The Canonical Reduction Method for Symplectic Structures and Its Applications
The canonical reduction method is analized in detail and applied to Maxwell and Yang– Mills equations considered as Hamiltonian systems on some fiber bundles with symplectic and connection structures. The minimum interaction principle is proved to have geometric origin within the reduction method...
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Цитувати: | The Canonical Reduction Method for Symplectic Structures and Its Applications / A.K. Prykarpatsky, V.H. Samoilenko // Нелінійні коливання. — 2001. — Т. 4, № 3. — С. 354-367. — Бібліогр.: 10 назв. — англ. |
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irk-123456789-1746942021-01-28T01:26:23Z The Canonical Reduction Method for Symplectic Structures and Its Applications Prykarpatsky, A.K. Samoilenko, V.H. The canonical reduction method is analized in detail and applied to Maxwell and Yang– Mills equations considered as Hamiltonian systems on some fiber bundles with symplectic and connection structures. The minimum interaction principle is proved to have geometric origin within the reduction method devised. 2001 Article The Canonical Reduction Method for Symplectic Structures and Its Applications / A.K. Prykarpatsky, V.H. Samoilenko // Нелінійні коливання. — 2001. — Т. 4, № 3. — С. 354-367. — Бібліогр.: 10 назв. — англ. 1562-3076 http://dspace.nbuv.gov.ua/handle/123456789/174694 en Нелінійні коливання Інститут математики НАН України |
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The canonical reduction method is analized in detail and applied to Maxwell and Yang–
Mills equations considered as Hamiltonian systems on some fiber bundles with symplectic and
connection structures. The minimum interaction principle is proved to have geometric origin
within the reduction method devised. |
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Article |
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Prykarpatsky, A.K. Samoilenko, V.H. |
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Prykarpatsky, A.K. Samoilenko, V.H. The Canonical Reduction Method for Symplectic Structures and Its Applications Нелінійні коливання |
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Prykarpatsky, A.K. Samoilenko, V.H. |
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Prykarpatsky, A.K. |
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The Canonical Reduction Method for Symplectic Structures and Its Applications |
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The Canonical Reduction Method for Symplectic Structures and Its Applications |
title_full |
The Canonical Reduction Method for Symplectic Structures and Its Applications |
title_fullStr |
The Canonical Reduction Method for Symplectic Structures and Its Applications |
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The Canonical Reduction Method for Symplectic Structures and Its Applications |
title_sort |
canonical reduction method for symplectic structures and its applications |
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Інститут математики НАН України |
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2001 |
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http://dspace.nbuv.gov.ua/handle/123456789/174694 |
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The Canonical Reduction Method for Symplectic Structures and Its Applications / A.K. Prykarpatsky, V.H. Samoilenko // Нелінійні коливання. — 2001. — Т. 4, № 3. — С. 354-367. — Бібліогр.: 10 назв. — англ. |
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Нелінійні коливання |
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AT prykarpatskyak thecanonicalreductionmethodforsymplecticstructuresanditsapplications AT samoilenkovh thecanonicalreductionmethodforsymplecticstructuresanditsapplications AT prykarpatskyak canonicalreductionmethodforsymplecticstructuresanditsapplications AT samoilenkovh canonicalreductionmethodforsymplecticstructuresanditsapplications |
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2025-07-15T11:44:42Z |
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Nonlinear Oscillations, Vol. 4, No. 3, 2001
THE CANONICAL REDUCTION METHOD FOR SYMPLECTIC
STRUCTURES AND ITS APPLICATIONS
A. K. Prykarpats’ky
Institute of Applied Problems of Mechanics and Mathematics, NAS of Ukraine,
Naukova St., 3b, L’viv, Ukraine; and AGH, Krakow, 30059, Poland
e-mail: prykanat@cybergal.com
prykanat@start.com.au
V. Hr. Samoylenko
Kyiv National Taras Shevchenko University
Volodymyr’ska St., 64, Kyiv, 01033, Ukraine
e-mail: vsam@imath.kiev.ua
vsam@mail.univ.kiev.ua
The canonical reduction method is analized in detail and applied to Maxwell and Yang–
Mills equations considered as Hamiltonian systems on some fiber bundles with symplectic and
connection structures. The minimum interaction principle is proved to have geometric origin
within the reduction method devised.
AMS Subject Classification: 35 Q58, 58 F07
1. Preliminaries
We begin by reviewing the backgrounds of the reduction theory subject to Hamiltonian
systems with symmetry on principle fiber bundles. The material is partly available in [1 – 3], so
here we only sketch, but in the notation suitable for us, the necessary definitions and statements.
