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The Heavy–Light Classical Limit

The classical limit used for the CFT–ODE dictionary is a coordinated double scaling, not the instruction “make the central charge large.” The four background primaries and the selected intermediate channel become heavy, with weights of order b2b^{-2}, while the degenerate insertion Vb/2(z)V_{-b/2}(z) stays light, with weight of order one. The heavy part exponentiates into a classical four-point block; the light part survives as a probe wavefunction whose two degenerate fusion branches span a two-dimensional local solution space.

That factorization supplies the missing step in the five-insertion BPZ equation. The modulus derivative is not discarded. Acting on the heavy exponential, it becomes multiplication by a zz-independent accessory residue. Only its action on the finite probe factor is subleading.

Central charge and weights must scale together

Section titled “Central charge and weights must scale together”

For the simplest real reading, take b0+b\to0^+. For complex bb, fix a sector and an asymptotic branch; then cVirc_{\mathrm{Vir}} diverges in magnitude rather than approaching ++\infty in an ordered sense.

With

QL=b+b1,cVir=1+6QL2,Q_{\mathrm L} = b+b^{-1}, \qquad c_{\mathrm{Vir}} = 1+6Q_{\mathrm L}^2,

one has the exact expansion

cVir=6b2+13+6b2.c_{\mathrm{Vir}} = \frac{6}{b^2} +13 +6b^2.

Thus b0b\to0 implies cVirc_{\mathrm{Vir}}\to\infty, but that alone does not specify a classical block. The external and internal weights must scale so that their ratios to cVirc_{\mathrm{Vir}} remain finite.

For every heavy label

j{0,t,1,,0t},j\in \left\{ 0,t,1,\infty,0t \right\},

use the centered momentum from the book conventions and choose

aL,j=θj2b.a_{\mathrm L,j} = \frac{\theta_j}{2b}.

Since ΔCFT(α)=QL2/4aL2\Delta^{\mathrm{CFT}}(\alpha) =Q_{\mathrm L}^2/4-a_{\mathrm L}^2,

ΔjCFT=1θj24b2+12+b24=δjb2+O(1),δj:=1θj24.\begin{aligned} \Delta_j^{\mathrm{CFT}} &= \frac{1-\theta_j^2}{4b^2} +\frac12 +\frac{b^2}{4} \\ &= \frac{\delta_j}{b^2} +O(1), \qquad \delta_j := \frac{1-\theta_j^2}{4}. \end{aligned}

More generally, 2baL,j=θj+O(b2)2b\,a_{\mathrm L,j}=\theta_j+O(b^2) gives the same leading result. In the uncentered momentum, write ηj:=limb0bαj\eta_j:=\lim_{b\to0}b\alpha_j. Then

ηj=1+θj2,δj=ηj(1ηj).\eta_j = \frac{1+\theta_j}{2}, \qquad \delta_j = \eta_j(1-\eta_j).

Alternatively, the exact finite-bb lift αj=ηj/b\alpha_j=\eta_j/b gives

ΔjCFT=ηj(1ηj)b2+ηj.\Delta_j^{\mathrm{CFT}} = \frac{\eta_j(1-\eta_j)}{b^2} +\eta_j.

Holding ηj\eta_j exactly fixed and holding θj\theta_j exactly fixed are two different finite-bb lifts with the same leading δj\delta_j. The leading oper is insensitive to that distinction; its first correction need not be. The centered lift is especially useful here because it exposes the ODE exponent difference immediately.

The chosen degenerate field really is light

Section titled “The chosen degenerate field really is light”

A convenient fixed-weight light representative has uncentered momentum

α=bσ,\alpha_\ell = b\sigma_\ell,

or by its reflection QLαQ_{\mathrm L}-\alpha_\ell. Its weight is

ΔCFT=σ+b2σ(1σ).\Delta_\ell^{\mathrm{CFT}} = \sigma_\ell +b^2\sigma_\ell(1-\sigma_\ell) .

By contrast, holding a generic uncentered momentum α=O(1)\alpha_\ell=O(1) gives ΔCFT=O(b1)\Delta_\ell^{\mathrm{CFT}}=O(b^{-1}). That is small relative to cVir=O(b2)c_{\mathrm{Vir}}=O(b^{-2}), but it is not the fixed-weight light scaling used here.

