Abstract
We present a deautonomization procedure for partial difference and differential-difference equations (with the latter defining symmetries of the former) which uses the integrability conditions as integrability detector. This procedure is applied to Hirota’s Korteweg–de Vries and all the ABS equations and leads to non-autonomous equations and their non-autonomous generalized symmetries of order two, all of which depend on arbitrary periodic functions and are related to the same two-quad equation and its symmetries. We show how reductions of the derived differential-difference equations lead to alternating QRT maps, and periodic reductions of the difference equations result to non-autonomous maps and discrete Painlevé type equations.
Communicated by: Prof. Nalini Joshi
1. Introduction
There exist several criteria and methods to test the integrability of a given difference equation and to derive discrete integrable systems. Multidimensional consistency [1], algebraic entropy [2], singularity confinement [3] and integrability conditions (existence of infinite hierarchies of generalized symmetries and canonical conservation laws) [4, 5] are some of these criteria and, for instance, multidimensional consistency has been used to classify integrable equations in [6, 7], and singularity confinement has been employed for the deautonomization of known autonomous equations [3, 8–10].
These criteria apply to any difference equation and there is a plethora of autonomous equations which satisfy them and can be characterized as integrable. For instance, the discrete potential Korteweg–de Vries (KdV) equation, aka H1,
(un,m−un+1,m+1)(un+1,m−un,m+1)=α−β
is multidimensionally consistent [
6], it admits infinite hierarchies of symmetries in both directions [
11], its movable singularities are confined [
3] and its algebraic entropy vanishes [
12]. Moreover, its deautonomized counterpart
is also multidimensionally consistent, with confined singularities [
13] and vanishing algebraic entropy [
12] but it does not admit any generalized symmetries for generic functions
αn
and
βm
but only for specific choices of these two functions [
14]. So the question we try to answer here is if we can systematically specify any arbitrary functions of the independent variables in a given deautonomized equation so that the resulting equation to admit hierarchies of symmetries and canonical conservation laws in both lattice directions as its autonomous counterpart.
To answer this question, we are going to employ the integrability conditions [4, 5] which not only test the integrability of the equation under consideration but also serve as determining equations for its generalized symmetries. So this approach allows us not only to derive integrable non-autonomous partial difference equations but also to construct their symmetries (differential-difference equations) and conservation laws which will also depend explicitly on n
and m
.
Specifically we start with known integrable partial difference equations in a generic deautonimized form and employ the integrability conditions to separate the integrable cases, i.e. the ones admitting generalized symmetries and conservation laws in both lattice directions. For our purposes, it is sufficient to consider only the first of these conditions which for the symmetries in the
n
direction can be written as
Here, S
and T
are the shift operators in the first and second direction, respectively, Qn,m
stands for the defining function of the d
-quad equation under consideration, and R
is a function of n
, m
and variables un−N,m
, …
, un+N,m
.
As N
depends on the order of the symmetry (i.e. the number of forward and backwards shifted values of u
involved in the symmetry generator) and there is no way to choose N
a priori, we start our investigations with N=1
(first order symmetries) and then proceed to second order ones (N=2
). In every step N
, we separate the integrable equations as the ones admitting symmetries of order N
and none of lower order (when N>1
). This procedure determines completely the introduced functions of n
and m
. Finally, employing more of the integrability conditions, we construct the lowest order symmetries which are non-autonomous differential-difference equations of order two.
We applied this procedure to equations (
1), and the deautonomized Hirota’s KdV [
15]
as well as to the ABS list, the sine-Gordon and the Hietarinta–Viallet equations (see (
31) and (
33) below). The only integrable cases for
N=1
are the original autonomous equations. For symmetries of order two, it turns out that the arbitrary functions must be periodic with period two.
The most interesting phenomenon is that most of these deautonomized equations, we analysed are related via Miura transformations to the
same non-autonomous quadratic one-quad equation (see equation (
6) below) which can be autonomized leading to the
two-quad equation where
ϕn,m=zn,m+zn+1,m+zn,mzn+1,m
. Moreover, under the same Miura transformation the symmetries of the aforementioned quad equations are transformed to symmetries of the two-quad equation (
4). In particular, the first symmetry is given by the differential-difference equation
where
cn
is a periodic function with period 2, i.e.
cn+2=cn
. This is an integrable equation not only because it satisfies the corresponding integrability conditions but also because it admits a
local master symmetry (see (
10) below). Moreover (
5) may be viewed as a generalization of the differential-difference equation presented recently by Adler [
16] and corresponds to the choice
cn=1
. The fact that all these second order differential-difference equations we found are mapped to (
5) suggests that the latter plays a role of universal object in the theory as it was pointed in [
17].
