SLIDE 1
Reflections on conformal spectra
Petr Kravchuk
with Hyungrok Kim and Hirosi Ooguri
Walter Burke Institute for Theoretical Physics, Caltech
CERN, 14 Dec 2015
SLIDE 2 Outline
- 1. Convergence bounds for large ∆
- 2. Cardy-like formula for large ∆
- 3. A convergence bound for finite ∆
SLIDE 3 The problem
Consider the state in a Euclidean CFTd | ri = (r) |i ,
- r the four point function on the real line with x = ¯
x = r2 G4(x) = h| (1)(x, ¯ x) |i / h r| ri .
SLIDE 4 The problem
Consider the state in a Euclidean CFTd | ri = (r) |i ,
- r the four point function on the real line with x = ¯
x = r2 G4(x) = h| (1)(x, ¯ x) |i / h r| ri . Using ⇥ OPE, one can decompose | ri = X
O
COVO(r) |Oi G4(x) = X
O
C 2
Ox2∆φF∆,`(x) /
X
O
C 2
O hO| V † O(r)VO(r) |Oi
SLIDE 5
The problem
Suppose we want to understand | ri = X
O
COVO(r) |Oi .
SLIDE 6
The problem
Suppose we want to understand | ri = X
O
COVO(r) |Oi . Consider the CDF F(∆⇤, x) = h r| P∆O<∆∗ | ri h r| ri = 1 G ∆∗
4
(x) G4(x) , where G ∆∗
4
(x) = X
O,∆O>∆∗
C 2
Ox2∆φF∆,`(x)
[Pappadopulo,Rychkov,Espin,Rattazzi ’12; Rychkov,Yvernay ’15]
SLIDE 7
A simpler problem
Ignore conformal symmetry, use only scaling symmetry ! “scaling blocks”, G4(x) = X
O
C 2
Ox∆O2∆φ =
Z 1 x∆2∆φg(s)(∆)d∆.
SLIDE 8
A simpler problem
Ignore conformal symmetry, use only scaling symmetry ! “scaling blocks”, G4(x) = X
O
C 2
Ox∆O2∆φ =
Z 1 x∆2∆φg(s)(∆)d∆. From [PRER ’12], in a given theory, for sufficiently large ∆⇤ G ∆∗
4
(x) . 1 Γ(2∆ + 1)∆2∆φ
⇤
x∆∗2∆φ. Can we obtain more information on the structure of F(∆⇤, x)?
SLIDE 9
Crossing symmetry
Using a different channel for OPE expansion one finds G4(x) = G4(1 x), and so @nG4(x) = (@)nG4(1 x).
SLIDE 10
Crossing symmetry
Using a different channel for OPE expansion one finds G4(x) = G4(1 x), and so @nG4(x) = (@)nG4(1 x). At x = 1/2 one obtains Z 1 [∆ 2∆](2k+1)(s)
1/2(∆)d∆ = 0,
[↵](n) = x↵+n@nx↵ = ↵(↵ 1) . . . (↵ n + 1) (s)
x (∆) = x∆2∆φg(s)(∆)
SLIDE 11
Crossing symmetry
Suppose ∆ 1 in Z 1 [∆ 2∆](2k+1)(s)
1/2(∆)d∆ = 0,
Then for k ⌧ p∆ approximate [∆ 2∆](2k+1) ' (∆ 2∆)2k+1, Z 1
2∆φ
w2k+1(s)
1/2(w + 2∆)dw ' 0.
This suggests that (s)
1/2(w + 2∆) is approximately symmetric
around w = 0.
SLIDE 12
Reflection symmetry
Suppose the symmetry is exact, (s)
1/2(∆) = (s) 1/2(4∆ ∆).
SLIDE 13
Reflection symmetry
Suppose the symmetry is exact, (s)
1/2(∆) = (s) 1/2(4∆ ∆).
Normalize R (s)
1/2(∆)d∆ = 1.
Then F(∆⇤, 1/2) = R ∆∗ (s)
1/2(∆)d∆ is antisymmetric up to a
constant.
SLIDE 14 Reflection symmetry
Suppose the symmetry is exact, (s)
1/2(∆) = (s) 1/2(4∆ ∆).
