The Double Copy of a Point Charge Ricardo Monteiro Queen Mary - - PowerPoint PPT Presentation

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The Double Copy of a Point Charge Ricardo Monteiro Queen Mary - - PowerPoint PPT Presentation

The Double Copy of a Point Charge Ricardo Monteiro Queen Mary University of London QCD meets Gravity UCLA, 12 December 2019 Based on arXiv:1912.02177 with Kwangeon Kim, Kanghoon Lee, Isobel Nicholson, David Peinador Veiga Ricardo Monteiro


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SLIDE 1

The Double Copy of a Point Charge

Ricardo Monteiro

Queen Mary University of London QCD meets Gravity UCLA, 12 December 2019

Based on arXiv:1912.02177 with Kwangeon Kim, Kanghoon Lee, Isobel Nicholson, David Peinador Veiga

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 1 / 16

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SLIDE 2

Motivation

Simple gauge theory solution: Coulomb. Schwarzschild is natural double copy of Coulomb. Full story? Dilaton?

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 2 / 16

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Motivation

Simple gauge theory solution: Coulomb. Schwarzschild is natural double copy of Coulomb. Full story? Dilaton? Double-copy structure of Einstein equations? double copy double field theory

Gravity = YM × YM doubled geometry (xµ, ˜

xµ)

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 2 / 16

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SLIDE 4

Double copy of Coulomb: perturbative approach

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 3 / 16

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Gravity ∼ (Yang-Mills) 2

Scattering amplitudes

[Kawai, Lewellen, Tye ’86; Bern, Carrasco, Johansson ’08; . . . ]

YM states: A a

µ = eik·x ǫµ T a ,

ǫµ has D − 2 dof.

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 4 / 16

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SLIDE 6

Gravity ∼ (Yang-Mills) 2

Scattering amplitudes

[Kawai, Lewellen, Tye ’86; Bern, Carrasco, Johansson ’08; . . . ]

YM states: A a

µ = eik·x ǫµ T a ,

ǫµ has D − 2 dof. NS-NS gravity states: Hµν = eik·x εµν , εµν = ǫµ ˜ ǫν

  • r linear comb.

(D − 2)2 dof: graviton hµν + dilaton φ + B-field Bµν .

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 4 / 16

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SLIDE 7

Gravity ∼ (Yang-Mills) 2

Scattering amplitudes

[Kawai, Lewellen, Tye ’86; Bern, Carrasco, Johansson ’08; . . . ]

YM states: A a

µ = eik·x ǫµ T a ,

ǫµ has D − 2 dof. NS-NS gravity states: Hµν = eik·x εµν , εµν = ǫµ ˜ ǫν

  • r linear comb.

(D − 2)2 dof: graviton hµν + dilaton φ + B-field Bµν . Interactions Agrav(ε µν

i

) = AYM(ǫ µ

i ) ⊗dc AYM(˜

ǫ µ

i )

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 4 / 16

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SLIDE 8

Gravity ∼ (Yang-Mills) 2

Scattering amplitudes

[Kawai, Lewellen, Tye ’86; Bern, Carrasco, Johansson ’08; . . . ]

YM states: A a

µ = eik·x ǫµ T a ,

ǫµ has D − 2 dof. NS-NS gravity states: Hµν = eik·x εµν , εµν = ǫµ ˜ ǫν

  • r linear comb.

(D − 2)2 dof: graviton hµν + dilaton φ + B-field Bµν . Interactions Agrav(ε µν

i

) = AYM(ǫ µ

i ) ⊗dc AYM(˜

ǫ µ

i )

Strings insight: closed string ∼ (‘left’ open string) × (‘right’ open string)

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 4 / 16

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SLIDE 9

Gravity ∼ (Yang-Mills) 2

Scattering amplitudes

[Kawai, Lewellen, Tye ’86; Bern, Carrasco, Johansson ’08; . . . ]

YM states: A a

µ = eik·x ǫµ T a ,

ǫµ has D − 2 dof. NS-NS gravity states: Hµν = eik·x εµν , εµν = ǫµ ˜ ǫν

  • r linear comb.

(D − 2)2 dof: graviton hµν + dilaton φ + B-field Bµν . Interactions Agrav(ε µν

i

) = AYM(ǫ µ

i ) ⊗dc AYM(˜

ǫ µ

i )

Strings insight: closed string ∼ (‘left’ open string) × (‘right’ open string) Perturbative classical solutions First map free solutions (linear). Then correct solutions in double-copy-ish perturbation theory.

