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The E 11 origin of gauged maximal supergravities Fabio Riccioni - - PowerPoint PPT Presentation

The E 11 origin of gauged maximal supergravities Fabio Riccioni Kings College London based on work with Peter West arXiv:0705.0752 The E 11 origin ofgauged maximal supergravities p. 1/3 Introduction Massless maximal supergravities all


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SLIDE 1

The E11 origin of gauged maximal supergravities

Fabio Riccioni

King’s College London based on work with Peter West arXiv:0705.0752

The E11 origin ofgauged maximal supergravities – p. 1/3

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Introduction

Massless maximal supergravities all arise from dimensional reduction of 11-dimensional and IIB supergravities.

The E11 origin ofgauged maximal supergravities – p. 2/3

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Introduction

Massless maximal supergravities all arise from dimensional reduction of 11-dimensional and IIB supergravities. In any dimension, the theory is unique, and has a global symmetry G.

The E11 origin ofgauged maximal supergravities – p. 2/3

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Introduction

Massless maximal supergravities all arise from dimensional reduction of 11-dimensional and IIB supergravities. In any dimension, the theory is unique, and has a global symmetry G. The scalars parametrise the manifold G/H, where H is the maximal compact subgroup of G.

The E11 origin ofgauged maximal supergravities – p. 2/3

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Introduction

D G 10A

R+

10B

SL(2, R)

9

SL(2, R) × R+

8

SL(3, R) × SL(2, R)

7

SL(5, R)

6

SO(5, 5)

5

E6(+6)

4

E7(+7)

3

E8(+8)

The E11 origin ofgauged maximal supergravities – p. 3/3

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Introduction

Gauging: some of the vectors group to form the adjoint of a subgroup of G

The E11 origin ofgauged maximal supergravities – p. 4/3

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Introduction

Gauging: some of the vectors group to form the adjoint of a subgroup of G Correspondingly, a potential for the scalars arises, which contains mass parameters

→ Massive theories

The E11 origin ofgauged maximal supergravities – p. 4/3

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Introduction

Gauging: some of the vectors group to form the adjoint of a subgroup of G Correspondingly, a potential for the scalars arises, which contains mass parameters

→ Massive theories

Although some of these theories can be seen as Scherk-Schwarz compactifications, or as reductions with fluxes turned on, in general a complete understanding of such theories in terms of higher dimensional ones is lacking

The E11 origin ofgauged maximal supergravities – p. 4/3

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Introduction

Simplest example: Romans’ massive IIA (not actually a gauged theory)

The E11 origin ofgauged maximal supergravities – p. 5/3

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Introduction

Simplest example: Romans’ massive IIA (not actually a gauged theory) This theory describes the bulk of IIA in the presence of

D8-branes

The E11 origin ofgauged maximal supergravities – p. 5/3

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SLIDE 11

Introduction

Simplest example: Romans’ massive IIA (not actually a gauged theory) This theory describes the bulk of IIA in the presence of

D8-branes

This theory does not arise from 11-dimensional supergravity

The E11 origin ofgauged maximal supergravities – p. 5/3

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Introduction

Simplest example: Romans’ massive IIA (not actually a gauged theory) This theory describes the bulk of IIA in the presence of

D8-branes

This theory does not arise from 11-dimensional supergravity

E11 provides an 11-dimensional origin of all maximal

supergravities (and much more...)

The E11 origin ofgauged maximal supergravities – p. 5/3

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Plan

More about supergravities

The E11 origin ofgauged maximal supergravities – p. 6/3

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Plan

More about supergravities An introduction to E11

The E11 origin ofgauged maximal supergravities – p. 6/3

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Plan

More about supergravities An introduction to E11 The fields of E11

The E11 origin ofgauged maximal supergravities – p. 6/3

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Plan

More about supergravities An introduction to E11 The fields of E11

E11 and dimensional reduction

The E11 origin ofgauged maximal supergravities – p. 6/3

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Plan

More about supergravities An introduction to E11 The fields of E11

E11 and dimensional reduction

Some dynamics

The E11 origin ofgauged maximal supergravities – p. 6/3

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Plan

More about supergravities An introduction to E11 The fields of E11

E11 and dimensional reduction

Some dynamics Conclusions

The E11 origin ofgauged maximal supergravities – p. 6/3

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More about supergravities

In a series of papers, all the gauged maximal supergravities in D = 7, 6, . . . , 3 have been classified

de Wit, Samtleben and Trigiante, hep-th/0212239, hep-th/0412173, hep-th/0507289 Samtleben and Weidner, hep-th/0506237 Nicolai and Samtleben, hep-th/0010076

