Bootstrap for Large N Confining Gauge Theories Alexander Zhiboedov, - - PowerPoint PPT Presentation

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Bootstrap for Large N Confining Gauge Theories Alexander Zhiboedov, - - PowerPoint PPT Presentation

Bootstrap for Large N Confining Gauge Theories Alexander Zhiboedov, Harvard U IGST 2017, Paris, France with S. Caron-Huot, Z. Komargodski, A. Sever Introduction In this talk I discuss theories of weakly interacting higher spin particles in flat


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Bootstrap for Large N Confining Gauge Theories

Alexander Zhiboedov, Harvard U IGST 2017, Paris, France

with S. Caron-Huot, Z. Komargodski, A. Sever

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Introduction

In this talk I discuss theories of weakly interacting higher spin particles in flat space (d>2).

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Introduction

In this talk I discuss theories of weakly interacting higher spin particles in flat space (d>2). These are characterized by: spectrum of particles mi three-point couplings fijk i j k

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Introduction

In this talk I discuss theories of weakly interacting higher spin particles in flat space (d>2). This data is combined into 2-2 scattering amplitude

A(s, t)

These are characterized by: spectrum of particles mi three-point couplings fijk i j k

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What is WIHS?

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What is WIHS?

A(s, t) =

Two-to-two scattering amplitude

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What is WIHS?

A(s, t) =

Two-to-two scattering amplitude

  • weakly coupled ≡

meromorphic

fssφ

fφss

θ

m2

φ, J

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What is WIHS?

A(s, t) =

Two-to-two scattering amplitude

  • weakly coupled ≡

meromorphic

fssφ

fφss

θ

m2

φ, J

  • unitarity

A(s, t)|s'm2

φ ' f 2

ssφ

PJ(1 +

2t m2

φ4m2 s )

s m2

φ positive

cos θ

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What is WIHS?

A(s, t) =

Two-to-two scattering amplitude

  • weakly coupled ≡

meromorphic

fssφ

fφss

θ

m2

φ, J

  • unitarity

A(s, t)|s'm2

φ ' f 2

ssφ

PJ(1 +

2t m2

φ4m2 s )

s m2

φ positive

cos θ

A(s, t) = A(t, s)

  • crossing
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Examples

  • QFT

A(s, t) = 1 s − m2 + 1 t − m2

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Examples

  • fundamental strings

[Veneziano]

A(s, t) = Γ(−s)Γ(−t) Γ(−s − t)

  • QFT

A(s, t) = 1 s − m2 + 1 t − m2

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Examples

  • fundamental strings

[Veneziano]

A(s, t) = Γ(−s)Γ(−t) Γ(−s − t)

  • QFT

A(s, t) = 1 s − m2 + 1 t − m2

  • confining gauge theories/large N QCD

[Kronfeld]

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Examples

  • fundamental strings

[Veneziano]

A(s, t) = Γ(−s)Γ(−t) Γ(−s − t)

  • QFT

A(s, t) = 1 s − m2 + 1 t − m2

  • confining gauge theories/large N QCD

[Kronfeld]

  • something else???
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  • soft high energy limit

lim

s→∞ A(s, t0) < sJ0

J0 t s

What is WIHS?

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  • soft high energy limit

lim

s→∞ A(s, t0) < sJ0

J0 t s

What is WIHS?

clash with unitarity!

A(s, t) ∼ sJ0 ⇒

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  • soft high energy limit

lim

s→∞ A(s, t0) < sJ0

J0 t s

  • no accumulation point in the spectrum

#{of particles mi < E} < ∞

What is WIHS?

clash with unitarity!

A(s, t) ∼ sJ0 ⇒

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  • soft high energy limit

lim

s→∞ A(s, t0) < sJ0

J0 t s

  • no accumulation point in the spectrum

#{of particles mi < E} < ∞

What is WIHS?

clash with unitarity!

