k.
3.2 Hypergeometric extensions
Let s be such that s t = at for some a Î k*.
Proposition 2 [[9]]
If for all w in k * and n >0 we have s w ¹ a n
w, then t is transcendental over k and the following equalities
hold: k(t) s = ks and k[t] s = k[t]
s * = { c tm| c Î k, m³ 0 }.
For example, in C[n], let s be such that s n = q n for
some q Î C *. The property holds whenever q is not a root
of unity. Or we can consider C[n,t], with s such that
s| C = idC, s n = n+1 and s t = (n+1)
t; in other words t represents n!.
4 Dispersion
Definition 2
Let K be a field of characteristic 0.
Let f: K[X] ® K[X] be a function.
Let p and q be non-zero polynomials in K[X].
One defines
-
the spread of p and q with respect to f:
Spr |
|
(p,q) = { m ³ 0 such that p
and f m q have a non trivial gcd } |
- the dispersion of p and q with respect to f:
Dis |
|
(p,q)= |
|
-1 |
|
max(Spr(p,q)) |
if Spr |
|
(p,q) is a finite
nonempty set; |
|
+ ¥ |
if Spr |
|
(p,q) is an infinite
set. |
|
|
|
These definitions are specialized to the case p=q: Sprf(p) = Sprf(p,p) and Disf(p)=Disf(p,p).
Examples are:
-
Disd/dx (p(x)) is
the maximum of the multiplicity of a root of p minus 1;
- Sprn ® n+1
(p(n)) is finite (and then Disn ® n+1
(p(n)) < + ¥);
- Disn ® qn
(n) is infinite.
Let s be an automorphism of k[t] such that s k Í
k.
Then the dispersion Diss(q) is infinite if and only if there exists p in
k[t]s * \ k such that p divides q.
Also, the dispersion Diss(h,q) is infinite if and only if there exists p in
k[t]s * \ k such that p divides q and
s n p divides h.
Example 1
Let a=2n7 + 19n6+63n5+81n4+27n3 be in Q[n] and f be the
automorphism of Q[n] over Q that maps n to n+1.
The resultant of a and f m a is 4m19 (2m+5)3 (2m+1)3
(2m-1)3 (2m-5)3 (m-3)9 (m+3)9,
implying that
Sprf(a)={0,3} and Disf(a)=3
4.1 Splitting factorization
One now extends the splitting factorization of polynomials to
difference field: let q in k[t] be decomposed into two factors q
= q¥ q such that
-
the gcd of q¥ and q is equal to 1,
- for all irreducible factor p of q, p divides q¥
if p is in k[t] s *,
- and for all irreducible factor p of q, p divides q
if p is not in k[t] s *.
The polynomial q¥ is the infinite part of q, and
q is its finite part.
We note that the dispersion Diss
(q) is finite, the dispersion
Diss(q¥) is infinite, and
for all h the dispersion
Diss(h,q) is finite.
4.2 s-Orbits
Given a and b in a field K, the problem of the orbit is
to find m ³ 0 such that a m = b. A bound for the
smallest m such that a m = b is given in
[3]. The main ideas are as follows: if there exists d
such that a d =1 then one can test whether a i = b
for 0 £ i £ d. If it is not the case, then the orbit problem
has no solution, otherwise its solutions consist of all the integers
of the form i0 + kd0 where k ³ 0, i0 is the smallest i
³ 0 such that a i = b and d0 is the smallest d >0
such that a d =1. One can now assume that a is not a
root of unity, which implies that the orbit problem has at most one
solution. If a is transcendental over Q, the orbit problem
has a solution if and only if b is algebraic over
Q(a). Looking at the degree at which a appears in
b gives at most one candidate solution for the orbit problem.
One can now assume that a is algebraic over Q. This
generalizes to find m ³ 0 such that a m,s = a
( s a ) ... (
s m-1 a) = b (see [3]).
4.3 Computation of the dispersion
Let s: K[X] ® K[X] be an automorphism such that
s K Í K. Then
Spr |
|
æ ç ç è |
|
|
p |
|
, |
|
q |
|
|
ö ÷ ÷ ø |
=
|
|
Spr |
|
(pi,qj)
and
Dis |
|
æ ç ç è |
|
|
p |
|
, Õ |
j q |
|
|
ö ÷ ÷ ø |
= |
|
Dis |
|
(pi,qj).
|
The computation of the dispersion reduces to the computation of the
dispersion of two irreducible polynomials.
Let p and q be irreducible polynomials.