Normalize R (s)
1/2(∆)d∆ = 1.
Then F(∆⇤, 1/2) = R ∆∗ (s)
1/2(∆)d∆ is antisymmetric up to a
constant.
2 Δϕ 4 Δϕ
Δ
1 2
1 ℱ
SLIDE 15 Reflection symmetry
Suppose the symmetry is exact, (s)
1/2(∆) = (s) 1/2(4∆ ∆).
Normalize R (s)
1/2(∆)d∆ = 1.
Then F(∆⇤, 1/2) = R ∆∗ (s)
1/2(∆)d∆ is antisymmetric up to a
constant.
2 Δϕ 4 Δϕ
Δ
1 2
1 ℱ
SLIDE 16 Reflection symmetry
Suppose the symmetry is exact, (s)
1/2(∆) = (s) 1/2(4∆ ∆).
Normalize R (s)
1/2(∆)d∆ = 1.
Then F(∆⇤, 1/2) = R ∆∗ (s)
1/2(∆)d∆ is antisymmetric up to a
constant.
2 Δϕ 4 Δϕ
Δ
1 2
1 ℱ
G4(x) = x2∆φ2∆φ or G4(x) = x2∆φ + (1 x)2∆φ
SLIDE 17
Reflection symmetry
For general x the reflection is between (s)
x
and (s)
1x, relating
∆ 2∆ x $ ∆ 2∆ 1 x
SLIDE 18
Reflection symmetry
For general x the reflection is between (s)
x
and (s)
1x, relating
∆ 2∆ x $ ∆ 2∆ 1 x Let x > 1/2, ∆x = 2∆φ
1x . Then (s) 1x(∆) = 0 for ∆ < 0 )
(s)
x (∆) ' 0 for ∆ ∆x.
Δx
Δ
1 ℱ
SLIDE 19
Saddle point interpretation
The same relation for general x can be obtained if one assumes that the four-point function is dominated by a saddle point at ∆ = ∆(x), ∆(x) = 2∆ + @ log G4(x) @ log x .
SLIDE 20
Saddle point interpretation
The same relation for general x can be obtained if one assumes that the four-point function is dominated by a saddle point at ∆ = ∆(x), ∆(x) = 2∆ + @ log G4(x) @ log x . G4(x) = G4(1 x) ) ∆(x) 2∆ x = ∆(1 x) 2∆ 1 x
SLIDE 21
Threshold bound
Can we compute a bound on the tail which exhibits ∆x threshold?
SLIDE 22
Threshold bound
Can we compute a bound on the tail which exhibits ∆x threshold? Consider the linear programming formulation [Rattazzi,Rychkov,Tonni,Vichi 2008] (s)
1/2(∆) 0
Z 1 (s)
1/2(∆)d∆ = 1
Z 1 [∆ 2∆](2k+1)(s)
1/2(∆)d∆ = 0
max Z 1
∆∗
(s)
1/2(∆)d∆ =?
SLIDE 23
Threshold bound
Can we compute a bound on the tail which exhibits ∆x threshold? Consider the linear programming formulation [Rattazzi,Rychkov,Tonni,Vichi 2008] (s)
1/2(∆) 0
Z 1 (s)
1/2(∆)d∆ = 1
Z 1 [∆ 2∆](2k+1)(s)
1/2(∆)d∆ = 0
max Z 1
∆∗
(s)
1/2(∆)d∆ =?
This is of the form A~ x = ~ b, x 0 max ~ c · ~ x =?
SLIDE 24
Linear programming duality
The linear programming problem of the form A~ x = ~ b, x 0, max ~ c · ~ x =?, is dual to another problem, AT~ y ~ c, min ~ b · ~ y =?
SLIDE 25
Linear programming duality
The linear programming problem of the form A~ x = ~ b, x 0, max ~ c · ~ x =?, is dual to another problem, AT~ y ~ c, min ~ b · ~ y =? With the property that ~ c · ~ x ~ b · ~ y.
SLIDE 26
Linear programming duality
The linear programming problem of the form A~ x = ~ b, x 0, max ~ c · ~ x =?, is dual to another problem, AT~ y ~ c, min ~ b · ~ y =? With the property that ~ c · ~ x ~ b · ~ y. ~ c · ~ x ~ y · A~ x = ~ y · ~ b.