Let G denote a given Lie group with the unity element e ∈ G and the corresponding Lie
algebra G ' Te(G). Consider a principal fiber bundle p : (M,ϕ) → N with the structure group
G and a base manifold N on which the Lie group G acts by means of a mapping ϕ : M ×G →
M. Namely, for each g ∈ G there is a group diffeomorphism ϕg : M → M, generating for any
fixed u ∈ M the following induced mapping: û : G → M , where û(g) = ϕg(u).
On the principal fiber bundle p : (M,ϕ) → N there is assigned a connection Γ(A) by
means of such a morphism A :(T (M), ϕg∗) → (G, Adg−1) that for each u ∈ M , the mapping
A(u) : Tu(M) → G is a left inverse of the mapping û∗(e) : G → Tu(M), that is
A(u)û∗(e) = 1. (1)
As usual, denote by ϕ∗g : T ∗(M) → T ∗(M) the corresponding lift of the mapping ϕg :
M → M at any g ∈ G. If α(1) ∈ Λ1(M) is the canonical G-invariant 1-form on M, the
canonical symplectic structure ω(2) ∈ Λ2(T ∗(M)), given by formula
ω(2) := dpr∗α(1),
354 c© A. K. Prykarpats’ky, V. Hr. Samoylenko, 2001
THE CANONICAL REDUCTION METHOD FOR SYMPLECTIC STRUCTURES . . . 355
generates the corresponding momentum mapping l : T ∗(M) → G∗, where
l(α(1))(u) = û∗(e)α
(1)(u) (2)
for all u ∈ M.
Remark here that the principal fiber bundle structure p : (M,ϕ) → N means, in part, the
exactness of the following sequences of mappings:
0 → G û∗(e)→ Tu(M)
p∗(u)→ Tp(u)(N) = 0,
that is,
p∗(u)û∗(e) = 0 = û∗(e)p∗(u) (3)
for all u ∈ M.
Combining (3) with (1) and (2), one obtains the following embedding for the canonical
1-form α(1) ∈ Λ1(M) at u ∈ M :
[1−A∗(u)û∗(e)]α(1)(u) ∈ range p∗(u). (4)
The expression (4) means that
û∗(e)[1−A∗(u)û∗(e)]α(1)(u) = 0
for all u ∈ M.
Taking now into account that the mapping p∗(u) : T ∗(N) → T ∗(M) for each u ∈ M is
injective, we conclude that it has a unique inverse mapping (p∗(u))−1 on its image p∗(u)T ∗p(u)(N)
⊂ T ∗u (M). Thereby, for each u ∈ M one can define a morphism pA : (T ∗(M), ϕ∗g) → T ∗(N) by
pA(u) : α(1)(u) → (p∗(u))−1[1−A∗(u)û∗(e)]α(1)(u). (5)
Based on definition (5), one can easily check that the diagram
T ∗(M)
pA→ T ∗(N)
prM↓ ↓prN
M
p→ N
is commutative.
Let an element ξ ∈ G∗ be G-invariant, that is, Ad∗g−1ξ = ξ for all g ∈ G. Denote also by
pξA the restriction of mapping (5) to the subset l−1(ξ) ∈ T ∗(M), that is, pξA : l−1(ξ) → T ∗(N),
where, for all u ∈ M , we have
pξA(u) : l−1(ξ) → (p∗(u))−1 [1−A∗(u)û∗(e)]l−1(ξ).
Now one can characterize the structure of the reduced phase space l−1(ξ)/G by means of
the following lemma.
356 A.K. PRYKARPATS’KY, V.HR. SAMOYLENKO
Lemma 1. The mapping pξA(u) : l−1(ξ) → T ∗(N) is a principal fiber G-bundle with the
reduced space l−1(ξ)/G being diffeomorphic to T ∗(N).
Denote by 〈·, ·〉G the standard Ad-invariant nondegenerate scalar product on G∗ ×G. Based
on Lemma 1, one deduces the following characterization theorem.
Theorem 1. Given a principal fiber G-bundle with a connection Γ(A) and a G-invariant
element ξ ∈ G∗, then every such a connection Γ(A) defines a symplectomorphism νξ : l−1(ξ)/G →
T ∗(N) between the reduced phase space l−1(ξ)/G and the cotangent bundle T ∗(N), where l :
T ∗(M) → G∗ is the naturally associated momentum mapping for the group G-action
on M.