A(s, t) ∼ sJ0 ⇒

  • interacting higher spin ≡ exchange of a particle with spin > 2

(softness is causality)

J=2 - Shapiro time delay

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Examples

  • QFT

A(s, t) = 1 s − m2 + 1 t − m2

high energy is not soft

lim

s→∞ A(s, t0) < sJ0

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Examples

  • QFT

A(s, t) = 1 s − m2 + 1 t − m2

high energy is not soft

lim

s→∞ A(s, t0) < sJ0

  • fundamental strings

Very non-generic:

  • linear Regge trajectories
  • spectrum degeneracy

[Veneziano]

A(s, t) = Γ(−s)Γ(−t) Γ(−s − t)

lim

s→∞ A(s, t) ∼ sα0t

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Examples

  • QFT

A(s, t) = 1 s − m2 + 1 t − m2

high energy is not soft

lim

s→∞ A(s, t0) < sJ0

  • confining gauge theories
  • Regge trajectories are not linear
  • spectrum is not degenerate
  • fundamental strings

Very non-generic:

  • linear Regge trajectories
  • spectrum degeneracy

[Veneziano]

A(s, t) = Γ(−s)Γ(−t) Γ(−s − t)

lim

s→∞ A(s, t) ∼ sα0t

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Goal

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Goal

In principle, this is a well-defined math problem and such functions are subject to a classification.

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Goal

In principle, this is a well-defined math problem and such functions are subject to a classification. In practice, almost nothing is known.

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Goal

In principle, this is a well-defined math problem and such functions are subject to a classification. In practice, almost nothing is known. Can we bootstrap it?

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Goal

In principle, this is a well-defined math problem and such functions are subject to a classification. In practice, almost nothing is known. Can we bootstrap it?

  • 1. Universal properties
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Goal

In principle, this is a well-defined math problem and such functions are subject to a classification. In practice, almost nothing is known. Can we bootstrap it?

  • 1. Universal properties

[El-Showk, Paulos, Poland, Rychkov, Simmons-Duffin, Vichi]

  • 2. Special points
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Hint

What fundamental strings and YM strings have in common?

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Hint

What fundamental strings and YM strings have in common? What do we mean by strings?

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t j(t)

ST

(mass) (spin)

lim

s→∞ A(s, t) ∼ sj(t)

spectrum scattering

The Regge Trajectory j(t)

Γ(−s)Γ(−t) Γ(−t − s)

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t j(t)

ST Y M

(mass) (spin)

lim

s→∞ A(s, t) ∼ sj(t)

spectrum scattering

The Regge Trajectory j(t)

Γ(−s)Γ(−t) Γ(−t − s)

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t j(t)

ST Y M

(mass) (spin)

lim

s→∞ A(s, t) ∼ sj(t)

spectrum

non-universal

?

scattering

The Regge Trajectory j(t)

Γ(−s)Γ(−t) Γ(−t − s)

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t j(t)

ST Y M

(mass) (spin)

lim

s→∞ A(s, t) ∼ sj(t)

universal

spectrum

non-universal

?

scattering

The Regge Trajectory j(t)

Γ(−s)Γ(−t) Γ(−t − s)

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s

t u

s c a t t e r i n g scattering s c a t t e r i n g spectrum s p e c t r u m s p e c t r u m

Mandelstam Plane

Universal/Imaginary Angles Non-universal/Real Angles Key idea: scattering at imaginary angles is universal

s, t > 0

s > 0, − s < t < 0

s + t + u = 0

s = E2

cm

t = −E2

cm

2 (1 − cos θ)

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Part I

Asymptotic Uniqueness of the Veneziano amplitude

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Result Part I

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞ s/t fixed

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Result Part I

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞ s/t fixed

∼ E2

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Result Part I

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form

limit of the Veneziano amplitude

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞ s/t fixed

∼ E2

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Result

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞ s/t fixed

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Result

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞ s/t fixed

  • amplitude is exponentially large (unitarity universality)

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Result

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞ s/t fixed

  • stringy. Infinitely many asymptotically linear Regge trajectories
  • bject of transverse size

= a string

∼ log(s)

b

j(t) = α0t + corrections +parallel trajectories

Im A(s, b) ∼ e−

b2 α0 log s

  • amplitude is exponentially large (unitarity universality)

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Result

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞ s/t fixed

  • stringy. Infinitely many asymptotically linear Regge trajectories
  • bject of transverse size