SLIDE 27
Linear programming duality
Any feasible solution to the dual problem provides an upper bound for the primal problem. In our case the dual problem is Q(∆) = y0 + X
k
yk[∆ 2∆](2k1), Q(∆) 0, 8∆ 0, Q(∆) 1, 8∆ ∆⇤, min y0 =?,
SLIDE 28 Linear programming duality
Any feasible solution to the dual problem provides an upper bound for the primal problem. In our case the dual problem is Q(∆) = y0 + X
k
yk[∆ 2∆](2k1), Q(∆) 0, 8∆ 0, Q(∆) 1, 8∆ ∆⇤, min y0 =?,
Q(∆) = X
k
k[∆ 2∆](2k1), Q(∆) 1, 8∆ 0, Q(∆) Q0, 8∆ ∆⇤, min 1 Q0 + 1 =?.
SLIDE 29
Large ∆
Q(∆) = X
k
k[∆ 2∆](2k1), Q(∆) 1, 8∆ 0, Q(∆) Q0, 8∆ ∆⇤, min 1 Q0 + 1 =?.
SLIDE 30
Large ∆
Q(∆) = X
k
k[∆ 2∆](2k1), Q(∆) 1, 8∆ 0, Q(∆) Q0, 8∆ ∆⇤, min 1 Q0 + 1 =?. For large ∆ we truncate at k = n ⌧ p∆ to find an approximate truncated version (v = (∆ 2∆0)/2∆) q(v) 2 Podd
n
, q(v) 1, 8v 1, q(v) q0, 8v v⇤, min 1 q0 + 1 =?
SLIDE 31
Large ∆
q(v) 2 Podd
2n1,
q(v) 1, 8v 1, q(v) q0, 8v v⇤, min 1 q0 + 1 =?
SLIDE 32
Large ∆
q(v) 2 Podd
2n1,
q(v) 1, 8v 1, q(v) q0, 8v v⇤, min 1 q0 + 1 =? For v⇤ > 1 the solution is given by the Chebyshev polynomial, q(v) = T2n1(v).
SLIDE 33
Large ∆
q(v) 2 Podd
2n1,
q(v) 1, 8v 1, q(v) q0, 8v v⇤, min 1 q0 + 1 =? For v⇤ > 1 the solution is given by the Chebyshev polynomial, q(v) = T2n1(v). 1 F(∆⇤, 1/2) 1 1 + T2n1 ⇣ ∆∗2∆φ
2∆φ
⌘, ∆⇤ 4∆
SLIDE 34
Large ∆
1 F(∆⇤, 1/2) 1 1 + T2n1 ⇣ ∆∗2∆φ
2∆φ
⌘, ∆⇤ 4∆
SLIDE 35
Large ∆
1 F(∆⇤, 1/2) 1 1 + T2n1 ⇣ ∆∗2∆φ
2∆φ
⌘, ∆⇤ 4∆ 1 F(∆⇤, x) 2 1 + T2n1 ⇣
∆∗∆x/2 ∆x/2
⌘, ∆⇤ ∆x
SLIDE 36
Large ∆
1 F(∆⇤, 1/2) 1 1 + T2n1 ⇣ ∆∗2∆φ
2∆φ
⌘, ∆⇤ 4∆ 1 F(∆⇤, x) 2 1 + T2n1 ⇣
∆∗∆x/2 ∆x/2
⌘, ∆⇤ ∆x GFF with ∆ = 100 and T5 bound
Δ2/3=6Δϕ
Δ
1 ℱ
SLIDE 37 Other cases
The essential ingredient in the above analysis was the formula @nef (x) = [f 0(x)]nef (x) 1 + O(n21)
We had = ∆ 2∆0 and f (x) = log x. More generally, the same approach works for many other cases when there is a UV-IR crossing-like equation and a large parameter limit. The analysis can be extended to
- 1. Conformal block expansion, (∆x = 2∆/p1 x)
- 2. “Scaling block” expansion in ⇢ coordinate
(∆x = 2∆/p1 x)
- 3. Large space-time dimension limit of conformal block
expansion (∆x is more complicated)
- 4. Large central charge limit of modular-invariant partition
function in CFT2 (∆⌧ = (1 + |⌧|2)c/12)
SLIDE 38
Cardy-like formula
In [PRER ’12] an asymptotic formula for the OPE coefficients was found, similar in spirit to Cardy formula. At large central charge and under an additional sparse light spectrum condition Cardy formula can be shown to work for operators ∆ ⇠ c [Hartman,Keller,Stoica ’14].