× ∼

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 4 / 16

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Double copy for Coulomb?

Linearised “fat graviton”:

[Luna, RM, Nicholson, Ochirov, O’Connell, White, Westerberg 16]

Hµν =

  • hµν − 1

2 h + Pµν[h]

  • + Bµν + Pµν [φ]

(graviton + B-field + dilaton) (Pµν is coord. space projector)

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 5 / 16

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Double copy for Coulomb?

Linearised “fat graviton”:

[Luna, RM, Nicholson, Ochirov, O’Connell, White, Westerberg 16]

Hµν =

  • hµν − 1

2 h + Pµν[h]

  • + Bµν + Pµν [φ]

(graviton + B-field + dilaton) (Pµν is coord. space projector) Coulomb usual gauge: Aa

µ = −qa

r uµ uµ = (1, 0, 0, 0) , ∂µqa = 0 . Natural double copy: Hµν = M r uµ uν both graviton and dilaton.

[also Goldberger, Ridgway 16] Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 5 / 16

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SLIDE 12

Double copy for Coulomb?

Linearised “fat graviton”:

[Luna, RM, Nicholson, Ochirov, O’Connell, White, Westerberg 16]

Hµν =

  • hµν − 1

2 h + Pµν[h]

  • + Bµν + Pµν [φ]

(graviton + B-field + dilaton) (Pµν is coord. space projector) Coulomb usual gauge: Aa

µ = −qa

r uµ uµ = (1, 0, 0, 0) , ∂µqa = 0 . Natural double copy: Hµν = M r uµ uν both graviton and dilaton.

[also Goldberger, Ridgway 16]

Coulomb different gauge: Aa

µ = qa

r kµ k = dt + dr , k2 = 0 . Natural double copy: hµν = 2M r kµ kν exact Schwarzschild! Kerr-Schild double copy.

[RM, O’Connell, White 14] Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 5 / 16

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Double copy for Coulomb?

Linearised “fat graviton”:

[Luna, RM, Nicholson, Ochirov, O’Connell, White, Westerberg 16]

Hµν =

  • hµν − 1

2 h + Pµν[h]

  • + Bµν + Pµν [φ]

(graviton + B-field + dilaton) (Pµν is coord. space projector) Coulomb usual gauge: Aa

µ = −qa

r uµ uµ = (1, 0, 0, 0) , ∂µqa = 0 . Natural double copy: Hµν = M r uµ uν both graviton and dilaton.

[also Goldberger, Ridgway 16]

Coulomb different gauge: Aa

µ = qa

r kµ k = dt + dr , k2 = 0 . Natural double copy: hµν = 2M r kµ kν exact Schwarzschild! Kerr-Schild double copy.

[RM, O’Connell, White 14]

Both consistent with ‘convolution’ idea [Anastasiou, Borsten, Duff, Hughes, Nagy 14] : Aa

µ ∗ inv(Φ)a˙ a ∗ A˙ a ν

  • (1/r) ∗ inv(1/r) ∗ (1/r) = (1/r)

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 5 / 16

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Double copy for Coulomb: JNW solution

Clue from momentum states: take polarisations ǫµ , ˜ ǫµ . ǫ · k = ˜ ǫ · k = 0 Simplest double copy: εµν = ǫµ˜ ǫν .

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 6 / 16

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Double copy for Coulomb: JNW solution

Clue from momentum states: take polarisations ǫµ , ˜ ǫµ . ǫ · k = ˜ ǫ · k = 0 Simplest double copy: εµν = ǫµ˜ ǫν . ǫ · q = ˜ ǫ · q = q2 = 0 Why not ǫ(µ˜ ǫν) , ǫ[µ˜ ǫν] , ǫ · ˜ ǫ ∆µν ? ∆µν = ηµν − kµqν + kνqµ k · q

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 6 / 16

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Double copy for Coulomb: JNW solution

Clue from momentum states: take polarisations ǫµ , ˜ ǫµ . ǫ · k = ˜ ǫ · k = 0 Simplest double copy: εµν = ǫµ˜ ǫν . ǫ · q = ˜ ǫ · q = q2 = 0 Why not ǫ(µ˜ ǫν) , ǫ[µ˜ ǫν] , ǫ · ˜ ǫ ∆µν ? ∆µν = ηµν − kµqν + kνqµ k · q General: graviton + B-field + dilaton. εµν = C(h)

  • ǫ(µ˜

ǫν) − ∆µν D − 2 ǫ · ˜ ǫ

  • + C(B) ǫ[µ˜

ǫν] + C(φ) ∆µν D − 2 ǫ · ˜ ǫ .

