Jacobi-Lie Hamiltonian systems
on
real low-dimensional
Jacobi-Lie groups and their
Lie symmetries
**H. Amirzadeh-Fard1 ** 111 e-mail: [email protected],
Gh. Haghighatdoost2 222 e-mail: [email protected],
**A.
Rezaei-Aghdam3 333 e-mail: [email protected]
1,2***Department
of Mathematics, Azarbaijan Shahid Madani University, 53714-161, Tabriz, Iran
3Department of Physics, Azarbaijan Shahid Madani
University, 53714-161, Tabriz, Iran
Abstract
We study Jacobi-Lie Hamiltonian systems admitting Vessiot-Guldberg Lie algebras of Hamiltonian vector
fields related to Jacobi structures on
real low-dimensional
Jacobi-Lie groups. Also,
we find some examples
of Jacobi-Lie Hamiltonian systems on
real two- and three- dimensional Jacobi-Lie groups.
Finally, we present
Lie symmetries of Jacobi-Lie Hamiltonian systems on some three-dimensional real Jacobi-Lie groups.
keywords: Jacobi-Lie group, Jacobi manifold, Lie system, Jacobi-Lie Hamiltonian system, Lie symmetry.
1 Introduction
A Lie system is a non-independent system of first-order ODEs that possesses a superposition rule. In other words,
a Lie system amounts to a non-autonomous vector field that takes values in a finite-dimensional real Lie algebra of vector fields,
referred to as Vessiot-Guldberg Lie algebra
(VG Lie algebra)
of the system, with respect to a geometric
structure.
At the end of the 19th century, the study
of Lie systems was
carried out by Sophus Lie,
who pioneered the study of systems of
ODEs
admitting superposition rules [References].
Then about a century, the study of this problem was silent.
After the work of
Winternitz [References],
many authors have recently
investigated this problem [References-References].
Some results have been obtained for Lie systems admitting
a VG Lie algebra of Hamiltonian vector fields relative to
symplectic and Poisson structures
[References].
A particular class of Lie systems on Poisson manifolds, the so-called Lie-Hamilton systems, that admit a VG Lie algebra of Hamiltonian vector fields with
respect to a Poisson structure was studied in [References].
Recently Lie systems possessing a VG Lie algebras of Hamiltonian
vector fields with respect to Jacobi structures [References, References, References]
were
referred to as the Jacobi-Lie systems are studied and exactly introduced in [References].
It is well known that
the symplectic
manifold is a particular case of the
Poisson manifold
so that the Poisson bracket
is not necessarily assumed to be non-degenerate.
In order that the Jacobi bracket is not necessarily assumed to be derivation,
the
Jacobi manifold
is a generalization of
the Poisson manifold
[References, References].
To wrap up the discussion,
Lie-Hamiltonian systems
are a generalization of Hamiltonian systems
and
a particular case of
the Jacobi-Lie Hamiltonian systems.
In this work, we study Lie systems with VG Lie algebras
of Hamiltonian vector fields with respect to Jacobi-Lie groups
[References],
especially
on real two and three-dimensional Jacobi-Lie
groups [References, References].
The outline of the paper is as follows:
In section 2, we recall several definitions
and results in Lie systems and Jacobi structures on Jacobi-Lie
groups [References]
and Jacobi-Lie Hamiltonian system on a Jacobi manifold [References].
In Section 3 we exemplify results of Sections 2 on real two- and three-dimensional
Jacobi-Lie groups [References, References].
Finally, in Section 4 we study
Lie symmetry of Jacobi-Lie Hamiltonian system on some three-dimensional real Jacobi-Lie groups.
2 Definitions and Notations on Lie and Jacobi-Lie Hamiltonian system
For simplicity,
all functions and geometric
structures throughout this paper
are assumed to be real, smooth, and globally defined.
In order to highlight the main aspects of our results, let
us omit minor technical problems.
Here,
for self-containment of the paper, we review some basic
concepts of Lie, Lie-Hamiltonian [References, References] and
Jacobi-Lie Hamiltonian systems [References].
2.1 Lie systems and Lie-Hamiltonian systems
Let
a and b
be two vector subspaces of Lie algebra g,
and let [a,b] denote the vector
space spanned by the Lie brackets between elements of a and b,
respectively.
We define Lie(a,g,[.,.]) to be the smallest Lie subalgebra of
(g,[.,.]) containing a
and represent it with
Lie(a).
Definition 2.1
A t-dependent vector field on a manifold M is a map
[TABLE]
satisfying τMoX=π2,
where
π2 and τM
are the projections from R×M and TM onto M, respectively.
Using this definiition, we can identify every t-dependent vector field
with a family {Xt}t∈R of vector fields
Xt:M⟶TM,x↦Xt(x)=X(t,x),
and vice versa.
Definition 2.2
The minimal Lie algebra of X on a manifold M is the smallest
real Lie algebra, gX, containing the vector fields {Xt}t∈R. In other words,
gX=Lie({Xt}t∈R).
Definition 2.3
An integral curve of X is an
integral curve
α:R⟶R×M,t↦(t,x(t)),
of the suspension of X [References], i.e. for the vector field
[TABLE]
we have
dtdx(t)=X(t,x).
Definition 2.4
A Lie system is a system
X
on a manifold M
whose
gX
is finite-dimensional [References].
Definition 2.5
A superposition rule
depending on n particular solutions
for a system X on a manifold M is a function Ψ:Mn×M⟶M,
(x(1),...,x(n);k)⟼x,
such that the general solution x(t) of X can be
written as
[TABLE]
where x(1)(t),...,x(n)(t) is any generic
collection
of particular solutions to X and k=(k1,...,km)
is a point of M to
be related to initial conditions
of X [References].
Theorem 2.6
*(The Lie-Scheffers Theorem) ***
A system X on M admits a superposition
rule if and only if
it can
be written in the form
[TABLE]
for a set b1(t),...,br(t) of t-dependent functions and a family of vector fields X1,...,Xr on
M spanning an r-dimensional real Lie algebra: a VG Lie algebra of X.
That is to say,
a system X on M possesses a superposition rule if
and only if it is a Lie system
[References,References].
Definition 2.7
A manifold M endowed with bivector structure P∈Γ(⋀2TM)
satisfying that
[P,P]=0
is called a Poisson manifold
(M,P),
where
[., .]
is the Schouten-Nijenhius bracket
444[X1∧...∧Xp,Y1∧...∧Yq]=i=1∑pj=1∑q(−1)i+j[Xi,Xj]∧X1∧...∧Xi^∧...∧Xp∧Y1∧...∧Yj^∧...∧Yq
and
Γ(⋀2TM)
is the space of sections of
⋀2TM [References].
The bivector P has a bundle morphism
P#:TM∗⟶TM
is defined by
β(P#α)=P(α,β)∀α,β∈TM∗.
Definition 2.8
A vector field X on M with the
bivector P
is said to be a Hamiltonian vector field
if
it can be written as
X=P#(df)
where f is a function on M, called the Hamiltonian;
conversely, every function f is called the Hamiltonian function of a unique
Hamiltonian vector field Xf.
