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Irregular States and Confluent BPZ Equations

A regular CFT puncture is labeled by a highest-weight module. When two punctures collide with their momenta held fixed, they ordinarily produce another regular insertion—or one puncture simply disappears from the outer equation. An irregular puncture appears only when positions and momenta scale together so that higher stress-tensor moments survive.

This page performs the first such collision. Two regular insertions merge at infinity into a rank-one Virasoro irregular state. A light degenerate probe then obeys an exact BPZ equation with two regular singularities and one irregular end. In the heavy–light limit, the scale derivative of an irregular classical block becomes the remaining oper coefficient, and an explicit scalar gauge gives the DLMF confluent Heun equation.

A rank-one irregular state remembers two Virasoro moments

Section titled “A rank-one irregular state remembers two Virasoro moments”

Place the irregular insertion at infinity and use an algebraic dual state Iμ,Λ\langle\mathcal I_{\mu,\Lambda}|. In the convention used on this page, it is defined by

Iμ,ΛL0=ΛΛIμ,Λ,Iμ,ΛL1=μΛIμ,Λ,Iμ,ΛL2=Λ24Iμ,Λ,Iμ,ΛLn=0,n>2.\begin{aligned} \langle\mathcal I_{\mu,\Lambda}|L_0 &= \Lambda\partial_\Lambda \langle\mathcal I_{\mu,\Lambda}|, \\ \langle\mathcal I_{\mu,\Lambda}|L_{-1} &= \mu\Lambda \langle\mathcal I_{\mu,\Lambda}|, \\ \langle\mathcal I_{\mu,\Lambda}|L_{-2} &= -\frac{\Lambda^2}{4} \langle\mathcal I_{\mu,\Lambda}|, \\ \langle\mathcal I_{\mu,\Lambda}|L_{-n} &=0, \qquad n>2. \end{aligned}

The first line is an operator identity: L0L_0 differentiates the scale dependence of the family of states. It is not an eigenvalue equation. Likewise, μ\mu and Λ\Lambda are irregular-state parameters, not the weight of a hidden highest-weight vector.

The distinction from an ordinary primary is structural:

State at infinityAction of the negative modes
Dual highest-weight state $\langle\Delta$
Rank-one irregular state $\langle\mathcal I_{\mu,\Lambda}$

The Virasoro commutators make these conditions compatible. For example,

[L1,L2]=L3.[L_{-1},L_{-2}] = L_{-3}.

The two prescribed eigenvalues commute, so the left-hand side vanishes on Iμ,Λ\langle\mathcal I_{\mu,\Lambda}| and forces the displayed L3L_{-3} constraint. Commutators with still lower modes propagate the vanishing conditions.

For an irregular ket at the origin, the mode indices reverse: L1L_1 and L2L_2 act diagonally and LnL_n vanishes for n>2n>2. This bra-versus-ket reversal is a convention, not a change of irregular rank.

The label “rank one” is not a substitute for these equations. Sources can rescale (μ,Λ)(\mu,\Lambda), reverse signs, or use a different rank label for an L1L_1-only state. Comparisons should begin with the nonzero Virasoro modes and their eigenvalues.

The collision keeps finite first and second moments

Section titled “The collision keeps finite first and second moments”

Use the book’s centered Liouville momentum aLa_{\mathrm L}, for which

ΔCFT=QL24aL2.\Delta^{\mathrm{CFT}} = \frac{Q_{\mathrm L}^2}{4} -a_{\mathrm L}^2.

Introduce a collision parameter RR and choose

aL,(R)=μ+R2,aL,t(R)=Rμ2,t=RΛ.\begin{aligned} a_{\mathrm L,\infty}(R) &= -\frac{\mu+R}{2}, \\ a_{\mathrm L,t}(R) &= \frac{R-\mu}{2}, \\ t &= \frac{R}{\Lambda}. \end{aligned}

Thus RR\to\infty sends the moving insertion at tt into infinity while both conformal weights diverge. After an explicit power normalization,

Iμ,ΛlimRtΔtCFT(R)ΔCFT(R)Δ(R)VΔt(R)(t).\begin{aligned} \langle\mathcal I_{\mu,\Lambda}| \propto \lim_{R\to\infty} t^{ \Delta_t^{\mathrm{CFT}}(R) -\Delta_\infty^{\mathrm{CFT}}(R) } \langle\Delta_\infty(R)| V_{\Delta_t(R)}(t). \end{aligned}

The proportionality sign is intentional. An RR-dependent but Λ\Lambda-independent scalar renormalization may first be needed to make a chosen analytic normalization finite. Once it is fixed, a finite function of the remaining momenta and of μ\mu fixes the residual three-point normalization. Neither factor changes the Virasoro constraints.