= a string

∼ log(s)

b

j(t) = α0t + corrections +parallel trajectories

Im A(s, b) ∼ e−

b2 α0 log s

  • amplitude is exponentially large (unitarity universality)

  • insensitive to the microscopic spectrum degeneracy
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Bootstrap (Leading Order)

For s,t large and positive a thermodynamic picture emerges

s, t → ∞ s/t fixed

lim log A ((1 + i✏)s, (1 + i✏)t)

[Caron-Huot, Komargodski, Sever, AZ] 1

−1

J even J odd

PJ(x)

we are here

Partial wave

Complex s plane at fixed real t

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Bootstrap (Leading Order)

For s,t large and positive a thermodynamic picture emerges

s, t → ∞ s/t fixed

lim log A ((1 + i✏)s, (1 + i✏)t)

[Caron-Huot, Komargodski, Sever, AZ] 1

−1

J even J odd

PJ(x)

we are here

Partial wave

⇒ • All residues are positive

Complex s plane at fixed real t

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Bootstrap (Leading Order)

For s,t large and positive a thermodynamic picture emerges

s, t → ∞ s/t fixed

lim log A ((1 + i✏)s, (1 + i✏)t)

[Caron-Huot, Komargodski, Sever, AZ] 1

−1

J even J odd

PJ(x)

we are here

Partial wave

⇒ • At least one zero between every two poles

  • There could be more zeros

⇒ • All residues are positive

Complex s plane at fixed real t

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Bootstrap (Leading Order)

For s,t large and positive a thermodynamic picture emerges

s, t → ∞ s/t fixed

lim log A ((1 + i✏)s, (1 + i✏)t)

[Caron-Huot, Komargodski, Sever, AZ] 1

−1

J even J odd

PJ(x)

we are here

Partial wave

⇒ • At least one zero between every two poles

  • There could be more zeros

⇒ • All residues are positive

log A(s, t) ' j(t) log s ⇒ j(t) = Diss log A = X (zeros − poles) Complex s plane at fixed real t

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poles zeros

Bootstrap (Leading Order)

For s,t large and positive a thermodynamic picture emerges

−t

s

We are here

s, t → ∞ s/t fixed

lim log A ((1 + i✏)s, (1 + i✏)t)

distribution of excess zeros ρ

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Bootstrap (Leading Order)

log A = Z d2z ρ(t; z, ¯ z) log(z − s) The amplitude takes the form

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Bootstrap (Leading Order)

log A = Z d2z ρ(t; z, ¯ z) log(z − s) The amplitude takes the form

dimensional analysis at large s,t

ρ(t; z, ¯ z) = j(t) t2 ρ(z/t, ¯ z/t)

In the large t limit we can write for the distribution

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Bootstrap (Leading Order)

log A = Z d2z ρ(t; z, ¯ z) log(z − s)

log A(s, t) = j(t) Z d2z ρ(z, ¯ z) log(1 − s tz )

normalization unitarity

ρ(z, ¯ z) ≥ 0 Z d2z ρ(z, ¯ z) = 1

The amplitude takes the form

dimensional analysis at large s,t

ρ(t; z, ¯ z) = j(t) t2 ρ(z/t, ¯ z/t)

In the large t limit we can write for the distribution

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Bootstrap (Leading Order)

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Unitarity

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Unitarity

The distribution of the zeros comes from a sum of Legendre polynomials with positive coefficients

j(t)

X

n=0

C2

nPn (1 + 2β)

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Unitarity

  • 1
  • 0.015

0.015

together with the Regge limit (3pt couplings cannot be too small) implies finite support of the excess zeros

β = s t

  • β + 1

2

  • ≤ 1

The distribution of the zeros comes from a sum of Legendre polynomials with positive coefficients

j(t)

X

n=0

C2

nPn (1 + 2β)

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Bootstrap (Leading Order)

log A(s, t) = j(t) Z d2z ρ(z, ¯ z) log(1 − s tz )

normalization unitarity

ρ(z, ¯ z) ≥ 0 Z d2z ρ(z, ¯ z) = 1

Assume

j(t) = tk

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Bootstrap (Leading Order)