Definition 2.9
A Lie-Hamiltonian system on a Poisson manifold M is a Lie system X whose
gX
consists of
Hamiltonian vector fields relative to a Poisson bivector
P
[References].
2.2 Jacobi and Jacobi-Lie structures
The study of the Jacobi manifolds was made by Lichnerowicz and Kirillov [References, References].
Definition 2.10
A Jacobi manifold is a triple (M,Λ,E), where Λ is a 2-vector field and E
is a vector field on M (called the Reeb vector
field) such that
[TABLE]
where
the bracket is that of Schouten-Nijenhuis bracket.
The space (C∞(M),{.,.}Λ,E) is
a local Lie algebra in the sense of Kirillov [References] with the Jacobi bracket
[TABLE]
This Lie bracket is a Poisson bracket
if and only if the vector field
E identically vanishes.
Iglesias and Marrero have proved in [References] that if Lie group G is a connected simply connected with Lie algebra g and
the pair((g,ϕ0),(g∗,X0)) is a Jacobi-Lie bialgebra then G
is Jacobi-Lie group and
has a special Jacobi
structure.
Definition 2.11
A Jacobi-Lie bialgebra is a pair ((g,ϕ0),(g∗,X0)), where g is a finite dimensional real Lie algebra with Lie bracket [,]g and g∗ is dual space of g with Lie bracket [,]g∗; also, ϕ0∈g∗ and
X0∈g are 1-cocycles on g and g∗, respectively, such that
for all X,Y∈g
satisfying the following properties:
[TABLE]
[TABLE]
[TABLE]
where
[TABLE]
moreover,
d∗ is the Chevalley-Eilenberg differential
of g∗ and d∗X0 is the X0-differential of
g∗
as well as the operation [,]ϕ0g is the ϕ0-Schouten-Nijenhuis bracket
[References].
Theorem 2.12
Let the pair ((g,ϕ0),(g∗,X0)) be a Jacobi-Lie bialgebra and Lie group
G be a connected
simply connected admitting Lie algebra g. Then, there exists a unique multiplicative
function σ:G⟶R and a unique σ-multiplicative bivector
Λ on G satisfying (dσ)(e)=ϕ0
and the intrinsic derivative of bivector at e is −d∗X0, i.e.,
deΛ=−d∗X0.
Furthermore, the following identity holds
[TABLE]
where E=−X~0
and the pair (Λ,E) is a Jacobi structure on G;
in addition,
both
X~ and Xˉ are the right and left invariant vector field such that
X~0(e)=Xˉ0(e)=X0
[References].
Definition 2.13
A Coboundary Jacobi-Lie bialgebra is a Jacobi-Lie bialgebra
such that d∗X0 is a 1-coboundary that is, there exists r∈∧2g satisfying that
[TABLE]
(for more details, see [References]).
A Jacobi structure on G was determined by Iglesias and Marrero in [References], as follows:
[TABLE]
Where both
r~ and rˉ are
right and left invariant 2-vector on
the Lie group G
as well as X~0 is right invariant vector field on G.
Furthermore,
(dσ)(e)=ϕ0.
The relation (12)
can
be expressed in terms of coordinate on M as follows
[References]:
[TABLE]
and
[TABLE]
Where both XiR
and XiL are the ith coordinates of the right and left invariant vector fields on
the Lie group G. Moreover, rij is calculated from the relation r=21rijXi∧Xj
, and multiplicative
function σ:G⟶R is defined as
(dσ)(e)=ϕ0
as well as
αi is obtained from the relation
X0=αiXi
where
{Xi} is
the basis of the Lie algebra
g.
Now, using
the results in [References] and relations
(13) and (14), one can calculate the vector field E and 2-vector Λ related to real two- and three- dimensional Jacobi-Lie bialgebras. The results are listed in Tables 1-3.
The first column gives the names of the real two- and three-dimensional Jacobi-Lie bialgebras according to [References], and the second column gives the
Jacobi structure on Lie
group G related to Lie
algebra g.
Note
that in [References] the bi-r-matrix Jacobi-Lie bialgebras as
Jacobi-Lie bialgebras being coboundary in two directions, that is,
((g,ϕ0),(g∗,X0)) and
((g∗,X0),(g,ϕ0)) having classical r-matrices r and r~ have been classified. Nevertheless, they
classified coboundary Jacobi-Lie bialgebras having r or r~.
2.3 Jacobi-Lie Hamiltonian systems
Jacobi-Lie Hamiltonian systems
were introduced in [References].
In other words,
Lie systems possessing a Vessiot-Guldberg Lie algebra of Hamiltonian functions with
respect to a Jacobi structure.
One of the most useful constructions on Jacobi manifolds is in a sense analogue of the gradient, defined as follows.
Definition 2.14
A vector field X on the manifold M with the
Jacobi structure
is said to be a Hamiltonian
if there exists a function f, referred to as Hamiltonian, such that
[TABLE]
where
the bracket is that of Schouten-Nijenhuis bracket[References].
If Ef=0 (that is,
the derivative of the function f in the direction of the vector field E is equal
to zero), then the function f is called a good Hamiltonian function and Xf
a good Hamiltonian vector field [References].
Let f be a smooth function on the Jacobi manifold M.
There exists a unique vector field Xf on M, referred to as
Hamiltonian vector field associated with f,
such that the following equality is satisfied
[TABLE]
However, a vector field
Xf
can possess several Hamiltonian functions.
Obviously,
(Ham(M,Λ,E),[.,.]) is a Lie algebra,
where
the bracket is that of vector fields bracket
and
Ham(M,Λ,E) is the space of Hamiltonian vector fields of Jacobi manifold.
Definition 2.15
A Jacobi-Lie system is a quadruple (M,Λ,E,X) where (M,Λ,E)
is a Jacobi manifold and a Lie system X such that gX⊂Ham(M,Λ,E) [References].
Definition 2.16
A Jacobi-Lie Hamiltonian system is a quadruple (M,Λ,E,f) where (M,Λ,E)
is a Jacobi manifold
and f:R×M⟶M,(t,x)↦ft(x)
is a
t-dependent function and Lie({ft}t∈R,{.,.}Λ,E) is finite-dimensional. The vector field X on M is said to be Jacobi-Lie Hamiltonian system (M,Λ,E,f)
if Xft is a Hamiltonian vector field with Hamiltonian function ft (relative to
Jacobi manifold)
∀t∈R
[References].
Theorem 2.17
If (M,Λ,E,f) is a Jacobi-Lie Hamiltonian system, then the system
X of the form
Xt=Xft,∀t∈R,
is a Jacobi-Lie system (M,Λ,E,X). If
X is a Lie system whose {Xt}t∈R are good Hamiltonian vector fields, then X possesses
a Jacobi-Lie Hamiltonian [References].