Two elementary checks expose the scaling:

ΔtCFT(R)ΔCFT(R)=μR,\Delta_t^{\mathrm{CFT}}(R) -\Delta_\infty^{\mathrm{CFT}}(R) = \mu R,

while

t1R=Λ.t^{-1}R=\Lambda.

The divergent weights and the vanishing inverse position combine into finite first and second moments, μΛ\mu\Lambda and Λ2/4-\Lambda^2/4. Those are precisely the L1L_{-1} and L2L_{-2} eigenvalues above. If the weights were held fixed while tt\to\infty, both moments would vanish and the generic rank-one irregular type would not survive.

One can audit the modes before taking the limit. Put s=ΔtCFTΔCFTs=\Delta_t^{\mathrm{CFT}}-\Delta_\infty^{\mathrm{CFT}} and denote the power-normalized state at finite RR by IR\langle I_R|. The primary commutator gives, for k1k\geq1,

IRLk=tk[tt+(1k)ΔtCFTs]IR.\begin{aligned} \langle I_R|L_{-k} = -t^{-k} \left[ t\partial_t +(1-k)\Delta_t^{\mathrm{CFT}} -s \right] \langle I_R|. \end{aligned}

At fixed RR, tt=ΛΛt\partial_t=-\Lambda\partial_\Lambda. The derivative term is suppressed by tkt^{-k}, while the divergent part of ΔtCFT\Delta_t^{\mathrm{CFT}} survives only for k2k\leq2. Substitution gives μΛ\mu\Lambda, Λ2/4-\Lambda^2/4, and zero for k>2k>2, respectively.

A scaled collision of two regular punctures produces a rank-one irregular state, a confluent BPZ equation, and then the confluent Heun oper.

A collision is a correlated limit of position and momenta. Fixed weights make the distant puncture disappear; scaled centered momenta retain the finite Virasoro moments μΛ\mu\Lambda and Λ2/4-\Lambda^2/4, which become the formal data of the rank-one irregular end.

This construction is an analytic chiral limit. The intermediate regular weights need not lie in a unitary spectrum, and a full Liouville correlator requires additional structure constants, antiholomorphic data, and a contour prescription.

The exact confluent BPZ equation is still a PDE

Section titled “The exact confluent BPZ equation is still a PDE”

Throughout this finite-bb subsection, Δj\Delta_j abbreviates ΔjCFT\Delta_j^{\mathrm{CFT}}; in particular, Δ2,1\Delta_{2,1} is the weight of the (2,1)(2,1) degenerate field.

Insert the book’s light degenerate field Vb/2(z)V_{-b/2}(z) between a regular state at zero, a regular primary at one, and the irregular bra:

G(z,Λ):=Iμ,ΛV1(1)Vb/2(z)Δ0.\mathcal G(z,\Lambda) := \left\langle \mathcal I_{\mu,\Lambda} \right| V_1(1) V_{-b/2}(z) \left| \Delta_0 \right\rangle.

The null relation and the irregular Ward identities give

0=[b2z2(1z+1z1)z+ΛΛΔ2,1Δ1Δ0z(z1)+Δ1(z1)2+Δ0z2+μΛzΛ24]G.\begin{aligned} 0 ={}& \left[ b^{-2}\partial_z^2 - \left( \frac1z+\frac1{z-1} \right)\partial_z \right. \\ &\left. + \frac{ \Lambda\partial_\Lambda -\Delta_{2,1} -\Delta_1 -\Delta_0 }{ z(z-1) } \right. \\ &\left. + \frac{\Delta_1}{(z-1)^2} + \frac{\Delta_0}{z^2} + \frac{\mu\Lambda}{z} - \frac{\Lambda^2}{4} \right] \mathcal G. \end{aligned}

This is the confluent analogue of the five-insertion BPZ equation. The regular modulus has been replaced by the irregular scale Λ\Lambda, but its derivative has not disappeared. At finite bb the equation is a PDE in (z,Λ)(z,\Lambda).