Since all the second order differential-difference equations, we derive depend on periodic functions of
n
, certain reductions of them lead to alternating QRT maps [
18,
19] with first integrals following from the conserved forms of the equations involved. On the other hand,
(k,−1)
periodic reductions of the non-autonomous partial difference equations lead to families of ordinary difference equations the form of which depends on the parity of
k
. In particular, the even order reductions of (
3) with
an,m=αn
are non-autonomous extensions of some of the maps discussed recently in [
20], and are related via a Bäcklund transformation to the corresponding reductions of (
1) with
βm=0
. But the odd order reductions of equation (
3) lead to the family of equations
the first member (
p=1
) of which coincides with the first two-periodic Lyness recurrence [
21], and the corresponding reductions of (
1) result to equations
where
α
,
β
and
γ
are real constants.
The article is organized as follows. Section 2 presents the non-autonomous quadratic quad equation and its autonomous two-quad counterpart and some of their integrability aspects. Section 3 deals with the procedure of deautonomization using Hirota’s and the discrete potential KdV equations as illustrative examples and presents the relative results for all the ABS equations, the deformed H list, as well as for the discrete sine-Gordon and the Hietarinta-Viallet equations. Section 4 presents reductions for some of the derived non-autonomous differential-difference equations and their relations to alternating QRT maps. Section 5 deals with the (k,−1)
periodic reductions of the deautonomized KdV equations. The final section gives an overall evaluation of our results and the appendix contains outcomes from our analysis in Section 3 and some canonical conservation laws we employ in section 5.
2. Two difference equations and their symmetries
In this section, we present two difference equations, derive their relation and discuss their integrability properties. In particular, we present their lowest order generalized symmetries in the first lattice direction (of order two) and compute the first two canonical conserved densities. The importance of these two equations stems from the fact that both of them are related to the deautonomized equations we are discussing in the next section.
The first equation is non-autonomous, quadratic and defined on an elementary quadrilateral of the lattice and has the following form.
where
and
An+2=An
,
An+1≠An
and
B
is a constant. The second condition for
An
is essential because if
An=A∈R
, then equation is linearizable since
Wn,m(A,A,B)=(A−B)(ϕn,m+1−ϕn,m)(zn,mzn+1,m+1−zn+1,mzn,m+1)
.
An interesting property of this equation is that we can remove function
An
from our considerations using its periodicity and the pair of equations
Wn,m(An,An+1,B)=0
,
Wn+1,m(An+1,An,B)=0
. The elimination of
An
and
An+1
from this pair leads to a polynomial equation that can be factorized as a product of two polynomials, each of which is linear in
zn,m
,
zn,m+1
,
zn+2,m
and
zn+2,m+1
. The first factor leads to
which is a trivial equation since it is equivalent to
(T−1)(S2−1)log(zn,m−zn−2,m)=0
. The second factor however yields the two-quad equation
This is an integrable equation, as we explain below, and can be solved uniquely with respect to any corner value of z
(hence, we can solve uniquely the initial value problem if initial data are given for instance along one horizontal line and two consecutive vertical lines).
A manifestation of the integrability of equations (
6) and (
8) is that they admit the same hierarchy of generalized symmetries in the
n
direction with the lowest symmetry being of order two. More precisely the first member of this hierarchy is given by
where
cn
is a periodic function with period 2, i.e.
cn+2=cn
. We can construct the higher order members of this hierarchy by considering commutators with the
local master symmetry which is another symmetry of equation (
8) and was derived using the integrability conditions for equation (
8). Moreover using the same conditions one may derive a hierarchy of canonical conservation laws and here we present (the equivalent to) the first two canonical conservation laws for (
9).
First canonical conservation law
where
∂tρ(0)=(S−1)(σ(0))
.
Second canonical conservation law
where
∂tρ(1)=(S2−1)(σ(1))
.
For difference equation (
8) the first canonical conservation law is equivalent to
with
(T−1)logϱ(0)=(S−1)logψ(0)
, and for the second law the density
ρ(1)
is given in (
12) but the flux is omitted here because of its length.
The symmetries in the vertical direction for the quadratic equation (6) can be derived by exploiting its relation to the quad equations presented in the next section. However, for equation (8) we do not know any symmetries in the m
direction.
3. Deautonomizations
Integrability conditions provide us the means not only to test if a given equation is integrable but also to find its generalized symmetries [5]. In this context, we employ equation (2) to find non-autonomous integrable generalizations of known partial difference equations defined on an elementary quadrilateral on the lattice. We describe our approach by using Hirota’s KdV and discrete potential KdV equations as illustrative examples and then present some results about the ABS equations [6] and their deformed counterparts [22].