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 6 / 16

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Double copy for Coulomb: JNW solution

Clue from momentum states: take polarisations ǫµ , ˜ ǫµ . ǫ · k = ˜ ǫ · k = 0 Simplest double copy: εµν = ǫµ˜ ǫν . ǫ · q = ˜ ǫ · q = q2 = 0 Why not ǫ(µ˜ ǫν) , ǫ[µ˜ ǫν] , ǫ · ˜ ǫ ∆µν ? ∆µν = ηµν − kµqν + kνqµ k · q General: graviton + B-field + dilaton. εµν = C(h)

  • ǫ(µ˜

ǫν) − ∆µν D − 2 ǫ · ˜ ǫ

  • + C(B) ǫ[µ˜

ǫν] + C(φ) ∆µν D − 2 ǫ · ˜ ǫ . Linearised (Coulomb)2: no B-field, M ∼ C(h) graviton, Y ∼ C(φ) dilaton. Hµν = M uµuν r − Pµν u2 r

  • + Y Pµν

u2 r

  • Pµν
  • u2

r

  • = −1

2 r (ηµν − qµlν − qνlµ)

Y = 0: linearised Schwarzschild solution. Any Y: linearised JNW solution [Janis, Newman, Winicour ’68].

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 6 / 16

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Perturbative construction

Starting point: H(0)

µν is linearised solution, H(1) µν is first non-linear correction.

H(1) =

H(0) H(0)

Gauge theory field Aa

µ

A(1)aµ(−p1) = i 2p2

1

  • dDp2dDp3δD(p1 + p2 + p3)

f abc V µβγ A(0)b

β

(p2)A(0)c

γ

(p3) YM vertex V(p1, p2, p3)µβγ = (p1 − p2)γηµβ + (p2 − p3)µηβγ + (p3 − p1)βηγµ

Gravity field Hµν ∼ graviton + dilaton + B-field

H(1)µµ′(−p1) = 1 4p2

1

  • dDp2dDp3δD(p1 + p2 + p3)

V µβγ V µ′β′γ′ H(0)

ββ′(p2)H(0) γγ′(p3) Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 7 / 16

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Perturbative construction

Starting point: H(0)

µν is linearised solution, H(1) µν is first non-linear correction.

H(1) =

H(0) H(0)

Gauge theory field Aa

µ

A(1)aµ(−p1) = i 2p2

1

  • dDp2dDp3δD(p1 + p2 + p3)

f abc V µβγ A(0)b

β

(p2)A(0)c

γ

(p3) YM vertex V(p1, p2, p3)µβγ = (p1 − p2)γηµβ + (p2 − p3)µηβγ + (p3 − p1)βηγµ

Gravity field Hµν ∼ graviton + dilaton + B-field

H(1)µµ′(−p1) = 1 4p2

1

  • dDp2dDp3δD(p1 + p2 + p3)

V µβγ V µ′β′γ′ H(0)

ββ′(p2)H(0) γγ′(p3)

Simplification: index factorisation.

[analogous to Bern, Grant 99; Hohm 11; Cheung, Remmen 16] Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 7 / 16

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SLIDE 20

Perturbative construction

Starting point: H(0)

µν is linearised solution, H(1) µν is first non-linear correction.

H(1) =

H(0) H(0)

Gauge theory field Aa

µ

A(1)aµ(−p1) = i 2p2

1

  • dDp2dDp3δD(p1 + p2 + p3)

f abc V µβγ A(0)b

β

(p2)A(0)c

γ

(p3) YM vertex V(p1, p2, p3)µβγ = (p1 − p2)γηµβ + (p2 − p3)µηβγ + (p3 − p1)βηγµ

Gravity field Hµν ∼ graviton + dilaton + B-field

H(1)µµ′(−p1) = 1 4p2

1

  • dDp2dDp3δD(p1 + p2 + p3)

V µβγ V µ′β′γ′ H(0)

ββ′(p2)H(0) γγ′(p3)

Simplification: index factorisation.