The singularity structure is already visible:

PointExact BPZ behavior
z=0z=0Regular singularity controlled by Δ0\Delta_0
z=1z=1Regular singularity controlled by Δ1\Delta_1
z=z=\inftyIrregular terms μΛ/zΛ2/4\mu\Lambda/z-\Lambda^2/4

If the insertion at one is omitted, the same Ward calculation gives the one-regular-point equation

[b2z21zz+Δ0z2+μΛzΛ24]GW=0.\left[ b^{-2}\partial_z^2 -\frac1z\partial_z +\frac{\Delta_0}{z^2} +\frac{\mu\Lambda}{z} -\frac{\Lambda^2}{4} \right]\mathcal G_{\mathrm W} =0.

After a scalar power gauge this is Whittaker’s equation. It is the rigid confluent-hypergeometric benchmark behind the nonrigid confluent-Heun problem.

More explicitly, set

Δ0CFT=QL24aL,02,x=bΛz,GW=zb2/2w(x).\Delta_0^{\mathrm{CFT}} = \frac{Q_{\mathrm L}^2}{4} -a_{\mathrm L,0}^2, \qquad x=b\Lambda z, \qquad \mathcal G_{\mathrm W} = z^{b^2/2}w(x).

Then

 ⁣d2w ⁣dx2+[14+bμx+14b2aL,02x2]w=0.\frac{\dd^2w}{\dd x^2} + \left[ -\frac14 +\frac{b\mu}{x} +\frac{ \frac14-b^2a_{\mathrm L,0}^2 }{x^2} \right]w =0.

The two regular-end branches are proportional to

zb2/2Mbμ,±baL,0(bΛz).z^{b^2/2} M_{b\mu,\,\pm b a_{\mathrm L,0}} (b\Lambda z).

Whittaker WW-type solutions instead encode sectorial asymptotics at the irregular end. Their connection coefficients are not needed for the confluent-Heun derivation below.

Heavy–light factorization produces the irregular oper

Section titled “Heavy–light factorization produces the irregular oper”

Take b0b\to0 in a fixed complex sector and scale

baL,0θ02,baL,1θ12,bμm,bΛL.\begin{aligned} b\,a_{\mathrm L,0} &\longrightarrow \frac{\theta_0}{2}, & b\,a_{\mathrm L,1} &\longrightarrow \frac{\theta_1}{2}, \\ b\mu&\longrightarrow m, & b\Lambda&\longrightarrow L. \end{aligned}

Then

δi:=limb0b2ΔiCFT=1θi24,i{0,1}.\delta_i := \lim_{b\to0}b^2\Delta_i^{\mathrm{CFT}} = \frac{1-\theta_i^2}{4}, \qquad i\in\{0,1\}.

Fix a heavy internal channel as well:

b2ΔintCFTδint=1θint24.b^2\Delta_{\mathrm{int}}^{\mathrm{CFT}} \longrightarrow \delta_{\mathrm{int}} = \frac{1-\theta_{\mathrm{int}}^2}{4}.

Let Birr(Λ)\mathcal B_{\mathrm{irr}}(\Lambda) be the background irregular block obtained by removing the degenerate probe. Define its classical scale coordinate directly by

u(L):=limb0b2ΛΛ\LogBirr(Λ)Λ=L/b.u(L) := \lim_{b\to0} b^2\Lambda\partial_\Lambda \Log\mathcal B_{\mathrm{irr}}(\Lambda) \bigg|_{\Lambda=L/b}.

This derivative definition is safer than taking limb2\LogBirr(L/b)\lim b^2\Log\mathcal B_{\mathrm{irr}}(L/b) directly: the leading power can leave an LL-independent term proportional to \Logb\Log b. After choosing an LL-independent subtraction, introduce a primitive firrf_{\mathrm{irr}} by

u(L)=LLfirr(L).u(L) = L\partial_Lf_{\mathrm{irr}}(L).

