Invariants of Diffeomorphism Groups Actions Valentin Lychagin and - - PowerPoint PPT Presentation

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Invariants of Diffeomorphism Groups Actions Valentin Lychagin and - - PowerPoint PPT Presentation

Invariants of Diffeomorphism Groups Actions Valentin Lychagin and Valery Yumaguzhin Russian Academy of Sciences, Russia & University of Troms, Norway Workshop on Infinite-dimensional Riemannian geometry January 12 16, 2015,


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Invariants of Diffeomorphism Groups Actions

Valentin Lychagin and Valery Yumaguzhin

Russian Academy of Sciences, Russia & University of Tromsø, Norway

Workshop on “Infinite-dimensional Riemannian geometry ” January 12 — 16, 2015, Vienna, Austria

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

The field of relativistic invariants.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

The field of relativistic invariants. Hilbert and Poincare functions for relativistic invariants.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

The field of relativistic invariants. Hilbert and Poincare functions for relativistic invariants. Factor Einstein Equations and the equivalence problem for Einstein metrics.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

The field of relativistic invariants. Hilbert and Poincare functions for relativistic invariants. Factor Einstein Equations and the equivalence problem for Einstein metrics.

Einstein - Maxwell equations

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

The field of relativistic invariants. Hilbert and Poincare functions for relativistic invariants. Factor Einstein Equations and the equivalence problem for Einstein metrics.

Einstein - Maxwell equations

The field of electromagnetic invariants.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

The field of relativistic invariants. Hilbert and Poincare functions for relativistic invariants. Factor Einstein Equations and the equivalence problem for Einstein metrics.

Einstein - Maxwell equations

The field of electromagnetic invariants. Hilbert and Poincare functions for electromagnetic invariants.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Overview

Diffeomorphisms and Naturality Principle in Physics Metrics (and Gravity)

The field of rational differential invariants. Hilbert and Poincare functions for metrics. Factor Equations and the equivalence problem for metrics.

Vacuum Einstein equations.

The field of relativistic invariants. Hilbert and Poincare functions for relativistic invariants. Factor Einstein Equations and the equivalence problem for Einstein metrics.

Einstein - Maxwell equations

The field of electromagnetic invariants. Hilbert and Poincare functions for electromagnetic invariants. Factor Einstein-Maxwell Equations and the equivalence problem for solutions of Einstein - Maxwell equations.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Differential Groups

M is a smooth manifold.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Differential Groups

M is a smooth manifold. πk : Jk

0 (M, M) → M × M - the bundle of k-jets of local

diffeomorphisms (of M ).

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Differential Groups

M is a smooth manifold. πk : Jk

0 (M, M) → M × M - the bundle of k-jets of local

diffeomorphisms (of M ). The bundles πk,k−1 : Jk

0 (M, M) → Jk−1

(M, M) are affine, when k ≥ 2, and the associated vector bundles are SkT∗ ⊗ T.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Differential Groups

M is a smooth manifold. πk : Jk

0 (M, M) → M × M - the bundle of k-jets of local

diffeomorphisms (of M ). The bundles πk,k−1 : Jk

0 (M, M) → Jk−1

(M, M) are affine, when k ≥ 2, and the associated vector bundles are SkT∗ ⊗ T. Fix a ∈ M, then

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Differential Groups

M is a smooth manifold. πk : Jk

0 (M, M) → M × M - the bundle of k-jets of local

diffeomorphisms (of M ). The bundles πk,k−1 : Jk

0 (M, M) → Jk−1

(M, M) are affine, when k ≥ 2, and the associated vector bundles are SkT∗ ⊗ T. Fix a ∈ M, then

fibres Dk = π−1

k,0 (a, a)

are algebraic Lie groups, (differential group of order k )

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Differential Groups

M is a smooth manifold. πk : Jk

0 (M, M) → M × M - the bundle of k-jets of local

diffeomorphisms (of M ). The bundles πk,k−1 : Jk

0 (M, M) → Jk−1

(M, M) are affine, when k ≥ 2, and the associated vector bundles are SkT∗ ⊗ T. Fix a ∈ M, then

fibres Dk = π−1

k,0 (a, a)

are algebraic Lie groups, (differential group of order k ) projections πk,k−1 : Dk → Dk−1 are Lie group epimorphisms, and

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Differential Groups

M is a smooth manifold. πk : Jk

0 (M, M) → M × M - the bundle of k-jets of local

diffeomorphisms (of M ). The bundles πk,k−1 : Jk

0 (M, M) → Jk−1

(M, M) are affine, when k ≥ 2, and the associated vector bundles are SkT∗ ⊗ T. Fix a ∈ M, then

fibres Dk = π−1

k,0 (a, a)

are algebraic Lie groups, (differential group of order k ) projections πk,k−1 : Dk → Dk−1 are Lie group epimorphisms, and kernels ∆k = ker (πk,k−1 : Dk → Dk−1) are abelian Lie groups,and ∆k SkT∗ ⊗ T.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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D0 = e; D1 = GL ( TM) .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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D0 = e; D1 = GL ( TM) . For k ≥ 2 0 → SkT∗ ⊗ T →Dk → Dk−1 → e

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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D0 = e; D1 = GL ( TM) . For k ≥ 2 0 → SkT∗ ⊗ T →Dk → Dk−1 → e In words: Dk is an extension of Dk−1 by Abelian group SkT∗ ⊗ T.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Quadratic differential forms

Let q : S2T∗M → M be the symmetric power of the cotangent bundle.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Quadratic differential forms

Let q : S2T∗M → M be the symmetric power of the cotangent bundle. Smooth sections C ∞ (q) are quadratic differential forms on M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Quadratic differential forms

Let q : S2T∗M → M be the symmetric power of the cotangent bundle. Smooth sections C ∞ (q) are quadratic differential forms on M. Let Jk (q) be the manifold of k-jets of quadratic differential forms, and qk : Jk (q) → M the bundles of jets.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Quadratic differential forms