Let m be in Sprs(p,q). This means that
the greatest common divisor of p and s m q is not trivial. The polynomials being irreducible,
this is equivalent to the existence of u in K * such that
s m q = u p. This implies that deg p=deg q.
One just has to consider irreducible polynomials with common
degree.
Let p and q be monic irreducible polynomials of k[t] with degree n:
p = tn + åi=0n-1 pi ti and q = tn + åi=0n-1
qi ti.
Assume that s t = at for some a Î k*.
Then m is in Sprs(p,q) implies aim,s = bi for all
i such that pi qi ¹ 0, where bi =qi/pi and
ai = a n-i qi / s qi.
Therefore, if Sprs(p,q) is not empty then
pi and qi vanish simultaneously.
If p=q=t then Dis(p,q)=+¥.
Otherwise, this reduces to the orbit problem a m,s = b
for a, b in k* and m in Spr(p,q).
Remark that if s w ¹ a d w for all w in k* and
d>0 then a d ¹ 1 for all d>0. So, the orbit problem has
at most one solution and then Sprs(p,q) has
at most one element.
One can extend the computation of the dispersion to rational functions:
let f = p/q with relatively prime p and q in C[n].
Let Diss(f) = max ( Diss (p), Diss(p,q) , Diss(q,p) , Diss (q)) and n ¥(f) =
deg q - deg p.
Then n¥ (f m,s) = m n ¥(f).
And if f is not in C then Diss(f
m,s) = Diss(f) + m -1.
This last equality allows us to reduce orbit problems to dispersions
whenever a is not constant.
5 Rational Solutions of Difference Equations
Let t be a monomial over k=C(n).
Let s be such that s n = n+1 and s t = at for
some a in k such that s w ¹ a d w, for all w in
k* and d >0.
Let L = åi=0N ai s i be a linear difference operator, with
the ai's in k[t] and both a0 and aN not equal to 0.
Let b be in k[t].
The aim of this section is to described an algorithm to find y in
k(t) such that L(y)=b (if there exists such a y).
5.1 Denominator of a rational solution
The first problem is to find a bound for the finite part of any y in
k(t) such that L(y)=b. This means to compute a polynomial q in
k[t] such that if L(y)=b then yq = p/d¥ where p is in
k[t] and d¥ in k[t] s *. We outline the
ideas here, proofs and technical details are given in [5].
Let a0 be decomposed: a0 = a0,¥ a0.
Let y be in k(t) such that L(y) = b, where y=p/d and
d = d¥ d.
Then Diss(d)£max(-1, Diss
(aN,a0) - N).
Let h >0 be an integer.
One can compute an operator Lh = bs ssh + bs-1 s
(s-1)h + ... + b0 such that Lh = RL for some R in
k(t)[s].
It follows that Lh(y) = Rb for any b in k[t] and any solution y
in k(t) of L(y)=b.
We get that every solution y in k(t) of L(y)=b satisfies an
equation of the form cs s hs(y) + ... + c1 s
h(y) = dh
where c0,...,cs,dh are in k[t] and cs ¹ 0.
If h was chosen such that
Diss(d) < h then d
divides gcd0 £ i £ s ( s -ih ci ).
This gives us a polynomial q such that if L(y) = b then qy =
p/d¥ with p in k[t] and d¥ in
k[t] s *
Example 2
Consider y(n+2) - (n! + n) y(n+1) + n(n!
-1) y(n) =0.
If we define s by s n=n+1 and s t = (n+1) t then
the associated difference operator is s 2 - (t+n) s + n(t
-1).
aN = 1, a0 = a0 = n(t-1) and
Diss(aN,a0) = -1.
Then Diss(d) £ -1 and d Î C(n).
So, if there exists y Î C(n)(t) such that L(y)=b then y is in C(n)[t,t-1].
Remark 1
The same results holds for the q-difference equation:
let q be transcendental over Q.
Let s be such that s x = qx.
Consider the q-difference equation
|
q3 (qx+1) y(q2x) - 2 q2 (x+1) y(qx) + (x+q) y(x)=0 |
We have a0=x+q, a2 = q3 (qx+1).
The resultant of a2 and s m (a0) is q3 (q2 -
qm), which implies that
Diss(a2,a0)=2 hence that any
solution of (1) has a denominator of the form xn
d where Diss(d) £ 0.
Using the bound h=1, we get Lh = L and d divides the
greatest common divisor of gcd0 £ i £ 2 ( s-i ai)
= gcd (x+q,s -1 (q2 (x+1)),s-2 (q3
(qx+1))) = gcd(x+q,q(x+q),q2(x+q))=x+q.