Now factor

G(z,Λ)=Birr(Λ)Ψb(z;L).\mathcal G(z,\Lambda) = \mathcal B_{\mathrm{irr}}(\Lambda) \Psi_b(z;L).

Assume that Ψb\Psi_b and its first two zz-derivatives converge locally uniformly to ψ\psi, and that

b2ΛΛΨb0b^2\Lambda\partial_\Lambda\Psi_b \longrightarrow 0

locally uniformly on the same domain. This is the derivative-compatible irregular heavy–light hypothesis.

After multiplying the exact BPZ equation by b2b^2, every surviving term has a transparent origin:

Finite-bb quantityClassical limit
b2ΔiCFTb^2\Delta_i^{\mathrm{CFT}}δi\delta_i
b2ΛΛ\LogBirrb^2\Lambda\partial_\Lambda\Log\mathcal B_{\mathrm{irr}}uu
b2μΛb^2\mu\LambdamLmL
b2Λ2b^2\Lambda^2L2L^2
b2Δ2,1b^2\Delta_{2,1} and the first-derivative term00

The limiting probe equation is

[z2+Tirr(z;L)]ψ(z;L)=0,\left[ \partial_z^2 +T_{\mathrm{irr}}(z;L) \right]\psi(z;L) =0,

with

Tirr(z;L)=δ0z2+δ1(z1)2+uδ0δ1z(z1)+mLzL24.\begin{aligned} T_{\mathrm{irr}}(z;L) ={}& \frac{\delta_0}{z^2} + \frac{\delta_1}{(z-1)^2} \\ &+ \frac{ u-\delta_0-\delta_1 }{ z(z-1) } + \frac{mL}{z} - \frac{L^2}{4}. \end{aligned}

This is the rank-one irregular counterpart of the four-pole oper on the preceding page. The single coefficient uu is supplied by a scale derivative rather than a position derivative.

The leading irregular power must be retained

Section titled “The leading irregular power must be retained”

Suppose the full and unit-leading irregular blocks are related by

Birr(Λ)=ΛΔintB^irr(Λ).\mathcal B_{\mathrm{irr}}(\Lambda) = \Lambda^{\Delta_{\mathrm{int}}} \widehat{\mathcal B}_{\mathrm{irr}}(\Lambda).

After absorbing an LL-independent normalization into the chosen branch,

firr(L)=δint\LogL+f^irr(L),f_{\mathrm{irr}}(L) = \delta_{\mathrm{int}}\Log L +\widehat f_{\mathrm{irr}}(L),

and therefore

u(L)=δint+LLf^irr(L).u(L) = \delta_{\mathrm{int}} +L\partial_L\widehat f_{\mathrm{irr}}(L).

For a unit-leading small-LL series,

u(L)=δint+O(L).u(L) = \delta_{\mathrm{int}} +O(L).

At L=0L=0 the irregular terms vanish and the oper reduces to the three-regular-point coefficient

T0(z)=δ0z2+δ1(z1)2+δintδ0δ1z(z1).\begin{aligned} T_0(z) ={}& \frac{\delta_0}{z^2} + \frac{\delta_1}{(z-1)^2} \\ &+ \frac{ \delta_{\mathrm{int}} -\delta_0 -\delta_1 }{ z(z-1) }. \end{aligned}

Thus the collision family returns to its hypergeometric boundary with the chosen internal exponent at infinity. Dropping the leading irregular power would fail this check.

Pole order and formal exponentials identify rank one

Section titled “Pole order and formal exponentials identify rank one”

For large zz, the normal-form coefficient has the expansion

Tirr(z;L)=L24+mLz+uz2+O(z3).T_{\mathrm{irr}}(z;L) = -\frac{L^2}{4} +\frac{mL}{z} +\frac{u}{z^2} +O(z^{-3}).

Under inversion w=1/zw=1/z, the projective connection transforms as

T~(w)=w4Tirr(1/w),\widetilde T(w) = w^{-4}T_{\mathrm{irr}}(1/w),

because inversion is Möbius and its Schwarzian vanishes. Hence

T~(w)=L24w4+mLw3+uw2+O(w1).\widetilde T(w) = -\frac{L^2}{4w^4} +\frac{mL}{w^3} +\frac{u}{w^2} +O(w^{-1}).