Moreover, the following equality:
(pξA)(d pr∗β(1) + pr∗Ω
(2)
ξ ) = d pr∗α(1)
∣∣∣
l−1(ξ)
(6)
holds for the canonical 1-forms β(1) ∈ Λ1(N) and α(1) ∈ Λ1(M), where Ω
(2)
ξ := 〈Ω(2), ξ〉G is
the ξ-component of the corresponding curvature form Ω(2) ∈ Λ(2)(N)⊗ G.
Proof. On l−1(ξ) ⊂ M due to (5), we have
p∗(u)pξA(α(1)(u)) = p∗(u)β(1)(prN (u)) = α(1)(u)−A∗(u)û∗(e)α(1)(u)
for any β(1) ∈ T ∗(N) and all u ∈ Mξ := pM l
−1(ξ) ⊂ M. Thus we easily get that
α(1)(u) = (pξA)−1β(1)(pN (u)) = p∗(u)β(1) (prN (u)) + 〈A(u), ξ〉
for all u ∈ Mξ. Recall now that in virtue of (6), one gets on Mξ
p prMξ
= prN p
ξ
A, pr∗Mξ
p∗ = (pξA)∗ pr∗N .
Therefore we can write now that
pr∗Mξ
α(1)(u) = pr∗Mξ
β(1)(pN (u)) + pr∗Mξ
〈A(u), ξ〉
= (pξA)∗(pr∗Nβ
(1))(u) + pr∗Mξ
〈A(u), ξ〉.
Whence taking the external differential, one arrives at the following equality:
d pr∗Mξ
α(1)(u) = (pξA)∗d(pr∗Nβ
(1))(u) + pr∗Mξ
〈dA(u), ξ〉
= (pξA)∗d(pr∗Nβ
(1))(u) + pr∗Mξ
〈Ω(p(u)), ξ〉
= (pξA)∗d(pr∗Nβ
(1))(u) + pr∗Mξ
p∗〈Ω, ξ〉(u)
= (pξA)∗d(pr∗Nβ
(1))(u) + (pξA)∗pr∗N 〈Ω, ξ〉(u)
= (pξA)∗[d(pr∗Nβ
(1))(u) + pr∗N 〈Ω, ξ〉(u)].
THE CANONICAL REDUCTION METHOD FOR SYMPLECTIC STRUCTURES . . . 357
When deriving the above expression we made use of the following property satisfied by the
curvature 2-form Ω ∈ Λ2(M)⊗ G :
〈dA(u), ξ〉 = 〈dA(u) +A(u) ∧ A(u), ξ〉 − 〈A(u) ∧ A(u), ξ〉
= 〈Ω(pN (u)), ξ〉 = 〈p∗NΩ, ξ〉(u) (7)
at any u ∈ Mξ, since for any A,B ∈ G, 〈[A,B], ξ〉 = 〈B, (Ad A)∗ξ〉 = 0 in virtue of the
invariance condition AdGξ = ξ. Thereby the proof is finished.
Remark . Since the canonical 2-form dpr∗α(1) ∈ Λ(2)(T ∗(M)) is G-invariant on T ∗(M),
due to the construction, it is evident that its restriction to the G-invariant submanifold l−1(ξ) ⊂
T ∗(M) will be effectively defined only on the reduced space l−1(ξ)/G, which ensures the vali-
dity of the equality sign in (6).
As a consequence of Theorem 1 one can formulate the following results useful enough for
applications.
Theorem 2. Let an element ξ ∈ G∗ have the isotropy group Gξ acting on the subset
l−1(ξ) ⊂ T ∗(M) freely and properly, so that the reduced phase space (l−1(ξ)/Gξ , σ
(2)
ξ ) is
symplectic, where by the definition,
σ
(2)
ξ := dpr∗α(1)
∣∣∣
l−1(ξ)
.
If the principal fiber bundle p : (M,ϕ) → N has the structure group coinciding with Gξ, then
the reduced symplectic space (l−1(ξ)/Gξ, σ
(2)
ξ ) is symplectomorphic to the cotangent symplectic
space (T ∗(N), ω
(2)
ξ ), where
ω
(2)
ξ = d pr∗β(1) + pr∗Ω
(2)
ξ ,
and the corresponding symplectomorphism is given by a relation similar to (6).
Theorem 3. In order that two symplectic spaces (l−1(ξ)/G, σ
(2)
ξ ) and (T ∗(N), dpr∗β(1))
were symplectomorphic, it is necessary and sufficient that the element ξ ∈ ker h, where for a
G-invariant element ξ ∈ G∗, the mapping h : ξ → [Ω
(2)
ξ ] ∈ H2(N ;Z), with H2(N ;Z) being
the cohomology class of 2-forms on the manifold N.