[analogous to Bern, Grant 99; Hohm 11; Cheung, Remmen 16]

Case Y = M [Luna, RM, Nicholson, Ochirov, O’Connell, White, Westerberg 16]. Case Y = M [Kim, Lee, RM, Nicholson, Veiga 19]. Comparison to exact solution messy (gauge choices, field redefinitions).

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 7 / 16

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General point charge: JNW solution

Unique static, spherically symmetric, asymptotically flat solution

  • f Einstein + minimally coupled scalar.

Two parameters (M, Y) or (ρ0, γ). Found by Janis, Newman, Winicour ’68: ds2 = −

  • 1 − ρ0

ρ γ dt2 +

  • 1 − ρ0

ρ −γ dρ2 +

  • 1 − ρ0

ρ 1−γ ρ2dΩ2 φ = Y ρ0 log

  • 1 − ρ0

ρ

  • ρ0 = 2
  • M2 + Y 2

γ = M √ M2 + Y 2 Y = 0: vacuum gravity → Schwarzschild (usual coords) Y = 0: naked singularity at origin ρ = ρ0, cf. no-hair theorems

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 8 / 16

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General point charge: JNW solution

Unique static, spherically symmetric, asymptotically flat solution

  • f Einstein + minimally coupled scalar.

Two parameters (M, Y) or (ρ0, γ). Found by Janis, Newman, Winicour ’68: ds2 = −

  • 1 − ρ0

ρ γ dt2 +

  • 1 − ρ0

ρ −γ dρ2 +

  • 1 − ρ0

ρ 1−γ ρ2dΩ2 φ = Y ρ0 log

  • 1 − ρ0

ρ

  • ρ0 = 2
  • M2 + Y 2

γ = M √ M2 + Y 2 Y = 0: vacuum gravity → Schwarzschild (usual coords) Y = 0: naked singularity at origin ρ = ρ0, cf. no-hair theorems General JNW not Kerr-Schild. Exact double copy map? Yes.

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 8 / 16

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General point charge: JNW solution

Unique static, spherically symmetric, asymptotically flat solution

  • f Einstein + minimally coupled scalar.

Two parameters (M, Y) or (ρ0, γ). Found by Janis, Newman, Winicour ’68: ds2 = −

  • 1 − ρ0

ρ γ dt2 +

  • 1 − ρ0

ρ −γ dρ2 +

  • 1 − ρ0

ρ 1−γ ρ2dΩ2 φ = Y ρ0 log

  • 1 − ρ0

ρ

  • ρ0 = 2
  • M2 + Y 2

γ = M √ M2 + Y 2 Y = 0: vacuum gravity → Schwarzschild (usual coords) Y = 0: naked singularity at origin ρ = ρ0, cf. no-hair theorems General JNW not Kerr-Schild. Exact double copy map? Yes. Solution above is in Einstein frame. In string frame, gS

µν = e2φ gE µν .

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 8 / 16

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Double copy of Coulomb: exact map with double field theory

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 9 / 16

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Classical double copy: exact

Kerr-Schild double copy

[RM, O’Connell, White 14] [with Luna, Nicholson 15-18]

“Exact perturbation” gµν = ηµν + φ kµkν where kµ is null and geodesic wrt ηµν and gµν. (kµ = gµνkν = ηµνkν)

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 10 / 16

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Classical double copy: exact

Kerr-Schild double copy

[RM, O’Connell, White 14] [with Luna, Nicholson 15-18]

“Exact perturbation” gµν = ηµν + φ kµkν where kµ is null and geodesic wrt ηµν and gµν. (kµ = gµνkν = ηµνkν) Einstein equations linearise: gµν = ηµν − φ kµkν Rµν = 1

2∂α [∂µ (φkαkν) + ∂ν (φkαkµ) − ∂α (φkµkν)]

∂µ ≡ ηµν∂ν

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 10 / 16

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SLIDE 27

Classical double copy: exact

Kerr-Schild double copy

[RM, O’Connell, White 14] [with Luna, Nicholson 15-18]

“Exact perturbation” gµν = ηµν + φ kµkν where kµ is null and geodesic wrt ηµν and gµν. (kµ = gµνkν = ηµνkν) Einstein equations linearise: gµν = ηµν − φ kµkν Rµν = 1

2∂α [∂µ (φkαkν) + ∂ν (φkαkµ) − ∂α (φkµkν)]