For L0L\neq0, the fourth-order pole is the scalar normal-form signature of an unramified rank-one irregular singularity.

The two formal branches begin as

ψ^±(z)=exp(±Lz2)zm[1+O(z1)].\widehat\psi_\pm(z) = \exp\left( \pm\frac{Lz}{2} \right) z^{\mp m} \left[ 1+O(z^{-1}) \right].

The exponent difference is LzLz. Its real part changes sign on Re(Lz)=0\operatorname{Re}(Lz)=0, so different sectors have different dominant branches. Actual analytic solutions asymptotic to ψ^±\widehat\psi_\pm are sectorial and are related across sector boundaries by Stokes matrices. The parameter mm is formal monodromy data; it is not a pair of ordinary Frobenius exponents at infinity.

The DLMF confluent-Heun dictionary is exact

Section titled “The DLMF confluent-Heun dictionary is exact”

Use the DLMF confluent Heun equation

y+(γCz+δCz1+ϵC)y+αCzqCz(z1)y=0.\begin{aligned} y'' &+ \left( \frac{\gamma_{\mathrm C}}z + \frac{\delta_{\mathrm C}}{z-1} + \epsilon_{\mathrm C} \right)y' \\ &+ \frac{ \alpha_{\mathrm C}z-q_{\mathrm C} }{ z(z-1) }y =0. \end{aligned}

The subscript C\mathrm C keeps these canonical parameters distinct from CFT weights and centered momenta. On a simply connected patch, set

y(z)=exp(ϵCz2)zγC/2(1z)δC/2ψ(z).\begin{aligned} y(z) ={}& \exp\left( -\frac{\epsilon_{\mathrm C}z}{2} \right) z^{-\gamma_{\mathrm C}/2} (1-z)^{-\delta_{\mathrm C}/2} \psi(z). \end{aligned}

The exact inverse dictionary from the irregular oper is

γC=1θ0,δC=1θ1,ϵC=L,αC=L(m+γC+δC2),\begin{aligned} \gamma_{\mathrm C} &= 1-\theta_0, & \delta_{\mathrm C} &= 1-\theta_1, \\ \epsilon_{\mathrm C} &= L, & \alpha_{\mathrm C} &= L \left( m+\frac{\gamma_{\mathrm C}+\delta_{\mathrm C}}2 \right), \end{aligned}

together with

qC=14(γC+δC1)24+L(m+γC2)u.\begin{aligned} q_{\mathrm C} ={}& \frac14 - \frac{ \left( \gamma_{\mathrm C}+\delta_{\mathrm C}-1 \right)^2 }{4} \\ &+ L \left( m+\frac{\gamma_{\mathrm C}}2 \right) -u. \end{aligned}

Equivalently, the forward accessory map is

u=14qC+αC(γC+δC1)24δCϵC2.\begin{aligned} u ={}& \frac14 -q_{\mathrm C} +\alpha_{\mathrm C} \\ &- \frac{ \left( \gamma_{\mathrm C}+\delta_{\mathrm C}-1 \right)^2 }{4} - \frac{ \delta_{\mathrm C}\epsilon_{\mathrm C} }{2}. \end{aligned}

The regular standard-form exponents are

z=00, 1γC=θ0z=10, 1δC=θ1.\begin{array}{c|c} z=0 & 0,\ 1-\gamma_{\mathrm C}=\theta_0 \\ z=1 & 0,\ 1-\delta_{\mathrm C}=\theta_1 \end{array}.

For L=ϵC0L=\epsilon_{\mathrm C}\neq0, the two standard-form asymptotic branches at infinity are instead

y+(z)zαC/ϵC,y(z)exp(ϵCz)zαC/ϵCγCδC.\begin{aligned} y_+(z) &\sim z^{-\alpha_{\mathrm C}/\epsilon_{\mathrm C}}, \\ y_-(z) &\sim \exp(-\epsilon_{\mathrm C}z) z^{ \alpha_{\mathrm C}/\epsilon_{\mathrm C} -\gamma_{\mathrm C} -\delta_{\mathrm C} }. \end{aligned}

Dividing by the scalar gauge recovers ψ^±\widehat\psi_\pm. This simultaneously checks the exponential signs and the definition of mm. At L=0L=0, the dictionary also has αC=0\alpha_{\mathrm C}=0: the equation lies on its hypergeometric boundary, and mm is no longer an independent differential-equation parameter.