3.1 Hirota’s KdV equation
We start with equation [
15]
and try to find the functions
an,m
for which it admits infinite hierarchies of symmetries in both lattice directions.
We start our analysis with the symmetries in the first direction in which case condition (
2) with
d=1
becomes
Assuming that equation (
13) admits a first order formal recursion operator, the analysis of (
14) with
N=1
leads to a linear system of first order partial differential equations for
R
which is consistent if and only if either
R=0
or
an+1,m=an,m
. Hence,
an,m
must be independent of
n
for the equation to admit symmetries of order one in the
n
direction. Working in the same way in the
m
direction we find also
an,m+1=an,m
. Hence, the only member of the family (
13) which satisfies the first order integrability conditions in both directions is Hirota’s KdV equation
which corresponds to
an,m=α
.
To find the equations in the family (13) the lowest generalized symmetries of which are of order two (at least in the n
direction), we consider the determining equation (14) with N=2
along with the requirement an+1,m≠an,m
to exclude any symmetries of order one. A linear system of differential equations for R
can be derived which is consistent provided that an+2,m=an,m
. Moving to symmetries in the m
direction and assuming that they are of order one, then our previous analysis implies that an,m+1=an,m
. However, assuming that the equation admits symmetries of order two in the m
direction, our analysis yields two constraints, namely an,m+2=an,m
and an+1,m+1+an,m=an+1,m+an,m+1
, which imply that an,m
must separate variables and be periodic with period two with respect to each variable.
We can summarize the above analysis for the symmetries of equation (13) in the following statement which can be proven by direct computations.
Theorem 3.1.
Let function an,m
be such that an+1,m+1+an,m=an+1,m+an,m+1
. Then in the n
direction, equation (13) admits
1.First order symmetries provided that
an+1,m=an,m
, which are generated by
where the
y
flow is a master symmetry of the
x
one.
2.Second order symmetries if
an+2,m=an,m
and
an+1,m≠an,m
, given by
and
where
F(±)=vn±1vn,m−an,m
and
ωn,m=vn+1,mv2n,mvn−1,m−an+1,mvn,m(vn+1,m+vn−1,m)+an,man+1,m
.
3.If
an,m
is periodic in
n
with period two and independent of
m
, i.e.
an+2,m=an,m
,
an+1,m≠an,m
and
an,m+1=an,m
, then there is one more second order symmetry, namely
In the m
direction, the lowest order symmetries of equation (13) are of order one if an,m+1=an,m
, and of order two if an,m+2=an,m
and an,m+1≠an,m
. The formulae for these symmetries follow from (16) to (19) by applying the changes (vn+i,m,an+i,m,n,S)→(vn,m+i,−an,m+i,m,T)
.
When
an+2,m=an,m
, equation (
13) and its symmetries are related to the equations in the previous section by the Miura transformation
Specifically it maps equation (13) to Wn,m(an+1,m,an,m,0)=0
in (6), and symmetries (17) and (18) to (9) with cn=1
and cn=(−1)n
, respectively.
Finally, at the limit an,m→α
, equation (13) reduces to (15) and in the same way (17)–(19) reduce to symmetries of the latter equation. Specifically, (19) reduces to the n
dependent symmetry in (16), (17) becomes the second order symmetry of (15) and (18) after multiplying it with the constant (an,m−an+1,m)(−1)n
leads to the first order autonomous symmetry in (16).
3.2 The discrete potential KdV equation
The next family of equations, we are going to consider is
This is a generic choice since equation
(un,m−un+1,m+1)(un+1,m−un,m+1)−fn,m=0
and the symmetry analysis imply that
fn,m
must separate variables, i.e.
fn,m=αn−βm
. Moreover, the covariance of the equation allows us to perform the symmetry analysis in one direction and then apply changes
(un+i,m+j,αn+i,βm+i,n,m)→(un+j,m+i,βm+i,αn+i,m,n)
to derive the results in the other direction. Herein, we present the analysis for the first direction using condition (
2) which now becomes
Assuming that equation (21) admits a first order formal recursion operator, condition (22) with N=1
leads to a system of partial differential equations which is consistent provided that either R=0
or αn+1=αn
. Hence equation (21) admits symmetries of order one only if αn+1=αn
and they can be found in [23]. To find the equations in family (21) admitting symmetries of order two but not of order one, we consider (22) with N=2
, along with αn+1≠αn
to exclude symmetries of lower order. The analysis of this equation implies that αn
must be a function of period two, αn+2=αn
, and for the corresponding symmetries we can state the following result which can be shown by direct computations.