In case where a Lie group G is given the tangent space T (G) is also Lie group isomorphic
to the semidirect product G̃ := G ⊗Ad G of the Lie group G and its Lie algebra G under the
adjoint Ad-action of G on G.
The Lie algebra G̃ of G̃ is, correspondingly, the semidirect product of G with itself, regarded
as a trivial Abelian Lie algebra, under the adjoint ad-action and thus has the bracket defined by
[(a1,m1), (a2,m2)] := ([a1, a2], [a1,m2] + [a2,m1])
for all (aj ,mj) ∈ G ⊗ad G, j = 1, 2.
358 A.K. PRYKARPATS’KY, V.HR. SAMOYLENKO
Take now any element ξ ∈ G∗ and compute its isotropy group Gξ under the coadjoint
action Ad∗ of G on G∗, and denote by Gξ its Lie algebra.
The cotangent bundle T ∗(G) is obviously diffeomorphic to M := G× G∗ on which the Lie
group Gξ acts freely and properly (due to the construction) by left translation on the first factor
and Ad∗-action on the second one.
The corresponding momentum mapping l : G× G∗ → G∗ξ is obtained as
l(h, α) = Ad∗h−1α
∣∣
G∗ξ
with no critical points.
Let now η ∈ G∗ and η(ξ) := η|G∗ξ . Therefore, the reduced space (l−1(η(ξ))/G
η(ξ)
ξ , σ
(2)
ξ ) has
to be symplectic due to the well known Marsden – Weinstein reduction theorem [4, 5], where
G
η(ξ)
ξ is the isotropy subgroup of the Gξ-coadjoint action on η(ξ) ∈ G∗ξ and the symplectic
form σ
(2)
ξ := dpr∗α(1)
∣∣
l−1(η(ξ))
is naturally induced from the canonical symplectic structure on
T ∗(G).
Define now for η(ξ) ∈ G∗ξ the one-form α
(1)
η(ξ) ∈ Λ1(G) by
α
(1)
η(ξ)(h) := R∗hη(ξ), (8)
where Rh : G → G is the right translation by an element h ∈ G.
It is easy to check that element (8) is rightG-invariant and leftGη(ξ)ξ -invariant, thus inducing
a one-form on the quotient Nξ := G/G
η(ξ)
ξ .
Denote by pr∗α
(1)
η(ξ) its pull-back to T ∗(Nξ) and form the symplectic manifold (T ∗(Nξ),
dpr∗β(1) + dpr∗α
(1)
η(ξ)), where dpr∗β(1) ∈ Λ(2)(T ∗(Nξ)) is the canonical symplectic form on
T ∗(Nξ).
The construction above can now be summarized as the following theorem.
Theorem 4. Let ξ, η ∈ G∗ and η(ξ) := η|G∗ξ be fixed. Then the reduced symplectic mani-
fold (l−1(η(ξ))/G
η(ξ)
ξ , σ
(2)
ξ ) is a symplectic covering of the coadjoint orbit Or(ξ, η(ξ); G̃) and
symplectically embeds onto a subbundle over G/Gη(ξ)ξ of (T ∗(G/G
η(ξ)
ξ ), ω
(2)
ξ ), with
ω
(2)
ξ := dpr∗β(1) + dpr∗α
(1)
η(ξ) ∈ Λ2(T ∗(G/G
η(ξ)
ξ ).
The statement above fits into the conditions of Theorem 2 if one defines a connection 1-form
A(g) : Tg(G) → Gξ as follows:
〈A(g), ξ〉G := R∗gη(ξ) (9)
for any g ∈ G.
Expression (9) generates a completely horizontal 2-form d〈A(g), ξ〉G on the Lie group
G, which immediately gives rise to the symplectic structure ω(2)
ξ on the reduced phase space
T ∗(G/G
η(ξ)
ξ ).
THE CANONICAL REDUCTION METHOD FOR SYMPLECTIC STRUCTURES . . . 359
2. The Maxwell Electromagnetic Equations
Under the Maxwell electromagnetic equations we understand the following relationships
on the cotangent phase space T ∗(N) with N ⊂ T (D;R3) being a manifold of vector fields on
some almost everywhere smooth enough domain D ⊂ R3 :
∂E/∂t = rotB, ∂B/∂t = −rotE,
(10)
divE = ρ, divB = 0,
where (E,B) ∈ T ∗(N) is a vector of electric and magnetic fields and ρ ∈ C(D;R) is some fixed
density function for a smeared out ambient charge.
Aiming to repesent equations (10) as those on reduced symplectic space, define as in [6]
an appropriate configuration space, M ⊂ T (D;R3), with a vector potential field coordinate
A ∈ M.