The ODE confluence mirrors the CFT collision

Section titled “The ODE confluence mirrors the CFT collision”

The coefficient limit can be checked independently of CFT. Let the fourth regular singularity of the general Heun equation be AA\to\infty and fix target confluent parameters with ϵC0\epsilon_{\mathrm C}\neq0. Scale

ϵG=AϵC,αG=αCϵC,βG=AϵC+γC+δC1αCϵC,qG=AqC.\begin{aligned} \epsilon_{\mathrm G} &= -A\epsilon_{\mathrm C}, \\ \alpha_{\mathrm G} &= \frac{\alpha_{\mathrm C}}{\epsilon_{\mathrm C}}, \\ \beta_{\mathrm G} &= -A\epsilon_{\mathrm C} +\gamma_{\mathrm C} +\delta_{\mathrm C} -1 -\frac{\alpha_{\mathrm C}}{\epsilon_{\mathrm C}}, \\ q_{\mathrm G} &= -Aq_{\mathrm C}. \end{aligned}

The general-Heun Fuchs relation holds exactly. For fixed zz away from 00 and 11,

ϵGzAϵC,\frac{\epsilon_{\mathrm G}}{z-A} \longrightarrow \epsilon_{\mathrm C},

and

αGβGzqGz(z1)(zA)αCzqCz(z1).\frac{ \alpha_{\mathrm G}\beta_{\mathrm G}z-q_{\mathrm G} }{ z(z-1)(z-A) } \longrightarrow \frac{ \alpha_{\mathrm C}z-q_{\mathrm C} }{ z(z-1) }.

This is the same mechanism as the CFT collision: a point moves to infinity while selected parameters diverge so that finite first and second moments remain. The Heun confluence page proves local-uniform coefficient and initial-value solution convergence and records the O(A1)O(A^{-1}) remainder.

The matching concerns the equation and fixed-base-point solutions on an outer domain. Frobenius bases attached to the moving singularity generally need singular normalization before they approach sectorial bases of the irregular equation.

The regular accessory has a finite irregular remainder

Section titled “The regular accessory has a finite irregular remainder”

The same collision can be checked directly in normal form. Start from the four-pole oper

TA(z)=δ0z2+δ1(z1)2+δA(zA)2+ΞAz(z1)+A(A1)cAz(z1)(zA),\begin{aligned} T_A(z) ={}& \frac{\delta_0}{z^2} +\frac{\delta_1}{(z-1)^2} +\frac{\delta_A}{(z-A)^2} \\ &+ \frac{\Xi_A}{z(z-1)} + \frac{ A(A-1)c_A }{ z(z-1)(z-A) }, \end{aligned}

where

ΞA=δδ0δAδ1.\Xi_A = \delta_\infty-\delta_0-\delta_A-\delta_1.

Choose exponent representatives and the accessory scaling

θA=ALm,θ=ALm,cA=mLuA+O(A2),δν=1θν24.\begin{aligned} \theta_A&=AL-m, & \theta_\infty&=-AL-m, \\ c_A&=-mL-\frac{u}{A}+O(A^{-2}), & \delta_\nu&=\frac{1-\theta_\nu^2}{4}. \end{aligned}

Then ΞA=ALmδ0δ1\Xi_A=-ALm-\delta_0-\delta_1, and direct expansion gives TATirrT_A\to T_{\mathrm{irr}} locally uniformly away from 00 and 11. In this normalization the irregular energy is the finite remainder

u=limAA(cA+mL).u = -\lim_{A\to\infty} A\left(c_A+mL\right).

Thus the regular accessory itself tends to mL-mL; subtracting that collision term and rescaling extracts the classical irregular-block coordinate. Here cA=(Afreg){δν}c_A=(\partial_A f_{\mathrm{reg}})_{\{\delta_\nu\}} is defined with the regular weights held fixed. Differentiating along the collision path without accounting for their variation gives a different—and incorrect—remainder.

What changes when a regular point becomes irregular

Section titled “What changes when a regular point becomes irregular”

The collision changes the correct local data, not merely the function name.