For the book’s (2,1)(2,1) presentation,

V2,1(z):=Vb/2(z),V_{2,1}(z) := V_{-b/2}(z),

and

Δd=ΔCFT(b2)=123b24.\Delta_{\mathrm d} = \Delta^{\mathrm{CFT}} \left( -\frac b2 \right) = -\frac12 -\frac{3b^2}{4}.

Its weight remains finite while the background weights grow as b2b^{-2}. Its null relation,

(L12+b2L2)Vb/2=0,\left( L_{-1}^2+b^2L_{-2} \right)V_{-b/2}=0,

is precisely the presentation whose BPZ equation retains a finite second derivative after multiplication by b2b^2.

The dual degenerate field behaves differently in this same limit:

ΔCFT(12b)=1234b2.\Delta^{\mathrm{CFT}} \left( -\frac{1}{2b} \right) = -\frac12 -\frac{3}{4b^2}.

It is heavy, and its null relation contains b2L2b^{-2}L_{-2}. It becomes the light presentation only after the dual exchange bb1b\leftrightarrow b^{-1}; the Kac label alone does not license swapping the two fields.

The finite-bb fusion power adjacent to a heavy insertion is

ρi,ϵi=bQL2+ϵibaL,i,ϵi=±1.\rho_{i,\epsilon_i} = \frac{bQ_{\mathrm L}}2 + \epsilon_i b\,a_{\mathrm L,i}, \qquad \epsilon_i=\pm1.

Under the centered heavy scaling,

ρi,ϵi=1+b2+ϵiθi21+ϵiθi2.\rho_{i,\epsilon_i} = \frac{ 1+b^2+\epsilon_i\theta_i }{2} \longrightarrow \frac{1+\epsilon_i\theta_i}{2}.

This agrees with the indicial equation of a normal-form oper having double-pole coefficient δi\delta_i:

r(r1)+δi=0,r±=1±θi2.r(r-1)+\delta_i=0, \qquad r_\pm=\frac{1\pm\theta_i}{2}.

The CFT fusion branches therefore become the two local Frobenius powers of the limiting ODE. This is an independent check of both the sign in δi=(1θi2)/4\delta_i=(1-\theta_i^2)/4 and the branch order fixed on the degenerate-fusion page.

Fix the 0t0t channel, the internal heavy weight, the branch of \Logt\Log t, and the normalization of the four-point chiral block V0t(t;b)\mathcal V_{0t}(t;b). Its classical block is defined by

f0t(t):=limb0b2\LogV0t(t;b),f_{0t}(t) := \lim_{b\to0} b^2 \Log \mathcal V_{0t}(t;b),

when this limit exists on the chosen branch. At minimum, the definition implies

\LogV0t(t;b)=f0t(t)b2+o(b2).\Log\mathcal V_{0t}(t;b) = \frac{f_{0t}(t)}{b^2} +o(b^{-2}).

On a regular generic semiclassical branch one often has the stronger expansion

\LogV0t=f0tb2+g0t+O(b2).\Log\mathcal V_{0t} = \frac{f_{0t}}{b^2} +g_{0t} +O(b^2).

This sign convention is a definition. Sources that write exp[cVirS/6]\exp[-c_{\mathrm{Vir}}S/6] use the opposite leading convention, f0t=Sf_{0t}=-S, because cVir/6b2c_{\mathrm{Vir}}/6\sim b^{-2}. Exponentiation of a generic four-heavy block is established independently of the mixed degenerate probe. The five-point factorization used below is a selected-branch semiclassical statement, explicitly realized in the references, rather than a theorem of global uniformity over the entire tt-plane.

Recall the exact normalization

V0t(t;b)=tΔ0tCFTΔ0CFTΔtCFTV^0t(t;b),V^0t(0;b)=1.\mathcal V_{0t}(t;b) = t^{ \Delta_{0t}^{\mathrm{CFT}} - \Delta_0^{\mathrm{CFT}} - \Delta_t^{\mathrm{CFT}} } \widehat{\mathcal V}_{0t}(t;b), \qquad \widehat{\mathcal V}_{0t}(0;b)=1.