The cotangent space T ∗(M) may be identified with pairs (A, Y ) ∈ T ∗(M), where Y ∈
T ∗(D;R3) is a vector field density in D.
On the space T ∗(M) there exists the canonical symplectic form ω(2) ∈ Λ2(T ∗(M), where
ω(2) := dpr∗α(1), and
α(1)(A, Y ) =
∫
D
d3x〈Y, dA〉 := (Y, dA), (11)
where by 〈·, ·〉 we denote the standard scalar product in R3 endowed with the measure d3x,
and by pr : T ∗(M) → M we denote the usual basepoint projection upon the base space M.
Define now a Hamiltonian function H ∈ D(T ∗(M)) by
H(A, Y ) =
1
2
((Y, Y ) + (rotA, rotA)), (12)
which is evidently invariant with respect to the following symmetry group G acting on the base
manifold M and lifted to T ∗(M) : for any ψ ∈ G ⊂ C(1)(D;R) and (A, Y ) ∈ T ∗(M)
ϕψ(A) := A+∇ψ, Φψ(Y ) = Y. (13)
Under the transformation (13) the 1-form (11) is evidently invariant too, since
ϕ∗ψ α
(1)(A, Y ) = (Y, dA+∇dψ) = (Y, dA)− (div Y, dψ) = α(1)(A, Y ),
where we made use of the condition that dψ ' 0 in Λ1(M).
Thus the corresponding momentum mapping (2) is given as l(A, Y ) = −div Y for all
(A, Y ) ∈ T ∗(M).
If ρ ∈ G∗, one can define the reduced space l−1(ρ)/G, since evidently the isotropy group
Gρ = G due to its commutativity.
Consider now a principal fiber bundle p : M → N with the Abelian structure group G
and a base manifold N taken to be N := {B ∈ T (D;R3) : divB = 0}, where, by definition,
p(A) := B = rotA.
360 A.K. PRYKARPATS’KY, V.HR. SAMOYLENKO
Over this bundle, one can build a connection 1-form A : T (M) → G, where for all A ∈ M ,
A(A) · Â∗(l) = 1, d〈A(A), ρ〉G = Ω(2)
ρ (B)
in virtue of commutativity of the Lie algebra G.
Then, due to Theorem 2, the cotangent manifold T ∗(N) is symplectomorphic to the reduced
phase space
l−1(ρ)/G ∼= {(B,S) ∈ T ∗(N) : divE(S) = ρ, divB = 0}
with the canonical symplectic 2-form
ω(2)
ρ (B,S) = (dS,∧dB) + d 〈A(A), ρ〉G , (14)
where we put rotS−F = −E and, by definition, divF = ρ for some mapping F ∈ C1(D;R3).
The Hamiltonian (12) is correspondingly reduced to the following classical form:
H(B,E) =
1
2
((B,B) + (E,E)). (15)
As a result, the Maxwell equations (9) become a Hamiltonian system on the reduced phase
space T ∗(N) endowed with the quasicanonical symplectic structure (14) and the new Hami-
ltonian function (15).
It is well known that Maxwell equations (10) admit a one more canonical symplectic structure
on T ∗(N), namely,
ω̄(2) := (dB,∧dE), (16)
with respect to which they are Hamiltonian too and whose ”helicitylike” conservative Hami-
ltonian function is
H̄(B,E) =
1
2
((rotE,E) + (rotB,B)), (17)
where (B,E) ∈ T ∗(N).
It easy to see that (17) is also an invariant function with respect to the Maxwell equations
(10). Subject to the Maxwell equations (10), a group theoretical interpretation of the symplectic
structure (16) is still waiting for search.
Notice finally that both symplectic structure (16) and Hamiltonian (17) are invariant with
respect to the following Abelian group G2 = G×G-action:
G2 3 (ψ, χ) : (B,E) → (B +∇ψ,E +∇χ) (18)
for all (B,E) ∈ T ∗(N).
THE CANONICAL REDUCTION METHOD FOR SYMPLECTIC STRUCTURES . . . 361
Corresponding to (18), the momentum mapping l : T ∗(N) → G∗×G∗ is calculated as
l(B,E) = (divE,−divB) (19)
for any (B,E) ∈ T ∗(N).
Fixing a value in (19) as l(B,E) = ξ := (ρ, 0), that is,
divE = ρ, divB = 0, (20)
one obtains the reduced phase space l−1(ξ)/G2, since the isotropy subgroup G2
ξ of the element
ξ ∈ G∗×G∗ coincides with entire group G2.