Theorem 3.2
The lowest order symmetries of equation (
21) with
αn+2=αn
and
αn+1≠αn
are generated by
where
hn,m=(un,m−un+2,m)(un+1,m−un−1,m)−αn+αn+1
. Moreover, the Miura transformation
maps (
21) to
Wn,m(αn,αn+1,βm)=0
in (
6), and symmetry (
23) to (
9) with
cn=gn/(αn−αn+1)2
.
Symmetries (23), as well as (28) below, were first given in an equivalent form in [14].
3.3 Deautonomization of the ABS equations
We can go through the same analysis starting with any of the ABS equations H1–H3, Q1–Q31 [6] or the deformed H equations dH1–dH3 [22] and derive corresponding integrable equations depending on a periodic function of n
. We summarize these results in the following statement which can be verified by direct computations.
Theorem 3.3
Consider the equation
where
Q(un,m+1,un,m,un+1,m,un+1,m+1;α,β)
is the defining polynomial of any of the equations H1–H3, Q1–Q3 or dH1–dH3.
1. If αn
is constant, αn+1=αn
, then equation (25) admits first order symmetries in the n
direction [22, 23]
2. If
αn+2=αn
and
αn+1≠αn
, then the lowest order symmetries of (
25) are generated by
where
and functions
Pn,m=P(n,m,un−1,m,un,m,un+1,m)
are given in the following table.
Equation | Pn,m |
---|
H1 | 1 |
dH1 | 1−ϵ(un−1,mun+1,mXn,m+u2n,mYn,m) |
H2 | un−1,m+2un,m+un+1,m+αn+αn+1 |
dH2 | un−1,m+2un,m+un+1,m+αn+αn+1−4ϵ((αnun−1,m+αn+1un+1,m)Xn,m+α2n2 |
| (αnαn+1+un−1,mun+1,m)X2n,m+(α2n+α2n+12+(αn+αn+1)un,m+u2n,m)Y2n,m) |
H3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1) |
dH3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1)−ϵ(un−1,mun+1,mXn,m+α2n+α2n+12αnαn+1u2n,mYn,m) |
Q1 | (un,m−un−1,m)(un,m−un+1,m)−δ2αnαn+1 |
Q2 | (un,m−un−1,m)(un,m−un+1,m)−α2n+1un+1,m+(α2n+α2n+1−4αnαn+1)un,m−α2nun−1,m+α2nα2n+1 |
Q3 | αnαn+1un−1,mun+1,m−(αn(α2n+1+1)2un+1,m+αn+1(α2n+1)2un−1,m)un,m+α2n+α2n+12u2n,m+δ2(α2n−1)(α2n+1−1)4 |
Equation | Pn,m |
---|
H1 | 1 |
dH1 | 1−ϵ(un−1,mun+1,mXn,m+u2n,mYn,m) |
H2 | un−1,m+2un,m+un+1,m+αn+αn+1 |
dH2 | un−1,m+2un,m+un+1,m+αn+αn+1−4ϵ((αnun−1,m+αn+1un+1,m)Xn,m+α2n2 |
| (αnαn+1+un−1,mun+1,m)X2n,m+(α2n+α2n+12+(αn+αn+1)un,m+u2n,m)Y2n,m) |
H3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1) |
dH3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1)−ϵ(un−1,mun+1,mXn,m+α2n+α2n+12αnαn+1u2n,mYn,m) |
Q1 | (un,m−un−1,m)(un,m−un+1,m)−δ2αnαn+1 |
Q2 | (un,m−un−1,m)(un,m−un+1,m)−α2n+1un+1,m+(α2n+α2n+1−4αnαn+1)un,m−α2nun−1,m+α2nα2n+1 |
Q3 | αnαn+1un−1,mun+1,m−(αn(α2n+1+1)2un+1,m+αn+1(α2n+1)2un−1,m)un,m+α2n+α2n+12u2n,m+δ2(α2n−1)(α2n+1−1)4 |
Equation | Pn,m |
---|
H1 | 1 |
dH1 | 1−ϵ(un−1,mun+1,mXn,m+u2n,mYn,m) |
H2 | un−1,m+2un,m+un+1,m+αn+αn+1 |
dH2 | un−1,m+2un,m+un+1,m+αn+αn+1−4ϵ((αnun−1,m+αn+1un+1,m)Xn,m+α2n2 |
| (αnαn+1+un−1,mun+1,m)X2n,m+(α2n+α2n+12+(αn+αn+1)un,m+u2n,m)Y2n,m) |
H3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1) |
dH3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1)−ϵ(un−1,mun+1,mXn,m+α2n+α2n+12αnαn+1u2n,mYn,m) |
Q1 | (un,m−un−1,m)(un,m−un+1,m)−δ2αnαn+1 |
Q2 | (un,m−un−1,m)(un,m−un+1,m)−α2n+1un+1,m+(α2n+α2n+1−4αnαn+1)un,m−α2nun−1,m+α2nα2n+1 |
Q3 | αnαn+1un−1,mun+1,m−(αn(α2n+1+1)2un+1,m+αn+1(α2n+1)2un−1,m)un,m+α2n+α2n+12u2n,m+δ2(α2n−1)(α2n+1−1)4 |
Equation | Pn,m |
---|
H1 | 1 |
dH1 | 1−ϵ(un−1,mun+1,mXn,m+u2n,mYn,m) |
H2 | un−1,m+2un,m+un+1,m+αn+αn+1 |
dH2 | un−1,m+2un,m+un+1,m+αn+αn+1−4ϵ((αnun−1,m+αn+1un+1,m)Xn,m+α2n2 |
| (αnαn+1+un−1,mun+1,m)X2n,m+(α2n+α2n+12+(αn+αn+1)un,m+u2n,m)Y2n,m) |