∂µ ≡ ηµν∂ν Stationary vacuum case (take k0 = 1): 0 = Rµ

0 = 1

2 ∂νF µν for F = dA Aµ = φ kµ

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 10 / 16

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SLIDE 28

Classical double copy: exact

Kerr-Schild double copy

[RM, O’Connell, White 14] [with Luna, Nicholson 15-18]

“Exact perturbation” gµν = ηµν + φ kµkν where kµ is null and geodesic wrt ηµν and gµν. (kµ = gµνkν = ηµνkν) Einstein equations linearise: gµν = ηµν − φ kµkν Rµν = 1

2∂α [∂µ (φkαkν) + ∂ν (φkαkµ) − ∂α (φkµkν)]

∂µ ≡ ηµν∂ν Stationary vacuum case (take k0 = 1): 0 = Rµ

0 = 1

2 ∂νF µν for F = dA Aµ = φ kµ Simplest example: Schwarzschild ∼ (Coulomb) × (Coulomb) Why abelian? Exact linear Einstein exact linear YM, i.e., Maxwell.

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 10 / 16

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SLIDE 29

Classical double copy: exact

Kerr-Schild double copy

[RM, O’Connell, White 14] [with Luna, Nicholson 15-18]

“Exact perturbation” gµν = ηµν + φ kµkν where kµ is null and geodesic wrt ηµν and gµν. (kµ = gµνkν = ηµνkν) Einstein equations linearise: gµν = ηµν − φ kµkν Rµν = 1

2∂α [∂µ (φkαkν) + ∂ν (φkαkµ) − ∂α (φkµkν)]

∂µ ≡ ηµν∂ν Stationary vacuum case (take k0 = 1): 0 = Rµ

0 = 1

2 ∂νF µν for F = dA Aµ = φ kµ Simplest example: Schwarzschild ∼ (Coulomb) × (Coulomb) Why abelian? Exact linear Einstein exact linear YM, i.e., Maxwell. Rest of the talk Vacuum here. Kerr-Schild-type ansatz for NS-NS gravity? Why is this double copy?

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 10 / 16

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SLIDE 30

Classical double copy: exact

Double Field Theory

[Siegel ’93] [Hull, Zwiebach ’09 + Hohm ’10]

For our purposes: fancy formulation of NS-NS gravity. Motivation: low-energy effective theory of closed string exhibiting T-duality.

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 11 / 16

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Classical double copy: exact

Double Field Theory

[Siegel ’93] [Hull, Zwiebach ’09 + Hohm ’10]

For our purposes: fancy formulation of NS-NS gravity. Motivation: low-energy effective theory of closed string exhibiting T-duality. Doubled space XM = (xµ, ˜ xµ) , dim = 2D . String on torus: quantised momenta, winding. Mixed by T-duality. DFT idea: (xµ, ˜ xµ) conjugate to (momenta, winding). T-duality: O(D, D). ΛM N ∈ O(D, D) : (Λ)T(J )(Λ) = (J ) . JMN = δµν δµν

  • is O(D, D) metric.

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 11 / 16

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SLIDE 32

Classical double copy: exact

Double Field Theory

[Siegel ’93] [Hull, Zwiebach ’09 + Hohm ’10]

For our purposes: fancy formulation of NS-NS gravity. Motivation: low-energy effective theory of closed string exhibiting T-duality. Doubled space XM = (xµ, ˜ xµ) , dim = 2D . String on torus: quantised momenta, winding. Mixed by T-duality. DFT idea: (xµ, ˜ xµ) conjugate to (momenta, winding). T-duality: O(D, D). ΛM N ∈ O(D, D) : (Λ)T(J )(Λ) = (J ) . JMN = δµν δµν

  • is O(D, D) metric.

T-duality manifest: O(D, D) covariance. Section condition, e.g., ∂/∂˜ xµ = 0 : correct dof, breaks covariance.

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 11 / 16

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SLIDE 33

Classical double copy: exact

Double Field Theory

[Siegel ’93] [Hull, Zwiebach ’09 + Hohm ’10]

For our purposes: fancy formulation of NS-NS gravity. Motivation: low-energy effective theory of closed string exhibiting T-duality. Doubled space XM = (xµ, ˜ xµ) , dim = 2D . String on torus: quantised momenta, winding. Mixed by T-duality. DFT idea: (xµ, ˜ xµ) conjugate to (momenta, winding). T-duality: O(D, D). ΛM N ∈ O(D, D) : (Λ)T(J )(Λ) = (J ) . JMN = δµν δµν

  • is O(D, D) metric.