Define the normalized classical block by

f^0t(t):=limb0b2\LogV^0t(t;b).\widehat f_{0t}(t) := \lim_{b\to0} b^2\Log \widehat{\mathcal V}_{0t}(t;b).

On the declared branch of \Logt\Log t,

f0t(t)=(δ0tδ0δt)\Logt+f^0t(t).f_{0t}(t) = \left( \delta_{0t} -\delta_0 -\delta_t \right) \Log t + \widehat f_{0t}(t).

Consequently,

tf0t=δ0tδ0δtt+tf^0t.\partial_t f_{0t} = \frac{ \delta_{0t}-\delta_0-\delta_t }{t} + \partial_t\widehat f_{0t}.

This elementary shift is why an accessory formula is meaningless until the OPE prefactor has been stated.

The first sewing coefficient checks the scaling

Section titled “The first sewing coefficient checks the scaling”

The level-one coefficient derived on the Virasoro-block page gives

f^0t(t)=κ1t+O(t2),\widehat f_{0t}(t) = \kappa_1t +O(t^2),

where

κ1=(δ0t+δtδ0)(δ0t+δ1δ)2δ0t.\kappa_1 = \frac{ \left( \delta_{0t}+\delta_t-\delta_0 \right) \left( \delta_{0t}+\delta_1-\delta_\infty \right) }{ 2\delta_{0t} }.

Indeed, the quantum level-one coefficient grows as b2κ1b^{-2}\kappa_1. At higher levels the claim is much stronger: powers more singular than b2b^{-2} must cancel in the logarithm of the block. Semiclassical exponentiation is this nontrivial reorganization, not a termwise replacement of every weight by δ/b2\delta/b^2.

The degenerate insertion factors off the heavy background

Section titled “The degenerate insertion factors off the heavy background”

Choose one local degenerate branch and compatible chiral-vertex normalizations for the five-point block B5,ϵ(z,t;b)\mathscr B_{5,\epsilon}(z,t;b) and the background four-point block. The heavy–light statement is that their ratio has a finite leading limit,

ψϵ(z;t):=limb0B5,ϵ(z,t;b)V0t(t;b).\psi_\epsilon(z;t) := \lim_{b\to0} \frac{ \mathscr B_{5,\epsilon}(z,t;b) }{ \mathcal V_{0t}(t;b) }.

Write the exact ratio as B5,ϵ=V0tΨb,ϵ\mathscr B_{5,\epsilon} =\mathcal V_{0t}\Psi_{b,\epsilon}. The required statement is Ψb,ϵψϵ\Psi_{b,\epsilon}\to\psi_\epsilon. When a regular even-power expansion exists, this refines to Ψb,ϵ=ψϵ+b2ψϵ,1+\Psi_{b,\epsilon} =\psi_\epsilon+b^2\psi_{\epsilon,1}+\cdots. The heavy exponential remains entirely inside V0t\mathcal V_{0t}, including any finite zz-independent correction eg0t\ee^{g_{0t}}.

On compact probe domains away from the punctures, assume that Ψb,ϵψϵ\Psi_{b,\epsilon}\to\psi_\epsilon locally uniformly in zz. Holomorphy then gives convergence of its first two zz-derivatives. In the modulus direction, the reduction below requires

b2t\LogV0ttf0t,Ψb,ϵψϵ,b2tΨb,ϵ0.\begin{aligned} b^2\partial_t \Log\mathcal V_{0t} &\longrightarrow \partial_t f_{0t}, \\ \Psi_{b,\epsilon} &\longrightarrow \psi_\epsilon, \\ b^2\partial_t\Psi_{b,\epsilon} &\longrightarrow 0. \end{aligned}

Pointwise convergence of b2\LogV0tb^2\Log\mathcal V_{0t} alone does not imply the first derivative limit.

A vanishing momentum shift can leave a finite factor

Section titled “A vanishing momentum shift can leave a finite factor”

In a branch in which the degenerate probe fuses with the insertion at z=0z=0,

aL,0[ϵ]=aL,0ϵb2.a_{\mathrm L,0}^{[\epsilon]} = a_{\mathrm L,0} -\epsilon\frac b2.

For the scaled exponent difference this is

θ0[ϵ]=2baL,0[ϵ]=θ0ϵb2.\theta_0^{[\epsilon]} = 2b\,a_{\mathrm L,0}^{[\epsilon]} = \theta_0-\epsilon b^2.