Let q : S2T∗M → M be the symmetric power of the cotangent bundle. Smooth sections C ∞ (q) are quadratic differential forms on M. Let Jk (q) be the manifold of k-jets of quadratic differential forms, and qk : Jk (q) → M the bundles of jets. Exact sequences of vector bundles 0 → SkT∗ ⊗ S2T∗→ Jk (q) → Jk−1 (q) → 0.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Actions

φ : M → M - local diffeomorphism, g - is a quadratic differential form: φ : g → φ (g) = φ∗−1 (g) the natural action.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Actions

φ : M → M - local diffeomorphism, g - is a quadratic differential form: φ : g → φ (g) = φ∗−1 (g) the natural action. Jet -level. Let φ(a) = a, [φ]k+1

a

∈ Dk+1 (k + 1) -jet of φ at the point a, and [g]k

a ∈ Jk a (q) k -jet of g at the point a. Then

[φ]k+1

a

: [g]k

a → [φ(g)]k a

defines Dk+1 -action on Jk

a (q) .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Important algebraic structure

For any smooth bundle π : E (π) → M fibres of projections πk,0 : Jk (π) → J0 (π) = E (π) are algebraic manifolds wrt canonical jet-coordinates.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Important algebraic structure

For any smooth bundle π : E (π) → M fibres of projections πk,0 : Jk (π) → J0 (π) = E (π) are algebraic manifolds wrt canonical jet-coordinates. The structure is natural in the sence that smooth bundle automorphisms induce birational isomorphisms of the algebraic manifolds.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Important algebraic structure

For any smooth bundle π : E (π) → M fibres of projections πk,0 : Jk (π) → J0 (π) = E (π) are algebraic manifolds wrt canonical jet-coordinates. The structure is natural in the sence that smooth bundle automorphisms induce birational isomorphisms of the algebraic manifolds. Important:

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Important algebraic structure

For any smooth bundle π : E (π) → M fibres of projections πk,0 : Jk (π) → J0 (π) = E (π) are algebraic manifolds wrt canonical jet-coordinates. The structure is natural in the sence that smooth bundle automorphisms induce birational isomorphisms of the algebraic manifolds. Important:

Jk

a (q) - algebraic manifolds,

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Important algebraic structure

For any smooth bundle π : E (π) → M fibres of projections πk,0 : Jk (π) → J0 (π) = E (π) are algebraic manifolds wrt canonical jet-coordinates. The structure is natural in the sence that smooth bundle automorphisms induce birational isomorphisms of the algebraic manifolds. Important:

Jk

a (q) - algebraic manifolds,

Dk+1 - algebraic groups,

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Important algebraic structure

For any smooth bundle π : E (π) → M fibres of projections πk,0 : Jk (π) → J0 (π) = E (π) are algebraic manifolds wrt canonical jet-coordinates. The structure is natural in the sence that smooth bundle automorphisms induce birational isomorphisms of the algebraic manifolds. Important:

Jk

a (q) - algebraic manifolds,

Dk+1 - algebraic groups, Dk+1 × Jk

a (q) → Jk a (q) -algebraic actions.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Rational differential invariants

Rosenlicht theorem = ⇒ rational invariants of the Dk+1 -action on Jk

a (q) separate regular orbits.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Rational differential invariants

Rosenlicht theorem = ⇒ rational invariants of the Dk+1 -action on Jk

a (q) separate regular orbits.

We call the rational Dk+1−invariants metric invariants.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Rational differential invariants

Rosenlicht theorem = ⇒ rational invariants of the Dk+1 -action on Jk

a (q) separate regular orbits.

We call the rational Dk+1−invariants metric invariants. Let Fk the field of metric invariants, then trdeg (Fk) = codim (regular Dk+1 − orbit) .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Rational differential invariants

Rosenlicht theorem = ⇒ rational invariants of the Dk+1 -action on Jk

a (q) separate regular orbits.

We call the rational Dk+1−invariants metric invariants. Let Fk the field of metric invariants, then trdeg (Fk) = codim (regular Dk+1 − orbit) . Metric Hilbert function: k → H(k) = trdeg (Fk) − trdeg (Fk−1) the "number of metric invariants of pure order k" .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Rational differential invariants

Rosenlicht theorem = ⇒ rational invariants of the Dk+1 -action on Jk

a (q) separate regular orbits.

We call the rational Dk+1−invariants metric invariants. Let Fk the field of metric invariants, then trdeg (Fk) = codim (regular Dk+1 − orbit) . Metric Hilbert function: k → H(k) = trdeg (Fk) − trdeg (Fk−1) the "number of metric invariants of pure order k" . Metric Poincaré function: Π (t) = ∑

k≥0

H (k) tk.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Orbits

Denote by ζk the following operator ζk : Sk+1T∗ ⊗ T

δ

→ SkT∗ ⊗ T∗ ⊗ T

sym

→ SkT∗ ⊗ S2T∗, where δ is the Spencer δ-operator.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Orbits

Denote by ζk the following operator ζk : Sk+1T∗ ⊗ T

δ

→ SkT∗ ⊗ T∗ ⊗ T

sym

→ SkT∗ ⊗ S2T∗, where δ is the Spencer δ-operator. The tangent space Tθ (∆k+1θ) to the orbit ∆k+1θ, θ ∈ Jk

a (q)

coinside with the image of ζk : Tθ (∆k+1θ) = Im ζk.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Orbits

Denote by ζk the following operator ζk : Sk+1T∗ ⊗ T

δ

→ SkT∗ ⊗ T∗ ⊗ T

sym

→ SkT∗ ⊗ S2T∗, where δ is the Spencer δ-operator. The tangent space Tθ (∆k+1θ) to the orbit ∆k+1θ, θ ∈ Jk

a (q)

coinside with the image of ζk : Tθ (∆k+1θ) = Im ζk. The normal space to the orbit ∆k+1θ is Coker ζk. We call Coker ζk, k ≥ 2, space of curvature tensors of order k. Coker ζ2 is the space of so-called algebraic curvature tensors.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Orbits

