The analytic bootstrap and AdS superhorizon locality
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Citations
Solving the 3D Ising Model with the Conformal Bootstrap
The Conformal Bootstrap: Theory, Numerical Techniques, and Applications
Convexity and Liberation at Large Spin
Solving the 3d Ising Model with the Conformal Bootstrap II. c-Minimization and Precise Critical Exponents
Causality Constraints on Corrections to the Graviton Three-Point Coupling
References
The Large N limit of superconformal field theories and supergravity
Anti De Sitter Space And Holography
Gauge Theory Correlators from Non-Critical String Theory
Anti de sitter space and holography
Infinite Conformal Symmetry in Two-Dimensional Quantum Field Theory
Related Papers (5)
Frequently Asked Questions (13)
Q2. What are the future works mentioned in the paper "The analytic bootstrap and ads superhorizon locality" ?
Thus far much of the work on the bootstrap has been numerical and has focused on questions of phenomenological interest, so further studies of superconformal theories [ 12 ], AdS/CFT setups [ 10 ], and even quantum gravity [ 41 ] may yield important results. Perhaps in the future the results of [ 44, 45 ] could be used to prove these statements. Through further work it should be possible to use their results to shed light on the convergence properties of the CFT bootstrap in Mellin space. A more precise version of this observation could be useful for further work using the CFT bootstrap, both analytically and numerically.
Q3. What is the non-trivial content of this theorem?
The non-trivial content of this theorem is that positivity and linearity imply that the density so-constructed is unique, and gives the correct value of the functional on any set with compact support.
Q4. How can the authors obtain a bound on the conformal block coefficients?
Since the authors explicitly know the leading and sub-leading behavior as u → 0, the authors can obtain a bound on the conformal block coefficients using the crossing symmetry relation, eq. (2.29).
Q5. What is the power law in the large l sum?
the authors stress that all the authors need in order to expand v γ(n,ℓ) 2 in log v in the large ℓ sum is the property that it is power law suppressed as ℓ→ ∞, which is true even if the coefficients γn are O(1) or larger.
Q6. What is the key feature of eq. (2.12)?
Note that z → 0 at fixed z̄ is equivalent to u→ 0 at fixed v. A key feature of eq. (2.12) is that the ℓ, z dependence of gτ,ℓ factorizes from the τ, v dependence in the limit z → 0, ℓ → ∞.
Q7. What is the reason why there is no operator in this theory?
Now the authors see why there are no operators in this theory with twist τ = 2∆σ: the existence of this low-twist tower means that the identity operator can be (and is) cancelled by contributions on the same side of the crossing relation.
Q8. What is the simplest way to calculate the dimensions of double-trace operators?
The calculation of anomalous dimensions of double-trace operators starting with a perturbative AdS description is usually simplest for the lowest-spin states [16, 55], and becomes increasingly more involved for higher spins.
Q9. How do the authors interpret the state of a particle?
So the authors need to study very large ℓ to create a large separation in AdS units.– 17 –J H E P 1 2 ( 2 0 1 3 ) 0 0 4In the absence of large N , the authors certainly cannot interpret the state |φ〉 as a bulk particle, but the authors can still view it as some de-localized blob in AdS.
Q10. What is the simplest way to constrain the dimensions of operators in a scalar?
In [8], the authors used numerical boostrap methods to constrain the dimensions of operators appearing in the OPE of a scalar φ with itself in 3d CFTs.
Q11. What is the power-law dependence on l?
In this case the authors obtain a specific power-law dependence on ℓ that can be written asγ(n, ℓ) = γn ℓτm ∝ γn exp [ −τm bRAdS], (3.3)so the interactions between the blobs are shutting off exponentially at large, superhorizon distances in AdS.
Q12. What would be the extension to the nightmann theorem?
Another interesting extension would involve studying further sub-leading corrections to the bootstrap as u→ 0; analyzing these corrections could lead to a more general proof of the Nachtmann theorem that does not rely on conformal symmetry breaking in the IR.
Q13. What is the reason why the u log v term is absent?
15Note that if instead one considers the s-channel expansion of the correlator 〈Φ†ΦΦ†Φ〉 then there is no longer a relative sign between the even and odd spins in the superconformal block [12], so a u1 log v term is present.