3 Jacobi-Lie Hamiltonian systems on
real low-dimensional
Jacobi-Lie groups
Now, we consider some Jacobi structures obtained by using the real two and three dimensional
Jacobi-Lie groups
related to
Jacobi-Lie
bialgebras (see table 1, 3 below).
In these examples, we consider the Lie group G related to the Jacobi-Lie bialgebra
((g,ϕ0),(g∗,X0)).
For
this propose we use the formalisms mentioned in the previous section for calculation of
Jacobi-Lie Hamiltonian systems
on real low dimensional Jacobi-Lie groups.
Example 1.
Real two-dimensional bi-r-matrix Jacobi-Lie bialgebra
((A2,bX~2),(A2.i,−bX1))[References]:
Consider
the Lie group
A2 (with the coordinates x,y) related to Lie algebra
A2.
For this example, the
Jacobi structure and Reeb vector have the following forms (see table 1):
[TABLE]
Simple calculations show that they satisfying in
[TABLE]
where [.,.] is the Schouten-Nijenhuis bracket.
Thus, (A2,ΛA2,EA2)
is a Jacobi manifold.
It is easy to check
that
[TABLE]
span Lie algebra A2(i.e.,[X1H,X2H]=X1H) of Hamiltonian vector fields
on A2.
Consider now the
system on A2
defined by
[TABLE]
for arbitrary t-dependent functions bi(t).
XA2 is a Lie system
since the associated t-dependent vector field
XA2=∑i=12bi(t)XiH takes values in the Lie algebra
[X1H,X2H]=X1H,namely, Lie algebra A2.
We now illustrate that the Lie system (18)
is a Jacobi-Lie
system.
Indeed, X1H and X2H are Hamiltonian vector fields
with respect to
(A2,ΛA2,EA2)
with Hamiltonian
functions
f1=eb−x
and
f2=1, respectively ( i.e.,
XiH=Λ#(dfi)+fiE);
consequently,
(A2,ΛA2,EA2,XA2)
is a Jacobi-Lie
system.
Since
f=∑i=12bi(t)fi=b1(t)eb−x+b2(t)
is a Hamiltonian
function of
XA2 for every t∈R and the
functions
f1 and f2
satisfy the commutation
relation
{f1,f2}ΛA2,EA2=f1,
then
the functions {ft}t∈R span a finite-dimensional real Lie algebra
of functions
with respect to the Lie bracket induced by
(17). Consequently, XA2
admits a Jacobi-Lie
Hamiltonian
system
(A2,ΛA2,EA2,f).
Example 2.
Real three-dimensional bi-r-matrix Jacobi-Lie bialgebra
((\@slowromancapiii@,−bX~2+bX~3),(\@slowromancapiii@.iv,bX1)) [References]:
Consider
the Lie group
\@slowromancapiii@ (with the coordinates x,y,z) related to Lie algebra
\@slowromancapiii@.
For this example, the
Jacobi structure and Reeb vector have the following forms (see table 2):
[TABLE]
Obviously,
[Λ\@slowromancapiii@,Λ\@slowromancapiii@]=−2b(y+z)eb(y−z)∂x∧∂y∧∂z=2E\@slowromancapiii@∧Λ\@slowromancapiii@
and
[E\@slowromancapiii@,Λ\@slowromancapiii@]=0.
As a result,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@)
is a Jacobi manifold.
It is straightforward to verify
that
the Lie algebra, \@slowromancapii@, of Hamiltonian vector fields
on \@slowromancapiii@ is
spanned by
[TABLE]
[TABLE]
where
Ei(1,−b(y+z))=∫−b(y+z)∞xe−xdx
The system on \@slowromancapiii@ can be defined as
[TABLE]
for arbitrary t-dependent functions bi(t).
So that the associated t-dependent vector field
X\@slowromancapiii@=∑i=13bi(t)XiH
takes values in the Lie algebra \@slowromancapii@
,that is, [X2H,X3H]=X1H
; so X\@slowromancapiii@ is a Lie system.
We now manifest that
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,X\@slowromancapiii@)
is a Jacobi-Lie system. Infact, X1H and X2H,and X3H are Hamiltonian vector fields
relative to
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@)
with good Hamiltonian
functions
f1=1
and
f2=y, and f3=−e−2byEi(1,−b(y+z) respectively ( i.e.,
XiH=Λ#(dfi)+fiE);
subsequently,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,X\@slowromancapiii@)
is a Jacobi-Lie system.
Because
f=∑i=12bi(t)fi=b1(t)+b2(t)y−b3(t)e−2byEi(1,−b(y+z)
is a Hamiltonian
function of
X\@slowromancapiii@ for every t∈R, and the
functions
f1,f2
and
f3 satisfy the commutation
relations
{f2,f3}Λ\@slowromancapiii@,E\@slowromancapiii@=f1,
then
the functions {ft}t∈R span a finite-dimensional real Lie algebra
of functions
with respect to the Lie bracket induced by
(19). Consequently, X\@slowromancapiii@
admits a Jacobi-Lie Hamiltonian system
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,f).
Example 3.
Real three-dimensional bi-r-matrix Jacobi-Lie bialgebra
((\@slowromancapiii@,0),(\@slowromancapiii@.v,21X2−21X3)) [References]:
Consider
the Lie group
\@slowromancapiii@ (with the coordinates x,y,z) related to Lie algebra
\@slowromancapiii@.
For this example, the
Jacobi structure and Reeb vector have the following forms (see table 2):
[TABLE]
one can show that
[TABLE]
So
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@)
is a Jacobi manifold.
A simple calculation shows that
X_{1}^{H}=-\frac{1}{2}\,\left(2\,x-3\,y-z-2\right)\left(-1+{e}^{2\,x}\right)\partial_{x}+\Big{(}\frac{3}{2}\,{e}^{2\,x}y+\frac{1}{2}\,{e}^{2\,x}z+{e}^{2\,x}+\frac{y}{2}-\frac{z}{2}-1-{e}^{2\,x}x-x\Big{)}\partial_{y}+\Big{(}-\frac{3}{2}\,{e}^{2\,x}y-\frac{1}{2}\,{e}^{2\,x}z-{e}^{2\,x}+\frac{3}{2}\,y+\frac{5}{2}\,z+1+{e}^{2\,x}x+{y}^{2}+2\,yz+{z}^{2}+x\Big{)}\partial_{z},\,X_{2}^{H}=\Big{(}\frac{1}{2}-\frac{1}{2}e^{2x}\Big{)}\partial_{x}-\frac{1}{2}e^{2x}\,\partial_{y}+\frac{1}{2}\,e^{2x}\,\partial_{z}
and
X3H=−21∂y+21∂z
span the Lie algebra \@slowromancapiii@ of Hamiltonian vector fields
on \@slowromancapiii@.
The system on \@slowromancapiii@ can be written as
[TABLE]
for arbitrary t-dependent functions bi(t).