T-duality manifest: O(D, D) covariance. Section condition, e.g., ∂/∂˜ xµ = 0 : correct dof, breaks covariance. NS-NS fields packaged as tensor and scalar wrt to O(D, D). Generalised metric: HMN =

  • gµν

−gµρBρν Bµρgρν gµν − BµρgρσBσν

  • ∈ O(D, D) .

DFT dilaton d : e−2d = √−g e−2φ .

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 11 / 16

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SLIDE 34

Classical double copy: exact

Kerr-Schild-inspired ansatz

Recall Kerr-Schild ansatz: gµν = ηµν + ϕ kµkν kµ null and geodesic. DFT version: take H0MN = HMN (gµν =ηµν, Bµν =0) ,

[Lee 18] [Cho, Lee 19] [Kim, Lee, RM, Nicholson, Veiga 19]

HMN = H0MN + ϕ

  • KM ¯

KN + KN ¯ KM

  • −1

2 ϕ2 ¯ K 2KMKN KM = 1 √ 2 kµ ηµνkν

  • ¯

KM = 1 √ 2

  • ¯

kµ −ηµν¯ kν

  • where kµ and ¯

kµ are null and satisfy diff. contraints (or ¯ kµ not null).

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 12 / 16

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SLIDE 35

Classical double copy: exact

Kerr-Schild-inspired ansatz

Recall Kerr-Schild ansatz: gµν = ηµν + ϕ kµkν kµ null and geodesic. DFT version: take H0MN = HMN (gµν =ηµν, Bµν =0) ,

[Lee 18] [Cho, Lee 19] [Kim, Lee, RM, Nicholson, Veiga 19]

HMN = H0MN + ϕ

  • KM ¯

KN + KN ¯ KM

  • −1

2 ϕ2 ¯ K 2KMKN KM = 1 √ 2 kµ ηµνkν

  • ¯

KM = 1 √ 2

  • ¯

kµ −ηµν¯ kν

  • where kµ and ¯

kµ are null and satisfy diff. contraints (or ¯ kµ not null). gµν = ηµν − ϕ 1 + ϕ

2 (k · ¯

k) k(µ¯ kν) , Bµν = ϕ 1 + ϕ

2 (k · ¯

k) k[µ¯ kν] . First examples of exact double copy with dilaton and B-field. [Lee 18] JNW solution: fits ansatz, B-field is pure gauge.

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 12 / 16

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SLIDE 36

Classical double copy: exact

Double Field Theory versus Double Copy

Generalised metric HM N induces chirality: PM

N = 1

2

  • δM

N + HM N

, ¯ PM

N = 1

2

  • δM

N − HM N

. Project into chiral and anti-chiral sectors

Ricardo Monteiro (Queen Mary) Double Copy of a Point Charge 13 / 16

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SLIDE 37

Classical double copy: exact

Double Field Theory versus Double Copy

Generalised metric HM N induces chirality: PM

N = 1

2

  • δM

N + HM N

, ¯ PM

N = 1

2

  • δM

N − HM N

. Project into chiral and anti-chiral sectors = left and right moving sectors! (pullback to worldsheet) Kerr-Schild-like ansatz HMN = H0MN + ϕ

  • KM ¯

KN + KN ¯ KM

  • + . . .

Satisfy definite chiralities: (P0)M NKN = KM , (¯ P0)M N ¯ KN = ¯ KM . Double-copy interpretation: KM Aµ ¯ KM ¯ Aµ

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slide-38
SLIDE 38

Classical double copy: exact

Double Field Theory versus Double Copy

Generalised metric HM N induces chirality: PM

N = 1

2

  • δM

N + HM N

, ¯ PM

N = 1

2

  • δM

N − HM N

. Project into chiral and anti-chiral sectors = left and right moving sectors! (pullback to worldsheet) Kerr-Schild-like ansatz HMN = H0MN + ϕ

  • KM ¯

KN + KN ¯ KM

  • + . . .

Satisfy definite chiralities: (P0)M NKN = KM , (¯ P0)M N ¯ KN = ¯ KM . Double-copy interpretation: KM Aµ ¯ KM ¯ Aµ KLT picture of Kerr-Schild double copy!