The E11 origin ofgauged maximal supergravities – p. 7/3

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SLIDE 20

More about supergravities

In a series of papers, all the gauged maximal supergravities in D = 7, 6, . . . , 3 have been classified

de Wit, Samtleben and Trigiante, hep-th/0212239, hep-th/0412173, hep-th/0507289 Samtleben and Weidner, hep-th/0506237 Nicolai and Samtleben, hep-th/0010076

Gauging:

Dµ = ∂µ − AM

µ ΘM αtα

The embedding tensor Θ belongs to a reducible representation of G

The E11 origin ofgauged maximal supergravities – p. 7/3

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SLIDE 21

More about supergravities

In a series of papers, all the gauged maximal supergravities in D = 7, 6, . . . , 3 have been classified

de Wit, Samtleben and Trigiante, hep-th/0212239, hep-th/0412173, hep-th/0507289 Samtleben and Weidner, hep-th/0506237 Nicolai and Samtleben, hep-th/0010076

Gauging:

Dµ = ∂µ − AM

µ ΘM αtα

The embedding tensor Θ belongs to a reducible representation of G The fact that the gauge symmetry is a Lie group, as well as supersymmetry, pose constraints on Θ

The E11 origin ofgauged maximal supergravities – p. 7/3

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More about supergravities

Example: D = 5

The E11 origin ofgauged maximal supergravities – p. 8/3

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More about supergravities

Example: D = 5

Aµ,M belongs to the 27 of E6

The E11 origin ofgauged maximal supergravities – p. 8/3

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More about supergravities

Example: D = 5

Aµ,M belongs to the 27 of E6

The embedding tensor belongs to

27 ⊗ 78 = 27 ⊕ 351 ⊕ 1728

The Jacobi identities and the constraints from supersymmetry restrict the embedding tensor to be in the

351

The E11 origin ofgauged maximal supergravities – p. 8/3

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More about supergravities

Field strength:

∂µAν,M − 1 2Aµ,NΘN α(tα)M PAν,P − 2ZMNAµνaN

where

ZMN = Z[MN] ZMNΘN

α = 0

The E11 origin ofgauged maximal supergravities – p. 9/3

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More about supergravities

Field strength:

∂µAν,M − 1 2Aµ,NΘN α(tα)M PAν,P − 2ZMNAµνaN

where

ZMN = Z[MN] ZMNΘN

α = 0

Gauge invariance:

δAa,M = 4ZMNΛaN

The E11 origin ofgauged maximal supergravities – p. 9/3

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SLIDE 27

More about supergravities

Field strength:

∂µAν,M − 1 2Aµ,NΘN α(tα)M PAν,P − 2ZMNAµνaN

where

ZMN = Z[MN] ZMNΘN

α = 0

Gauge invariance:

δAa,M = 4ZMNΛaN

The vectors that do not belong to the adjoint of the gauge group are gauged away, i.e. dualised to 2-forms. The 2-forms are massive and satisfy massive self-duality conditions

The E11 origin ofgauged maximal supergravities – p. 9/3

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More about supergravities

This result is more general: some dualisations are needed in order to determine the most general embedding tensor. Simple examples: D = 4 and D = 3

The E11 origin ofgauged maximal supergravities – p. 10/3

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More about supergravities

This result is more general: some dualisations are needed in order to determine the most general embedding tensor. Simple examples: D = 4 and D = 3 In D = 9 all the gauged supergravities have been classified via a case-by-case analysis

Bergshoeff, de Wit, Gran, Linares, Roest, hep-th/0209205

The E11 origin ofgauged maximal supergravities – p. 10/3

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More about supergravities

D G Masses 9

SL(2, R) × R+ 2 ⊕ 3

8

SL(3, R) × SL(2, R)

? 7

SL(5, R) 15 ⊕ 40

6

SO(5, 5) 144

5

E6(+6) 351

4

E7(+7) 912

3

E8(+8) 1 ⊕ 3875

The E11 origin ofgauged maximal supergravities – p. 11/3

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SLIDE 31

More about supergravities

Supersymmetry algebra of IIB: democratic formulation. All the fields appear together with their magnetic duals