Since the associated t-dependent vector field
X\@slowromancapiii@=∑i=13bi(t)XiH takes values in the Lie algebra \@slowromancapiii@
,that is, [X1H,X2H]=−(X2H+X3H),[X1H,X3H]=−(X2H+X3H)
, then X\@slowromancapiii@ is a Lie system.
We now prove that
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,X\@slowromancapiii@)
is a Jacobi-Lie system. As a matter of fact, X1H and X2H,and X3H are Hamiltonian vector fields
relative to
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@)
with Hamiltonian
functions
f1=2(y+z+2)(−y+x)
and
f2=1+y+z, and f3=1 respectively ( i.e.,
XiH=Λ#(dfi)+fiE); subsequently,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,,X\@slowromancapiii@)
is a Jacobi-Lie system.
Using the Lie bracket induced by
Λ\@slowromancapiii@ and E\@slowromancapiii@ of Lie group \@slowromancapiii@,
we can write
{f1,f2}Λ\@slowromancapiii@,E\@slowromancapiii@=−f2−f3,{f1,f3}Λ\@slowromancapiii@,E\@slowromancapiii@=−f2−f3.
Therefore,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,f=∑i=13bi(t)fi)
for X\@slowromancapiii@
is a Jacobi-Lie Hamiltonian system,
where Λ\@slowromancapiii@ and E\@slowromancapiii@
are those appearing in (21).
Example 4.
Real three-dimensional bi-r-matrix Jacobi-Lie bialgebra
((\@slowromancapiv@,−X~1),(\@slowromancapiii@.vi,−X2−X3)) [References]:
Consider
the Lie group
\@slowromancapiv@ (with the coordinates x,y,z) related to Lie algebra
\@slowromancapiv@.
For this example, the
Jacobi structure and Reeb vector have the following forms (see table 2):
[TABLE]
Then one can show that
[TABLE]
so,
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@)
is a Jacobi manifold.
A short calculation shows that
[TABLE]
and
[TABLE]
span the Lie algebra ,\@slowromancapiv@, of Hamiltonian vector fields
on \@slowromancapiv@.
The system on \@slowromancapiv@ can be considered as
[TABLE]
for arbitrary t-dependent functions bi(t).
Since the associated t-dependent vector field
X\@slowromancapiv@=∑i=13bi(t)XiH takes values in the Lie algebra \@slowromancapiv@
,that is, [X1H,X2H]=−(X2H−X3H),[X1H,X3H]=−X3H
; then, X\@slowromancapiv@ is a Lie system.
We now exhibits that
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@,X\@slowromancapiv@)
is a Jacobi-Lie system. Actually, X1H and X2H,and X3H are Hamiltonian vector fields
relative to
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@)
with Hamiltonian
functions
f1=x(2y−z)e−x
and
f2=1, and f3=−x1 respectively ( i.e.,
XiH=Λ#(dfi)+fiE); subsequently
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@,X\@slowromancapiv@)
is a Jacobi-Lie system.
Using the Lie bracket induced by
Λ\@slowromancapiv@ and E\@slowromancapiv@ of Lie group \@slowromancapiv@, the
functions
f1,f2
and
f3 satisfy the commutation
relations
{f1,f2}Λ\@slowromancapiv@,E\@slowromancapiv@=−f2+f3,{f1,f3}Λ\@slowromancapiv@,E\@slowromancapiv@=−f3.
Therefore,
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiii@,f=∑i=13bi(t))
for X\@slowromancapiv@
is a Jacobi-Lie Hamiltonian system,
where Λ\@slowromancapiv@ and E\@slowromancapiv@
are those appearing in (23).
4 Lie symmetry for Jacobi-Lie Hamiltonian systems
We now present some examples of Jacobi-Lie Hamiltonian systems on three-dimensional real Jacobi-Lie groups
whose distribution associated with their systems is of dimension two. Then, there exists a constant of motion
for their systems. We obtain a time-independent Lie symmetry [References] for their systems to illustrate our procedure.
Let X be a
t-dependent vector field on M, the associated distribution of X is the generalised distribution ΔX on M spanned by the vector fields of gX. In other words,
[TABLE]
and the associated co-distribution of X is the generalised co-distribution
(ΔX)⊥
on M of the form
[TABLE]
where (ΔxX)⊥ is the annihilator of ΔxX.
The function
ρX:M⟶N∪{0},x↦dimΔxX
is a lower semicontinuous at x since it cannot decrease in a neighbourhood of x.
In addition, ρX(x)
is constant on the
connected components of dense and an open subset UX of M ( cf. [References, p. 19] ),
where ΔX becomes a regular involutive distribution. Also,
(ΔxX)⊥ becomes a
regular co-distribution on each connected component
since
dim(ΔxX)⊥=dimM−ρX(x).
Proposition 4.1
A function h:UX⟶R is a local t-independent constant of motion for a t-dependent vector field X if
and only if dh∈(ΔxX)⊥∣UX [References].
Definition 4.2
Let X be a Jacobi-Lie system with a Jacobi-Lie Hamiltonian structure (M,Λ,E,f).
Then,
one can define its symmetry distribution
as follows:
(SΛ,EX)x=Λ#(dhi)+hiE∈TxM,
where dhi∈(ΔxX)⊥∣U.
Now using the symmetry distribution, we study the t-independent
Lie symmetries of Jacobi-Lie Hamiltonian systems on real
low dimensional Jacobi-Lie groups.
The following proposition is the same as the proposition 1 in [References], except that Hamiltonian functions are not
necessarily a good.
Proposition 4.3
Let X be a Jacobi-Lie system possessing a Jacobi-Lie Hamiltonian structure (M,Λ,E,f).
The
smooth function h on the Jacobi manifold M
is a constant of motion for X if and only if it commutes with all
elements of
Lie({ft}t∈R,{.,.}Λ,E) relative to {.,.}Λ,E.
Proof. Let h be a t-independent constant of motion for X, i.e.
[TABLE]
Using (25) and the Jacobi identity, we get
{h,{ft,ft′}Λ,E}Λ,E={ft,{h,ft′}Λ,E}Λ,E+{{h,ft}Λ,E,ft′}Λ,E=0∀t,t′∈R.
By the inductive procedure,
h commutes with the whole successive Jacobi brackets of elements of
{ft}t∈R relative to {.,.}Λ,E and their linear combinations.
Since {ft}t∈R span Lie({ft}t∈R,{.,.}Λ,E), we obtain that h
commutes with Lie({ft}t∈R,{.,.}Λ,E) relative to {.,.}Λ,E.
Let us prove the converse. If h commutes with Lie({ft}t∈R,{.,.}Λ,E) relative to {.,.}Λ,E, it commutes with the elements {ft}t∈R
relative to {.,.}Λ,E.
By applying (25), the function h is a constant of motion of X.
Lemma 4.4
The mappinq
[TABLE]
is a homomorphism Lie algebras, i.e.
φ{f,g}Λ,E=[Xf,Xg].
Proposition 4.5
Let X be a Jacobi-Lie system admitting a Jacobi-Lie Hamiltonian structure (M,Λ,E,f).