Regular point before collisionRank-one irregular point after collision
Two Frobenius powersTwo formal exponential-power branches
One local monodromy matrixFormal monodromy plus Stokes matrices
Punctured diskOverlapping sectors
Resonance from an integer exponent differenceFormal resonance and Stokes degeneracies, analyzed separately
Frobenius-normalized connection matrixSectorially normalized connection or Stokes matrix

The classical irregular block supplies uu, hence the differential equation. It does not by itself specify sector labels, summation directions, asymptotic normalizations, Stokes multipliers, or a regular-to- irregular connection matrix. Chapter 7 adds the irregular fusion factors and normalization data needed for those connection problems.

Sending a puncture away with fixed weights. Then its polar moments vanish on the outer domain. The generic confluent equation requires a compensating momentum and accessory scaling.

Calling the irregular state a highest-weight state. Its L0L_0 action is a scale derivative, and two higher moments act diagonally. It belongs to a Whittaker-type Virasoro module rather than an ordinary Verma module.

Treating the exact confluent BPZ equation as an ODE. The term ΛΛ\Lambda\partial_\Lambda survives at finite bb. It becomes the number uu only after a derivative-compatible classical factorization.

Using a unit-leading block without restoring its power. The full scale derivative contains δint\delta_{\mathrm{int}}. Omitting it gives the wrong L0L\to0 hypergeometric boundary.

Writing qC=uq_{\mathrm C}=u. The irregular block derivative is the normal-form coordinate uu. The standard confluent-Heun accessory qCq_{\mathrm C} differs by the displayed scalar-gauge shift.

Assigning Frobenius exponents to the irregular end. Infinity has formal exponential powers and Stokes sectors for L0L\neq0. The regular limit L=0L=0 is a different singularity stratum.

1. Check the irregular Virasoro constraints

Section titled “1. Check the irregular Virasoro constraints”

Use the Virasoro commutator to show that the prescribed L1L_{-1} and L2L_{-2} eigenvalues imply Iμ,ΛL3=0\langle\mathcal I_{\mu,\Lambda}|L_{-3}=0.

Solution

Since

[L1,L2]=L3,[L_{-1},L_{-2}] = L_{-3},

the left-hand side acts by

(μΛ)(Λ24)(Λ24)(μΛ)=0.(\mu\Lambda) \left( -\frac{\Lambda^2}{4} \right) - \left( -\frac{\Lambda^2}{4} \right) (\mu\Lambda) =0.

Therefore the action of L3L_{-3} vanishes. Commuting L1L_{-1} with LnL_{-n} then propagates the higher vanishing constraints.

Starting from the two centered momenta, compute ΔtCFTΔCFT\Delta_t^{\mathrm{CFT}}-\Delta_\infty^{\mathrm{CFT}}.

Solution

The common QL2/4Q_{\mathrm L}^2/4 cancels, so

ΔtCFTΔCFT=(μR)24+(μ+R)24=μR.\begin{aligned} \Delta_t^{\mathrm{CFT}} -\Delta_\infty^{\mathrm{CFT}} &= -\frac{(\mu-R)^2}{4} +\frac{(\mu+R)^2}{4} \\ &= \mu R. \end{aligned}

Thus the normalizing power is tμRt^{\mu R}. Together with t=R/Λt=R/\Lambda, it removes the divergent dilation weight while leaving finite Λ\Lambda-dependent Virasoro moments.

3. Recover the classical oper term by term

Section titled “3. Recover the classical oper term by term”

Multiply the exact BPZ equation by b2b^2, insert the heavy–light factorization, and recover TirrT_{\mathrm{irr}}.

Solution

The background logarithmic derivative gives

b2ΛΛ\LogBirru.b^2\Lambda\partial_\Lambda \Log\mathcal B_{\mathrm{irr}} \longrightarrow u.

The heavy weights give δ0\delta_0 and δ1\delta_1, while

b2μΛmL,b2Λ2L2.b^2\mu\Lambda\to mL, \qquad b^2\Lambda^2\to L^2.

The light degenerate weight and the first-derivative term are multiplied by b2b^2 and vanish. The coefficient of 1/[z(z1)]1/[z(z-1)] is therefore uδ0δ1u-\delta_0-\delta_1, giving exactly the displayed oper.

