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Tauberian Theorems and Asymptotic Spectral Data

A Tauberian theorem turns a singular limit of a positive spectral transform into an asymptotic statement about an integrated spectral measure. In conformal bootstrap applications, this is the rigorous bridge from crossed-channel identity dominance to averaged high-dimension or large-spin data. It does not normally determine individual operator dimensions or coefficients.

Required background. The lightcone OPE and large-spin expansion supplies the crossed-channel singularity and the large-spin interpretation. Asymptotic scales, remainders, and uniformity distinguishes a leading equivalent from a pointwise expansion.

Helpful background. Bounded, compact, and integral operators provides language for kernels and spectral measures, although positivity rather than compactness is the decisive Tauberian input here.

Let dμ(E)0d\mu(E)\ge0 be a spectral measure and

F(t)=0etEdμ(E),t>0.F(t)=\int_0^\infty e^{-tE}\,d\mu(E), \qquad t>0.

If the cumulative measure satisfies

M(E)μ([0,E])AΓ(γ+1)Eγ,M(E)\equiv\mu([0,E]) \sim \frac{A}{\Gamma(\gamma+1)}E^\gamma,

then integration by parts and y=tEy=tE give

F(t)Atγ(t0+).F(t)\sim A\,t^{-\gamma} \qquad(t\to0^+).

This forward, or Abelian, implication follows by inserting known spectral growth into the transform. Bootstrap reasoning needs the converse: infer M(E)M(E) from the singularity of F(t)F(t). Oscillating signed measures can have the same leading transform while very different cumulative behavior, so the converse requires a Tauberian hypothesis such as nonnegativity or monotonicity.

For a Hermitian scalar in a reflection-positive one-dimensional CFT, use

ϕ(0)ϕ(z)ϕ(1)ϕ()=z2ΔϕG(z),\langle\phi(0)\phi(z)\phi(1)\phi(\infty)\rangle =z^{-2\Delta_\phi}\mathcal G(z),

and the block expansion on 0<z<10<z<1,

G(z)=0dΔp(Δ)GΔ(z),p(Δ)0,GΔ(z)=zΔ2F1(Δ,Δ;2Δ;z).\mathcal G(z)=\int_0^\infty d\Delta\, p(\Delta)G_\Delta(z), \qquad p(\Delta)\ge0, \qquad G_\Delta(z)=z^\Delta{}_2F_1(\Delta,\Delta;2\Delta;z).

Assume the crossed identity is separated by a positive gap, so

G(1x)x2Δϕ(x0+).\mathcal G(1-x)\sim x^{-2\Delta_\phi} \qquad(x\to0^+).

At large Δ\Delta with xΔ=O(1)\sqrt{x}\,\Delta=O(1),

GΔ(1x)C(Δ)K0(2xΔ),C(Δ)=4ΔΔπ.G_\Delta(1-x) \sim C(\Delta)K_0(2\sqrt{x}\,\Delta), \qquad C(\Delta)=4^\Delta\sqrt{\frac{\Delta}{\pi}}.

Define the weighted cumulative primary density

Q(Y)=0YdΔC(Δ)p(Δ).Q(Y)=\int_0^Yd\Delta\,C(\Delta)p(\Delta).

The conformal Tauberian theorem then gives

Q(Y)YγAγ,γ=4Δϕ,A=14Γ ⁣(γ2)2.Q(Y)\sim\frac{Y^\gamma}{A\gamma}, \qquad \gamma=4\Delta_\phi, \qquad A=\frac14\Gamma\!\left(\frac\gamma2\right)^2.

This exact prefactor follows from

0dttγ1K0(2t)=14Γ ⁣(γ2)2.\int_0^\infty dt\,t^{\gamma-1}K_0(2t) =\frac14\Gamma\!\left(\frac\gamma2\right)^2.

The proof first controls replacement of the exact block by its Bessel kernel, then uses a Wiener-type Tauberian theorem to replace that smooth kernel by a sharp cutoff. The nonvanishing Fourier transform of the logarithmically rescaled kernel is essential Qiao and Rychkov 2017, §§2–5.

For a discrete spectrum, p(Δ)=iaiδ(ΔΔi)p(\Delta)=\sum_i a_i\delta(\Delta-\Delta_i), so the theorem states

ΔiYC(Δi)aiY4ΔϕΔϕΓ(2Δϕ)2.\sum_{\Delta_i\le Y} C(\Delta_i)a_i \sim\frac{Y^{4\Delta_\phi}} {\Delta_\phi\Gamma(2\Delta_\phi)^2}.

It determines a cumulative weighted count. For any fixed η>0\eta>0, subtraction of two cumulative equivalents also fixes a multiplicative window:

Q((1+η)Y)Q(Y)(1+η)γ1AγYγ.Q((1+\eta)Y)-Q(Y) \sim\frac{(1+\eta)^\gamma-1}{A\gamma}Y^\gamma.