Bergshoeff, de Roo, Kerstan, F .R., hep-th/0506013

The E11 origin ofgauged maximal supergravities – p. 12/3

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More about supergravities

Supersymmetry algebra of IIB: democratic formulation. All the fields appear together with their magnetic duals

Bergshoeff, de Roo, Kerstan, F .R., hep-th/0506013

The forms one gets are

2

A4 Aα

6

A(αβ)

8

A(αβγ)

10

10

The E11 origin ofgauged maximal supergravities – p. 12/3

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More about supergravities

Supersymmetry algebra of IIB: democratic formulation. All the fields appear together with their magnetic duals

Bergshoeff, de Roo, Kerstan, F .R., hep-th/0506013

The forms one gets are

2

A4 Aα

6

A(αβ)

8

A(αβγ)

10

10

The 9-branes belong to a non-linear doublet out of the quadruplet

Bergshoeff, de Roo, Kerstan, Ortin, F .R., hep-th/0601128

This leads to an SL(2, R)-invariant formulation of brane effective actions

Bergshoeff, de Roo, Kerstan, Ortin, F .R., hep-th/0611036

The E11 origin ofgauged maximal supergravities – p. 12/3

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More about supergravities

Same analysis for IIA

Bergshoeff, Kallosh, Ortin, Roest, Van Proeyen, hep-th/0103233 Bergshoeff, de Roo, Kerstan, Ortin, F .R., hep-th/0602280

The E11 origin ofgauged maximal supergravities – p. 13/3

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More about supergravities

Same analysis for IIA

Bergshoeff, Kallosh, Ortin, Roest, Van Proeyen, hep-th/0103233 Bergshoeff, de Roo, Kerstan, Ortin, F .R., hep-th/0602280

The algebra closes among the rest on a 9-form (field strength dual to Romans cosmological constant) and two 10-forms

The E11 origin ofgauged maximal supergravities – p. 13/3

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SLIDE 36

More about supergravities

Same analysis for IIA

Bergshoeff, Kallosh, Ortin, Roest, Van Proeyen, hep-th/0103233 Bergshoeff, de Roo, Kerstan, Ortin, F .R., hep-th/0602280

The algebra closes among the rest on a 9-form (field strength dual to Romans cosmological constant) and two 10-forms The algebra describes both massless and massive IIA If m = 0 the algebra does not arise from 11-dimensions

The E11 origin ofgauged maximal supergravities – p. 13/3

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More about supergravities

Same analysis for IIA

Bergshoeff, Kallosh, Ortin, Roest, Van Proeyen, hep-th/0103233 Bergshoeff, de Roo, Kerstan, Ortin, F .R., hep-th/0602280

The algebra closes among the rest on a 9-form (field strength dual to Romans cosmological constant) and two 10-forms The algebra describes both massless and massive IIA If m = 0 the algebra does not arise from 11-dimensions The D8-branes are electrically charged with respect to the 9-form

The E11 origin ofgauged maximal supergravities – p. 13/3

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An introduction to E11

Starting point: gravity as a non-linear realisation

Borisov, Ogievetsky, 1974

g = exp(xaPa) exp(habKab)

with

[Kab, Kcd] = δc

bKad − δa dKcb

[Kab, Pc] = δa

c Pb

Gravity is formulated as the non-linear realisation of the closure of this group with the conformal group

The E11 origin ofgauged maximal supergravities – p. 14/3

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SLIDE 39

An introduction to E11

Starting point: gravity as a non-linear realisation

Borisov, Ogievetsky, 1974

g = exp(xaPa) exp(habKab)

with

[Kab, Kcd] = δc

bKad − δa dKcb

[Kab, Pc] = δa

c Pb

Gravity is formulated as the non-linear realisation of the closure of this group with the conformal group The theory is invariant under

g → g0gh−1

The E11 origin ofgauged maximal supergravities – p. 14/3

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SLIDE 40

An introduction to E11

Maurer-Cartan form:

V = g−1dg − ω ω: spin connection. It transforms as ω → hωh−1 + hdh−1

As a result, V transforms as

V → hVh−1

The E11 origin ofgauged maximal supergravities – p. 15/3

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An introduction to E11

Maurer-Cartan form:

V = g−1dg − ω ω: spin connection. It transforms as ω → hωh−1 + hdh−1

As a result, V transforms as

V → hVh−1

One gets

V = dxµ(eµaPa + ΩµabKab)

The E11 origin ofgauged maximal supergravities – p. 15/3

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An introduction to E11

Similar analysis for the bosonic sector of 11-dimensional supergravity:

[Rabc, Rdef] = Rabcdef

group element:

g = exp(xaPa) exp(habKab) exp(AabcRabc + AabcdefRabcdef)

The E11 origin ofgauged maximal supergravities – p. 16/3

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An introduction to E11

Similar analysis for the bosonic sector of 11-dimensional supergravity:

[Rabc, Rdef] = Rabcdef

group element:

g = exp(xaPa) exp(habKab) exp(AabcRabc + AabcdefRabcdef)

Field equations: duality relations

West, hep-th/0005270

The E11 origin ofgauged maximal supergravities – p. 16/3

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An introduction to E11

Similar analysis for the bosonic sector of 11-dimensional supergravity:

[Rabc, Rdef] = Rabcdef

group element:

g = exp(xaPa) exp(habKab) exp(AabcRabc + AabcdefRabcdef)

Field equations: duality relations

West, hep-th/0005270

E11 is the smallest Kac-Moody group that contains this

group

West, hep-th/0104081

The E11 origin ofgauged maximal supergravities – p. 16/3

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An introduction to E11

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

1 2 3 4 5 6 7 8 9 10 11

The E11 origin ofgauged maximal supergravities – p. 17/3

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An introduction to E11

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

1 2 3 4 5 6 7 8 9 10 11

Cartan matrix with Minkowskian signature → The algebra is infinite-dimensional

The E11 origin ofgauged maximal supergravities – p. 17/3

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An introduction to E11

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

1 2 3 4 5 6 7 8 9 10 11

Cartan matrix with Minkowskian signature → The algebra is infinite-dimensional A complete list of the generators is lacking, not to mention

  • ther representations...

The E11 origin ofgauged maximal supergravities – p. 17/3

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SLIDE 48

An introduction to E11

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

1 2 3 4 5 6 7 8 9 10 11

Cartan matrix with Minkowskian signature → The algebra is infinite-dimensional A complete list of the generators is lacking, not to mention

  • ther representations...

Idea: write each positive root in terms of the simple roots of

A10 and the simple root α11 α =

10

  • i=1

niαi + lα11 l = level

The E11 origin ofgauged maximal supergravities – p. 17/3

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SLIDE 49

An introduction to E11

A necessary condition for the occurrence of a representation of A10 with highest weight

j pjλj is that this

weight arises in a root of E11. One then gets

α2 = − 2 11l2 +

  • i,j

pi(Aij)−1pj

The E11 origin ofgauged maximal supergravities – p. 18/3

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An introduction to E11

A necessary condition for the occurrence of a representation of A10 with highest weight

j pjλj is that this

weight arises in a root of E11. One then gets

α2 = − 2 11l2 +

  • i,j

pi(Aij)−1pj

The fact that E11 is a Kac-Moody algebra with symmetric Cartan matrix imposes the constraint

α2 = 2, 0, −2, −4 . . .

The E11 origin ofgauged maximal supergravities – p. 18/3

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SLIDE 51

An introduction to E11

A necessary condition for the occurrence of a representation of A10 with highest weight

j pjλj is that this

weight arises in a root of E11. One then gets

α2 = − 2 11l2 +

  • i,j

pi(Aij)−1pj

The fact that E11 is a Kac-Moody algebra with symmetric Cartan matrix imposes the constraint

α2 = 2, 0, −2, −4 . . .

