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Gravitational Scattering via Twistor Theory Tim Adamo DAMTP, University of Cambridge Frontiers of Fundamental Physics 14 14 July 2014 Work with L. Mason [arXiv:1307.5043, 1308.2820] T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 1 / 15

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Page 1: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Gravitational Scattering via Twistor Theory

Tim AdamoDAMTP, University of Cambridge

Frontiers of Fundamental Physics 14

14 July 2014

Work with L. Mason [arXiv:1307.5043, 1308.2820]

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 1 / 15

Page 2: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Motivation

Why gravity scattering amplitudes?

Provide important constraints on any theory of quantum gravity

Theoretical ‘data’

May point to novel formulations of underlying theory or new ways tocompute observables

c.f., ongoing progress in (planar) gauge theory

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 2 / 15

Page 3: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Motivation

Why gravity scattering amplitudes?

Provide important constraints on any theory of quantum gravity

Theoretical ‘data’

May point to novel formulations of underlying theory or new ways tocompute observables

c.f., ongoing progress in (planar) gauge theory

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 2 / 15

Page 4: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Today: tree-level (semi-classical) scattering amplitudes.

Defined by the classical action of a theory:

Definition (Tree-level amplitudes)

Given an action functional S [φ], non-linear solution to the FEs(‘background’) φcl, and n solutions φi to the linearized FEs (‘scatteringstates’), then the tree-level scattering amplitude for the φi on φcl is:

M0n(φ1, . . . , φn) =

∂nS[φcl −

∑i εiφi

]∂ε1 · · · ∂εn

∣∣∣∣∣ε1=···εn=0

Usually compute by summing Feynman diagrams...hard!

Resulting formulae (drastically) simpler than expected! [DeWitt,

Berends-Giele-Kuijf, Mason-Skinner, Nguyen-Spradlin-Volovich-Wen, Hodges, Cachazo-Skinner,

Cachazo-He-Yuan, ...]

Many of these simplifications are related to expressing amplitudes intwistor theory.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 3 / 15

Page 5: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Today: tree-level (semi-classical) scattering amplitudes.

Defined by the classical action of a theory:

Definition (Tree-level amplitudes)

Given an action functional S [φ], non-linear solution to the FEs(‘background’) φcl, and n solutions φi to the linearized FEs (‘scatteringstates’), then the tree-level scattering amplitude for the φi on φcl is:

M0n(φ1, . . . , φn) =

∂nS[φcl −

∑i εiφi

]∂ε1 · · · ∂εn

∣∣∣∣∣ε1=···εn=0

Usually compute by summing Feynman diagrams...hard!

Resulting formulae (drastically) simpler than expected! [DeWitt,

Berends-Giele-Kuijf, Mason-Skinner, Nguyen-Spradlin-Volovich-Wen, Hodges, Cachazo-Skinner,

Cachazo-He-Yuan, ...]

Many of these simplifications are related to expressing amplitudes intwistor theory.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 3 / 15

Page 6: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Today: tree-level (semi-classical) scattering amplitudes.

Defined by the classical action of a theory:

Definition (Tree-level amplitudes)

Given an action functional S [φ], non-linear solution to the FEs(‘background’) φcl, and n solutions φi to the linearized FEs (‘scatteringstates’), then the tree-level scattering amplitude for the φi on φcl is:

M0n(φ1, . . . , φn) =

∂nS[φcl −

∑i εiφi

]∂ε1 · · · ∂εn

∣∣∣∣∣ε1=···εn=0

Usually compute by summing Feynman diagrams...hard!

Resulting formulae (drastically) simpler than expected! [DeWitt,

Berends-Giele-Kuijf, Mason-Skinner, Nguyen-Spradlin-Volovich-Wen, Hodges, Cachazo-Skinner,

Cachazo-He-Yuan, ...]

Many of these simplifications are related to expressing amplitudes intwistor theory.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 3 / 15

Page 7: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Questions to Answer:

Is there some classical action principle giving rise to thesesimplifications?