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slide-39
SLIDE 39

Classical double copy: exact

Double Field Theory versus Double Copy

Generalised metric HM N induces chirality: PM

N = 1

2

  • δM

N + HM N

, ¯ PM

N = 1

2

  • δM

N − HM N

. Project into chiral and anti-chiral sectors = left and right moving sectors! (pullback to worldsheet) Kerr-Schild-like ansatz HMN = H0MN + ϕ

  • KM ¯

KN + KN ¯ KM

  • + . . .

Satisfy definite chiralities: (P0)M NKN = KM , (¯ P0)M N ¯ KN = ¯ KM . Double-copy interpretation: KM Aµ ¯ KM ¯ Aµ KLT picture of Kerr-Schild double copy! Usual DFT basis: (xµ, 0) , (0, ˜ xµ). Mixed by O(D, D). Double-copy basis:

1 2(xµ + ˜

xµ, xµ + ˜ xµ) ,

1 2(xµ − ˜

xµ, ˜ xµ − xµ) .

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SLIDE 40

Classical double copy: exact

DFT equations of motion

‘Generalised diffeomorphisms’ − → curvature tensors: RMN, R. With section condition (∂/∂˜ xµ = 0), NS-NS equations of motion: R(µν) = 0 for metric gµν R[µν] = 0 for B-field Bµν R = 0 for DFT dilaton d

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slide-41
SLIDE 41

Classical double copy: exact

DFT equations of motion

‘Generalised diffeomorphisms’ − → curvature tensors: RMN, R. With section condition (∂/∂˜ xµ = 0), NS-NS equations of motion: R(µν) = 0 for metric gµν R[µν] = 0 for B-field Bµν R = 0 for DFT dilaton d As in Kerr-Schild double copy, assume stationarity (Killing ∂0), k0 = ¯ k0 = 1: 4e−2d Rµ0 = ∂νFνµ = 0 , F = dA , Aµ = e−2dϕ kµ + Cµ , 4e−2d R0µ = ∂ν ¯ Fνµ = 0 , ¯ F = d ¯ A , ¯ Aµ = e−2dϕ ¯ kµ + ¯ Cµ . Cµ , ¯ Cµ absorb non-linearities, non-local.

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SLIDE 42

Classical double copy: exact

DFT equations of motion

‘Generalised diffeomorphisms’ − → curvature tensors: RMN, R. With section condition (∂/∂˜ xµ = 0), NS-NS equations of motion: R(µν) = 0 for metric gµν R[µν] = 0 for B-field Bµν R = 0 for DFT dilaton d As in Kerr-Schild double copy, assume stationarity (Killing ∂0), k0 = ¯ k0 = 1: 4e−2d Rµ0 = ∂νFνµ = 0 , F = dA , Aµ = e−2dϕ kµ + Cµ , 4e−2d R0µ = ∂ν ¯ Fνµ = 0 , ¯ F = d ¯ A , ¯ Aµ = e−2dϕ ¯ kµ + ¯ Cµ . Cµ , ¯ Cµ absorb non-linearities, non-local. Kerr-Schild-like (gµν, Bµν, d) ∼ (‘left-moving’ Aµ) × (‘right-moving’ ¯ Aµ) JNW ∼ (‘left-moving’ Coulomb) × (‘right-moving’ Coulomb)

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SLIDE 43

Conclusion

Conclusion

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SLIDE 44

Conclusion

Conclusion

Double copy of classical solutions possible. Perturbative double copy: generic but messy. Exact double copy: fully non-linear but not generic. JNW ∼ (left-moving Coulomb) × (right-moving Coulomb) Double field theory convenient setting for double copy. KLT interpretation of Kerr-Schild-type double copy

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SLIDE 45

Conclusion

Conclusion

Double copy of classical solutions possible. Perturbative double copy: generic but messy. Exact double copy: fully non-linear but not generic. JNW ∼ (left-moving Coulomb) × (right-moving Coulomb) Double field theory convenient setting for double copy. KLT interpretation of Kerr-Schild-type double copy Much more to explore Larger classes of solutions, duality transf., asymptotic symmetries, . . .

[Luna et al 15; Luna et al 18] [Godazgar et al; Huang et al; Alawadhi et al; Banerjee et al 19]

Aim: general formulation of fully non-linear double copy.

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