We can solve this level by level

The E11 origin ofgauged maximal supergravities – p. 18/3

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SLIDE 52

An introduction to E11

Solutions, using qj = p11−j:

Kab l = 0 Rabc l = 1, q3 = 1 Ra1...a6, l = 2, q6 = 1 Ra1...a8,b, l = 3, q1 = 1, q8 = 1

The E11 origin ofgauged maximal supergravities – p. 19/3

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SLIDE 53

An introduction to E11

Solutions, using qj = p11−j:

Kab l = 0 Rabc l = 1, q3 = 1 Ra1...a6, l = 2, q6 = 1 Ra1...a8,b, l = 3, q1 = 1, q8 = 1

The (8,1) generator is associated to the dual graviton

The E11 origin ofgauged maximal supergravities – p. 19/3

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SLIDE 54

An introduction to E11

Solutions, using qj = p11−j:

Kab l = 0 Rabc l = 1, q3 = 1 Ra1...a6, l = 2, q6 = 1 Ra1...a8,b, l = 3, q1 = 1, q8 = 1

The (8,1) generator is associated to the dual graviton All the generators arise from multiple commutators of Rabc The level is the number of times Rabc occurs

The E11 origin ofgauged maximal supergravities – p. 19/3

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SLIDE 55

An introduction to E11

Non-linear realisation: To each positive level generator we associate a gauge field

The E11 origin ofgauged maximal supergravities – p. 20/3

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An introduction to E11

Non-linear realisation: To each positive level generator we associate a gauge field The field equations are first order duality relations

The E11 origin ofgauged maximal supergravities – p. 20/3

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An introduction to E11

Non-linear realisation: To each positive level generator we associate a gauge field The field equations are first order duality relations At level 4 one gets the solution q10 = 1, q1 = 2 corresponding to the gauge field

A10,1,1

The E11 origin ofgauged maximal supergravities – p. 20/3

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SLIDE 58

An introduction to E11

Non-linear realisation: To each positive level generator we associate a gauge field The field equations are first order duality relations At level 4 one gets the solution q10 = 1, q1 = 2 corresponding to the gauge field

A10,1,1

Dimensional reduction → A9, that is Romans theory!

Schnakenburg and West, hep-th/0204207

The E11 origin ofgauged maximal supergravities – p. 20/3

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SLIDE 59

An introduction to E11

Non-linear realisation: To each positive level generator we associate a gauge field The field equations are first order duality relations At level 4 one gets the solution q10 = 1, q1 = 2 corresponding to the gauge field

A10,1,1

Dimensional reduction → A9, that is Romans theory!

Schnakenburg and West, hep-th/0204207

The theory is unique, gravity emerges from the choice of the background

compare with: Julia, hep-th/9805083

The E11 origin ofgauged maximal supergravities – p. 20/3

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D = 10A

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 21/3

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D = 10B

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 22/3

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SLIDE 62

D = 9

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 23/3

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SLIDE 63

D = 8

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 24/3

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SLIDE 64

D = 7

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 25/3

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SLIDE 65

D = 6

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 26/3

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SLIDE 66

D = 5

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 27/3

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SLIDE 67

D = 4

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 28/3

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SLIDE 68

D = 3

✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐ ✐

The E11 origin ofgauged maximal supergravities – p. 29/3

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The fields of E11

A partial classification of the generators of E11 has recently been performed

F .R. and West, hep-th/0612001

The E11 origin ofgauged maximal supergravities – p. 30/3

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The fields of E11

A partial classification of the generators of E11 has recently been performed

F .R. and West, hep-th/0612001

Basic idea: the sum of the indices of each field has to be equal to 3l:

11n +

  • j

jqj = 3l

The E11 origin ofgauged maximal supergravities – p. 30/3

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SLIDE 71

The fields of E11

A partial classification of the generators of E11 has recently been performed

F .R. and West, hep-th/0612001

Basic idea: the sum of the indices of each field has to be equal to 3l:

11n +

  • j

jqj = 3l

Propagating fields have n = q10 = 0. One gets

A9,9,...,9,3 A9,9,...,9,6 A9,9,...,9,8,1

That is we get infinitely many dual descriptions of the same fields

The E11 origin ofgauged maximal supergravities – p. 30/3

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The fields of E11

We want to determine all the forms that arise from dimensional reduction. The propagating fields in lower dimensions arise from the propagating fields in D = 11. We study the dimensional reduction to D.