Denote by ζk the following operator ζk : Sk+1T∗ ⊗ T

δ

→ SkT∗ ⊗ T∗ ⊗ T

sym

→ SkT∗ ⊗ S2T∗, where δ is the Spencer δ-operator. The tangent space Tθ (∆k+1θ) to the orbit ∆k+1θ, θ ∈ Jk

a (q)

coinside with the image of ζk : Tθ (∆k+1θ) = Im ζk. The normal space to the orbit ∆k+1θ is Coker ζk. We call Coker ζk, k ≥ 2, space of curvature tensors of order k. Coker ζ2 is the space of so-called algebraic curvature tensors. Ker ζk = 0, when k ≥ 1 and n = dim M ≥ 3.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Invariants

Computing dimensions of Coker ζk leads us to the following formulae for metric Hilbert function.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Invariants

Computing dimensions of Coker ζk leads us to the following formulae for metric Hilbert function. The Hilbert function of metric invariants is: Hn (2) = n (n + 3) (n − 1) (n − 2) 12 , Hn (k) = n (k − 1) 2 n + k − 1 k + 1

  • ,

when n = dim M ≥ 3 and k ≥ 3.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Invariants

Computing dimensions of Coker ζk leads us to the following formulae for metric Hilbert function. The Hilbert function of metric invariants is: Hn (2) = n (n + 3) (n − 1) (n − 2) 12 , Hn (k) = n (k − 1) 2 n + k − 1 k + 1

  • ,

when n = dim M ≥ 3 and k ≥ 3. In the case dim M = 2, H2 (2) = H2 (3) = 1, H2 (k) = k − 1, when k ≥ 4.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Invariants

Computing dimensions of Coker ζk leads us to the following formulae for metric Hilbert function. The Hilbert function of metric invariants is: Hn (2) = n (n + 3) (n − 1) (n − 2) 12 , Hn (k) = n (k − 1) 2 n + k − 1 k + 1

  • ,

when n = dim M ≥ 3 and k ≥ 3. In the case dim M = 2, H2 (2) = H2 (3) = 1, H2 (k) = k − 1, when k ≥ 4. The above formulae have been obtained by Zorawski, K. (1892), for the case n = 2, and by Haskins, C.N. (1902), for the case n ≥ 3.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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For small dimensions (n ≤ 4) and low orders (k ≤ 9), we have the following table of values of the Hilbert function: n\k 2 3 4 5 6 7 8 9 2 1 1 3 4 5 6 7 8 3 3 15 27 42 60 71 105 132 4 14 60 126 224 360 540 770 1056

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Tresse derivations

Total differential. For f ∈ C ∞ Jkπ

  • we denote by

df the total differential of f :

  • df =

n

i=1

df dxi dxi, where

d dxi total derivatives.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Tresse derivations

Total differential. For f ∈ C ∞ Jkπ

  • we denote by

df the total differential of f :

  • df =

n

i=1

df dxi dxi, where

d dxi total derivatives.

We say that functions f1, ..., fn ∈ C ∞ Jkπ

  • , where n = dim M, are

in general position if

  • df1 ∧ · · · ∧

dfn = 0 in an open domain.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Tresse derivations

For functions f1, ..., fn in general position and arbitrary f ∈ C ∞ Jkπ

  • we have
  • df = λ1

df1 + · · · + λn dfn in the domain of definition.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Tresse derivations

For functions f1, ..., fn in general position and arbitrary f ∈ C ∞ Jkπ

  • we have
  • df = λ1

df1 + · · · + λn dfn in the domain of definition. Functions λ1, ..., λn ∈ C ∞ Jk+1π

  • are said to be Tresse derivatives
  • f f and will be denoted

Df Df1 , ...., Df Dfn .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Tresse derivations

For functions f1, ..., fn in general position and arbitrary f ∈ C ∞ Jkπ

  • we have
  • df = λ1

df1 + · · · + λn dfn in the domain of definition. Functions λ1, ..., λn ∈ C ∞ Jk+1π

  • are said to be Tresse derivatives
  • f f and will be denoted

Df Df1 , ...., Df Dfn . Important observation: If f1, ..., fn are metric invariants of order k then Df Dfi are metric invariants too for any metric invariant f .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Tresse derivations

For functions f1, ..., fn in general position and arbitrary f ∈ C ∞ Jkπ

  • we have
  • df = λ1

df1 + · · · + λn dfn in the domain of definition. Functions λ1, ..., λn ∈ C ∞ Jk+1π

  • are said to be Tresse derivatives
  • f f and will be denoted

Df Df1 , ...., Df Dfn . Important observation: If f1, ..., fn are metric invariants of order k then Df Dfi are metric invariants too for any metric invariant f . Remark that order of Df

Dfi , as a rule, higher then order of f .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Data Formally integrable algebraic PDEs system Ek ⊂ Jkπ. That is, fibres of projection πk,0 : Ek → J0π are irreducible algebraic manifolds.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Data Formally integrable algebraic PDEs system Ek ⊂ Jkπ. That is, fibres of projection πk,0 : Ek → J0π are irreducible algebraic manifolds. Algebraic Lie pseudo group G of symmetries of E, acting in a transitive way on J0π. That is, a Lie pseudogroup given by algebraic differential equations.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Data Formally integrable algebraic PDEs system Ek ⊂ Jkπ. That is, fibres of projection πk,0 : Ek → J0π are irreducible algebraic manifolds. Algebraic Lie pseudo group G of symmetries of E, acting in a transitive way on J0π. That is, a Lie pseudogroup given by algebraic differential equations. By rational differerential G-invariants of order ≤ l we mean fibrewise rational functions on prolongation El = E(l−k)

k

⊂ Jlπ which are G-invariant. Denote by Fl the field of invariants of order ≤ l.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Lie -Tresse Theorem

Statement

There are basic invariants: Q1, ..., Qn, P1, ..., Pm, such that any rational differential G-invariant is a rational function of Q, P and the Tresse derivatives D|σ|P DQσ .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 61

Lie -Tresse Theorem

Statement

There are basic invariants: Q1, ..., Qn, P1, ..., Pm, such that any rational differential G-invariant is a rational function of Q, P and the Tresse derivatives D|σ|P DQσ . Rational differential G-invariants separate regular orbits.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 62