2d “electric field”

ρ(z, ¯ z)

2d “electric potential” for a positive distribution of charge

V (β) = log A(s, t) j(t) = Z d2z ρ(z, ¯ z) log(1 − β z ) =

E(β) = t ∂sV (s/t) = Z d2z ρ(z, ¯ z) β − z =

s/t

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Bootstrap (Leading Order)

2d “electric field”

ρ(z, ¯ z)

2d “electric potential” for a positive distribution of charge E(β) analytic where ρ = 0 crossing

+

E(β) = 1 β 2F1(k, k, k + 1; −1/β) = 1 β − k2 k + 1 1 β2 + . . .

M1

V (β) = log A(s, t) j(t) = Z d2z ρ(z, ¯ z) log(1 − β z ) =

E(β) = t ∂sV (s/t) = Z d2z ρ(z, ¯ z) β − z =

s/t

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Bootstrap (Leading Order)

2d “electric field”

ρ(z, ¯ z)

2d “electric potential” for a positive distribution of charge E(β) analytic where ρ = 0 crossing

+

E(β) = 1 β 2F1(k, k, k + 1; −1/β) = 1 β − k2 k + 1 1 β2 + . . .

M1

V (β) = log A(s, t) j(t) = Z d2z ρ(z, ¯ z) log(1 − β z ) =

E(β) = t ∂sV (s/t) = Z d2z ρ(z, ¯ z) β − z =

s/t

k ≤ 1

lim

β→∞ E(β) = 1

β + . . . ⇒ lim

β→0 E(β) = −k βk−1 log β + . . .

k ≤ 1 ⇒

crossing

β

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Bootstrap (Leading Order)

mathematical identity

∂2

θ log

X

n

C2

n Pn(cos θ) ≥ 0

M1 ≥ 1 2

k ≥ 1

k = 1

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Bootstrap (Leading Order)

mathematical identity

∂2

θ log

X

n

C2

n Pn(cos θ) ≥ 0

M1 ≥ 1 2

k ≥ 1

k = 1

for ρ(x, x) = 1

The unique solution is

−t

s

log A(s, t) = α0t

1

Z dxρ(x) log ⇣ 1 + s tx ⌘ = α0 [(s + t) log(s + t) − s log s − t log t]

−1 < x < 0

= classical string theory

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Part II

Universal Correction to the Veneziano Amplitude

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Result Part II

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

∼ E2

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Result Part II

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

∼ E2

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Result Part II

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

∼ E

1 2

∼ E2

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Result Part II

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form

elliptic integral of the first kind EllipticK[x]

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

∼ E

1 2

∼ E2

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Result Part II

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form

elliptic integral of the first kind EllipticK[x] correction due to the slowdown of the string (massive endpoints)/spectrum non-degeneracy

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

∼ E

1 2

∼ E2

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Result Part II

The high energy limit of WIHS amplitudes at imaginary scattering angles takes the form

elliptic integral of the first kind EllipticK[x] correction due to the slowdown of the string (massive endpoints)/spectrum non-degeneracy corrections are O(1)

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

∼ E

1 2

∼ E2

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Result

δ log A(s, t) = −16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

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Result

δ log A(s, t) = −16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

  • worldsheet: slowdown of the string endpoints

m m

[Chodos, Thorn, 74’]

j(t) = α0 ✓ t − 8√π 3 m3/2t1/4 + ... ◆

[Sonnenschein et al.] [Wilczek] [Baker, Steinke]

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Result

δ log A(s, t) = −16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

  • bootstrap: removal of the spectrum degeneracy

jsub−leading(t) 6= jleading(t) + integer

  • worldsheet: slowdown of the string endpoints

m m

[Chodos, Thorn, 74’]

j(t) = α0 ✓ t − 8√π 3 m3/2t1/4 + ... ◆

[Sonnenschein et al.] [Wilczek] [Baker, Steinke]

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  • Scattering of Strings With Massive Endpoints
  • Universality (Holography & EFT of Long Strings)
  • Bootstrap
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Worldsheet Computation (review)

s/t fixed |s|, |t| → ∞

lim A(s, t) = e−SE(s,t)