It does not fix a window whose relative width shrinks with YY, and it does not imply the pointwise density

C(Δ)p(Δ)?A1Δγ1.C(\Delta)p(\Delta)\stackrel{?}{\sim}A^{-1}\Delta^{\gamma-1}.

Delta functions already make that pointwise statement meaningless for a generic discrete CFT. Additional regularity, spacing, or remainder hypotheses are needed for local spectral information.

OPE convergence is what permits the positive block expansion to be used away from coincident points; its exponential tail bound is a separate result from the Tauberian asymptotic Pappadopulo et al. 2012, §§3–5.

MethodPositivity or analyticity inputTransform and limiting variableArc, subtraction, or smoothingSupported domainUncontrolled data
Hardy–Littlewood for powersNonnegative primary-plus-descendant coefficientsLaplace variable t=logz0t=\lvert\log z\rvert\to0Sharp cumulative count obtained from a positive exponential kernelIntegrated descendant-weighted densityIndividual degeneracies and shrinking windows
Conformal-block Tauberian theoremp(Δ)0p(\Delta)\ge0 and crossed identity dominance with a gapBessel kernel with x0x\to0, xΔ2=O(1)x\Delta^2=O(1)Smooth Bessel average replaced by a sharp cutoffQ(Y)Q(Y) with the exact leading prefactorPointwise primary density and generic subleading terms
Lightcone application in d>2d>2Positive collinear spectral measure in the chosen reflection-positive configuration1zˉ01-\bar z\to0 and large spin at bounded twistFixed-twist or smeared spectral sector must be isolatedAveraged large-spin OPE weightAn individual trajectory without extra analytic input
Lorentzian inversionDeclared double discontinuity and Regge bound, not a Tauberian positivity theoremComplex spin and spectral dimensionArc vanishes only above a spin thresholdMeromorphic data above that thresholdLow spins and zero-discontinuity terms
Subtracted dispersionCut-plane analyticity plus polynomial growthCorrelator cross-ratiosExplicit subtraction/contact basisCorrelator modulo supplied constantsContact coefficients not fixed by cuts

This comparison matters: inversion can establish individual analytic trajectories under stronger Lorentzian assumptions, while a Tauberian theorem gives a robust averaged result from positivity. One conclusion cannot be silently promoted into the other.

Generalized-free bosonic data have

Δn=2Δϕ+2n,\Delta_n=2\Delta_\phi+2n,

and known positive OPE coefficients. At large Δ\Delta their weighted density is a comb with spacing two. Summing the comb up to YY reproduces the power and prefactor of Q(Y)Q(Y) above, whereas the unsmeared density continues to oscillate between delta-function support and zero. This simultaneously checks the theorem and displays why the conclusion must be cumulative Qiao and Rychkov 2017, app. B.

If

G(1x)=x2Δϕ(1+O(xα)),\mathcal G(1-x)=x^{-2\Delta_\phi} \bigl(1+O(x^\alpha)\bigr),

it is tempting to append an O(Y2α)O(Y^{-2\alpha}) relative error to Q(Y)Q(Y). That conclusion does not follow from the leading Tauberian theorem. Subleading terms can mix with discreteness and oscillatory spectral structure; a quantitative remainder theorem needs explicit hypotheses on the transform, kernel, and smoothing window. Slowly varying factors can sometimes be carried through by an appropriate generalized theorem, but they must be stated rather than inferred by pattern matching.

Take Δϕ=1/2\Delta_\phi=1/2. Compute γ\gamma, AA, and the leading weighted cumulative density Q(Y)Q(Y). Then state what the theorem predicts for the fixed multiplicative window [Y,2Y][Y,2Y].

Solution

Here γ=2\gamma=2 and A=Γ(1)2/4=1/4A=\Gamma(1)^2/4=1/4. Therefore Q(Y)Y2/(Aγ)=2Y2Q(Y)\sim Y^2/(A\gamma)=2Y^2. The window contains weighted mass Q(2Y)Q(Y)2(41)Y2=6Y2Q(2Y)-Q(Y)\sim2(4-1)Y^2=6Y^2. The theorem says nothing pointwise about an individual coefficient inside the window.

  • Pappadopulo, Duccio, Slava Rychkov, Johnny Espin, and Riccardo Rattazzi. “OPE Convergence in Conformal Field Theory.” Physical Review D 86, no. 10 (2012): 105043. doi:10.1103/PhysRevD.86.105043.
  • Qiao, Jiaxin, and Slava Rychkov. “A Tauberian Theorem for the Conformal Bootstrap.” Journal of High Energy Physics 2017, no. 12 (2017): 119. doi:10.1007/JHEP12(2017)119.