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Introduction Outline Geometry of T T Intrinsic - - PowerPoint PPT Presentation

ArXiv:1203.0493 Gil Cavalcanti Utrecht University Poisson Geometry in Mathematics and Physics Utrecht 2012 Introduction Outline Geometry of T T Intrinsic torsion Hodge theory Deformations


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ArXiv:1203.0493

Gil Cavalcanti

Utrecht University

Poisson Geometry in Mathematics and Physics Utrecht 2012

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

Introduction — SKT structures

K¨ ahler structure with torsion: Hermitian structure (g, I) with a connection ∇ with Tor(∇) = H ∈ Ω3(M) such that ∇g = ∇I = 0. K¨ ahler structure with strong torsion (SKT): dH = 0. SKT structure: Hermitian structure (g, I) such that ddcω = 0. H = dcω.

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

Examples

K¨ ahler manifolds; Compact even dimensional Lie groups; Compact complex surfaces (Gauduchon); Instanton moduli space over compact complex surfaces; Instanton moduli space over Hermitian manifolds with Gauduchon metrics; Classification on 6-nilmanifolds;

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

K¨ ahler vs. SKT

K¨ ahler SKT Decomposition of cohomology

  • Hodge theory
  • Fr¨
  • licher spectral seq. degenerates
  • Formality
  • Unobstructed deformations
  • Fino, Parton and Salamon. Families of strong KT structures in

six dimensions. Comment. Math. Helv. 2004. (arXiv:math/0209259)

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

K¨ ahler vs. SKT

K¨ ahler SKT Decomposition of cohomology

Hodge theory

Fr¨

  • licher spectral seq. degenerates

Formality

Unobstructed deformations

Fino, Parton and Salamon. Families of strong KT structures in six dimensions. Comment. Math. Helv. 2004. (arXiv:math/0209259)

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

K¨ ahler vs. SKT

K¨ ahler SKT Decomposition of cohomology

Hodge theory

Fr¨

  • licher spectral seq. degenerates

Formality

Unobstructed deformations ✪ ✪ Fino, Parton and Salamon. Families of strong KT structures in six dimensions. Comment. Math. Helv. 2004. (arXiv:math/0209259)

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

K¨ ahler vs. SKT

K¨ ahler SKT Decomposition of cohomology

  • Hodge theory
  • Fr¨
  • licher spectral seq. degenerates
  • Formality

Unobstructed deformations ✪ ✪

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

K¨ ahler vs. GK vs. SKT

K¨ ahler GK SKT Decomposition of cohomology

  • Hodge theory
  • Fr¨
  • licher spectral seq. degenerates
  • Formality

✪ Unobstructed deformations ✪ ✪ ✪

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

Main insights

SKT structures are also generalized structures ` a la Hitchin. Description of intrinsic torsion of generalized almost Hermitian structures.

SKT geometry Cavalcanti

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Introduction Outline Geometry of T ⊕ T∗ Intrinsic torsion Hodge theory Deformations

Outline of Topics

1

Geometry of T ⊕ T∗

2

Nijenhuis tensor and intrinsic torsion

3

Hodge theory

4

Deformations

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Natural pairing

Natural pairing X + ξ, Y + η = 1 2(η(X) + ξ(Y)). Action of T ⊕ T∗ on ∧•T∗: (X + ξ) · ϕ = ιXϕ + ξ ∧ ϕ. Extends to an action of Clif(T ⊕ T∗) on ∧•T∗: v · (v · ϕ) = v, vϕ. ∧•T∗ ❀ spinors. Spin invariant pairing: (·, ·)Ch : ∧•T∗ ⊗ ∧•T∗ − → ∧topT∗.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Generalized metric

A generalized metric is an orthogonal, self-adjoint bundle isomorphism: G : T ⊕ T∗ − → T ⊕ T∗; such that Gv, v > 0. G−1 = Gt = G ⇒ G2 = Id. G is determined by its +1-eigenspace V+.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Generalized Hodge star

Generalized metric + orientation ⇒ generalized Hodge star ⋆ (ϕ, ⋆ϕ)Ch > 0. ⋆2 = (−1)

m(m−1) 2

. SD forms = −i

m(m−1) 2

  • eigenspace;

ASD forms = i

m(m−1) 2

  • eigenspace;

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Gen. almost complex structure

Generalized almost complex structure: J : T ⊕ T∗ − → T ⊕ T∗; J 2 = −Id; J is orthogonal. J ⇔ L ⊂ (T ⊕ T∗) ⊗ C, maximal isotropic L ∩ L = {0}. J t = J −1 = −J ⇒ J ∈ ∧2(T ⊕ T∗) = spin(T ⊕ T∗). J splits ∧•T∗ into its ik-eigenspaces: ∧•T∗

CM = ⊕−n≤k≤nUk.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Gen. almost Hermitian str.