SLIDE 39
Cardy-like formula
In [PRER ’12] an asymptotic formula for the OPE coefficients was found, similar in spirit to Cardy formula. At large central charge and under an additional sparse light spectrum condition Cardy formula can be shown to work for operators ∆ ⇠ c [Hartman,Keller,Stoica ’14]. Consider a situation in which ∆ is large and the OPE coefficients with light operators are sufficiently small so that for x < 1/2 we have log G4(x) = 2∆ log x + O(1), I.e. essentially the contribution from the identity operator.
SLIDE 40
Cardy-like formula
In [PRER ’12] an asymptotic formula for the OPE coefficients was found, similar in spirit to Cardy formula. At large central charge and under an additional sparse light spectrum condition Cardy formula can be shown to work for operators ∆ ⇠ c [Hartman,Keller,Stoica ’14]. Consider a situation in which ∆ is large and the OPE coefficients with light operators are sufficiently small so that for x < 1/2 we have log G4(x) = 2∆ log x + O(1), I.e. essentially the contribution from the identity operator. It then follows from the approximate reflection symmetry that we should expect the dominant contribution for x > 1/2 to come from ∆ = ∆x = 2∆/(1 x). This implies an asymptotic formula for the OPE coefficients for operators of dimension ∆ > ∆1/2 = 4∆.
SLIDE 41 Cardy-like formula
Using the technology of [HKS ’14] one shows for ∆ > 4∆ ¯ g(s)(∆) = exp ∆ log ✓ 1 2∆ ∆ ◆ + 2∆ log ✓ ∆ 2∆0 1 ◆ + O(∆↵
)
where ¯ g(s) is g(s) averaged over interval of size ⇠ ∆↵
with
1/2 < ↵ < 1.
SLIDE 42
Finite ∆
Chebyshev bound shows only a polynomial decay, but we know that it should be exponential in the end. Can we find a similar bound which would be exponentially small?
SLIDE 43
Finite ∆
Chebyshev bound shows only a polynomial decay, but we know that it should be exponential in the end. Can we find a similar bound which would be exponentially small? Recall the exact dual problem Q(∆) = X
k
k[∆ 2∆](2k1), Q(∆) 1, 8∆ 0, Q(∆) Q0, 8∆ ∆⇤, min 1 Q0 + 1 =?
SLIDE 44 Finite ∆
Chebyshev bound shows only a polynomial decay, but we know that it should be exponential in the end. Can we find a similar bound which would be exponentially small? Recall the exact dual problem Q(∆) = X
k
k[∆ 2∆](2k1), Q(∆) 1, 8∆ 0, Q(∆) Q0, 8∆ ∆⇤, min 1 Q0 + 1 =? Take Q(∆) / [∆ 2∆](2k1) for some optimal k. This gives (interpolation weakens the bound) 1 F(∆, 1/2) 1 1 + Γ(∆2∆φ1)Γ(2∆φ)
Γ( ∆+3
2 )Γ( ∆−1 2
)
SLIDE 45 Finite ∆
1 F(∆, 1/2) 1 1 + Γ(∆2∆φ1)Γ(2∆φ)
Γ( ∆+3
2 )Γ( ∆−1 2
)
- r, defining k(∆) = d(∆ 4∆ 3)/4e, without interpolation
1 F(∆, 1/2) 1 1 [∆2∆φ]2k(∆)+1
[2∆φ]2k(∆)+1
,
SLIDE 46 Finite ∆
1 F(∆, 1/2) 1 1 + Γ(∆2∆φ1)Γ(2∆φ)
Γ( ∆+3
2 )Γ( ∆−1 2
)
- r, defining k(∆) = d(∆ 4∆ 3)/4e, without interpolation
1 F(∆, 1/2) 1 1 [∆2∆φ]2k(∆)+1
[2∆φ]2k(∆)+1
, Asymptotically, 1 F(∆⇤, 1/2) p 2⇡ Γ(2∆)∆
2∆φ 1
2
⇤
✓1 2 ◆∆∗
SLIDE 47 Finite ∆
1 F(∆, 1/2) 1 1 + Γ(∆2∆φ1)Γ(2∆φ)
Γ( ∆+3
2 )Γ( ∆−1 2
)