Therefore, any rational solution of (1) can be written
as y=p/ (xn (x+q)) where n ³ 0 and p is in Q[x].
The indicial equation at x=0 is qZ2 -2q2Z+q3=0 (see
[2]). Its only solution of the form Z=qn is for
n=1, which implies that any rational solution of
(1) can be written as y=p/(x(x+q)).
Replacing y by this form, we get p(q2 x) - 2 p(qx)+p(x)=0 (whose
solution space is Q (q), which implies that the general rational
solution of (1) is y=C/(x(x+q)) for any
C in Q (q)).
5.2 Laurent polynomial solution
The problem of finding rational solutions y of L(y)=b is reduced
to finding y in k[t,t-1] such that L(y)=b, where b is in
k[t,t-1] and L =åi=0N ai s i is a difference
operator, with ai Î k[t] and non-zero a0 and aN. This
decomposes in two steps:
-
find a bound for the degree and the order in t of y;
- compute the coefficients of y, seen as a Laurent polynomial in t.
5.2.1 Bound for the degree and order of a polynomial solution
One rewrites L as åj=nd tj Lj where the Lj's are
in k[s] and Ln and Ld are not equal to zero. Let
y=ydtd+...+ygtg be in k[t,t-1]
for integers g and d satisfying g
³ d and such that neither yd nor yg is equal
to zero. Let b be in k[t,t-1]. If L(y)=b, then
-
either d ³ n(b) - n, or Ln(ydtd)=0;
- either g £ deg b-d, or Ld (ygtg)=0.
The problem is reduced to considering difference operators T =
åi=mM Ai s i with Ai Î C[n] for non-zero Am
and AM, and to searching bounds for gÎZ such that T(z
tg)=0 for some z in C(n). Let e =- n ¥
(s t/t) = n ¥(a). There are three possibilities:
-
if e > 0 then (degnAm -degnT)/e £ g £
(degnT - degnAM)/e;
- if e <0 then (degnT - degnAm)/e £ g £
(degnAm - degnT)/e;
- if e=0 then a = a(¥) Î C*. We
decompose Ai = ai,ai nai+ ··· .
We define Q(z) = åi|ai = maxj (aj)
ai,ai zi. We have Q(a g)=0. This problem can be solved if a d ¹
1 for all d ³ 0 (see section 4.2).
5.2.2 Coefficients of a Laurent polynomial solution
This is a generalization of the specialization given in [7].
We have found g and d such that if y is in
k[t,t-1] with L(y)=b then degt (y) £ g and valt(y)
³ d.
Let z=tdy. Note that degt(z) £ g -
d = J.
One has to consider the problem L(z) =b where L is in
k[t][s] and b in k[t].
Let L = åj=0d tj Lj with Lj in k[s], and
L0,Ld not equal to zero.
-
if J =0 then L(z) = åj=0d tj (Lj z). But Lj(z)
is in k so L(z)=b implies Lj(z) = bj for all j and this reduces
to difference equations with coefficients in C[n];
- if J >0 then one decomposes z = z0 + t z where
z0 = z(0) is in C(n).
Then L0(z0) = b0 and one can find z0.
So, L(z) = (L - L0) (z0) + L (t z ) + L0(z0) and L(z) = b implies
L ( t z ) |
= |
b - b0 - (L-L0) z0 |
|
= |
|
This gives us a new difference equation with a solution z
of degree strictly less than J. By induction, one can find z.
Example 3
Consider y(n+2) - (n! + n) y(n+1) + n(n!
-1) y(n) =0, which is associated to the difference operator
L= s 2 - ( t+n) s + n(t-1)= t ( n - s) + (s 2 - n s - n ) = t L1 + L0 |
Using the same notations as previously, e = - n ¥ (s
t/t) = - n ¥ (n+1) =1 and then y = y0 + y1 t. One
first considers L0(y0) = s 2 y0 - n s y0 -n y0 =0,
and finds that y0 = 0. Then:
L (t z1) = (n+2)(n+1) t s 2 (z1) -
(n+1)(t+n) t s(y1) + n(t-1) ty1,
from which follows that
|
(y1) =
(n+2)(n+1) s 2(y1) - (n+1)(t+n) s(y1) + n (t-1) y1 =0. |
This implies that y1 = c/n. Then y=y1 t = (c/n)n! = c(n-1)!.
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-
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-
Abramov (S. A.). --
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-
Abramov (Sergei) and Bronstein (Manuel). --
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