Generalized almost Hermitian structure: (G, J 1) GJ 1 = J 1G. J 2 = GJ 1 is a gcs and J 2J 1 = J 1J 2. (T ⊕ T∗) ⊗ C = V1,0

+ ⊕ V0,1 + ⊕ V1,0 − ⊕ V0,1 − .

∧•T∗

CM = ⊕p,qUp J 1 ∩ Uq J 2.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Gen. almost Hermitian str.

U0,3 U−1,2 U1,2 U−2,1 U0,1 U2,1 U−3,0 U−1,0 U1,0 U3,0 U−2,−1 U0,−1 U2,−1 U−1,−2 U1,−2 U0,−3 Spaces Up,q on a 6-dimensional generalized almost Hermitian structure.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Gen. almost Hermitian str.

Generalized almost Hermitian structure: (G, J 1) GJ 1 = J 1G. J 2 = GJ 1 is a gcs and J 2J 1 = J 1J 2. (T ⊕ T∗) ⊗ C = V1,0

+ ⊕ V0,1 + ⊕ V1,0 − ⊕ V0,1 − .

∧•T∗

CM = ⊕p,qUp J 1 ∩ Uq J 2.

⋆ = −e

πJ 1 2 e πJ 2 2

⋆|Up,q = −ip+q.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Gen. almost Hermitian str.

U0,3 U−1,2 U1,2 U−2,1 U0,1 U2,1 U−3,0 U−1,0 U1,0 U3,0 U−2,−1 U0,−1 U2,−1 U−1,−2 U1,−2 U0,−3 SD and ASD forms on a 6-dimensional generalized almost Hermitian structure.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Gen. almost Hermitian str.

U0,3 U−1,2 U1,2 U−2,1 U0,1 U2,1 U−3,0 U−1,0 U1,0 U3,0 U−2,−1 U0,−1 U2,−1 U−1,−2 U1,−2 U0,−3 SD and ASD forms on a 6-dimensional generalized almost Hermitian structure.

SKT geometry Cavalcanti

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Geometry of T ⊕ T∗ — Courant bracket

Courant bracket [ [X + ξ, Y + η] ]H = [X, Y] + LXη − ιYdξ − ιYιXH. [ [v1, v2] ]H · ϕ = {{v1, dH}, v2} · ϕ.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Given a gacs J , define N : Γ(L) × Γ(L) × Γ(L) − → Ω0(M; C) N(v1, v2, v3) = −2[ [v1, v2] ], v3. J is integrable iff N ≡ 0. N ∈ Γ(∧3L). Uk−3 Uk−2 Uk−1 Uk

N

  • ∂J 1
  • ∂J 1

N

  • Uk+1

Uk+2 Uk+3

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Up−3,q+3 Up−1,q+3 Up+1,q+3 Up+3,q+3 Up−3,q+1 Up−1,q+1 Up+1,q+1 Up+3,q+1 Up,q

N−

  • N1
  • N4
  • δ−
  • N3
  • δ+
  • N+
  • N2
  • N1
  • N−
  • δ−

N4 δ+

  • N3
  • N2
  • N+
  • Up−3,q−1

Up−1,q−1 Up+1,q−1 Up+3,q−1 Up−3,q−3 Up−1,q−3 Up+1,q−3 Up+3,q−3 Components of dH for a generalized almost Hermitian structure.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Up−1,q+3 Up+1,q+3 Up−1,q+1 Up+1,q+1 Up,q

N1

  • δ−
  • δ+
  • N2
  • N1
  • δ−

δ+

  • N2
  • Up−3,q−1

Up−1,q−1 Up−1,q−3 Up+1,q−3 Components of dH for a generalized Hermitian structure.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Up−1,q+1 Up+1,q+1 Up,q

δ−

  • δ+
  • δ−
  • δ+
  • Up−1,q−1

Up+1,q−1 Components of dH for a generalized K¨ ahler.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Definition

The tensors Nα, α = 1, 2, 3, 4 and ± are the components of the intrinsic torsion of a U(n) × U(n) structure.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Proposition (Gualtieri 04/Cavalcanti 06)

A (positive) SKT structure is a generalized metric G and complex structure I+ on V+ such that [ [Γ(V1,0

+ ), Γ(V1,0 + )]

] ⊂ Γ(V1,0

+ ).

Similarly, a (negative) SKT structure is a complex structure I− on V− such that [ [Γ(V1,0

− ), Γ(V1,0 − )]

] ⊂ Γ(V1,0

− ).