H3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1) |
dH3 | 12(αnun−1,mun,m+αn+1un,mun+1,m+2δαnαn+1)−ϵ(un−1,mun+1,mXn,m+α2n+α2n+12αnαn+1u2n,mYn,m) |
Q1 | (un,m−un−1,m)(un,m−un+1,m)−δ2αnαn+1 |
Q2 | (un,m−un−1,m)(un,m−un+1,m)−α2n+1un+1,m+(α2n+α2n+1−4αnαn+1)un,m−α2nun−1,m+α2nα2n+1 |
Q3 | αnαn+1un−1,mun+1,m−(αn(α2n+1+1)2un+1,m+αn+1(α2n+1)2un−1,m)un,m+α2n+α2n+12u2n,m+δ2(α2n−1)(α2n+1−1)4 |
3.For the non-autonomous ABS equations, the Miura transformation
maps the difference equation (
25) to the quadratic non-autonomous quad equation (
6) with parameters
and its symmetry (
26) to (
9) with
cn=gnp2n/k(αn+1,αn)2
.
4.If
αn+2=αn
with
αn+1≠αn
, and
βm=β∈R
, then equations H1 and H2 admit one more symmetry, namely
In the m
direction, the lowest order symmetries of equation (25) are of order one if βm+1=βm
, and of order two if βm+2=βm
and βm+1≠βm
. The formulae for latter symmetries follow from (26), (28) and (29) by applying the changes (un+i,m,αn+i)→(un,m+i,βm+i)
.
At the limit αn→α
, equation (25) reduces to the original autonomous equation and (26) yields the first two symmetries of the latter equation. Indeed, symmetry (26) with gn=1
reduces to the second order symmetry of the corresponding autonomous equation [4], whereas with gn
such that gn−gn+1=k(αn,αn+1)
it reduces to a linear combination of the first and the second order symmetry of the original equation. Finally, at the limit αn→α
, (28) and (29) lead to the n
dependent first order symmetries of the autonomous equations H1 and H2, respectively, given in [23].
Another interesting characteristic of (
26) with
gn=1
is that it can be interpreted as a non-autonomous extension of
where
h
is an affine linear polynomial possessing the symmetries of the square and
f(un,m,un+1,m)
is determined by
h(un−1,m,un,m,un+1,m,un+2,m)
in the similar way
fn,m
is determined from
hn,m
in (
26b). These equations were studied recently in [
17] in connection with seven point difference equations and Q4, whereas their relation to equation (
9) with
cn=1
is given by the Miura transformation (
27) with
pnk(αn+1,αn)=1
. The connection of
h
in (
30) with the defining polynomial of Q4 as described in [
17] as a limiting process differs from relation (
26b). We can think the latter as straightening an elementary quadrilateral by identifying parameter
β
with
αn−1=αn+1
and
un,m+1
,
un+1,m+1
with
un−1,m
and
un+2,m
, respectively.
3.4 Other deautonomized partial difference equations
We can apply the same procedure to other equations and derive their non-autonomous integrable counterparts which admit higher order symmetries. Herein, we present the discrete sine-Gordon and non-autonomous Hietarinta–Viallet equations, as well as the deautonomization of H1 admitting symmetries of order three in the n
direction.
3.4.1 Discrete sine-Gordon equation
The deautonomized discrete sine-Gordon equation
where
αn
and
βm
are non-constant periodic functions with period two, possesses generalized symmetries in both directions the lowest order of which is two. The first symmetry in the
n
direction is generated by
where
˜hn,m=αn+1(un+2,mun−1,m+un+1,mun,m)+αn(un+2,mun+1,m+un,mun−1,m)
, and the corresponding one in the other direction follows from (
32) by changing
un+i,m
to
un,m+i
and
αn+i
to
βm+1+i
. Up to a point transformation, differential-difference equation (
32) is the symmetry of the deautonomized H3 with
δ=0
.