Although the shift vanishes as b0b\to0, it occurs inside an exponential of order b2b^{-2}:

f0t(θ0ϵb2)=f0t(θ0)ϵb2θ0f0t+O(b4),exp[f0t(θ0ϵb2)f0t(θ0)b2]exp(ϵθ0f0t).\begin{aligned} f_{0t} \left( \theta_0-\epsilon b^2 \right) &= f_{0t}(\theta_0) -\epsilon b^2 \partial_{\theta_0}f_{0t} +O(b^4), \\ \exp \left[ \frac{ f_{0t}(\theta_0-\epsilon b^2) -f_{0t}(\theta_0) }{b^2} \right] &\longrightarrow \exp \left( -\epsilon \partial_{\theta_0}f_{0t} \right). \end{aligned}

This is one contribution to the normalization of ψϵ\psi_\epsilon. Local-coordinate powers and chiral-vertex conventions supply others. The leading oper needs only tf0t\partial_t f_{0t}, but connection coefficients can remember these finite momentum derivatives.

Power counting turns the BPZ PDE into an oper

Section titled “Power counting turns the BPZ PDE into an oper”

Write the exact finite-bb equation derived on the BPZ-equations page as

[b2z2p(z)z+K(z,t)t+Ub(z,t)]B5=0,\left[ b^{-2}\partial_z^2 -p(z)\partial_z +K(z,t)\partial_t +U_b(z,t) \right] \mathscr B_5 =0,

where

p(z)=1z+1z1,K(z,t)=t(t1)z(z1)(zt),p(z) = \frac1z+\frac{1}{z-1}, \qquad K(z,t) = \frac{ t(t-1) }{ z(z-1)(z-t) },

and

Ub(z,t)=Δ0CFTz2+ΔtCFT(zt)2+Δ1CFT(z1)2+ΔCFTΔ0CFTΔtCFTΔ1CFTΔdz(z1).\begin{aligned} U_b(z,t) ={}& \frac{\Delta_0^{\mathrm{CFT}}}{z^2} + \frac{\Delta_t^{\mathrm{CFT}}}{(z-t)^2} + \frac{\Delta_1^{\mathrm{CFT}}}{(z-1)^2} \\ &+ \frac{ \Delta_\infty^{\mathrm{CFT}} -\Delta_0^{\mathrm{CFT}} -\Delta_t^{\mathrm{CFT}} -\Delta_1^{\mathrm{CFT}} -\Delta_{\mathrm d} }{ z(z-1) }. \end{aligned}

Multiply the equation by b2b^2 and insert the derivative-compatible factorization B5,ϵ=V0tΨb,ϵ\mathscr B_{5,\epsilon} =\mathcal V_{0t}\Psi_{b,\epsilon}. After division by V0t\mathcal V_{0t}, the exact rescaled equation is

0=z2Ψb,ϵb2pzΨb,ϵ+b2UbΨb,ϵ+K(b2t\LogV0t)Ψb,ϵ+b2KtΨb,ϵ.\begin{aligned} 0={}& \partial_z^2\Psi_{b,\epsilon} -b^2p\,\partial_z\Psi_{b,\epsilon} +b^2U_b\Psi_{b,\epsilon} \\ &+ K \left( b^2\partial_t\Log\mathcal V_{0t} \right) \Psi_{b,\epsilon} +b^2K\,\partial_t\Psi_{b,\epsilon}. \end{aligned}

Every contribution now has an unambiguous order:

Contribution after multiplication by b2b^2Leading action on the factorized blockOrder
z2\partial_z^2z2ψϵ\partial_z^2\psi_\epsilon11
b2Ubb^2U_bHeavy weights give the classical pole potential11
b2Ktb^2K\partial_t on V0t\mathcal V_{0t}K(tf0t)ψϵK(\partial_t f_{0t})\psi_\epsilon11
b2Ktb^2K\partial_t on Ψb,ϵ\Psi_{b,\epsilon}b2KtΨb,ϵ0b^2K\partial_t\Psi_{b,\epsilon}\to0o(1)o(1); O(b2)O(b^2) under the regular expansion
b2pz-b^2p\partial_zb2pzψϵ-b^2p\partial_z\psi_\epsilonb2b^2
The light weight inside b2Ubb^2U_bb2Δdb^2\Delta_{\mathrm d}b2b^2

Power-counting diagram for the heavy–light reduction of the BPZ PDE. Three solid lanes retain the probe second derivative, the heavy-background modulus derivative, and the classical weight potential, while dashed lanes suppress the probe first derivative, residual modulus derivative, and light degenerate weight.