- r, defining k(∆) = d(∆ 4∆ 3)/4e, without interpolation
1 F(∆, 1/2) 1 1 [∆2∆φ]2k(∆)+1
[2∆φ]2k(∆)+1
, Asymptotically, 1 F(∆⇤, 1/2) p 2⇡ Γ(2∆)∆
2∆φ 1
2
⇤
✓1 2 ◆∆∗ Compare to G4(1/2) (1 F(∆⇤, 1/2)) . 1 Γ(2∆ + 1)∆2∆φ
⇤
✓1 2 ◆∆∗2∆φ
SLIDE 48 Finite ∆
T3, finite-∆ bounds and GFF at ∆ = 10
4 Δϕ 5 Δϕ 6 Δϕ
Δ
1 2
1 ℱ
SLIDE 49
Summary
I Approximate reflection symmetry in spectral decomposition
SLIDE 50 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
SLIDE 51 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
I A version of Cardy formula for weakly coupled light spectrum
SLIDE 52 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
I A version of Cardy formula for weakly coupled light spectrum I Non-asymptotic convergence bound
SLIDE 53 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
I A version of Cardy formula for weakly coupled light spectrum I Non-asymptotic convergence bound
SLIDE 54 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
I A version of Cardy formula for weakly coupled light spectrum I Non-asymptotic convergence bound
Questions
I What about spin? (Transverse derivatives)
SLIDE 55 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
I A version of Cardy formula for weakly coupled light spectrum I Non-asymptotic convergence bound
Questions
I What about spin? (Transverse derivatives) I Virasoro symmetry?
SLIDE 56 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
I A version of Cardy formula for weakly coupled light spectrum I Non-asymptotic convergence bound
Questions
I What about spin? (Transverse derivatives) I Virasoro symmetry? I Can we solve the case of scaling blocks exactly? (e.g. the tail
bound)
SLIDE 57 Summary
I Approximate reflection symmetry in spectral decomposition I Bound on scaling dimensions of dominant operators; e.g. 4∆0
p 2∆0 for x = 1/2.
I A version of Cardy formula for weakly coupled light spectrum I Non-asymptotic convergence bound
Questions
I What about spin? (Transverse derivatives) I Virasoro symmetry? I Can we solve the case of scaling blocks exactly? (e.g. the tail
bound)
I Or at least guess the result?
SLIDE 58 Conformal block for large ∆
We can find the form of the conformal block on real line x = ¯ x in the limit of large intermediate scaling dimension using the quartic Casimir equation with WKB-like approximation. This gives F∆,`(x) =(1 ⇢2)✏1(4⇢)∆ ⇥ exp 1 ∆ ⇢2 1 ⇢2 (1 + ✏ ✏2)∆2 + ✏(✏ 1)`2 ∆2 `2 + O(∆2)
✏ = d 2 2 , ⇢ = x (1 + p1 x)2
SLIDE 59 Large spacetime dimension
Unitarity bounds ∆ = 0
∆ d 2 2 ⇠ d 2
SLIDE 60 Large spacetime dimension
Unitarity bounds ∆ = 0
∆ d 2 2 ⇠ d 2 Reflection symmetry then implies ∆ = 0
d 2 ∆ ∆x
∆ = ∆0
x
SLIDE 61 Large spacetime dimension
Unitarity bounds ∆ = 0
∆ d 2 2 ⇠ d 2 Reflection symmetry then implies ∆ = 0
d 2 ∆ ∆x
∆ = ∆0
x
For ∆ = d
2 , ∆x = d 2 ) resembles free fied
SLIDE 62 Saturation of tail bound
2d global conformal blocks at Ising point ∆ = 1/8
2 4 6 8 10 10-5 10-4 0.001 0.010 0.100 1