3.4.2 Hietarinta–Viallet equation
Equation
is a deautonomization of
wn,mwn,m+1−wn,m+1wn+1,m+1+wn+1,mwn+1,m+1=0
, an equation due to Hietarinta and Viallet [
24]. Its lowest order generalized symmetries in the
n
direction are of order two generated by
where
χn,m:=wn+2,m(wn+1,m−αn+1wn−1,m)−αn+1wn,m(wn+1,m−αnwn−1,m)
, whereas the symmetries in the
m
direction are generated by
Moreover, the Miura transformation
maps equation (
33) to
Wn,m(αn,αn+1,0)=0
and its symmetries (
34a) and (
34b) to equation (
9) with
cn=1/(αn−αn+1)2
and
cn=(−1)n/(αn−αn+1)2
, respectively.
3.4.3 Discrete potential KdV equation and third order symmetries
In all our previous examples, we have considered equations admitting symmetries of order one or two. We can continue and consider deautonomized equations admitting symmetries of order three in the n
direction. But this is a very difficult computational task as the calculations are lengthy and cumbersome. We were able to partially analyse the discrete potential KdV equation, and we can present the outcome of our analysis in the following form.
Theorem 3.4
The lowest order generalized symmetries in the
n
direction of equation
are of order three. A symmetry is generated by
where
gn+3=gn
is an arbitrary function,
wn,m=un+1,m−un−1,m
and
Another symmetry is generated by
Symmetry (36) yields the first three generalized symmetries of H1 at the limit αn→α
. In particular, (36) with gn=1
reduces to third order symmetry of H1, with gn=αn+2
leads to a linear combination of the third and the second order symmetries, and with gn=αnαn+1
yields a linear combination of the first three symmetries of H1. On the other hand, (37) reduces to the first order n
dependent symmetry of the original potential KdV equation [23]. It should be noted that equation (35) was also discussed in [14] and a third order symmetry was given there (with some misprints) which corresponds to (36) with gn=αn+1(αn+1−αn+2)(αn−αn+2)
.
4. Differential-difference equations and reductions
Exact reductions of a differential-difference equation lead to ordinary difference equations and in particular, as it was conjectured in [25], every autonomous difference equation obtained by an exact reduction of the differential-difference equation is an integrable mapping. In this section, we present exact reductions of the non-autonomous equations (9), (17), (23), and of their conserved forms, which lead to non-autonomous ordinary difference equations and corresponding first integrals. As some of these reductions lead to alternating QRT maps [18, 19], these examples suggest that in certain cases the QRT conjecture is also valid for non-autonomous equations.
Example 1
We start with the stationary solutions of (
9) which satisfy the non-autonomous ordinary difference equation
∂tzn=0
(here and in the following examples, we suppress the second index
m
as it does not vary). We can readily integrate the resulting equation twice and then write it as
where
bn
is the constant of integration. Moreover this equation admits the first integral
which follows from the first canonical conservation (
11) of (
9) presented in
Section 2.
Example 2
We consider equation (
17) with
an,m=αn
being periodic with period two. Seeking for solutions of the form
v(n,t)=exp(μ(−1)nt)vn
, we substitute this form into (
17) and after one integration we find that
vn
is related to the solution
fn
of the alternating QRT map
a first integral of which is given by
where
sn=α2n−α2n+1−(αn−αn+1)(bn+bn+1)
and
rn=(2α2nα2n+1+αn(αn−αn+1)bnbn+1)/(αn+αn+1)
. Specifically, the relation between
vn
and
fn
is
where
bn=αn(1+(λ−μ(−1)n/2)αn+1(αn+1−αn))
is periodic with period two and
λ
is the constant of integration.
Remark 4.1
The first integral (41) is the reduction of the first canonical conservation law of (17) which can be derived from (11) after using the Miura transformation (20).
Example 3
We seek for solutions to the differential-difference equation (
23) of the form
u(n,t)=(λ+μ(−1)n)t+un
. Substituting into the equation and setting
(un+1−un−1)(un−un−2)+αn+1−αn=δ−1n
, we find that
δn
must satisfy equation
A first integral of this map is given by
On the other hand, searching for solutions to (
23) of the form
u(n,t)=exp(μ(−1)nt)un
, we introduce function
yn
as
unun+1=(αn−αn+1)yn
to find that it must satisfy the ordinary difference equation
where
Fn:=(yn+2+yn+1)(yn+1+yn)−yn+1
and
μn:=μ(αn−αn+1)2(−1)n
. Equation (
44) admits a two-integral
Jn
and a first integral
In
given by
respectively, where
Remark 4.2
The integrals follow from the reduction of the corresponding conserved forms of (23) which can be derived from (11) and (12) by employing the Miura transformation (24).