Lie -Tresse Theorem

Statement

There are basic invariants: Q1, ..., Qn, P1, ..., Pm, such that any rational differential G-invariant is a rational function of Q, P and the Tresse derivatives D|σ|P DQσ . Rational differential G-invariants separate regular orbits. trdeg (Fl) = codim (regular G-orbit in El) .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 63

Lie -Tresse Theorem

Application: metric invariants

n = 2. Basic invariants: Q1 = kg, Q2 = g (dkg, dkg ) , P1, P2, P3, where g = P1 dQ2

1 + 2P2

dQ1 · dQ2 + P3 dQ2

2

and kg is the curvature of g.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 64

Lie -Tresse Theorem

Application: metric invariants

n = 2. Basic invariants: Q1 = kg, Q2 = g (dkg, dkg ) , P1, P2, P3, where g = P1 dQ2

1 + 2P2

dQ1 · dQ2 + P3 dQ2

2

and kg is the curvature of g. Remark that Q1 is an invariant of order 2, Q2 -order 3, and P1, P2, P3 have order 4. All of them rational. Therefore, due to Rosenlicht theorem and Zorawski result (see above) they do generate the field of metric invariants of order 4.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 65

Lie -Tresse Theorem

Application: metric invariants

n = 2. Basic invariants: Q1 = kg, Q2 = g (dkg, dkg ) , P1, P2, P3, where g = P1 dQ2

1 + 2P2

dQ1 · dQ2 + P3 dQ2

2

and kg is the curvature of g. Remark that Q1 is an invariant of order 2, Q2 -order 3, and P1, P2, P3 have order 4. All of them rational. Therefore, due to Rosenlicht theorem and Zorawski result (see above) they do generate the field of metric invariants of order 4. Lie-Tresse theorem states that all metric invariants are rational functions of Q, P and Tresse derivatives D |σ|P

DQ σ .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 66

Lie -Tresse Theorem

Application: metric invariants

n = 2. Basic invariants: Q1 = kg, Q2 = g (dkg, dkg ) , P1, P2, P3, where g = P1 dQ2

1 + 2P2

dQ1 · dQ2 + P3 dQ2

2

and kg is the curvature of g. Remark that Q1 is an invariant of order 2, Q2 -order 3, and P1, P2, P3 have order 4. All of them rational. Therefore, due to Rosenlicht theorem and Zorawski result (see above) they do generate the field of metric invariants of order 4. Lie-Tresse theorem states that all metric invariants are rational functions of Q, P and Tresse derivatives D |σ|P

DQ σ .

Singularity condition has order 4 : Σ4 = { dQ1 ∧ dQ2 = 0} ⊂ J4q.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 67

Metric Invariants

n ≥ 3. Basic invariants: Q1 = Tr Ricg, Q2 = Tr Ric2

g, ..., Qn = Tr Ricn g,

Pij, where g = ∑

i,j

Pi,j dQi · dQj, and Ricg : T → T the Ricci operator.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 68

Metric Invariants

n ≥ 3. Basic invariants: Q1 = Tr Ricg, Q2 = Tr Ric2

g, ..., Qn = Tr Ricn g,

Pij, where g = ∑

i,j

Pi,j dQi · dQj, and Ricg : T → T the Ricci operator. Remark that Qi are invariants of order 2, and Pij have order 3. Obviously, they together with the Tresse derivatives generate the field

  • f metric invariants.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 69

Metric Invariants

n ≥ 3. Basic invariants: Q1 = Tr Ricg, Q2 = Tr Ric2

g, ..., Qn = Tr Ricn g,

Pij, where g = ∑

i,j

Pi,j dQi · dQj, and Ricg : T → T the Ricci operator. Remark that Qi are invariants of order 2, and Pij have order 3. Obviously, they together with the Tresse derivatives generate the field

  • f metric invariants.

Singularity condition has order 3 : Σ4 = { dQ1 ∧ ... ∧ dQn = 0} ⊂ J3q.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 70

Metric Factor Equation

Let n = 2, and let (M, g) be a fixed two-dimensional Riemannian manifold, and let Σg ⊂ M the set of singular points of g, (i.e. j4 (g) ∈ Σ4 ). Assume that Σg = M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 71

Metric Factor Equation

Let n = 2, and let (M, g) be a fixed two-dimensional Riemannian manifold, and let Σg ⊂ M the set of singular points of g, (i.e. j4 (g) ∈ Σ4 ). Assume that Σg = M. Take the plane R2 with fixed coordinates (x1, x2) and consider the following map (invariantization): I : M → R2, where x1 = Q1 (g) , x2 = Q2 (g) .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 72

Metric Factor Equation

Let n = 2, and let (M, g) be a fixed two-dimensional Riemannian manifold, and let Σg ⊂ M the set of singular points of g, (i.e. j4 (g) ∈ Σ4 ). Assume that Σg = M. Take the plane R2 with fixed coordinates (x1, x2) and consider the following map (invariantization): I : M → R2, where x1 = Q1 (g) , x2 = Q2 (g) . At regular points M Σg this mapping I is a covering over a domain Dg ⊂ R2 : I : M Σg → Dg ⊂ R2.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 73

Metric Factor Equation

Write down metric I−1∗ (g) in invariant coordinates h = P1 (g) dx2

1 + 2P2 (g) dx1 · dx2 + P3 (g) dx2 2 .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 74

Metric Factor Equation

Write down metric I−1∗ (g) in invariant coordinates h = P1 (g) dx2

1 + 2P2 (g) dx1 · dx2 + P3 (g) dx2 2 .

Then the metric h is invariantly related to g and satisfies the following factor equation Emetric: Curv (h) = x1, h (dx1, dx1) = x2.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Factor Equation

Write down metric I−1∗ (g) in invariant coordinates h = P1 (g) dx2

1 + 2P2 (g) dx1 · dx2 + P3 (g) dx2 2 .

Then the metric h is invariantly related to g and satisfies the following factor equation Emetric: Curv (h) = x1, h (dx1, dx1) = x2. Equivalence classes of metrics ⇐ ⇒ Solutions of PDEs system Emetric.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Example

We say that a Riemann surface (M, g) is orthogonal if the net Q1 (g) = constant, Q2 (g) = constant, is orthogonal, i.e. g( dk, d

  • g
  • dk,

dk

  • = 0.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Example

We say that a Riemann surface (M, g) is orthogonal if the net Q1 (g) = constant, Q2 (g) = constant, is orthogonal, i.e. g( dk, d

  • g
  • dk,

dk

  • = 0.