[Gross, Mende] [Gross, Mañes] [Alday, Maldacena]

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Worldsheet Computation (review)

s/t fixed |s|, |t| → ∞

lim A(s, t) = e−SE(s,t)

  • real scattering angles (amplitude is small)

SE 1

[Gross, Mende] [Gross, Mañes] [Alday, Maldacena]

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Worldsheet Computation (review)

s/t fixed |s|, |t| → ∞

lim A(s, t) = e−SE(s,t)

  • real scattering angles (amplitude is small)

SE 1

  • imaginary scattering angles (amplitude is large) SE 1

[Gross, Mende] [Gross, Mañes] [Alday, Maldacena]

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Worldsheet Computation (review)

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Worldsheet Computation (review)

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x − i X

j

kj · x(σj)

Flat space

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Worldsheet Computation (review)

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x − i X

j

kj · x(σj)

Flat space

  • general solution

0 = i

X

i

i log |z − σi|2

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Worldsheet Computation (review)

  • Virasoro (scattering equations)

X

j

ki · kj σi − σj = 0

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x − i X

j

kj · x(σj)

Flat space

  • general solution

0 = i

X

i

i log |z − σi|2

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Worldsheet Computation (review)

  • Virasoro (scattering equations)

X

j

ki · kj σi − σj = 0

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x − i X

j

kj · x(σj)

Flat space log A(s, t) = α0 [(s + t) log(s + t) − s log s − t log t] ⇒

s, t > 0

  • general solution

0 = i

X

i

i log |z − σi|2

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Adding The Mass

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Adding The Mass

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x + m Z dσ p |∂σx|2 − i X

j

kj · x(σj)

[Chodos, Thorn]

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Adding The Mass

Modified boundary condition: 1 2πα0 ∂τx + m ∂σ ∂σx √∂σx · ∂σx = i X

j

kj δ(σ − σj)

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x + m Z dσ p |∂σx|2 − i X

j

kj · x(σj)

[Chodos, Thorn]

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SLIDE 83

Adding The Mass

Modified boundary condition: 1 2πα0 ∂τx + m ∂σ ∂σx √∂σx · ∂σx = i X

j

kj δ(σ − σj) is zero for a free string!

∂σx0 · ∂σx0 = 0

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x + m Z dσ p |∂σx|2 − i X

j

kj · x(σj)

[Chodos, Thorn]

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Adding The Mass

Modified boundary condition: 1 2πα0 ∂τx + m ∂σ ∂σx √∂σx · ∂σx = i X

j

kj δ(σ − σj) is zero for a free string!

∂σx0 · ∂σx0 = 0

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x + m Z dσ p |∂σx|2 − i X

j

kj · x(σj)

[Chodos, Thorn]

The expansion reorganizes itself in terms of :

√m

xµ = xµ

0 + √m xµ 1 + ...

S = S0 + √mS1 + mS2 + m3/2S3

slide-85
SLIDE 85

Adding The Mass

Modified boundary condition: 1 2πα0 ∂τx + m ∂σ ∂σx √∂σx · ∂σx = i X

j

kj δ(σ − σj) is zero for a free string!

∂σx0 · ∂σx0 = 0

SE = 1 2πα0 Z d2z ∂x · ¯ ∂x + m Z dσ p |∂σx|2 − i X

j

kj · x(σj)

[Chodos, Thorn]

The expansion reorganizes itself in terms of :

√m

xµ = xµ

0 + √m xµ 1 + ...

