gravitational scattering via twistor theoryffp14.cpt.univ-mrs.fr/documents/slides/adamo_tim.pdf ·...
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/1.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/2.jpg)
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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/4.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/5.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/6.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/7.jpg)
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
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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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/10.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/11.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/12.jpg)
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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/14.jpg)
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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/16.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/17.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/18.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/19.jpg)
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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/21.jpg)
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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/23.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/24.jpg)
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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/26.jpg)
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
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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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/28.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/29.jpg)
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](https://reader030.vdocument.in/reader030/viewer/2022040409/5ec5009a220d2d1cbd768868/html5/thumbnails/30.jpg)
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
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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