Thus the reduced phase space, due to Theorem 2, is endowed with the canonical symplectic
structure
ω̄(2)(A, Y ) = (dY,∧ dA) + d 〈A(A), ξ〉G ,
where T ∗(M) 3 (A, Y ) are variables constituting the corresponding coordinates on the cotangent
space over an associated fibre bundle p̄ : N → M with a curvature 1-form A : T (N) → G ×G.
In virtue of (20) one can define the projection map p̄ : N → M as follows: p̄(B) :=
rot−1B = A for any A ∈ M ⊂ T (D;R3).
It is evident that the second condition of (20) is satisfied automatically on the cotangent
bundle T ∗(M).
Subject to the coadjoint variables Y ∈ T ∗A(M) and E ∈ T ∗B(N) for all A ∈ M and E ∈ N ,
one can easily obtain from the equality p̄∗β(1) = α(1) the expression
Y = −rotE
satisfying the evident condition div Y = 0. The Hamiltonians (15) and (17) take, correspondi-
ngly, on T ∗(M) the forms
H̄(A, Y ) =
1
2
(
(rot 3A,A) + (rot−1 Y, Y )
)
and
H(A, Y ) =
1
2
(
(rot−1 Y, rot−1 Y ) + (rotA, rotA)
)
,
being obviously invariant too with respect to common evolutions on T ∗(M).
As was mentioned in [1], the invariant like (17) admits the following geometrical interpretati-
on: its quantity is a helicity structure related with dynamical equations, that is a number of
closed linkages of the vortex lines present in the ambient phase space.
If one to consider now a motion of a charged particle under a Maxwell field, it is convenient
to introduce another fiber bundle structure p : M → N, namely, the one such thatM = N×G,
N := D ⊂ R3, and G := R\{0} being the corresponding (Abelian) structure Lie group.
An analysis similar to the above gives rise to a symplectic structure reduced to the space
l−1(ξ)/G ' T ∗(N), ξ ∈ G,
ω(2)(q, p) = 〈dp,∧dq〉+ d〈A(q, g), ξ〉G ,
362 A.K. PRYKARPATS’KY, V.HR. SAMOYLENKO
where
A(q, g) := 〈A(q), dq〉+ g−1dg
is a usual connection 1-form on M with (q, p) ∈ T ∗(N) and g ∈ G.
The corresponding canonical Poisson brackets on T ∗(N) are easily found to be
{qi, qj} = 0, {pj , qi} = δij , {pi, pj} = Fji(q)
for all (q, p) ∈ T ∗(N).
If one introduces a new momentum variable p̃ := p + A(q) on T ∗(N) 3 (q, p), it is easy to
verify that ω(2)
ξ → ω̃
(2)
ξ := 〈dp̃,∧dq〉, giving rise to the following Poisson brackets [7, 8]:
{qi, qj} = 0, {p̃j , qi} = δij , {p̃i, p̃j} = 0,
where i, j = 1, 3, iff for all i, j, k = 1, 3 the standard Maxwell field equations are satisfied
on N :
∂Fij
∂qk
+
∂Fjk
∂qi
+
∂Fki
∂qj
= 0
with the curvature tensor
Fij(q) :=
∂Aj
∂qi
− ∂Ai
∂qj
,
where i, j = 1, 3, q ∈ N.
Such a construction permits a natural generalization to the case of non-Abelian structure
Lie group yielding a description of Yang – Mills field equations within the reduction approach.
3. A Charged Particle Phase Space Structure and Yang – Mills Field Equations
As before, we start by defining a phase space M of a particle under a Yang – Mills field in a
region D ⊂ R3 as M := D ×G, where G is a Lie group (not in general semisimple) acting on
M from the right.
Over the space M one can define quite naturally a connection Γ(A) if to consider the
following trivial principal fiber bundle p : M → N, where N := D, with the structure group
G. Namely, if g ∈ G, q ∈ N, then a connection 1-form on M 3 (q, g) can be written [1, 3, 9] as
A(q; g) := g−1
(
d+
n∑
i=1
aiA
(i)(q)
)
g, (21)
where {ai ∈ G : i =1, n} is a basis of the Lie algebra G of the Lie group G, and Ai : D →
Λ1(D), i = 1, n, are the Yang – Mills fields in the physical space D ⊂ R3.
Now one defines the natural left invariant Liouville form on M by
α(1)(q; g) := 〈p, dq〉+ 〈y, g−1dg〉G , (22)
THE CANONICAL REDUCTION METHOD FOR SYMPLECTIC STRUCTURES . . . 363
where y ∈ T ∗(G) and 〈·, ·〉G denotes as before the usual Ad-invariant nondegenerate bilinear
form on G∗ × G, as evidently g−1dg ∈ Λ1(G)⊗ G.