S = S0 + √mS1 + mS2 + m3/2S3

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SLIDE 86

The on-shell action evaluates to

Adding The Mass

Lb = √ 2πα0 m Z dσ (∂2

σx0 · ∂2 σx0)1/4

SE = SGM + 2 3mLb + ...

slide-87
SLIDE 87

Gross-Mende solution

The on-shell action evaluates to

Adding The Mass

Lb = √ 2πα0 m Z dσ (∂2

σx0 · ∂2 σx0)1/4

SE = SGM + 2 3mLb + ...

slide-88
SLIDE 88

Gross-Mende solution

The on-shell action evaluates to

reparameterization invariant

Adding The Mass

Lb = √ 2πα0 m Z dσ (∂2

σx0 · ∂2 σx0)1/4

SE = SGM + 2 3mLb + ...

slide-89
SLIDE 89

Gross-Mende solution

The on-shell action evaluates to

reparameterization invariant

Adding The Mass

For four external particles

δ log A(s, t) = −16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + O(m5/2)

Lb = √ 2πα0 m Z dσ (∂2

σx0 · ∂2 σx0)1/4

SE = SGM + 2 3mLb + ...

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SLIDE 90

Gross-Mende solution

non-universal O(t−1/4)

The on-shell action evaluates to

reparameterization invariant

Adding The Mass

For four external particles

δ log A(s, t) = −16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + O(m5/2)

Lb = √ 2πα0 m Z dσ (∂2

σx0 · ∂2 σx0)1/4

SE = SGM + 2 3mLb + ...

slide-91
SLIDE 91

Emergent s-u Crossing Symmetry

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

slide-92
SLIDE 92

Emergent s-u Crossing Symmetry

The s-t crossing is manifest: log A(s, t) = log A(t, s)

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

slide-93
SLIDE 93

Emergent s-u Crossing Symmetry

The s-t crossing is manifest: log A(s, t) = log A(t, s) What about the s-u crossing?

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

slide-94
SLIDE 94

Emergent s-u Crossing Symmetry

The s-t crossing is manifest: log A(s, t) = log A(t, s) What about the s-u crossing? log A(s, t) = Re[log A(u, t)] u = −s − t

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

slide-95
SLIDE 95

Emergent s-u Crossing Symmetry

The s-t crossing is manifest: log A(s, t) = log A(t, s) What about the s-u crossing? log A(s, t) = Re[log A(u, t)] u = −s − t 1 2 3 4 1 2 3 4 ???

lim log A(s, t) = α0 [(s + t) log(s + t) − s log(s) − t log(t)]

s, t → ∞

s/t fixed

−16√π 3 α0m3/2 ✓ s t s + t ◆ 1

4 

K ✓ s s + t ◆ + K ✓ t s + t ◆ + . . .

slide-96
SLIDE 96

Emergent s-u Crossing Symmetry

[Komatsu]

1 2

3

4 1

2

3 4 ???

slide-97
SLIDE 97

Emergent s-u Crossing Symmetry

[Komatsu]

1 2

3

4 1

2

3 4 ???

slide-98
SLIDE 98

Asymptotic s-u Crossing

Equivalently, the asymptotic s-u crossing is: dDiscs log A(s, t) ≡ log A(−s − t + i✏, t) + log A(−s − t − i✏, t) − 2 log A(s, t) = 0 Double discontinuity is zero!

slide-99
SLIDE 99

Why is the correction universal?

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SLIDE 100

Why is the correction universal?

Why is the massive ends model physical?

slide-101
SLIDE 101

Holographic Argument

Holographic dual of a confining gauge theory: ds2 = dr2 + f(r) dx2

1,d−1

  • AdS in the UV

lim

r→∞ f(r) = e2r

  • Cutoff in the IR

f(0) = 1

[Sonnenschein] [Erdmenger et al.]

Holographic radial direction

r x

slide-102
SLIDE 102

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

IR r0 Holographic radial direction Flavor brane UV

slide-103
SLIDE 103

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

real scattering angles

[Polchinski, Strassler]

IR r0 Holographic radial direction Flavor brane UV

slide-104
SLIDE 104

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

real scattering angles imaginary scattering angles

[Polchinski, Strassler]