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Up−3,q+3 Up−1,q+3 Up−3,q+1 Up−1,q+1 Up+1,q+1 Up,q

N−

  • N1
  • N4
  • δ−
  • δ+
  • δ+
  • N1
  • N−
  • δ−

N4

Up−1,q−1 Up+1,q−1 Up+3,q−1 Up+1,q−3 Up+3,q−3

Components of dH for a (positive) SKT structure.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Up+1,q+3 Up+3,q+3 Up−1,q+1 Up+1,q+1 Up+3,q+1 Up,q

δ−

  • N3
  • δ+
  • N+
  • N2
  • δ−

δ+

  • N3
  • N2
  • N+
  • Up−3,q−1

Up−1,q−1 Up+1,q−1 Up−3,q−3 Up−1,q−3

Components of dH for a (negative) SKT structure.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Graphic proof of Gualtieri’s theorem

Theorem (Gualtieri 04)

A generalized K¨ ahler structure is equivalent to a pair of positive and negative SKT structures.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Up−3,q+3 Up−1,q+3 Up−3,q+1 Up−1,q+1 Up+1,q+1 Up,q

N−

  • N1
  • N4
  • δ−
  • δ+
  • δ+
  • N1
  • N−
  • δ−

N4

Up−1,q−1 Up+1,q−1 Up+3,q−1 Up+1,q−3 Up+3,q−3

Components of dH for a (positive) SKT structure.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Let Wk = ⊕p+q=kUp,q and Wk = Γ(Wk).

Proposition

A generalized almost Hermitian structure is an SKT structure if and

  • nly if

dH : Wk − → Wk−2 ⊕ Wk ⊕ Wk+2. δN

+ : Wk −

→ Wk+2; δN

+ : Wk −

→ Wk−2; / δ− : Wk − → Wk.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Up−1,q+3 Up−1,q+1 Up+1,q+1 Up,q

N

  • δ−
  • δ+
  • N
  • δ−

δ+

  • Up−1,q−1

Up+1,q−1 Up+1,q−3 Components of dH for a gen. cplx. extension of an SKT structure.

SKT geometry Cavalcanti

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Nijenhuis tensor and intrinsic torsion

Proposition

A generalized Hermitian structure is an SKT structure if and only if

dH : Up,q − → U p−1,q+3 ⊕ Up−1,q+1 ⊕ Up−1,q−1 ⊕ Up+1,q+1 ⊕ Up+1,q−1 ⊕ Up+1,q−3.

SKT geometry Cavalcanti

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Hodge theory

In (Mm, G, or) we define / D+ = 1 2(dH + (−1)m+1(dH)∗) / D− = 1 2(dH + (−1)m(dH)∗) Then: / D+ : Ω•

±(M) −

→ Ω•

∓(M)

/ D− : Ω•

±(M) −

→ Ω•

±(M)

(−1)m+1 / D2

+ = (−1)m /

D2

− = 1 4△dH.

SKT geometry Cavalcanti

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Hodge theory

Theorem

In a compact SKT manifold, the dH-cohomology splits according to the Wk decomposition of forms. Remark: The theorem also holds for parallel (almost) Hermitian structures with closed, skew torsion.

SKT geometry Cavalcanti

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Hodge theory

Proof:

Up−3,q+3 Up−1,q+3 Up−3,q+1 Up−1,q+1 Up+1,q+1 Up,q

N−

  • N1
  • N4
  • δ−
  • δ+
  • δ+
  • N1
  • N−
  • δ−

N4

Up−1,q−1 Up+1,q−1 Up+3,q−1 Up+1,q−3 Up+3,q−3 Components of dH for a (positive) SKT structure.

SKT geometry Cavalcanti

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Hodge theory

Proof:

Up−3,q+3 Up−1,q+3 Up−3,q+1 Up−1,q+1 Up+1,q+1 Up,q

N−

  • N1
  • N4
  • δ−
  • δ+
  • δ+
  • N1
  • N−
  • δ−

N4

Up−1,q−1 Up+1,q−1 Up+3,q−1 Up+1,q−3 Up+3,q−3 Components of dH for a (positive) SKT structure.

SKT geometry Cavalcanti

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Hodge theory

Up−3,q+3 Up−1,q+1 Up,q

N−

  • δ−
  • N−
  • δ−

Up+1,q−1 Up+3,q−3 Components of / D− for a (positive) SKT structure.

SKT geometry Cavalcanti

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Hodge theory

Proof: (Parallel case)

Up−3,q+3 Up−1,q+3 Up+3,q+3 Up−3,q+1 Up−1,q+1 Up+1,q+1 Up,q

N−

  • N1
  • N4
  • δ−
  • δ+
  • N+
  • N+
  • δ+
  • N1
  • N−
  • δ−

N4

Up−1,q−1 Up+1,q−1 Up+3,q−1 Up−3,q−3 Up+1,q−3 Up+3,q−3 Components of dH for a parallel positive Hermitian structure.

SKT geometry Cavalcanti

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Hodge theory

Corollary (Parallel bi-Hermitian structures)

Let (M, g) be a compact Riemannian manifold and H ∈ Ω3

cl(M). If

the metric connections with torsion ±H have holonomy in U(n) the dH-cohomology splits according to the Up,q decomposition of forms.