Can we learn anything about the associated twistor geometry?

Are there new expressions for ‘amplitudes’ in backgrounds that aren’tasymptotically flat (e.g., de Sitter space)?

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 4 / 15

Page 8: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Twistor Toolbox

Basic idea of twistor theory:

Physical info on M ⇔ Geometric data on PT

PT a (deformation of a) 3-dimensional complex projective manifold

Points x ∈ M ↔ holomorphic rational curves X ⊂ PT

x , y ∈ M null separated iff X ,Y ⊂ PT intersect.

Conformal structure on M ↔ C-structure on PT .

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 5 / 15

Page 9: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Twistor Toolbox

Basic idea of twistor theory:

Physical info on M ⇔ Geometric data on PT

PT a (deformation of a) 3-dimensional complex projective manifold

Points x ∈ M ↔ holomorphic rational curves X ⊂ PT

x , y ∈ M null separated iff X ,Y ⊂ PT intersect.

Conformal structure on M ↔ C-structure on PT .

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 5 / 15

Page 10: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Does a twistor space exist for every M?

No!

Basic result is [Penrose, Ward] :

Theorem (Non-linear Graviton)

∃ a 1:1 correspondence between:

M with self-dual holomorphic conformal structure, and

PT with integrable almost complex structure.

Thing to remember: ∂2 = 0 on PT ⇔ ΨABCD = 0 on M.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 6 / 15

Page 11: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Does a twistor space exist for every M?

No!

Basic result is [Penrose, Ward] :

Theorem (Non-linear Graviton)

∃ a 1:1 correspondence between:

M with self-dual holomorphic conformal structure, and

PT with integrable almost complex structure.

Thing to remember: ∂2 = 0 on PT ⇔ ΨABCD = 0 on M.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 6 / 15

Page 12: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Twistor theory good for describing self-duality

Is there a way to formulate GR as an expansion around the SD sector?

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 7 / 15

Page 13: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Twistor theory good for describing self-duality

Is there a way to formulate GR as an expansion around the SD sector?

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 7 / 15

Page 14: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Conformal Gravity

Start with an un-physical theory:

S [g ] =1

ε2

∫Mdµ Cµνρσ Cµνρσ

=2

ε2

∫Mdµ ΨABCD ΨABCD + top. terms

Conformally invariant, with 4th-order equations of motion (non-unitary):

(∇AA′∇B

B′ + ΦABA′B′)ΨABCD = (∇A′

A ∇B′B + ΦA′B′

AB )ΨA′B′C ′D′ = 0

Note: Einstein (ΦABA′B′ = 0 = ∇AA′

ΨABCD) and SD/ASD are subsectors ofsolutions.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 8 / 15

Page 15: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Conformal Gravity

Start with an un-physical theory:

S [g ] =1

ε2

∫Mdµ Cµνρσ Cµνρσ

=2

ε2

∫Mdµ ΨABCD ΨABCD + top. terms

Conformally invariant, with 4th-order equations of motion (non-unitary):

(∇AA′∇B

B′ + ΦABA′B′)ΨABCD = (∇A′

A ∇B′B + ΦA′B′

AB )ΨA′B′C ′D′ = 0

Note: Einstein (ΦABA′B′ = 0 = ∇AA′

ΨABCD) and SD/ASD are subsectors ofsolutions.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 8 / 15

Page 16: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Conformal Gravity

Start with an un-physical theory:

S [g ] =1

ε2

∫Mdµ Cµνρσ Cµνρσ

=2

ε2

∫Mdµ ΨABCD ΨABCD + top. terms

Conformally invariant, with 4th-order equations of motion (non-unitary):

(∇AA′∇B

B′ + ΦABA′B′)ΨABCD = (∇A′

A ∇B′B + ΦA′B′

AB )ΨA′B′C ′D′ = 0

Note: Einstein (ΦABA′B′ = 0 = ∇AA′

ΨABCD) and SD/ASD are subsectors ofsolutions.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 8 / 15

Page 17: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Upshot: Perturbative expansion around SD sector. [Berkovits-Witten]

Introduce Lagrange multiplier GABCD :

S [g ]→ S [g ,G ] =

∫Mdµ GABCD ΨABCD −

ε2

2

∫Mdµ GABCD GABCD

Field Equations:

ΨABCD = ε2 GABCD , (∇AA′∇B

B′ + ΦABA′B′)GABCD = 0

ε2 an expansion parameter around the SD sector.