IR r0 Holographic radial direction Flavor brane UV

slide-105
SLIDE 105

IR r0 Holographic radial direction Flavor brane UV

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-106
SLIDE 106

IR r0 Holographic radial direction Flavor brane UV

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-107
SLIDE 107

IR r0 Holographic radial direction Flavor brane UV

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-108
SLIDE 108

IR r0 Holographic radial direction Flavor brane UV

string in flat space

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-109
SLIDE 109

IR r0 Holographic radial direction Flavor brane UV

m

string in flat space

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-110
SLIDE 110

IR r0 Holographic radial direction Flavor brane UV

m

m m

effective description

m2α0 1

string in flat space

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-111
SLIDE 111

IR r0 Holographic radial direction Flavor brane UV

m

m m

effective description

m2α0 1

string in flat space

  • At the holographic model reduces to the string with massive ends

s, t 1

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-112
SLIDE 112

IR r0 Holographic radial direction Flavor brane UV

m

m m

effective description

m2α0 1

string in flat space

  • At the holographic model reduces to the string with massive ends

s, t 1

  • Insensitive to the details of the background

Polchinski-Strassler Mechanism

For mesons we add a space-filling flavor brane

[Polchinski, Strassler]

slide-113
SLIDE 113

EFT of Long Strings

[Aharony et al.] [Hellerman et al.] [Polchinski, Strominger] [Dubovsky et al.]

slide-114
SLIDE 114

EFT of Long Strings

[Aharony et al.] [Hellerman et al.] [Polchinski, Strominger] [Dubovsky et al.]

  • boundary corrections (open strings)

Unique in the effective theory of open strings

j(t) = α0 ✓ t − 8√π 3 m3/2t1/4 ◆

[Hellerman, Swanson]

slide-115
SLIDE 115

EFT of Long Strings

  • quantum corrections

Polchinski-Strominger term

(∂2x · ¯ ∂x)(∂x · ¯ ∂2x) (∂x · ¯ ∂x)2

[Aharony et al.] [Hellerman et al.] [Polchinski, Strominger] [Dubovsky et al.]

  • boundary corrections (open strings)

Unique in the effective theory of open strings

j(t) = α0 ✓ t − 8√π 3 m3/2t1/4 ◆

[Hellerman, Swanson]

slide-116
SLIDE 116

EFT of Long Strings

  • quantum corrections

Polchinski-Strominger term

(∂2x · ¯ ∂x)(∂x · ¯ ∂2x) (∂x · ¯ ∂x)2

  • higher derivative corrections (closed strings)

[Aharony et al.] [Hellerman et al.] [Polchinski, Strominger] [Dubovsky et al.]

  • boundary corrections (open strings)

Unique in the effective theory of open strings

j(t) = α0 ✓ t − 8√π 3 m3/2t1/4 ◆

[Hellerman, Swanson]

slide-117
SLIDE 117

EFT of Long Strings

  • quantum corrections

Polchinski-Strominger term

(∂2x · ¯ ∂x)(∂x · ¯ ∂2x) (∂x · ¯ ∂x)2

  • higher derivative corrections (closed strings)

[Aharony et al.] [Hellerman et al.] [Polchinski, Strominger] [Dubovsky et al.]

  • boundary corrections (open strings)

Unique in the effective theory of open strings

j(t) = α0 ✓ t − 8√π 3 m3/2t1/4 ◆

[Hellerman, Swanson]

slide-118
SLIDE 118

Bootstrap (Correction)

  • Spectrum Non-degeneracy/Support of excess zeros

−t

s

non-degeneracy zeros

slide-119
SLIDE 119

Bootstrap (Correction)

  • Spectrum Non-degeneracy/Support of excess zeros

−t

s

non-degeneracy zeros density>0

slide-120
SLIDE 120

Bootstrap (Correction)

  • Spectrum Non-degeneracy/Support of excess zeros

−t

s

non-degeneracy zeros

Indeed, the massive ends correction is of this form!

density>0

slide-121
SLIDE 121

Bootstrap (Assumptions)

slide-122
SLIDE 122
  • Unitarity and the s-t crossing are not enough

log A(s, t) = log A(t, s)

Bootstrap (Assumptions)

slide-123
SLIDE 123
  • Unitarity and the s-t crossing are not enough

log A(s, t) = log A(t, s)

Bootstrap (Assumptions)

  • Impose the s-u crossing

dDiscs log A(s, t) = 0

s

t

u

slide-124
SLIDE 124
  • Unitarity and the s-t crossing are not enough

log A(s, t) = log A(t, s)