Defining the finite-bb ratio Ψb,ϵ:=B5,ϵ/V0t\Psi_{b,\epsilon}:=\mathscr B_{5,\epsilon}/\mathcal V_{0t} separates the heavy block from the probe before the limit is taken. Here U0(z,t):=limb0b2Ub(z,t)U_0(z,t):=\lim_{b\to0}b^2U_b(z,t) is the classical pole potential; only the three solid lanes assemble the leading oper.

The modulus derivative survives at leading order through tf0t\partial_t f_{0t}. What disappears is only its action on the finite probe factor. The leading equation is

[z2+Top(z;t)]ψϵ(z;t)=0,\left[ \partial_z^2 +T_{\mathrm{op}}(z;t) \right] \psi_\epsilon(z;t) =0,

with

Top(z;t)=δ0z2+δt(zt)2+δ1(z1)2+δδ0δtδ1z(z1)+t(t1)ctopz(z1)(zt),\begin{aligned} T_{\mathrm{op}}(z;t) ={}& \frac{\delta_0}{z^2} + \frac{\delta_t}{(z-t)^2} + \frac{\delta_1}{(z-1)^2} \\ &+ \frac{ \delta_\infty-\delta_0-\delta_t-\delta_1 }{ z(z-1) } \\ &+ \frac{ t(t-1)c_t^{\mathrm{op}} }{ z(z-1)(z-t) }, \end{aligned}

where, for the unhatted block convention on this page,

ctop=tf0t.c_t^{\mathrm{op}} = \partial_t f_{0t}.

For the hatted block,

ctop=tf^0t+δ0tδ0δtt.c_t^{\mathrm{op}} = \partial_t\widehat f_{0t} + \frac{ \delta_{0t}-\delta_0-\delta_t }{t}.

The next page will compare this fixed-coordinate oper residue with other classical-block and standard-Heun accessory conventions. No such crosswalk should be inferred from the symbol “accessory” alone.

What the limiting statement does and does not guarantee

Section titled “What the limiting statement does and does not guarantee”

The derivation is local in parameter space. A safe version fixes:

  • a channel, internal weight, branch of \Logt\Log t, and branch of the classical block;
  • tt away from 00, 11, and \infty;
  • zz in compact subsets away from 00, tt, 11, and \infty;
  • a domain avoiding zeros of the chosen block when its logarithm is used;
  • generic weights away from singular Kac or resonant limits;
  • a derivative-compatible asymptotic expansion in one sector of the bb-plane.

Near a collision divisor, a bb-dependent boundary-layer scaling can change the power counting. Analytic continuation in tt can also exchange classical saddles or branches. Such saddle walls are not automatically the Stokes curves of an irregular ODE.

The internal weight of a fixed chiral block remains prescribed; no saddle over that weight is being taken. An internal-momentum saddle belongs instead to a full correlator after its structure constants, antiholomorphic pairing, and integration contour have been supplied.

For each fixed admissible tt, ψϵ(z;t)\psi_\epsilon(z;t) solves an ODE in zz and may still depend parametrically on tt. Its modulus-derivative contribution is subleading; under the regular even-power expansion above, it enters two orders later. At every nonzero bb, the original five-point equation remains a PDE.

Taking only cVirc_{\mathrm{Vir}}\to\infty. A classical block requires the external and selected internal weights to scale with cVirc_{\mathrm{Vir}}. Keeping them fixed defines a different large-central-charge regime.

Calling both degenerate presentations light. Under b0b\to0, Vb/2V_{-b/2} is light and V1/(2b)V_{-1/(2b)} is heavy. They are exchanged only with the simultaneous duality bb1b\leftrightarrow b^{-1}.