But we can formulate this in twistor space! [Mason]

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 9 / 15

Page 18: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Upshot: Perturbative expansion around SD sector. [Berkovits-Witten]

Introduce Lagrange multiplier GABCD :

S [g ]→ S [g ,G ] =

∫Mdµ GABCD ΨABCD −

ε2

2

∫Mdµ GABCD GABCD

Field Equations:

ΨABCD = ε2 GABCD , (∇AA′∇B

B′ + ΦABA′B′)GABCD = 0

ε2 an expansion parameter around the SD sector.

But we can formulate this in twistor space! [Mason]

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 9 / 15

Page 19: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Conformal Gravity in Twistor Space

Translation:

ΨABCD ↔ N[J] ∈ Ω0,2(PT ,TPT ), GABCD ↔ b ∈ Ω1,1(PT ,O(−4))

Action functional:

S [b, J] =

∫PT

D3Z ∧ Nyb − ε2

2

∫PT ×MPT

dµ ∧ b1 ∧ b2 (σ1σ2)4

Using standard results [Penrose, Atiyah-Hitchin-Singer] :

N[J] = ΨABCDσA ΣBC ∂

∂σD, GABCD =

∫XσAσBσCσD b|X

Implies FEs on twistor space equivalent to those on space-time.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 10 / 15

Page 20: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Conformal Gravity in Twistor Space

Translation:

ΨABCD ↔ N[J] ∈ Ω0,2(PT ,TPT ), GABCD ↔ b ∈ Ω1,1(PT ,O(−4))

Action functional:

S [b, J] =

∫PT

D3Z ∧ Nyb − ε2

2

∫PT ×MPT

dµ ∧ b1 ∧ b2 (σ1σ2)4

Using standard results [Penrose, Atiyah-Hitchin-Singer] :

N[J] = ΨABCDσA ΣBC ∂

∂σD, GABCD =

∫XσAσBσCσD b|X

Implies FEs on twistor space equivalent to those on space-time.

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 10 / 15

Page 21: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Why do we care?

Theorem (Anderson, Maldacena)

For M asymptotically de Sitter,

SCG[M] = −2 Λ2

3ε2Vren(M) = −Λκ2

3ε2SEHren [M] ,

and asymptotic Einstein states can be singled out in the conformal theory.

⇒ for tree-level amplitudes,

MEin =1

ΛMCG|Ein

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 11 / 15

Page 22: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Why do we care?

Theorem (Anderson, Maldacena)

For M asymptotically de Sitter,

SCG[M] = −2 Λ2

3ε2Vren(M) = −Λκ2

3ε2SEHren [M] ,

and asymptotic Einstein states can be singled out in the conformal theory.

⇒ for tree-level amplitudes,

MEin =1

ΛMCG|Ein

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 11 / 15

Page 23: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Why do we care?

Theorem (Anderson, Maldacena)

For M asymptotically de Sitter,

SCG[M] = −2 Λ2

3ε2Vren(M) = −Λκ2

3ε2SEHren [M] ,

and asymptotic Einstein states can be singled out in the conformal theory.