Invert z=1/wz=1/w and derive both the pole order and the leading formal branches.

Solution

The half-density transformation gives

T~(w)=w4T(1/w)=L24w4+mLw3+O(w2).\widetilde T(w) = w^{-4}T(1/w) = -\frac{L^2}{4w^4} +\frac{mL}{w^3} +O(w^{-2}).

For L0L\neq0, this is an unramified rank-one irregular singularity in scalar normal form. For a formal ansatz

ψ=exp(sLz2)zρ[1+O(z1)],s=±1,\psi = \exp\left( \frac{sLz}{2} \right)z^\rho \left[ 1+O(z^{-1}) \right], \qquad s=\pm1,

the constant terms cancel and the z1z^{-1} coefficient is L(sρ+m)L(s\rho+m). Hence ρ=sm\rho=-sm, which gives ψ^±\widehat\psi_\pm.

Assume Birr=ΛΔintB^irr\mathcal B_{\mathrm{irr}} =\Lambda^{\Delta_{\mathrm{int}}} \widehat{\mathcal B}_{\mathrm{irr}}. Find uu in terms of the unit-leading classical block.

Solution

Taking the logarithm, multiplying by b2b^2, and holding L=bΛL=b\Lambda fixed in the classical scaling gives

firr=δint\LogL+f^irrf_{\mathrm{irr}} = \delta_{\mathrm{int}}\Log L +\widehat f_{\mathrm{irr}}

up to an LL-independent term. Therefore

u=LLfirr=δint+LLf^irr.u = L\partial_Lf_{\mathrm{irr}} = \delta_{\mathrm{int}} +L\partial_L\widehat f_{\mathrm{irr}}.

Apply the scalar gauge to the DLMF equation and recover the displayed formula for uu.

Solution

For

p(z)=γCz+δCz1+ϵC,p(z) = \frac{\gamma_{\mathrm C}}z +\frac{\delta_{\mathrm C}}{z-1} +\epsilon_{\mathrm C},

the normal coefficient is

T=αCzqCz(z1)12p14p2.T = \frac{\alpha_{\mathrm C}z-q_{\mathrm C}}{z(z-1)} -\frac12p' -\frac14p^2.

Its double-pole coefficients are γC(2γC)/4\gamma_{\mathrm C}(2-\gamma_{\mathrm C})/4 and δC(2δC)/4\delta_{\mathrm C}(2-\delta_{\mathrm C})/4. Matching the constant and the sum of its simple-pole residues gives

L=ϵC,m=αCϵCγC+δC2.L=\epsilon_{\mathrm C}, \qquad m = \frac{\alpha_{\mathrm C}}{\epsilon_{\mathrm C}} -\frac{\gamma_{\mathrm C}+\delta_{\mathrm C}}2.

Matching the remaining 1/[z(z1)]1/[z(z-1)] coefficient gives

u=14qC+αC(γC+δC1)24δCϵC2.\begin{aligned} u ={}& \frac14-q_{\mathrm C}+\alpha_{\mathrm C} \\ &- \frac{ (\gamma_{\mathrm C}+\delta_{\mathrm C}-1)^2 }{4} - \frac{\delta_{\mathrm C}\epsilon_{\mathrm C}}2. \end{aligned}

7. Show why an unscaled moving pole is insufficient

Section titled “7. Show why an unscaled moving pole is insufficient”

Let AA\to\infty in the general Heun equation while every canonical parameter stays bounded. Determine the outer coefficient limit.

Solution

For fixed zz,

ϵGzA=O(A1),\frac{\epsilon_{\mathrm G}}{z-A} = O(A^{-1}),

and

αGβGzqGz(z1)(zA)=O(A1).\frac{ \alpha_{\mathrm G}\beta_{\mathrm G}z-q_{\mathrm G} }{ z(z-1)(z-A) } = O(A^{-1}).

The limiting equation is

y+(γGz+δGz1)y=0,y'' + \left( \frac{\gamma_{\mathrm G}}z + \frac{\delta_{\mathrm G}}{z-1} \right)y' =0,

a degenerate Fuchsian equation. The generic confluent-Heun terms survive only under the divergent parameter scaling used on this page.