If h is a t-independent constant of motion for X, then Xh=Λ#(dh)+hE is a t-independent Lie symmetry of
X.
Proof. In view of Lemma
4.4, we have
[Xh,Xft]=[Λ#(dh)+hE,Λ#(dft)+ftE]=φ{h,ft}Λ,E=−φ{ft,h}Λ,E=−φ(Xth)=0,∀t∈R.
Example 1.
Real three-dimensional bi-r-matrix Jacobi-Lie bialgebra
((\@slowromancapiii@,−bX~2+bX~3),(\@slowromancapiii@.iv,bX1)) [References]:
Let us Consider
the Lie group
\@slowromancapiii@ related to Lie algebra
\@slowromancapiii@ and the Jacobi structure given by (19).
A simple calculation shows that
[TABLE]
and
[TABLE]
span the Lie algebra ,A2, of Hamiltonian vector fields
on \@slowromancapiii@.
The system on \@slowromancapiii@ can be written as
[TABLE]
for arbitrary t-dependent functions bi(t).
Since the associated t-dependent vector field
X\@slowromancapiii@=∑i=12bi(t)XiH takes values in the Lie algebra A2
,that is, [X1H,X2H]=X1H
, then X\@slowromancapiii@ is a Lie system.
We now prove that
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,X\@slowromancapiii@)
is a Jacobi-Lie system. As a matter of fact, X1H and X2H are Hamiltonian vector fields
relative to
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@)
with Hamiltonian
functions
f1=x
and
f2=−bxln(x) respectively. Subsequently,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,,X\@slowromancapiii@)
is a Jacobi-Lie system.
Using the Lie bracket induced by
Λ\@slowromancapiii@ and E\@slowromancapiii@ of Lie group \@slowromancapiii@,
we can write
{f1,f2}Λ\@slowromancapiii@,E\@slowromancapiii@=f1;
therefore,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,f=∑i=12bi(t)fi)
for X\@slowromancapiii@
is a Jacobi-Lie Hamiltonian system.
It is easy check that
h=1−e−b(y−z)
is a t-independent constant of motion.
One can show that
[TABLE]
Then, the function h always Jacobi commutes with the whole Lie algebra Lie({ft}t∈R,{.,.}Λ\@slowromancapiii@,E\@slowromancapiii@), as expected.
By applying
proposition 4.5, Xh=Λ#(dh)+hE must be a Lie symmetry for this system. A short calculation shows
that
Xh=(y+z)b∂y+(y+z)b∂z.
It is easy to check that Xh commutes with X1H,X2H, and thus commutes with
every Xft, with t∈R, i.e. Xh is a Lie symmetry for X\@slowromancapiii@.
Example 2.
Real three-dimensional bi-r-matrix Jacobi-Lie bialgebra
((\@slowromancapiii@,0),(\@slowromancapiii@.v,21X2−21X3)) [References]:
Let us Consider
the Lie group
\@slowromancapiii@ related to Lie algebra
\@slowromancapiii@ and the Jacobi structure given by (21).
A simple calculation shows that
[TABLE]
and
[TABLE]
span the Lie algebra ,A2, of Hamiltonian vector fields
on \@slowromancapiii@.
The system on \@slowromancapiii@ can be written as
[TABLE]
for arbitrary t-dependent functions bi(t).
Since the associated t-dependent vector field
X\@slowromancapiii@=∑i=12bi(t)XiH takes values in the Lie algebra A2, that is, [X1H,X2H]=X1H
, then X\@slowromancapiii@ is a Lie system.
We now prove that
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,X\@slowromancapiii@)
is a Jacobi-Lie system. As a matter of fact, X1H and X2H are Hamiltonian vector fields
relative to
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@)
with Hamiltonian
functions
f1=y
and
f2=−2yln(y) respectively. Subsequently,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,,X\@slowromancapiii@)
is a Jacobi-Lie system.
Using the Lie bracket induced by
Λ\@slowromancapiii@ and E\@slowromancapiii@ of Lie group \@slowromancapiii@,
we can write
{f1,f2}Λ\@slowromancapiii@,E\@slowromancapiii@=f1;
therefore,
(\@slowromancapiii@,Λ\@slowromancapiii@,E\@slowromancapiii@,f=∑i=12bi(t)fi)
for X\@slowromancapiii@
is a Jacobi-Lie Hamiltonian system.
It is easy to show that
h=ln(e2x−1)−e−2xln(e2x−1)+y+z
is a t-independent constant of motion.
One can check that
[TABLE]
Then, the function h always Jacobi commutes with the whole Lie algebra Lie({ft}t∈R,{.,.}Λ\@slowromancapiii@,E\@slowromancapiii@), as expected.
By applying
proposition 4.5,
Xh=Λ#(dh)+hE must be a Lie symmetry for this system. A short calculation shows
that
Xh=21(1−e2x)∂x+e2x−1(e−2x+e2x−2)ln(e2x−1)−2e2x+e4x+1∂z.
It is easy to check that Xh commutes with X1H,X2H, and hence with
every Xft, with t∈R, i.e. Xh is a Lie symmetry for X\@slowromancapiii@.
Example 3.
Real three-dimensional bi-r-matrix Jacobi-Lie bialgebra
((\@slowromancapiv@,−X~1),(\@slowromancapiii@.vi,−X2−X3))[References]:
Let us Consider
the Lie group
\@slowromancapiv@ related to Lie algebra
\@slowromancapiv@ and the Jacobi structure given by (23).
A simple calculation shows that
[TABLE]
and
[TABLE]
span the Lie algebra ,A2, of Hamiltonian vector fields
on \@slowromancapiv@.
The system on \@slowromancapiv@ can be written as
[TABLE]
for arbitrary t-dependent functions bi(t).
Since the associated t-dependent vector field
X\@slowromancapiv@=∑i=12bi(t)XiH takes values in the Lie algebra A2
,that is, [X1H,X2H]=X1H
, then X\@slowromancapiv@ is a Lie system.
We now prove that
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@,X\@slowromancapiv@)
is a Jacobi-Lie system. As a matter of fact, X1H and X2H are Hamiltonian vector fields
relative to
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@)
with Hamiltonian
functions
f1=e−e−xy
and
f2=1 respectively. Subsequently,
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@,,X\@slowromancapiv@)
is a Jacobi-Lie system.
Using the Lie bracket induced by
Λ\@slowromancapiv@ and E\@slowromancapiv@ of Lie group \@slowromancapiv@,
we can write
{f1,f2}Λ\@slowromancapiv@,E\@slowromancapiv@=f1;
therefore,
(\@slowromancapiv@,Λ\@slowromancapiv@,E\@slowromancapiv@,f=∑i=12bi(t)fi)
for X\@slowromancapiv@
is a Jacobi-Lie Hamiltonian system.
It is easy to show that
h=ex+(x−1)y+z−1
is a t-independent constant of motion.