This equation is natural, and the factor equation for orthogonal surfaces has the form y4c2cxx + ycy + 2c + xy2c3 2 = 0 in coordinates (Q1, Q2) ⇔

  • x, y2

.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Example

We say that a Riemann surface (M, g) is orthogonal if the net Q1 (g) = constant, Q2 (g) = constant, is orthogonal, i.e. g( dk, d

  • g
  • dk,

dk

  • = 0.

This equation is natural, and the factor equation for orthogonal surfaces has the form y4c2cxx + ycy + 2c + xy2c3 2 = 0 in coordinates (Q1, Q2) ⇔

  • x, y2

. Orthogonal surfaces ⇐ ⇒solutions of the above equation

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Example

We say that a Riemann surface (M, g) is orthogonal if the net Q1 (g) = constant, Q2 (g) = constant, is orthogonal, i.e. g( dk, d

  • g
  • dk,

dk

  • = 0.

This equation is natural, and the factor equation for orthogonal surfaces has the form y4c2cxx + ycy + 2c + xy2c3 2 = 0 in coordinates (Q1, Q2) ⇔

  • x, y2

. Orthogonal surfaces ⇐ ⇒solutions of the above equation The factor equation has the scale symmetries (x, y, c) →

  • e2tx, e3ty, e−4tc
  • ,

which generate the Bäcklund type transformations on the class of

  • rthogonal surfaces.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Factor Equation

Let n ≥ 3, and let (M, g) be a fixed n-dimensional Riemannian manifold, and let Σg ⊂ M the set of Ricci singular points of g, (i.e. j3 (g) ∈ Σ3 ). Assume that Σg = M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 81

Metric Factor Equation

Let n ≥ 3, and let (M, g) be a fixed n-dimensional Riemannian manifold, and let Σg ⊂ M the set of Ricci singular points of g, (i.e. j3 (g) ∈ Σ3 ). Assume that Σg = M. Take space Rn with fixed coordinates (x1, ..., xn) and consider the invariantization mapping: I : M → Rn, where x1 = Q1 (g) , ..., xn = Qn (g) .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 82

Metric Factor Equation

Let n ≥ 3, and let (M, g) be a fixed n-dimensional Riemannian manifold, and let Σg ⊂ M the set of Ricci singular points of g, (i.e. j3 (g) ∈ Σ3 ). Assume that Σg = M. Take space Rn with fixed coordinates (x1, ..., xn) and consider the invariantization mapping: I : M → Rn, where x1 = Q1 (g) , ..., xn = Qn (g) . At regular points M Σg this mapping I is a covering over a domain Dg ⊂ Rn : I : M Σg → Dg ⊂ Rn.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Factor Equation

The factor equation Emetric is the following equation on a metric h on Rn : Tr Rich = x1, Tr Ric2

h = x2, ..., Tr Ricn h = xn.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Metric Factor Equation

The factor equation Emetric is the following equation on a metric h on Rn : Tr Rich = x1, Tr Ric2

h = x2, ..., Tr Ricn h = xn.

Equivalence classes of metrics ⇐ ⇒ Solutions of PDEs system Emetric.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 85

Einstein equation

Let M be an oriented 4-dimensional manifold, g be a Lorentzian metric on M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein equation

Let M be an oriented 4-dimensional manifold, g be a Lorentzian metric on M. The vacuum Einstein equation Gµν = 0 where Gµν = Rµν − R

2 gµν is the Einstein tensor, with Rµν-Ricci

curvature tensor and R the scalar curvature tensor.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein equation

Let M be an oriented 4-dimensional manifold, g be a Lorentzian metric on M. The vacuum Einstein equation Gµν = 0 where Gµν = Rµν − R

2 gµν is the Einstein tensor, with Rµν-Ricci

curvature tensor and R the scalar curvature tensor. Let E2 ⊂ J2q be a submanifold corresponding to the equation and let Ek = E(k−2)

2

⊂ Jkq be prolongations of the Einstein equation.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 88

Relativistic Invariants

Important remarks:

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Relativistic Invariants

Important remarks:

1

The Einstein equation is natural, i.e. invariant of the prolonged action

  • f the diffeomorphism group, and

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Relativistic Invariants

Important remarks:

1

The Einstein equation is natural, i.e. invariant of the prolonged action

  • f the diffeomorphism group, and

2

Formally integrable.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Relativistic Invariants

Important remarks:

1

The Einstein equation is natural, i.e. invariant of the prolonged action

  • f the diffeomorphism group, and

2

Formally integrable.

3

Fibres of the projections πk : Ek → M are irreducible algebraic manifolds and actions of the differential groups on these fibres are algebraic.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Relativistic Invariants

Important remarks:

1

The Einstein equation is natural, i.e. invariant of the prolonged action

  • f the diffeomorphism group, and

2

Formally integrable.

3

Fibres of the projections πk : Ek → M are irreducible algebraic manifolds and actions of the differential groups on these fibres are algebraic. A fibrewise rational function on the bundle πk : Ek → M we call relativistic invariant of order ≤ k if the function is invariant with respect to the prolonged action of the diffeomorphism group.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Weyl Operator

The Hodge operator ∗ : Λ2T∗ → Λ2T∗ defines the comlex structure in the bundle of differential 2-forms.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Weyl Operator

The Hodge operator ∗ : Λ2T∗ → Λ2T∗ defines the comlex structure in the bundle of differential 2-forms. The Weyl tensor, considered as operator, defines Weyl operator Wg : Λ2T∗ → Λ2T∗, which

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Weyl Operator

The Hodge operator ∗ : Λ2T∗ → Λ2T∗ defines the comlex structure in the bundle of differential 2-forms. The Weyl tensor, considered as operator, defines Weyl operator Wg : Λ2T∗ → Λ2T∗, which

commutes with ∗, i.e.Wg is a C-linear operator.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Weyl Operator

The Hodge operator ∗ : Λ2T∗ → Λ2T∗ defines the comlex structure in the bundle of differential 2-forms. The Weyl tensor, considered as operator, defines Weyl operator Wg : Λ2T∗ → Λ2T∗, which

commutes with ∗, i.e.Wg is a C-linear operator. TrC Wg = 0.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Weyl Operator

The Hodge operator ∗ : Λ2T∗ → Λ2T∗ defines the comlex structure in the bundle of differential 2-forms. The Weyl tensor, considered as operator, defines Weyl operator Wg : Λ2T∗ → Λ2T∗, which

commutes with ∗, i.e.Wg is a C-linear operator. TrC Wg = 0.