The E11 origin ofgauged maximal supergravities – p. 31/3

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The fields of E11

We want to determine all the forms that arise from dimensional reduction. The propagating fields in lower dimensions arise from the propagating fields in D = 11. We study the dimensional reduction to D. In order to determine the D − 1-forms, we also need to consider n = q9 = 0 q10 = 1

The E11 origin ofgauged maximal supergravities – p. 31/3

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The fields of E11

We want to determine all the forms that arise from dimensional reduction. The propagating fields in lower dimensions arise from the propagating fields in D = 11. We study the dimensional reduction to D. In order to determine the D − 1-forms, we also need to consider n = q9 = 0 q10 = 1 Finally, in order to determine the D-forms, we also need to consider q10 = q9 = 0 n = 1

The E11 origin ofgauged maximal supergravities – p. 31/3

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The fields of E11

We want to determine all the forms that arise from dimensional reduction. The propagating fields in lower dimensions arise from the propagating fields in D = 11. We study the dimensional reduction to D. In order to determine the D − 1-forms, we also need to consider n = q9 = 0 q10 = 1 Finally, in order to determine the D-forms, we also need to consider q10 = q9 = 0 n = 1 Remarkably, there are only a finite number of 11-dimensional fields that give rise to forms in any dimension above two

The E11 origin ofgauged maximal supergravities – p. 31/3

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The fields of E11

D field 10

ˆ g11 ˆ A3 ˆ A6 ˆ A8,1

8

ˆ A9,3

5

ˆ A9,6

3

ˆ A9,8,1

The E11 origin ofgauged maximal supergravities – p. 32/3

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The fields of E11

D field 10

ˆ A10,1,1

7

ˆ A10,4,1

5

ˆ A10,6,2

4

ˆ A10,7,1 ˆ A10,7,4 ˆ A10,7,7

3

ˆ A10,8 ˆ A10,8,2,1 ˆ A10,8,3 ˆ A10,8,5,1 ˆ A10,8,6 ˆ A10,8,7,2 ˆ A10,8,8,1 ˆ A10,8,8,4 ˆ A10,8,8,7

The E11 origin ofgauged maximal supergravities – p. 33/3

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SLIDE 78

The fields of E11

D field

µ

10

ˆ A11,1

1 8

ˆ A11,3,1

1 7

ˆ A11,4

1

ˆ A11,4,3

1 6

ˆ A11,5,1,1

1 5

ˆ A11,6,1

2

ˆ A11,6,3,1

1

ˆ A11,6,4

1

ˆ A11,6,6,1

1 4

ˆ A11,7

1

ˆ A11,7,2,1

1

ˆ A11,7,3

2

ˆ A11,7,4,2

1

ˆ A11,7,5,1

1

ˆ A11,7,6

2

ˆ A11,7,6,3

1

ˆ A11,7,7,2

1

ˆ A11,7,7,5

1

The E11 origin ofgauged maximal supergravities – p. 34/3

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SLIDE 79

E11 and dimensional reduction

Consider the 7-dimensional example

The E11 origin ofgauged maximal supergravities – p. 35/3

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SLIDE 80

E11 and dimensional reduction

Consider the 7-dimensional example 6-forms:

ˆ A6 → 1 ˆ A8,1 → 4 ⊕ 20 ˆ A9,3 → 6 ⊕ 10 ˆ A10,1,1 → 10 ˆ A10,4,1 → 4

  • f SL(4, R). This is 15 ⊕ 40 of SL(5, R)

The E11 origin ofgauged maximal supergravities – p. 35/3

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SLIDE 81

E11 and dimensional reduction

Consider the 7-dimensional example 6-forms:

ˆ A6 → 1 ˆ A8,1 → 4 ⊕ 20 ˆ A9,3 → 6 ⊕ 10 ˆ A10,1,1 → 10 ˆ A10,4,1 → 4

  • f SL(4, R). This is 15 ⊕ 40 of SL(5, R)

7-forms:

ˆ A8,1 → 6 ⊕ 10 ˆ A9,3 → 4 ⊕ 20 ˆ A10,1,1 → 4 ⊕ 36 ˆ A10,4,1 → 1 ⊕ 15 ˆ A11,1 → 4 ˆ A11,3,1 → 15 ˆ A11,4 → 1 ˆ A11,4,3 → 4

that is 5 ⊕ 45 ⊕ 70 of SL(5, R)