⇒ for tree-level amplitudes,

MEin =1

ΛMCG|Ein

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 11 / 15

Page 24: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Einstein Gravity in Twistor Space

Einstein degrees of freedom ⇒ break conformal invariance

Infinity twistor:

Iαβ =

(ΛεAB 0

0 εA′B′

), Iαβ =

(εAB 0

0 ΛεA′B′

)Obey IαβIβγ = Λδαγ , induce geometric structures:

τ = IαβZαdZβ ∈ Ω1,0(PT ,O(2)), ·, · = Iαβ∂α ∂β

(Like fixing the conformal factor for metric in Klein representation:

ds2 =εαβγδdX

αβ dXγδ

(Iαβ Xαβ)2)

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 12 / 15

Page 25: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Einstein Gravity in Twistor Space

Einstein degrees of freedom ⇒ break conformal invariance

Infinity twistor:

Iαβ =

(ΛεAB 0

0 εA′B′

), Iαβ =

(εAB 0

0 ΛεA′B′

)Obey IαβIβγ = Λδαγ , induce geometric structures:

τ = IαβZαdZβ ∈ Ω1,0(PT ,O(2)), ·, · = Iαβ∂α ∂β

(Like fixing the conformal factor for metric in Klein representation:

ds2 =εαβγδdX

αβ dXγδ

(Iαβ Xαβ)2)

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 12 / 15

Page 26: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Write complex structure on PT as finite deformation of ‘flat’ structure.

Compatability with Iαβ, Iαβ ⇒

∂ = ∂0 + Iαβ∂αh ∂β , h ∈ Ω0,1(PT ,O(2))

b → IαβZα dZβ h = τ h h ∈ Ω0,1(PT ,O(−6))

Action becomes:

S [b, J]→ S [h, h] = Λ

∫PT

D3Z ∧ h ∧(∂0h +

1

2h, h

)− ε2

2

∫PT ×MPT

dµ τ1 ∧ τ2 ∧ h1 ∧ h2 (σ1σ2)4

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 13 / 15

Page 27: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Write complex structure on PT as finite deformation of ‘flat’ structure.

Compatability with Iαβ, Iαβ ⇒

∂ = ∂0 + Iαβ∂αh ∂β , h ∈ Ω0,1(PT ,O(2))

b → IαβZα dZβ h = τ h h ∈ Ω0,1(PT ,O(−6))

Action becomes:

S [b, J]→ S [h, h] = Λ

∫PT

D3Z ∧ h ∧(∂0h +

1

2h, h

)− ε2

2

∫PT ×MPT

dµ τ1 ∧ τ2 ∧ h1 ∧ h2 (σ1σ2)4

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 13 / 15

Page 28: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

By earlier Theorem, Λ−1S [h, h] should compute tree-level Einstein gravityamplitudes. Is this actually true?

Yes! Lots of technical detail, but upshots are [Adamo-Mason] :

Second term is generating functional for MHV amplitudes

Flat space limit = Hodges formulae

New Λ 6= 0 formulae

Apparent MHV formalism induced on twistor space

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 14 / 15

Page 29: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

By earlier Theorem, Λ−1S [h, h] should compute tree-level Einstein gravityamplitudes. Is this actually true?

Yes! Lots of technical detail, but upshots are [Adamo-Mason] :

Second term is generating functional for MHV amplitudes

Flat space limit = Hodges formulae

New Λ 6= 0 formulae

Apparent MHV formalism induced on twistor space

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 14 / 15

Page 30: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Further Directions

Twistor action for Einstein gravity itself?

More general (i.e., NkMHV) amplitudes?

What do the Λ 6= 0 formulae mean?

Momentum space prescription for MHV formalism?

Thanks!

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 15 / 15

Page 31: Gravitational Scattering via Twistor Theoryffp14.cpt.univ-mrs.fr/DOCUMENTS/SLIDES/ADAMO_Tim.pdf · Why gravity scattering amplitudes? Provide important constraints on any theory of

Further Directions

Twistor action for Einstein gravity itself?

More general (i.e., NkMHV) amplitudes?

What do the Λ 6= 0 formulae mean?

Momentum space prescription for MHV formalism?

Thanks!

T Adamo (FFP14) Twistor Gravity Amplitudes 14 July 2014 15 / 15