Let TrC W2

g

= I1,g + √ −1I2,g, TrC W3

g

= I3,g + √ −1I4,g.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

They are rational and invariant under diffeomorphisms

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

They are rational and invariant under diffeomorphisms dim(Weyl tensors)-dim (so (1, 3)) = 10 − 6 = 4.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

They are rational and invariant under diffeomorphisms dim(Weyl tensors)-dim (so (1, 3)) = 10 − 6 = 4. Rosenlicht theorem = ⇒ I1, I2, I3, I4 generate relativistic invariants

  • rder 2.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 102

Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

They are rational and invariant under diffeomorphisms dim(Weyl tensors)-dim (so (1, 3)) = 10 − 6 = 4. Rosenlicht theorem = ⇒ I1, I2, I3, I4 generate relativistic invariants

  • rder 2.

We say that a 3-jet θ3 ∈ E3 is singular (resp. regular) if

  • dI1 ∧ ... ∧

dI4 = 0 (resp. dI1 ∧ ... ∧ dI4 = 0) at the point.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 103

Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

They are rational and invariant under diffeomorphisms dim(Weyl tensors)-dim (so (1, 3)) = 10 − 6 = 4. Rosenlicht theorem = ⇒ I1, I2, I3, I4 generate relativistic invariants

  • rder 2.

We say that a 3-jet θ3 ∈ E3 is singular (resp. regular) if

  • dI1 ∧ ... ∧

dI4 = 0 (resp. dI1 ∧ ... ∧ dI4 = 0) at the point. Denote ∑3 ⊂ E3 the set of all singular 3-jets, it is an algebraic variety.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 104

Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

They are rational and invariant under diffeomorphisms dim(Weyl tensors)-dim (so (1, 3)) = 10 − 6 = 4. Rosenlicht theorem = ⇒ I1, I2, I3, I4 generate relativistic invariants

  • rder 2.

We say that a 3-jet θ3 ∈ E3 is singular (resp. regular) if

  • dI1 ∧ ... ∧

dI4 = 0 (resp. dI1 ∧ ... ∧ dI4 = 0) at the point. Denote ∑3 ⊂ E3 the set of all singular 3-jets, it is an algebraic variety. At the regular points we write down g = ∑

i≤j

Gij dIi · dIj.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Basic Relativistics invariants

Denote by I1, I2, I3, I4 functions on E2 corresponding to Ii,g.

They are rational and invariant under diffeomorphisms dim(Weyl tensors)-dim (so (1, 3)) = 10 − 6 = 4. Rosenlicht theorem = ⇒ I1, I2, I3, I4 generate relativistic invariants

  • rder 2.

We say that a 3-jet θ3 ∈ E3 is singular (resp. regular) if

  • dI1 ∧ ... ∧

dI4 = 0 (resp. dI1 ∧ ... ∧ dI4 = 0) at the point. Denote ∑3 ⊂ E3 the set of all singular 3-jets, it is an algebraic variety. At the regular points we write down g = ∑

i≤j

Gij dIi · dIj. Then Gij are relativistic invariants of order 3.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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The field of relativistic invariants

Theorem

The field of relativistic invariants is generated by basic invariants (I1, I2, I3, I4) of order 2 and invariants Gij of order 3 and the Tresse derivatives. This field separates regular orbits. The Hilbert function of the field of relativistic invariants is HEin (k) = 2 (k + 3) (k − 1) ,for k ≥ 3.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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The field of relativistic invariants

Theorem

The field of relativistic invariants is generated by basic invariants (I1, I2, I3, I4) of order 2 and invariants Gij of order 3 and the Tresse derivatives. This field separates regular orbits. The Hilbert function of the field of relativistic invariants is HEin (k) = 2 (k + 3) (k − 1) ,for k ≥ 3. The Poincare function is PEin (t) =

2t2(3t3−9t2+6t+2) (1−t)3

.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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The field of relativistic invariants

Theorem

The field of relativistic invariants is generated by basic invariants (I1, I2, I3, I4) of order 2 and invariants Gij of order 3 and the Tresse derivatives. This field separates regular orbits. The Hilbert function of the field of relativistic invariants is HEin (k) = 2 (k + 3) (k − 1) ,for k ≥ 3. The Poincare function is PEin (t) =

2t2(3t3−9t2+6t+2) (1−t)3

. The table of numbers of independent relativistic invariants of pure

  • rder k for small values k :

k 2 3 4 5 6 7 8 9 HEin 4 24 42 64 90 120 154 192

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein Factor Equation

Let (M, g) be a fixed Einstein manifold, and let Σg ⊂ M the set of singular points of g, (i.e. j3 (g) ∈ Σ3 ). Assume that Σg = M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein Factor Equation

Let (M, g) be a fixed Einstein manifold, and let Σg ⊂ M the set of singular points of g, (i.e. j3 (g) ∈ Σ3 ). Assume that Σg = M. Take space C2 with fixed coordinates (z1, z2) and consider the invariantization mapping: I : M → C2, where z1 = I1,g + √ −1I2,g, z2 = I3,g + √ −1I4,g.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein Factor Equation

Let (M, g) be a fixed Einstein manifold, and let Σg ⊂ M the set of singular points of g, (i.e. j3 (g) ∈ Σ3 ). Assume that Σg = M. Take space C2 with fixed coordinates (z1, z2) and consider the invariantization mapping: I : M → C2, where z1 = I1,g + √ −1I2,g, z2 = I3,g + √ −1I4,g. At regular points M Σg this mapping is a covering over a domain Dg ⊂ C2 : I : M Σg → Dg ⊂ C2.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein Factor Equation

The factor equation EEin is the following equation on a metric h on C2 : Gh = 0, TrC W2

h = z1,

TrC W3

h = z2.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein Factor Equation

The factor equation EEin is the following equation on a metric h on C2 : Gh = 0, TrC W2

h = z1,

TrC W3

h = z2.