SKT geometry Cavalcanti

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Hodge theory

Proof:

Up−3,q+3 Up+3,q+3 Up−1,q+1 Up+1,q+1 Up,q

N−

  • δ−
  • δ+
  • N+
  • N+
  • δ+
  • N−
  • δ−

Up−1,q−1 Up+1,q−1 Up−3,q−3 Up+3,q−3 Components of dH for a parallel bi-Hermitian structure.

SKT geometry Cavalcanti

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Hodge theory

Theorem

Let (M, g) be a compact Riemannian manifold and H ∈ Ω3

cl(M). If

the metric connections with torsion ±H have holonomy in G± and g± ⊂ ∧2V± are the Lie algebras of G±, the dH-cohomology splits according to the irreducible representation of g+ × g− ⊂ ∧2V+ × ∧2V− ⊂ ∧2(T ⊕ T∗).

SKT geometry Cavalcanti

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K¨ ahler vs. GK vs. SKT vs. reduced holonomy

K¨ ahler GK SKT

  • red. hol.

Decomposition of cohomology

  • Hodge theory

Fr¨

  • licher spectral seq. deg.

Formality

✪ ?

  • Unobstr. deformations

✪ ✪ ✪ ?

SKT geometry Cavalcanti

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Hodge theory

Theorem

In a compact SKT manifold we have △δN

+ = △δN + = 1

4△dH. Proof: Integration by parts & ⋆|Up,q = −ip+q implies that (δN

+)∗ = −δN +.

/ D+ = δN

+ + δN + = δN + − δN∗ +

1 4△dH = − / D2

+ = −(δN + − δN∗ + )2 = △δN

+. SKT geometry Cavalcanti

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Hodge theory

Theorem

In a compact SKT manifold (M, g, I), the ∂ + i∂ω cohomology is isomorphic to the dH-cohomology. Proof: The automorphism of ∧•T∗

CM

Ψ : Ω•(M; C) − → Ω•(M; C) Ψ(ϕ) = eiωe

iω−1 2 ϕ

satisfies Ψ∂ = δ+ and Ψ(2i∂ω) = N

SKT geometry Cavalcanti

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Hodge theory

Corollary

In a compact SKT manifold (M, g, I), the spectral sequence correspoding to the decomposition dH = (∂ + i∂ω) + (∂ − i∂ω) degenerates at the second page.

SKT geometry Cavalcanti

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Deformations

Deformations are given by the action of SO(T ⊕ T∗). Small deformations are given by the action of (exponential

  • f) elements in the Lie algebra

Γ(spin(T ⊕ T∗)). It is natural to consider the question of deformations in the context of stability.

SKT geometry Cavalcanti

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Deformations

Question

Which deformations of J 1 can be completed with a deformation of G (or J 2) so that (G, J 1) is a positive SKT structure?

SKT geometry Cavalcanti

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Deformations

Deformations of J 1 are determined by eα, α ∈ Γ(∧2LJ 1) And lead to consider the operator e−αdHeα

linearization

{dH, α}.

with respect to the Up,q splitting. Here, the natural differential operators are ∂± = {δ±, ·}; ∂± = {δ±, ·} N = {N, ·}

SKT geometry Cavalcanti

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Deformations

Linear action of α is given by Un−2,2

δ−

  • δ+
  • Un−1,1

Un−2,0

δ−

  • δ+
  • Un,0

α−

  • α±
  • α+
  • Un−1,−1

Un−2,−2

δ−

  • δ+
  • SKT geometry

Cavalcanti

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Deformations

For J 2 U−2,n

N

  • U0,n

α+

  • α−
  • α±
  • U−1,n−1

U1,n−1 U−2,n−2

δ+

  • δ−
  • U0,n−2

U2,n−2 U−1,n−3 U1,n−3

SKT geometry Cavalcanti

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Deformations

Can change α by an element β ∈ Γ(V0,1

+ ⊗ V1,0 − ):

U−2,n

N

  • U0,n

β

  • α+
  • α−
  • α±
  • U−1,n−1

U1,n−1 U−2,n−2

δ+

  • δ−
  • U0,n−2

δ+

  • U2,n−2

U−1,n−3 U1,n−3 Need: ∂+β = −(∂−α+ + Nα±)

SKT geometry Cavalcanti

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Deformations

Theorem

The obstructions to deforming an SKT structure lie in H2,1

∂+(M). If

this space vanishes, any deformation of J 1 can be completed to a deformation of the SKT structure.

Theorem

If α = α− ∈ Γ(∧2V0,1

− ), then the deformed structure is still SKT

Corollary

If (M, I, ω) is K¨ ahler, deformations of the symplectic form turn it into an SKT structure.

SKT geometry Cavalcanti