The E11 origin ofgauged maximal supergravities – p. 35/3

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SLIDE 82

E11 and dimensional reduction

D G 1-forms 2-forms 3-forms 4-forms 5-forms 6-forms 7-forms 8-forms 9-forms 10-forms 10A R+ 1 1 1 1 1 1 1 1 1 1 10B SL(2, R) 2 1 2 3 4 2 9 SL(2, R) × R+ 2 2 1 1 2 2 3 3 4 2 1 1 1 2 2 8 SL(3, R) × SL(2, R) (3, 2) (3, 1) (1, 2) (3, 1) (3, 2) (15, 1) (8, 1) (6, 2) (3, 3) (1, 3) (3, 2) (3, 1) (3, 1) 7 SL(5, R) 10 5 5 10 24 40 70 45 15 5 6 SO(5, 5) 16 10 16 45 144 320 126 10 5 E6(+6) 27 27 78 351 1728 27 4 E7(+7) 56 133 912 8645 133 3 E8(+8) 248 3875 ? 1

The E11 origin ofgauged maximal supergravities – p. 36/3

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SLIDE 83

E11 and dimensional reduction

D G 1-forms 2-forms 3-forms 4-forms 5-forms 6-forms 7-forms 8-forms 9-forms 10-forms 10A R+ 1 1 1 1 1 1 1 1 1 1 10B SL(2, R) 2 1 2 3 4 2 9 SL(2, R) × R+ 2 2 1 1 2 2 3 3 4 2 1 1 1 2 2 8 SL(3, R) × SL(2, R) (3, 2) (3, 1) (1, 2) (3, 1) (3, 2) (15, 1) (8, 1) (6, 2) (3, 3) (1, 3) (3, 2) (3, 1) (3, 1) 7 SL(5, R) 10 5 5 10 24 40 70 45 15 5 6 SO(5, 5) 16 10 16 45 144 320 126 10 5 E6(+6) 27 27 78 351 1728 27 4 E7(+7) 56 133 912 8645 133 3 E8(+8) 248 3875 ? 1

3-forms in 3 dimensions: 248 ⊕ 3875 ⊕ 147250

Bergshoeff, De Baetselier, Nutma, arXiv:0705.1304

The E11 origin ofgauged maximal supergravities – p. 37/3

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SLIDE 84

Some dynamics

Consider the 5-dimensional example. G = E6

[Ra,M, Pb] = δa

b ΘM αRα

[RabM, Pc] = ZMN(δa

c Rb,N − δb cRa,N)

The E11 origin ofgauged maximal supergravities – p. 38/3

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SLIDE 85

Some dynamics

Consider the 5-dimensional example. G = E6

[Ra,M, Pb] = δa

b ΘM αRα

[RabM, Pc] = ZMN(δa

c Rb,N − δb cRa,N)

The term in the Cartan form proportional to the 1-form generator Ra,M is

∂µAa,M − 1 2Aµ,NΘN α(Dα)M PAa,P − 2ZMNAµaN

The scalar sector is the Cartan form of the gauged supergravity coset space

The E11 origin ofgauged maximal supergravities – p. 38/3

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SLIDE 86

Some dynamics

Consider the 5-dimensional example. G = E6

[Ra,M, Pb] = δa

b ΘM αRα

[RabM, Pc] = ZMN(δa

c Rb,N − δb cRa,N)

The term in the Cartan form proportional to the 1-form generator Ra,M is

∂µAa,M − 1 2Aµ,NΘN α(Dα)M PAa,P − 2ZMNAµaN

The scalar sector is the Cartan form of the gauged supergravity coset space The equations are first order duality relations. This reproduces the supergravity results

The E11 origin ofgauged maximal supergravities – p. 38/3

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SLIDE 87

Conclusions

E11 provides a completely unified description of all

supergravities and it encodes all their dynamical features

The E11 origin ofgauged maximal supergravities – p. 39/3

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SLIDE 88

Conclusions

E11 provides a completely unified description of all

supergravities and it encodes all their dynamical features It would be interesting to determine the D-forms in any dimension D below 10 from supersymmetry

The E11 origin ofgauged maximal supergravities – p. 39/3

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SLIDE 89

Conclusions

E11 provides a completely unified description of all

supergravities and it encodes all their dynamical features It would be interesting to determine the D-forms in any dimension D below 10 from supersymmetry Gauged supergravities in D = 8

The E11 origin ofgauged maximal supergravities – p. 39/3

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SLIDE 90

Conclusions

E11 provides a completely unified description of all

supergravities and it encodes all their dynamical features It would be interesting to determine the D-forms in any dimension D below 10 from supersymmetry Gauged supergravities in D = 8 Many other physical implications: uplifting of D8-branes, Horava-Witten...

The E11 origin ofgauged maximal supergravities – p. 39/3