Equivalence classes of Einstein metrics ⇐ ⇒ Solutions of system EEin.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein Factor Equation

The factor equation EEin is the following equation on a metric h on C2 : Gh = 0, TrC W2

h = z1,

TrC W3

h = z2.

Equivalence classes of Einstein metrics ⇐ ⇒ Solutions of system EEin. Remark on space-time problem.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein-Maxwell equation

Let M be an oriented 4-dimensional manifold, g be a Lorentzian metric and F be a differential 2-form on M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Einstein-Maxwell equation

Let M be an oriented 4-dimensional manifold, g be a Lorentzian metric and F be a differential 2-form on M. The Einstein-Maxwell equation: G = T , dF = 0, d ∗ F = 0, where G is the Einstein tensor, F is the Faraday tensor and ∗ is the Hodge operator.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 117

Einstein-Maxwell equation

Let M be an oriented 4-dimensional manifold, g be a Lorentzian metric and F be a differential 2-form on M. The Einstein-Maxwell equation: G = T , dF = 0, d ∗ F = 0, where G is the Einstein tensor, F is the Faraday tensor and ∗ is the Hodge operator. T is the energy-momentum tensor: Tij = 2k c4

  • −FikF k

j + 1

4gijFklF kl

  • ,

where k gravitational constant and c is the velocity of light.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 118

Einstein-Maxwell equation

Let τ(0,2) = S2T∗ ⊕ Λ2T∗ = T∗ ⊗ T∗ be the bundle of (0, 2)-tensors and let EM2 ⊂ J2τ(0,2) be the submanifold corresponding to Einstein-Maxwell equation.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 119

Einstein-Maxwell equation

Let τ(0,2) = S2T∗ ⊕ Λ2T∗ = T∗ ⊗ T∗ be the bundle of (0, 2)-tensors and let EM2 ⊂ J2τ(0,2) be the submanifold corresponding to Einstein-Maxwell equation. Denote by EMk = EM(k−2)

2

⊂ Jkτ(0,2) their prolongations.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 120

Electromagnetic Invariants

Note that Einstein-Maxwell equation is

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 121

Electromagnetic Invariants

Note that Einstein-Maxwell equation is

natural

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 122

Electromagnetic Invariants

Note that Einstein-Maxwell equation is

natural formally integrable

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 123

Electromagnetic Invariants

Note that Einstein-Maxwell equation is

natural formally integrable Fibres of the projections πk : EMk → M are irreducible algebraic manifolds and actions of the differential groups

  • n these fibres are algebraic.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 124

Electromagnetic Invariants

Note that Einstein-Maxwell equation is

natural formally integrable Fibres of the projections πk : EMk → M are irreducible algebraic manifolds and actions of the differential groups

  • n these fibres are algebraic.

A fibrewise rational function on the bundle πk : EMk → M we call electromagnetic invariant of order ≤ k if the function is invariant with respect to the prolonged action of the diffeomorphism group.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 125

Basic electromagnetic invariants

Let s = (g, F) ∈ τ(0,2). and let Ωg be the corresponding g unit volume form on M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 126

Basic electromagnetic invariants

Let s = (g, F) ∈ τ(0,2). and let Ωg be the corresponding g unit volume form on M. Then relations F ∧ F = I1 (s) Ωg, F ∧ ∗F = I2 (s) Ωg, define two electromagnetic invariants I1, I2 of order 0.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 127

Basic electromagnetic invariants

Let s = (g, F) ∈ τ(0,2). and let Ωg be the corresponding g unit volume form on M. Then relations F ∧ F = I1 (s) Ωg, F ∧ ∗F = I2 (s) Ωg, define two electromagnetic invariants I1, I2 of order 0. We say that point (ga, Fa) ∈ T(0,2)

a

, a ∈ M, is Rainich regular if (I1, I2) = 0 at this point.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 128

Basic electromagnetic invariants

Let s = (g, F) ∈ τ(0,2). and let Ωg be the corresponding g unit volume form on M. Then relations F ∧ F = I1 (s) Ωg, F ∧ ∗F = I2 (s) Ωg, define two electromagnetic invariants I1, I2 of order 0. We say that point (ga, Fa) ∈ T(0,2)

a

, a ∈ M, is Rainich regular if (I1, I2) = 0 at this point. At Rainich regular points one has splitting Ta = Ha ⊕ Ea

  • f the tangent space into the orthogonal sum of hyperbolic and

elliptic planes.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 129

Basic electromagnetic invariants

We say that a point in J1τ(0,2) is Rainich regular if its projection in τ(0,2) is regular and restrictions of the total differentials dI1 and dI2

  • n hyperbolic and elliptic planes are linear independent.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 130

Basic electromagnetic invariants

We say that a point in J1τ(0,2) is Rainich regular if its projection in τ(0,2) is regular and restrictions of the total differentials dI1 and dI2

  • n hyperbolic and elliptic planes are linear independent.

Denote by e∗

1, e∗ 2, e∗ 3, e∗ 4 the corresponding coframe.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 131

Basic electromagnetic invariants

We say that a point in J1τ(0,2) is Rainich regular if its projection in τ(0,2) is regular and restrictions of the total differentials dI1 and dI2

  • n hyperbolic and elliptic planes are linear independent.

Denote by e∗

1, e∗ 2, e∗ 3, e∗ 4 the corresponding coframe.

Remark that the dual frame defines invariant total derivations ∇1, ∇2, ∇3, ∇4 of order 1.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 132

Basic electromagnetic invariants

We say that a point in J1τ(0,2) is Rainich regular if its projection in τ(0,2) is regular and restrictions of the total differentials dI1 and dI2

  • n hyperbolic and elliptic planes are linear independent.