One can check that
[TABLE]
Then, the function h always Jacobi commutes with the whole Lie algebra Lie({ft}t∈R,{.,.}Λ\@slowromancapiv@,E\@slowromancapiv@), as expected.
By applying
proposition 4.5,
Xh=Λ#(dh)+hE must be a Lie symmetry for this system. A short calculation shows that
Xh=xex∂x+xyex∂y−x(xyex+e2x)∂z.
It is easy to check that Xh commutes with X1H,X2H, and subsequently with
every Xft, with t∈R, i.e. Xh is a Lie symmetry for X\@slowromancapiv@.
Example 4.
Real three-dimensional bi-r-matrix Jacobi-Lie bialgebra
((\@slowromancapvi@0,X~3),(\@slowromancapiii@.ix,−X1))[References]:
Let us Consider
the Lie group
\@slowromancapvi@0 related to Lie algebra
\@slowromancapvi@0 and the Jacobi structure given by
[TABLE]
Then one can show that
[TABLE]
so,
(\@slowromancapvi@0,Λ\@slowromancapvi@0,E\@slowromancapvi@0)
is a Jacobi manifold.
A simple calculation shows that
X1H=∂x
and
X2H=x∂x+(1+y−e−z)∂y+e−zsinh(z)∂z
span the Lie algebra ,A2, of Hamiltonian vector fields
on \@slowromancapvi@0.
The system on \@slowromancapvi@0 can be written as
[TABLE]
for arbitrary t-dependent functions bi(t).
Since the associated t-dependent vector field
X\@slowromancapvi@0=∑i=12bi(t)XiH takes values in the Lie algebra A2
,that is, [X1H,X2H]=X1H
, then X\@slowromancapvi@0 is a Lie system.
We now prove that
(\@slowromancapvi@0,Λ\@slowromancapvi@0,E\@slowromancapvi@0,X\@slowromancapvi@0)
is a Jacobi-Lie system. As a matter of fact, X1H and X2H are Hamiltonian vector fields
relative to
(\@slowromancapvi@0,Λ\@slowromancapvi@0,E\@slowromancapvi@0)
with Hamiltonian
functions
f1=1
and
f2=x respectively. Subsequently,
(\@slowromancapvi@0,Λ\@slowromancapvi@0,E\@slowromancapvi@0,,X\@slowromancapvi@0)
is a Jacobi-Lie system.
Using the Lie bracket induced by
Λ\@slowromancapvi@0 and E\@slowromancapvi@0 of Lie group \@slowromancapvi@0,
we can write
{f1,f2}Λ\@slowromancapvi@0,E\@slowromancapvi@0=f1;
therefore,
(\@slowromancapvi@0,Λ\@slowromancapvi@0,E\@slowromancapvi@0,f=∑i=12bi(t)fi)
for X\@slowromancapvi@0
is a Jacobi-Lie Hamiltonian system.
It is easy to show that
h=e2z−1
is a t-independent constant of motion.
One can check that
[TABLE]
Then, the function h always Jacobi commutes with the whole Lie algebra Lie({ft}t∈R,{.,.}Λ\@slowromancapvi@0,E\@slowromancapvi@0), as expected.
By applying
proposition 4.5,
Xh=Λ#(dh)+hE must be a Lie symmetry for this system. A short calculation shows that
Xh=(1−e2z)∂y.
It is easy to check that Xh commutes with X1H,X2H, and subsequently with
every Xft, with t∈R, i.e. Xh is a Lie symmetry for X\@slowromancapvi@0.
5 Concluding remarks
Using the realizations [References] of the complete list of Jacobi structures on real two and three- dimensional Jacobi-Lie
groups [References], we attained Hamiltonian vector fields and we achieved Jacobi-Lie Hamiltonian systems on real
low dimensional Jacobi-Lie groups.
Then we presented the Lie symmetries of these Jacobi-Lie Hamiltonian systems.
Table 1: vector field E and 2-vector Λ related to real two-dimensional bi-r-matrix Jacobi-Lie bialgebras.
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((A1,X~1),(A1,X2))
E=−∂y
Λ=(1−e−x)∂x∧∂y
((A2,bX~2),(A2.i,−bX1))
E=b∂x
Λ=(1−e−(b+1)y)∂x∧∂y
((A1,0),(A2,−X2))
E=∂y
Λ=0
Table 2: vector field E and 2-vector Λ related to real three-dimensional bi-r-matrix Jacobi-Lie bialgebras.
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapi@,−X~2+X~3),(\@slowromancapiii@,−2X1))
E=2∂x
Λ=(−1+ey−z)∂x∧∂y+(1−ey−z)∂x∧∂z
((\@slowromancapii@,0),(\@slowromancapi@,X1))
E=−∂x
Λ=−y∂x∧∂y−z∂x∧∂z
((\@slowromancapii@,0),(\@slowromancapv@,bX1))
E=−b∂x
Λ=−(1+b)y∂x∧∂y−(1+b)z∂x∧∂z
((\@slowromancapiii@,bX~1),(\@slowromancapiii@.i,−X2+X3))
E=∂y−∂z
\begin{array}[]{l}\Lambda=-\frac{1}{b}(1-e^{-bx})\partial_{x}\wedge\partial_{y}+\frac{1}{b}(1-e^{-bx})\partial_{x}\wedge\partial_{z}\\
\qquad-\frac{2}{b}(y+z)e^{-bx}\partial_{y}\wedge\partial_{z}\end{array}
Table 2: (Continued.)
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapiii@,−bX~2+bX~3),(\@slowromancapiii@.iv,bX1))
E=−b∂x
\begin{array}[]{l}\Lambda=\frac{1}{2}(1-e^{b(y-z)})\partial_{x}\wedge\partial_{y}-\frac{1}{2}(1-e^{b(y-z)})\partial_{x}\wedge\partial_{z}\\
\qquad+(y+z)e^{b(y-z)}\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapiii@,0),(\@slowromancapiii@.v,21X2−21X3))
E=−21∂y+21∂z
\begin{array}[]{l}\Lambda=\dfrac{e^{2x}-1}{4}\partial_{x}\wedge\partial_{y}+\dfrac{e^{2x}-1}{4}\partial_{x}\wedge\partial_{z}\\
\qquad-\frac{1}{2}(y+z+1-e^{2x})\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapiii@,0),(\@slowromancapiv@.iv,X2−X3))
E=−∂y+∂z
Λ=21(e2x−1)∂y∧∂z
((\@slowromancapiii@,−2X~1),(\@slowromancapv@.i,−X2−X3))
E=e2x∂y+e2x∂z
Λ=0
((\@slowromancapiii@,0),(\@slowromancapvi@0.iv,X2−X3))
E=−∂y+∂z
Λ=−2(y+z)∂y∧∂z
((\@slowromancapiii@,0),(\@slowromancapvi@a.vii,−X2+X3))
E=∂y−∂z
Λ=a−1−2(y+z)∂y∧∂z
((\@slowromancapiii@,0),(\@slowromancapvi@a.viii,−X2+X3))
E=∂y−∂z
Λ=a+12(y+z)∂y∧∂z
((\@slowromancapiv@,−X~1),(\@slowromancapiii@.vi,−X2−X3))
E=ex∂y+ex(1−x)∂z
Λ=−xex∂x∧∂z+ex(z−y−1+ex)∂y∧∂z
Table 2: (Continued.)