Deleting the modulus derivative. The term b2Ktb^2K\partial_t acts at order one on the heavy exponential. Only its action on the probe factor is suppressed.

Dropping the OPE prefactor silently. The hatted and unhatted classical blocks differ by an explicit logarithm, so their derivatives differ by a simple pole.

Ignoring a vanishing shift inside the exponent. A momentum shift of order b2b^2 changes f/b2f/b^2 by order one. Such terms affect normalized probe solutions and later connection coefficients.

Treating a local asymptotic as a global identity. The classical block has channel and analytic branches, and a fixed saddle need not dominate after arbitrary continuation in tt.

1. Separate the light and dual-degenerate weights

Section titled “1. Separate the light and dual-degenerate weights”

Expand cVirc_{\mathrm{Vir}}, Δ(b/2)\Delta(-b/2), and Δ(1/(2b))\Delta(-1/(2b)) as b0b\to0. Which degenerate field is light?

Solution

Direct substitution gives

cVir=6b2+13+6b2,Δ(b/2)=123b24,Δ(1/(2b))=1234b2.\begin{aligned} c_{\mathrm{Vir}} &= 6b^{-2}+13+6b^2, \\ \Delta(-b/2) &= -\frac12-\frac{3b^2}{4}, \\ \Delta(-1/(2b)) &= -\frac12-\frac{3}{4b^2}. \end{aligned}

Thus Vb/2V_{-b/2} has finite weight and is the light probe in this limit. The dual field has a weight of the same order as the heavy background.

2. Recover the oper coefficient and exponents

Section titled “2. Recover the oper coefficient and exponents”

Let aL=θ/(2b)a_{\mathrm L}=\theta/(2b). Derive δ\delta and the two limiting fusion powers.

Solution

The heavy weight is

ΔCFT=QL24θ24b2=1θ24b2+O(1),\Delta^{\mathrm{CFT}} = \frac{Q_{\mathrm L}^2}{4} -\frac{\theta^2}{4b^2} = \frac{1-\theta^2}{4b^2} +O(1),

so

δ=1θ24.\delta=\frac{1-\theta^2}{4}.

The two fusion powers are

ρϵ=1+b2+ϵθ21+ϵθ2.\rho_\epsilon = \frac{1+b^2+\epsilon\theta}{2} \longrightarrow \frac{1+\epsilon\theta}{2}.

They solve r(r1)+δ=0r(r-1)+\delta=0, as required by the normal-form oper.

3. Take the classical limit of the level-one coefficient

Section titled “3. Take the classical limit of the level-one coefficient”

Use the exact level-one sewing coefficient to recover κ1\kappa_1 in the small-tt expansion of f^0t\widehat f_{0t}.

Solution

Substitute ΔjCFT=δj/b2+O(1)\Delta_j^{\mathrm{CFT}}=\delta_j/b^2+O(1) into

V1=(Δ0t+ΔtΔ0)(Δ0t+Δ1Δ)2Δ0t.\mathcal V_1 = \frac{ \left( \Delta_{0t}+\Delta_t-\Delta_0 \right) \left( \Delta_{0t}+\Delta_1-\Delta_\infty \right) }{ 2\Delta_{0t} }.

The result is

V1=κ1b2+O(1),\mathcal V_1 = \frac{\kappa_1}{b^2} +O(1),

with

κ1=(δ0t+δtδ0)(δ0t+δ1δ)2δ0t.\kappa_1 = \frac{ \left( \delta_{0t}+\delta_t-\delta_0 \right) \left( \delta_{0t}+\delta_1-\delta_\infty \right) }{ 2\delta_{0t} }.

Since V^0t=exp(f^0t/b2+O(1))\widehat{\mathcal V}_{0t} =\exp(\widehat f_{0t}/b^2+O(1)), its coefficient of tt gives f^0t(t)=κ1t+O(t2)\widehat f_{0t}(t)=\kappa_1t+O(t^2).

Starting from V0t=tΔ0tΔ0ΔtV^0t\mathcal V_{0t} =t^{\Delta_{0t}-\Delta_0-\Delta_t}\widehat{\mathcal V}_{0t}, derive the relation between the two classical accessory derivatives.