5. Difference equations and periodic reductions
The difference equations we derived in the previous section can also be interpreted as defining certain group invariant solutions of the related partial difference equations. In this section, we consider some particular periodic reductions of the latter equations and show how they lead to families of non-autonomous ordinary difference equations. Since the periodic functions appearing in the equations are specific, our approach differs from similar considerations in [15, 26] where the reduction determines also the form of the arbitrary functions involved in the equations.
To be more precise, in this section, we discuss periodic reductions of equations
and
The former is (13) with an,m=αn
and the latter is (21) with βm=0
where in both cases αn
is a non-constant and periodic with period two, i.e. αn=a(−1)n+b
. According to our previous analysis (see Theorems 3.1 and 3.2), these equations admit symmetries of order one and two in the m
and n
direction, respectively, and corresponding canonical conservation laws can be found in the Appendix. Moreover, solutions of these two equations are related according to
Proposition 5.1.
The system of equations
defines a Bäcklund transformation between a solution
vn,m
of equation (
46) and a solution
un,m
of equation (
47).
We are going to consider the
(k,−1)
periodic reductions of equations (
46) and (
47). The choice of the steps in this reduction is motivated from the dependence of the equations on a periodic function of
n
. Such reductions amount to consider the equation along with the relation
un,m+1=un+k,m
and its consequences,
un+i,m+j=un+i+jk,m
. These relations clearly allow us to remove any dependence on
m
from the equation and derive a non-autonomous map with
n
as the independent variable. Specifically, equation (
46) becomes
whereas equation (
47) reduces to
In both equations, we have suppressed the second index of functions v
and u
since it does not vary.
Moreover, we can replace shift operator T
with Sk
in any conserved form of the original equations and potentially derive first integrals of the resulting maps. If (S−1)(pn)=(T−1)(qn)
is a conserved form of the equation, then the corresponding candidate for a first integral will be pn−qn−…−qn+k−1
. In the same way, we may derive a Lax pair for the reduced equations. More precisely, if system Ψn+1,m=Ln,mΨn,m
, Ψn,m+1=Mn,mΨn,m
is the Lax pair of the original equation and Ln,m+1Mn,m=Mn+1,mLn,m
is its compatibility condition, then in view of the (k,−1)
periodic reduction the latter relation becomes Ln+kMn=Mn+1Ln
, where we have omitted the second index. We may now define matrices Mn=Ln+k−1Ln+k−2⋯LnM−1n
and Ln=Ln+k
, and then write the reduced compatibility condition as Mn+1=LnMnL−1n
.
It should be noted though that we can construct first integrals and Lax pairs in the way we described above only when k
is a multiple of two. This is because the equations are non-autonomous and function αn
is periodic with period 2
. As a consequence we separate the two cases below and first we discuss the even reductions (k=2p)
for both equations and present their connections, and then we analyse the odd order reductions (k=2p+1)
.
Remark 5.2
The maps (49) may be considered a non-autonomous extension of the ones studied recently in [20]. Moreover, as a generalization of Proposition 4.2 in [20], one can easily prove
Proposition 5.3
Suppose that
vn=τnτn+k+1/(τn+1τn+k)
is a solution of equation (
49). Then, for any integer value of
k
, function
τn
satisfies the bilinear equation
If
k
is odd, then
τn
also satisfies
5.1 The even order reductions
5.1.1 Hirota’s KdV equation
If
k=2p
,
p∈Z>0
, equation (
49) becomes
and admits two first integrals and a two-integral which follow from our considerations and can be found in the Appendix, see relations (
A.3–
A.5). Moreover one additional integral follows from the equation itself since it is a total difference yielding the first integral
For these maps we can construct matrices
Mn
and
Ln
using as building blocks
The trace of matrix Mn
is a polynomial of the form p∑i=0F(i)nλ2i−2
, and the coefficients of λ
are first integrals of the map. For the cases, we have checked we found F(p)n=Jn
and F(0)n=In
, where Jn
and In
are given in (52) and (A.3), respectively.
Example 4
For
p=1
(or equivalently
k=2
), the map is
and it admits two functionally independent first integrals,
Example 5
For
p=2
(or equivalently
k=4
), the map is
and it admits two first integrals,
and the two-integral
Tn
(
A.5), which in this case has the following form,
Two more integrals can be derived from our considerations,
K′n
from the trace of the monodromy matrix, and
Kn
from the general formula (
A.4) in the Appendix. However, they are not functionally independent since
5.1.2 The potential KdV equation
Considering equation (
50) with
k=2p
, we introduce a new variable
wn=un+1−un
to derive
First integrals follow from the reduction of the conserved forms of equation (47) and can be found in the Appendix, see relations (A.9–A.11).