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapiv@,−X~1),(\@slowromancapiv@.i,−bX3))
E=bex∂z
Λ=ex(ex−1)∂y∧∂z
((\@slowromancapiv@,−X~1),(\@slowromancapiv@.ii,−bX3))
E=bex∂z
Λ=−ex(ex−1)∂y∧∂z
((\@slowromancapiv@,−X~1),(\@slowromancapvi@0.i,−X3))
E=ex∂z
Λ=−2yex∂y∧∂z
((\@slowromancapiv@,−X~1),(\@slowromancapvi@a.i,−X3))
E=ex∂z
Λ=a−12yex∂y∧∂z
((\@slowromancapiv@,−X~1),(\@slowromancapvi@a.ii,−X3))
E=ex∂z
Λ=−a+12yex∂y∧∂z
((\@slowromancapv@,−2X~1),(\@slowromancapv@.i,−2X2−2X3))
E=2ex∂y+2ex∂z
\begin{array}[]{l}\Lambda=e^{x}(1-e^{x})\partial_{x}\wedge\partial_{y}+e^{x}(1-e^{x})\partial_{x}\wedge\partial_{z}\\
\qquad+e^{2x}(z-y)\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapv@,−a−12aX~1),(\@slowromancapvi@a.i,−a−12aX3))
E=a−12aex∂z
Λ=(ex−ea−12ax)∂x∧∂z−yea−12ax∂y∧∂z
((\@slowromancapv@,−a+12aX~1),(\@slowromancapvi@a.ii,−a+12aX3))
E=a+12aex∂z
Λ=(ex−ea+12ax)∂x∧∂z−yea+12ax∂y∧∂z
Table 2: (Continued.)
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapvi@0,X~3),(\@slowromancapiii@.vii,−X1−X2))
E=∂x+∂y
\begin{array}[]{l}\Lambda=(y-x)\partial_{x}\wedge\partial_{y}+(1-e^{-2z})\partial_{x}\wedge\partial_{z}\\
\qquad+(1-e^{-2z})\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@0,X~3),(\@slowromancapiii@.ix,−X1))
E=∂x
\begin{array}[]{l}\Lambda=(1+y-e^{-z})\partial_{x}\wedge\partial_{y}+e^{-z}\sinh(z)\partial_{x}\wedge\partial_{z}\\
\qquad+(1-e^{-z}\cosh(z))\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@0,X~3),(\@slowromancapvi@0.ii,−X1+X2))
E=∂x−∂y
Λ=2(x+y)∂x∧∂y
((\@slowromancapvi@0,−2X~3),(\@slowromancapvi@0.ii,2X1−2X2))
E=−2∂x+2∂y
\begin{array}[]{l}\Lambda=-(x+y)\partial_{x}\wedge\partial_{y}+(1-e^{3z})\partial_{x}\wedge\partial_{z}\\
\qquad-(1-e^{3z})\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@0,X~3),(\@slowromancapvi@a.iii,−X1+X2))
E=∂x−∂y
Λ=−a−12(x+y)∂x∧∂y
((\@slowromancapvi@0,X~3),(\@slowromancapvi@a.iv,−X1+X2))
E=∂x−∂y
Λ=a+12(x+y)∂x∧∂y
((\@slowromancapvi@0,a−12X~3),(\@slowromancapvi@a.iii,−a−12(X1−X2)))
E=a−12∂x−a−12∂y
\begin{array}[]{l}\Lambda=-(x+y)\partial_{x}\wedge\partial_{y}+(1-e^{\frac{a-3}{a-1}z})\partial_{x}\wedge\partial_{z}\\
\qquad-(1-e^{\frac{a-3}{a-1}z})\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@0,−a+12X~3),(\@slowromancapvi@a.iv,a+12(X1−X2)))
E=−a+12∂x+a+12∂y
\begin{array}[]{l}\Lambda=-(x+y)\partial_{x}\wedge\partial_{y}+(1-e^{\frac{a+3}{a+1}z})\partial_{x}\wedge\partial_{z}\\
\qquad-(1-e^{\frac{a+3}{a+1}z})\partial_{y}\wedge\partial_{z}\end{array}
Table 2: (Continued.)
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapvi@a,−(a−1)X~1),(\@slowromancapiii@.ii,−a+1a−1(X2+X3)))
E=a+1a−1e(a+1)x∂y+a+1a−1e(a+1)x∂z
\begin{array}[]{l}\Lambda=\frac{1}{a+1}(e^{(a+1)x}-e^{(a-1)x})\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a+1}(e^{(a+1)x}-e^{(a-1)x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a+1}e^{(a-1)x}(1-a)(y-z)\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@a,−(a+1)X~1),(\@slowromancapiii@.v,a−11(X2−aX3)))
\begin{array}[]{l}E=\frac{1}{a-1}e^{ax}(-\cosh(x)+a\sinh(x))\partial_{y}\\
\qquad+\frac{1}{a-1}e^{ax}(-\sinh(x)+a\cosh(x))\partial_{z}\end{array}
\begin{array}[]{l}\Lambda=\frac{1}{a-1}e^{ax}\sinh(x)\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a-1}(e^{ax}\cosh(x)-e^{(a+1)x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a-1}(e^{2ax}-e^{(a+1)x}(1+ay+z))\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@a,−(a−1)X~1),(\@slowromancapiii@.v,a+11(X2−aX3)))
\begin{array}[]{l}E=\frac{1}{a+1}e^{ax}(-\cosh(x)+a\sinh(x))\partial_{y}\\
\qquad+\frac{1}{a+1}e^{ax}(-\sinh(x)+a\cosh(x))\partial_{z}\end{array}
\begin{array}[]{l}\Lambda=\frac{1}{a+1}e^{ax}\sinh(x)\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a+1}(e^{ax}\cosh(x)-e^{(a-1)x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a+1}(e^{2ax}-e^{(a-1)x}(1+ay+z))\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@a,−(a+1)X~1),(\@slowromancapiii@.x,−a−1a+1(X2−X3)))
E=a−1a+1e(a−1)x∂y−a−1a+1e(a−1)x∂z
\begin{array}[]{l}\Lambda=\frac{1}{a-1}(e^{(a-1)x}-e^{(a+1)x})\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a-1}(e^{(a+1)x}-e^{(a-1)x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a-1}e^{(a+1)x}(1+a)(y+z)\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@a,−(a+1)X~1),(\@slowromancapvi@b.v,−X2−X3))
E=e(a+1)x∂y+e(a+1)x∂z
Λ=(b−1)2e(a+1)x(y−z)∂y∧∂z
((\@slowromancapvi@a,−(a+1)X~1),(\@slowromancapvi@b.vi,−X2+X3))
E=e(a+1)x∂y+e(a+1)x∂z
Λ=−(b+1)2e(a+1)x(y−z)∂y∧∂z
Table 2: (Continued.)