The main assumption we need to make for the sequel is that the connection 1-form is in
accordance with the action of the Lie group G on M. The latter means that the condition
R∗hA(q; g) = Adh−1A(q; g)
is satisfied for all (q, g) ∈ M and h ∈ G, where Rh : G → G means the right translation by an
element h ∈ G on the Lie group G.
Having stated all preliminary conditions needed for the reduction Theorem 2 to be applied
to our model, suppose that the Lie group G canonical action on M is naturally lifted to that
on the cotangent space T ∗(M) endowed, due to (22), with the following G-invariant canonical
symplectic structure:
ω(2)(q, p; g, y) := dpr∗α(1)(q, p; g, y) = 〈dp,∧dq〉
+ 〈dy,∧g−1dg〉G + 〈ydg−1,∧dg〉G (23)
for all (q, p; g, y) ∈ T ∗(M).
Take now an element ξ ∈ G∗ and assume that its isotropy subgroupGξ = G, that is,Ad∗hξ =
ξ for all h ∈ G. In the general case such an element ξ ∈ G∗ can only be the trivial one, ξ = 0 as
it happens in the case of the Lie group G = SL2(R).
Then one can construct the reduced phase space l−1(ξ)/G symplectomorphic to (T ∗(N), ω
(2)
ξ ),
where due to (7) for any (q, p) ∈ T ∗(N) we have
ω
(2)
ξ (q, p) = 〈dp,∧dq〉+ 〈Ω(2)(q), ξ〉G
= 〈dp,∧dq〉+
n∑
s=1
3∑
i,j=1
esF
(s)
ij (q)dqi ∧ dqj . (24)
In the above we have expanded the element
G∗ 3 ξ =
n∑
i=1
eia
i
with respect to the biorthogonal basis {ai ∈ G∗ : 〈ai, aj〉G = δij , i, j = 1, n} with ei ∈ R, i =
1, 3, being some constants and we denoted by F (s)
ij (q), i, j = 1, 3, s = 1, n, the corresponding
curvature 2-form Ω(2) ∈ Λ2(N)⊗ G components, that is,
Ω(2)(q) :=
n∑
s=1
3∑
i,j=1
asF
(s)
ij (q)dqi ∧ dqj
for any point q ∈ N. Summarizing the above calculations we can formulate the following result.
364 A.K. PRYKARPATS’KY, V.HR. SAMOYLENKO
Theorem 5. Suppose a Yang – Mills field (21) on the fiber bundle p : M → N with M =
D × G is invariant with respect to the Lie group G-action G ×M → M. Suppose also that an
element ξ ∈ G∗ is chosen so that Ad∗Gξ = ξ. Then for the naturally constructed momentum
mapping l : T ∗(M) → G∗ (being equivariant) the reduced phase space l−1(ξ)/G ' T ∗(N)
is endowed with the canonical symplectic structure (24) having the following component-wise
Poissoin brackets form:
{pi, qj}ξ = δji , {q
i, qj}ξ = 0, {pi, pj}ξ =
n∑
s=1
esF
(s)
ji (q)
for all i, j = 1, 3 and (q, p) ∈ T ∗(N).
The correspondingly extended Poisson bracket on the whole cotangent space T ∗(M) amounts,
due to (23), to the following set of Poisson relations:
{ys, yk} =
n∑
r=1
crskyr, {pi, qj} = δji ,
(25)
{ys, pj} = 0 = {qi, qj}, {pi, pj} =
n∑
s=1
ysF
(s)
ji (q),
where i, j = 1, 3, crsk ∈ R, s, k, r = 1, n, are the structure constants of the Lie algebra G, and
we made use of the expansion
A(s)(q) =
3∑
j=1
A
(s)
j (q)dqj
as well made alternative values ei := yi, i = 1, n.
The result (25) can be seen easily if one rewrites expression (23) in an extended form,
ω(2) := ω
(2)
ext, where
ω
(2)
ext := ω(2)
∣∣∣
A0→A
, A0(g) := g−1dg, g ∈ G.