Denote by e∗

1, e∗ 2, e∗ 3, e∗ 4 the corresponding coframe.

Remark that the dual frame defines invariant total derivations ∇1, ∇2, ∇3, ∇4 of order 1. Let Gij and Fij the components of tensors g and F in this coframe. They are electromagnetic invariants of order 1.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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The field od electromagnetic invariants

Theorem

The field of relativistic electromagnetic invariants is generated by invariants: I1, I2 of order 0, invariants Gij , Fij of order 1 and invariant derivations ∇1, ∇2, ∇3, ∇4. This field separates Rainich regular orbits. The Hilbert function of the field of electromagnetic invariants is HEM (0) = 2, HEM (1) = 14, HEM (k) = 4k (k + 3) , for k ≥ 2.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 134

The field od electromagnetic invariants

Theorem

The field of relativistic electromagnetic invariants is generated by invariants: I1, I2 of order 0, invariants Gij , Fij of order 1 and invariant derivations ∇1, ∇2, ∇3, ∇4. This field separates Rainich regular orbits. The Hilbert function of the field of electromagnetic invariants is HEM (0) = 2, HEM (1) = 14, HEM (k) = 4k (k + 3) , for k ≥ 2. The Poincare function is PEM (t) = 2

  • 3t4 − 4t3 + 2t2 + 4t + 1
  • (1 − t)3

.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 135

Einstein-Maxwell factor equations

Let J = {J1, J2., J3, J4 } be for electromagnetic invariants. By regular jet we undersand jets where

  • dJ1 ∧ ... ∧

dJ4 = 0.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 136

Einstein-Maxwell factor equations

Let J = {J1, J2., J3, J4 } be for electromagnetic invariants. By regular jet we undersand jets where

  • dJ1 ∧ ... ∧

dJ4 = 0. Denote by ΣJ ⊂ Jkτ(0,2) the set of J-singular jets.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 137

Einstein-Maxwell factor equations

Let J = {J1, J2., J3, J4 } be for electromagnetic invariants. By regular jet we undersand jets where

  • dJ1 ∧ ... ∧

dJ4 = 0. Denote by ΣJ ⊂ Jkτ(0,2) the set of J-singular jets. Let (M, g, F) be a solution ofEinstein- Maxwell and let Σg,F ⊂ M be the set of J-singular points of s = (g, F). Assume that Σg,F = M.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 138

Einstein-Maxwell factor equations

Let J = {J1, J2., J3, J4 } be for electromagnetic invariants. By regular jet we undersand jets where

  • dJ1 ∧ ... ∧

dJ4 = 0. Denote by ΣJ ⊂ Jkτ(0,2) the set of J-singular jets. Let (M, g, F) be a solution ofEinstein- Maxwell and let Σg,F ⊂ M be the set of J-singular points of s = (g, F). Assume that Σg,F = M. Take space R4 with fixed coordinates (x1, x2, x3, x4) and consider the invariantization mapping: I : M → R4, where x1 = J1 (g, F) , x2 = J2 (g, F) , x3 = J3 (g, F) , x4 = J4 (g, F) .

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 139

Einstein-Maxwell factor equations

Define as above invariants Gij and Fij g = ∑

i,j

Gij dIi · dIj and F = ∑

i,j

Fij dIi ∧ dIj.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 140

Einstein-Maxwell factor equations

Define as above invariants Gij and Fij g = ∑

i,j

Gij dIi · dIj and F = ∑

i,j

Fij dIi ∧ dIj. At regular points M Σg,F this mapping is a covering over a domain Dg,F ⊂ R4 : I : M Σg,F → Dg,F ⊂ R4.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 141

Einstein-Maxwell factor equations

Define as above invariants Gij and Fij g = ∑

i,j

Gij dIi · dIj and F = ∑

i,j

Fij dIi ∧ dIj. At regular points M Σg,F this mapping is a covering over a domain Dg,F ⊂ R4 : I : M Σg,F → Dg,F ⊂ R4. The factor equation EEM is the following equation on a metric h and differenatial 2-form F on R4 : Gh = Th,F , dF = 0, d ∗ F = 0, J1 (g, F) = x1, J2 (g, F) = x2, J3 (g, F) = x3, J4 (g, F) = x4.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 142

Einstein-Maxwell factor equations

Define as above invariants Gij and Fij g = ∑

i,j

Gij dIi · dIj and F = ∑

i,j

Fij dIi ∧ dIj. At regular points M Σg,F this mapping is a covering over a domain Dg,F ⊂ R4 : I : M Σg,F → Dg,F ⊂ R4. The factor equation EEM is the following equation on a metric h and differenatial 2-form F on R4 : Gh = Th,F , dF = 0, d ∗ F = 0, J1 (g, F) = x1, J2 (g, F) = x2, J3 (g, F) = x3, J4 (g, F) = x4. Equivalence classes of Einstein - Maxwell solutions ⇐ ⇒ Solutions of PDEs

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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SLIDE 143

Einstein-Maxwell factor equations

Define as above invariants Gij and Fij g = ∑

i,j

Gij dIi · dIj and F = ∑

i,j

Fij dIi ∧ dIj. At regular points M Σg,F this mapping is a covering over a domain Dg,F ⊂ R4 : I : M Σg,F → Dg,F ⊂ R4. The factor equation EEM is the following equation on a metric h and differenatial 2-form F on R4 : Gh = Th,F , dF = 0, d ∗ F = 0, J1 (g, F) = x1, J2 (g, F) = x2, J3 (g, F) = x3, J4 (g, F) = x4. Equivalence classes of Einstein - Maxwell solutions ⇐ ⇒ Solutions of PDEs Remark on space-time problem.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Tables of Invariants

The tables of numbers of independent metric, relativistic and electromagnetic invariants of pure order k for small values k : k 1 2 3 4 5 6 7 Metric 14 60 126 224 360 540 Einstein 4 24 42 64 90 120 Einstein-Maxwell 2 14 40 72 112 160 216 280

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39

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Thank you for your attention.

Lychagin & Yumaguzhin (University of Tromso) Differential Invariants Workshop on “Infinite-dimensional Riemannia / 39