Bootstrap (Assumptions)

  • Impose the s-u crossing

dDiscs log A(s, t) = 0

s

t

u

  • boundary type

δ log A(s, t) = f(s, t) + f(t, s)

corrects the trajectory only in one channel

slide-125
SLIDE 125

Bootstrap (Integral Equation)

The extra condition leads to an integral equation δρk(y) =

1

Z dx [K(y, x) + K(1 − y, 1 − x)] δρk(x)

+(1 − y)k−1 π sin πk ✓ y x + y − x y + k log x (1 − y) x + y − x y ◆

δj(t) = tk

correction to the trajectory correction to the distribution

K(y, x) = cot πk π ✓ y P 1 x − y − k log x |x − y| ◆

slide-126
SLIDE 126

δρk(y) =

1

Z dx [K(y, x) + K(1 − y, 1 − x)] δρk(x)

Bootstrap (Integral Equation)

δj(t) = tk

slide-127
SLIDE 127
  • The correction we found obeys the equation

δρk(y) =

1

Z dx [K(y, x) + K(1 − y, 1 − x)] δρk(x)

Bootstrap (Integral Equation)

δj(t) = tk

slide-128
SLIDE 128
  • The correction we found obeys the equation

δρk(y) =

1

Z dx [K(y, x) + K(1 − y, 1 − x)] δρk(x)

Bootstrap (Integral Equation)

δj(t) = tk

  • One can show that the solution is of the form

ρs(x) = xk−1

X

n=0

xn(an log x + bn) .

slide-129
SLIDE 129
  • The correction we found obeys the equation
  • Easy to show that only k=1/4, k=3/4 are possible

δρk(y) =

1

Z dx [K(y, x) + K(1 − y, 1 − x)] δρk(x)

Bootstrap (Integral Equation)

δj(t) = tk

  • One can show that the solution is of the form

ρs(x) = xk−1

X

n=0

xn(an log x + bn) .

slide-130
SLIDE 130
  • The correction we found obeys the equation
  • Easy to show that only k=1/4, k=3/4 are possible

δρk(y) =

1

Z dx [K(y, x) + K(1 − y, 1 − x)] δρk(x)

Bootstrap (Integral Equation)

δj(t) = tk

  • One can show that the solution is of the form

ρs(x) = xk−1

X

n=0

xn(an log x + bn) .

  • To prove the uniqueness we do numerics

χ2 =

nmax

X

n=0

(aLHS

n

− aRHS

n

)2 + (bLHS

n

− bRHS

n

)2

Minimize

Truncation

slide-131
SLIDE 131

Conclusions and Open Questions

slide-132
SLIDE 132

Conclusions and Open Questions

  • Relax some assumptions
slide-133
SLIDE 133

Conclusions and Open Questions

  • Relax some assumptions
  • Removal of the degeneracy and Hagedorn
slide-134
SLIDE 134

Conclusions and Open Questions

  • Relax some assumptions
  • Non-universal regime

[Numerical bootstrap, graviton, DIS?]

  • Removal of the degeneracy and Hagedorn
slide-135
SLIDE 135

Conclusions and Open Questions

  • Relax some assumptions
  • Non-universal regime

[Numerical bootstrap, graviton, DIS?]

  • Bootstrap in AdS (Mellin space)

[Theories with accumulation?]

  • Removal of the degeneracy and Hagedorn
slide-136
SLIDE 136

Conclusions and Open Questions

  • Relax some assumptions
  • Non-universal regime

[Numerical bootstrap, graviton, DIS?]

  • Bootstrap in AdS (Mellin space)

[Theories with accumulation?]

  • Removal of the degeneracy and Hagedorn
  • Quantum theories

[Universal?]

slide-137
SLIDE 137

Conclusions and Open Questions

  • Relax some assumptions
  • Non-universal regime

[Numerical bootstrap, graviton, DIS?]

  • Bootstrap in AdS (Mellin space)

[Theories with accumulation?] thank you!

  • Removal of the degeneracy and Hagedorn
  • Quantum theories

[Universal?]

slide-138
SLIDE 138