Thereby one can obtain in virtue of the invariance properties of the connection Γ(A) that
ω
(2)
ext(q, p;u, y) = 〈dp,∧dq〉+ d〈y(g), Adg−1A(q; e)〉G
= 〈dp,∧dq〉+ 〈dAd∗g−1y(g),∧A(q; e)〉G
= 〈dp,∧dq〉+
n∑
s=1
dys ∧ dus + +
3∑
j=1
n∑
s=1
A
(s)
j (q)dys ∧ dq
− 〈Ad∗g−1y(g),A(q, e) ∧ A(q, e)〉G
+
n∑
k≥s=1
n∑
l=1
yl c
l
sk du
k ∧ dus +
n∑
s=1
3∑
i≥j=1
ysF
(s)
ij (q)dqi ∧ dqj , (26)
THE CANONICAL REDUCTION METHOD FOR SYMPLECTIC STRUCTURES . . . 365
where the coordinate points (q, p;u, y) ∈ T ∗(M) are defined as follows:
A0(e) :=
n∑
s=1
dui ai, Ad∗g−1y(g) = y(e) :=
n∑
s=1
ys a
s
for any element g ∈ G.
Whence one immediately gets the Poisson brackets (25) plus additional brackets connected
with the conjugated sets of variables {us ∈ R : s = 1, n} ∈ G∗ and {ys ∈ R : s = 1, n} ∈ G
of the following form:
{ys, uk} = δks , {uk, qj} = 0, {pj , us} = A
(s)
j (q), {us, uk} = 0, (27)
where j = 1, 3, k, s = 1, n, and q ∈ N.
Note here that the suggested above transition from the symplectic structure ω(2) on T ∗(N)
to its extension ω(2)
ext on T ∗(M) just consists formally in adding to the symplectic structure ω(2)
an exact part which transforms it into equivalent one.
Looking now at expressions (26), one can immediately infer that the element
ξ :=
n∑
s=1
esa
s ∈ G∗
will be invariant with respect to the Ad∗-action of the Lie group G iff
{ys, yk}|ys=es =
n∑
r=1
crsk er ≡ 0
identically for all s, k = 1, n, j = 1, 3 and q ∈ N.
In this and only this case, the reduction scheme elaborated above will go through.
Returning attention to the expression (27), one can easily write the following exact expressi-
on:
ω
(2)
ext(q, p;u, y) = ω(2)(q, p+
n∑
s=1
ysA
(s)(q);u, y), (28)
on the phase space T ∗(M) 3 (q, p;u, y), where we denoted for brevity 〈A(s)(q), dq〉 by
3∑
j=1
A
(s)
j (q) dqj .
The transformation like (28) was discussed within a somewhat different context in paper
[7] containing also a good background for the infinite-dimensional generalization of symplectic
structure techniques.
Having observed from (28) that the simple change of variable
p̃ := p+
n∑
s=1
ysA
(s)(q)
366 A.K. PRYKARPATS’KY, V.HR. SAMOYLENKO
of the cotangent space T ∗(N) recasts our symplectic structure (26) into the old canonical form
(23), one obtains the following new set of Poisson brackets on T ∗(M) 3 (q, p̃;u, y) of the form:
{ys, yk} =
n∑
r=1
crsk yr, {p̃i, p̃j} = 0, {p̃i, qj} = δji ,
{ys, qj} = 0 = {qi, qj}, {us, uk} = 0, {ys, p̃j} = 0,
{us, qi} = 0, {ys, uk} = δks , {us, p̃j} = 0,
where k, s = 1, n and i, j = 1, 3, holds iff the Yang – Mills equations
∂F
(s)
ij
∂ql
+
∂F
(s)
jl
∂qi
+
∂F
(s)
li
∂qj
+
n∑
k,r=1
cskr(F
(k)
ij A
(r)
l + F
(k)
jl A
(r)
i + F
(k)
li A
(r)
j ) = 0
are fulfilled for all s = 1, n and i, j, l = 1, 3 on the base manifold N.
This effect of complete reduction of Yang – Mills variables from the symplectic structure
(26) is known in literature [1, 7] as the principle of minimal interaction and appeared to be
useful enough for studying different interacting systems as in papers [6, 10]. In Part 2 of this
paper we shall continue a study of reduced symplectic structures connected with infinite di-
mensional coupled dynamical systems like Yang – Mills – Vlasov, Yang – Mills – Bogoliubov and
Yang – Mills – Josephson ones.
4. Acknowledgements
One of the authors (A.P.) is cordially indebted to Prof. B.A. Kupershmidt for sending a set
of inspiring reprints of his papers some of which are cited through this work as well as to Prof.
J. Zagrodzinski for sending his paper before publication.
Special thanks for nice hospitality and warm research atmosphere are due to the staff of
Department of Physics at the EMU of N.Cyprus, especially to Profs. M. Halilsoy, E. Aydiroglu,
Ufuk Taneri and Ping Zhang for valuable discussions of problems under study.
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Received 21.01.2001
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