Solution

Take a logarithm, multiply by b2b^2, and pass to the heavy limit:

f0t=(δ0tδ0δt)\Logt+f^0t.f_{0t} = \left( \delta_{0t}-\delta_0-\delta_t \right)\Log t +\widehat f_{0t}.

Therefore

tf0t=tf^0t+δ0tδ0δtt.\partial_t f_{0t} = \partial_t\widehat f_{0t} + \frac{ \delta_{0t}-\delta_0-\delta_t }{t}.

The difference is fixed and explicit, but only after the branch of \Logt\Log t and the block normalization have been declared.

5. Keep the correct part of the modulus derivative

Section titled “5. Keep the correct part of the modulus derivative”

Under the regular ansatz B5=ef/b2(ψ+b2ψ1+)\mathscr B_5=\ee^{f/b^2}(\psi+b^2\psi_1+\cdots), compute b2tB5b^2\partial_t\mathscr B_5 through relative order b2b^2.

Solution

Differentiation gives

b2tB5=ef/b2[(tf)ψ+b2(tψ+(tf)ψ1)+O(b4)].\begin{aligned} b^2\partial_t\mathscr B_5 = \ee^{f/b^2} \Bigl[ (\partial_t f)\psi \\ \qquad +b^2 \left( \partial_t\psi +(\partial_t f)\psi_1 \right) +O(b^4) \Bigr]. \end{aligned}

The first term survives and generates the accessory contribution. The derivative tψ\partial_t\psi is subleading; setting the whole modulus derivative to zero would remove the leading term as well.

6. Extract a finite factor from a vanishing fusion shift

Section titled “6. Extract a finite factor from a vanishing fusion shift”

Show that θ0θ0ϵb2\theta_0\mapsto\theta_0-\epsilon b^2 produces a finite exponential factor in a classical block.

Solution

Taylor expansion gives

f(θ0ϵb2)=f(θ0)ϵb2θ0f+O(b4).f(\theta_0-\epsilon b^2) = f(\theta_0) -\epsilon b^2\partial_{\theta_0}f +O(b^4).

Dividing the corresponding block by the unshifted block yields

exp[f(θ0ϵb2)f(θ0)b2]eϵθ0f.\exp \left[ \frac{ f(\theta_0-\epsilon b^2)-f(\theta_0) }{b^2} \right] \longrightarrow \ee^{-\epsilon\partial_{\theta_0}f}.

The shift is invisible in the leading heavy weight but remains in the finite normalization of the probe solution.

7. Identify where the reduction is nonuniform

Section titled “7. Identify where the reduction is nonuniform”

Give three situations in which the fixed-zz, fixed-tt power counting does not by itself justify the limiting oper.

Solution

Examples include:

  1. zz approaches 00, tt, 11, or \infty on a bb-dependent scale, so derivative and pole terms can rebalance.
  2. tt approaches a degeneration point 00, 11, or \infty, requiring a separate collision or matched limit.
  3. Analytic continuation crosses a classical saddle or branch wall, so the selected exponent f0tf_{0t} no longer describes the same asymptotic contribution.

Resonant or Kac-degenerate parameter limits also require coordinated basis limits. None of these effects changes the exact finite-bb PDE; they restrict where the displayed asymptotic reduction is uniform.

8. Show why pointwise exponentiation is insufficient

Section titled “8. Show why pointwise exponentiation is insufficient”

Consider a family defined locally by

\LogBb(t)=f(t)b2+sin(tb2).\Log B_b(t) = \frac{f(t)}{b^2} + \sin \left( \frac{t}{b^2} \right).

Show that b2\LogBbfb^2\Log B_b\to f pointwise while the scaled logarithmic derivative need not converge.

Solution

Multiplication by b2b^2 gives

b2\LogBb(t)=f(t)+b2sin(tb2)f(t).b^2\Log B_b(t) = f(t) + b^2 \sin \left( \frac{t}{b^2} \right) \longrightarrow f(t).

However,

b2t\LogBb(t)=f(t)+cos(tb2),b^2\partial_t\Log B_b(t) = f'(t) + \cos \left( \frac{t}{b^2} \right),

and the oscillating term has no limit for generic fixed tt. The PDE-to-oper reduction therefore needs convergence of the scaled logarithmic derivative, or sufficient locally uniform derivative bounds, not only pointwise convergence of the logarithm.