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapvi@a,−(a−1)X~1),(\@slowromancapvi@b.vii,−X2+X3))
E=e(a−1)x∂y−e(a−1)x∂z
Λ=−(b−1)2e(a−1)x(y+z)∂y∧∂z
((\@slowromancapvi@a,−(a−1)X~1),(\@slowromancapvi@b.viii,−X2+X3))
E=e(a−1)x∂y−e(a−1)x∂z
Λ=(b+1)2e(a−1)x(y+z)∂y∧∂z
((\@slowromancapvi@a,−b−12(ab+1)X~1),(\@slowromancapvi@b.v,−(a+1)(b−1)2(ab+1)(X2+X3)))
\begin{array}[]{l}E=\frac{2(ab+1)}{(a+1)(b-1)}e^{(a+1)x}\partial_{y}\\
\qquad+\frac{2(ab+1)}{(a+1)(b-1)}e^{(a+1)x}\partial_{z}\end{array}
\begin{array}[]{l}\Lambda=\frac{1}{a+1}(e^{(a+1)x}-e^{\frac{2(ab+1)}{b-1}x})\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a+1}(e^{(a+1)x}-e^{\frac{2(ab+1)}{b-1}x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a+1}e^{\frac{2(ab+1)}{b-1}x}(1-a)(y-z)\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@a,−b+12(ab−1)X~1),(\@slowromancapvi@b.vi,−(a+1)(b+1)2(ab−1)(X2+X3)))
\begin{array}[]{l}E=\frac{2(ab-1)}{(a+1)(b+1)}e^{(a+1)x}\partial_{y}\\
\qquad+\frac{2(ab-1)}{(a+1)(b+1)}e^{(a+1)x}\partial_{z}\end{array}
\begin{array}[]{l}\Lambda=\frac{1}{a+1}(e^{(a+1)x}-e^{\frac{2(ab-1)}{b+1}x})\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a+1}(e^{(a+1)x}-e^{\frac{2(ab-1)}{b+1}x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a+1}e^{\frac{2(ab-1)}{b+1}x}(1-a)(y-z)\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@a,−b−12(ab−1)X~1),(\@slowromancapvi@b.vii,−(a1)(b−1)2(ab−1)(X2−X3)))
\begin{array}[]{l}E=\frac{2(ab-1)}{(a-1)(b-1)}e^{(a-1)x}\partial_{y}\\
\qquad-\frac{2(ab-1)}{(a-1)(b-1)}e^{(a-1)x}\partial_{z}\end{array}
\begin{array}[]{l}\Lambda=\frac{1}{a-1}(e^{(a-1)x}-e^{\frac{2(ab-1)}{b-1}x})\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a-1}(-e^{(a-1)x}+e^{\frac{2(ab-1)}{b-1}x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a-1}e^{\frac{2(ab-1)}{b-1}x}(1+a)(y+z)\partial_{y}\wedge\partial_{z}\end{array}
((\@slowromancapvi@a,−b+12(ab+1)X~1),(\@slowromancapvi@b.viii,−(a−1)(b+1)2(ab+1)(X2−X3)))
\begin{array}[]{l}E=\frac{2(ab+1)}{(a-1)(b+1)}e^{(a-1)x}\partial_{y}\\
\qquad-\frac{2(ab+1)}{(a-1)(b+1)}e^{(a-1)x}\partial_{z}\end{array}
\begin{array}[]{l}\Lambda=\frac{1}{a-1}(e^{(a-1)x}-e^{\frac{2(ab+1)}{b+1}x})\partial_{x}\wedge\partial_{y}\\
\qquad+\frac{1}{a-1}(-e^{(a-1)x}+e^{\frac{2(ab+1)}{b+1}x})\partial_{x}\wedge\partial_{z}\\
\qquad+\frac{1}{a-1}e^{\frac{2(ab+1)}{b+1}x}(1+a)(y+z)\partial_{y}\wedge\partial_{z}\end{array}
Table 3: vector field E and 2-vector Λ related to real three dimensional coboundary Jacobi-Lie bialgebras.
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapi@,0),(\@slowromancapv@,−X1))
E=∂x
Λ=0
((\@slowromancapii@,−X~2+X~3),(\@slowromancapiii@,−2X1))
E=2∂x
Λ=(−1+ey−z)∂x∧∂y+(1−ey−z)∂x∧∂z
((\@slowromancapiii@,−X~2+X~3),(\@slowromancapiii@.iii,X2+X3))
E=−e2x∂y−e2x∂z
Λ=(−e2x+ey−z)∂y∧∂z
((\@slowromancapiii@,0),(\@slowromancapiii@.x,−X2+X3))
E=∂y−∂z
Λ=(y+z)∂y∧∂z
((\@slowromancapiv@,−X~1),(\@slowromancapiii@.v,−X3))
E=ex∂z
Λ=−(y+1−ex)ex∂y∧∂z
((\@slowromancapiv@,−2X~1),(\@slowromancapv@.ii,−2X3))
E=2ex∂z
Λ=(ex−e2x)∂x∧∂z−ye2x∂y∧∂z
((\@slowromancapiv@,−a−12aX~1),(\@slowromancapvi@a.i,−a−12aX3))
E=a−12aex∂z
Λ=(ex−ea−12ax)∂x∧∂z−yea−12ax∂y∧∂z
((\@slowromancapiv@,−a+12aX~1),(\@slowromancapvi@a.ii,−a+12aX3))
E=a+12aex∂z
Λ=(ex−ea+12ax)∂x∧∂z−yea+12ax∂y∧∂z
Table 3: (Continued.)
((g,ϕ0),(g∗,X0))
vector field E and 2-vector Λ
((\@slowromancapv@,−X~1),(\@slowromancapvi@0.i,−X3))
E=ex∂z
Λ=−2yex∂y∧∂z
((\@slowromancapv@,−X~1),(\@slowromancapvi@a.i,−X3))
E=ex∂z
Λ=a−12yex∂y∧∂z
((\@slowromancapv@,−X~1),(\@slowromancapvi@a.ii,−X3))
E=ex∂z
Λ=−a+12yex∂y∧∂z
((\@slowromancapvi@0,X~3),(\@slowromancapiii@.viii,−X1+X2))
E=∂x−∂y
Λ=(x+y)∂x∧∂y
((\@slowromancapvi@a,−(a+1)X~1),(\@slowromancapiii@.ii,−X2−X3))
E=e(a+1)x∂y+e(a+1)x∂z
Λ=−(y−z)e(a+1)x∂y∧∂z
((\@slowromancapvi@a,−(a−1)X~1),(\@slowromancapiii@.x,−X2+X3))
E=e(a−1)x∂y+e(a−1)x∂z
Λ=(y+z)e(a−1)x∂y∧∂z