Example 6
The reduced difference equation for
p=1
(k=2)
is
which may be viewed as a degenerated form of (the most general) discrete Painlevé I [
27], and admits the first-integral
5.1.3 Bäcklund transformations
One can derive connections among the maps constructed previously by applying the same periodic reduction to Proposition 5.1. It is not difficult to see that transformation (48) is compatible only with the even order reductions because of the periodicity of function αn
. So we state the following
Proposition 5.4
The system of equations
defines a transformation between a solution
vn
of (
51) and a solution
wn
of (
55).
Proof.
If we shift the second equation 2p
times and multiply the resulting relation with the first equation in (58), then we find that wn
satisfies (55). For the converse, let us denote with f
and g
the first and the second equation in (58), respectively. Then the combination S2p(g)−S(f)
yields wn+1+wn=vn+2p+1−αn/vn+2p
, whereas S(g)−S−2p(f)
leads to wn+1+wn=vn−αn+1/vn+1
. From the last two relations it follows that vn
must obey (51). □
5.2 The odd order reductions
5.2.1 Hirota’s KdV equation
When
k=2p+1
we introduce a new variable
xn=vnvn+1
in view of which map (
49) becomes
This map admits the first integral
which can be derived either from (
59) or from the reduction of the first conservation law (
A.2). We may consider
In=1
as our main equation which after the change
xn↦−α(p+1)/(2p+1)nαp/(2p+1)n+1xn
can be written as
where
bn=(−1)pα−(p+1)2/(2p+1)nα−p(p+1)/(2p+1)n+1
is periodic function with period 2. If we introduce even and odd variables
en
and
on
via the relations
en+i=x2n+2i
and
on+i=x2n+2i+1
, respectively, and denote
b2n+2i=α
,
b2n+2i+1=β
, then these variables will satisfy equations
Gp(en,α,β)=0
and
Gp(on,β,α)=0
, respectively, where
Example 7
For p=1
, the map (61) becomes xnxn+2−xn+1=bn
which is the second order periodic non-autonomous Lyness’ difference equation, an integrable map [21]. The corresponding odd-even variables decoupled system is the QRT map (fn−1fn−a)(fnfn+1−a)=fn+b
.
Example 8
When
p=2
the equation is
and the corresponding decoupled system of odd-even variables is related to solutions of the fourth order equation
5.2.2 The potential KdV equation
When
k=2p+1
the left hand side of (
50) can be written as
(S2p+1+1)(unun+1)−(S+1)(unun+2p+1)
. This allows us to integrate it once and then, upon the difference substitution
xn=(−1)nunun+1
, write the resulting equation as
where
γ
is the constant of integration. Since
αn
is a periodic function with period 2, we can choose without loss of generality
αn=−α(−1)n+2β
, change
γ→γ−α/2
and then write equation (
65) as
i.e. a family of discrete Painlevé type equations.
Example 9
The first member
(p=1)
of the family is
(xn+xn+1)(xn+1+xn+2)=znxn+1
which, upon the substitution
xn+1+xn=yn
becomes
xn=yn−ynyn+1/zn
and then leads to
6. Concluding remarks
We presented a method for the deautonomization of partial difference and differential-difference equations using the existence of infinite hierarchies of symmetries in both directions as integrability detector. In this way, we derived integrable non-autonomous difference equations along with compatible differential-difference equations (symmetries) and conservation laws. Our results include non-autonomous versions of various known quad equations and their second and third order non-autonomous symmetries which, as far as we are aware, are new and deviate from previous works [22, 28, 29] in which the first symmetries are of order one and related to Yamilov’s discrete non-autonomous Krichever–Novikov equation [30]. The most interesting phenomenon is that most of the deautonomized equations and their symmetries are related via Miura transformations to the two-quad equation (8) and its symmetries (9). Our results along with the ones in [16, 17, 31] justify the importance of equation (9) as it was already pointed in [17].
Reductions of the derived differential-difference equations led to integrable non-autonomous ordinary difference equations and in certain cases to alternating QRT maps, whereas the reductions of the corresponding conservation laws yielded integrals for the resulting equations. And the periodic reductions of equations (46) and (47) led to families of non-autonomous maps and discrete Painlevé type equations.
It would be interesting to apply this method for the derivation of non-autonomous differential-difference equations of order higher than two (with one such example provided by (36)), but also to extend it to systems of difference equations and their symmetries.
Acknowledgements
The author would like to thank Frank Nijhoff and Andy Hone for useful discussions and suggestions.
Appendix
In this section, we have collected three canonical conservation laws and their reductions for equations (46) and (47).
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