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Stage B: Canonical Sectorial Solutions and Local Connection Formulae

Page 3 divided the spatial surface into Stokes regions. A formal WKB branch in one such region is still not a canonical analytic solution. It becomes one only after the phase of \hbar, Borel direction, square-root sheet, normalization endpoint and path, spatial region, and lateral convention have all been fixed—and after the required summability theorem has been verified.

With those data in place, a simple turning point has a universal local answer. For a counterclockwise pair of adjacent regions, the turning-point-normalized bases are related by a unipotent triangular matrix whose nonzero off-diagonal entry is +i+\ii in the source-facing relation. The matrix that replaces the continued source frame by the canonical destination frame is its inverse and contains i-\ii. Rotated Airy functions fix this distinction exactly rather than mnemonically.

A simple pole is also a branch point of the WKB cover, but it is not an Airy turning point. In the standard meromorphic exact-WKB framework its multiplier is

2icos(πνs),νs2=1+4bs,2\ii\cos(\pi\nu_s), \qquad \nu_s^2=1+4b_s,

where bsb_s is the double-pole coefficient of the 2\hbar^2 correction in Schrödinger normal form. This page derives the associated modified Bessel model, states the precise local theorem, and stops before the Voros transports and wall-crossing rules needed for global products.

“Canonical” is a data package, not a preferred formula

Section titled ““Canonical” is a data package, not a preferred formula”

Retain the book’s normal form and Wronskian convention,

2ψ=R(z,)ψ,R(z,)=R0(z)+O(),Wr[f,g]=fgfg,λ0=R0(z) ⁣dz.\begin{aligned} \hbar^2\psi'' &=R(z,\hbar)\psi, \\ R(z,\hbar) &=R_0(z)+O(\hbar), \\ \Wr[f,g] &=fg'-f'g, \\ \lambda_0 &=\sqrt{R_0(z)}\,\dd z. \end{aligned}

The word canonical will always be relative to a declared passport. At minimum it contains

P=(Θ,Lθ,D,z^,N,Γ,s),\mathcal P = (\Theta_\hbar,L_\theta,D,\widehat z, N,\Gamma,\mathfrak s),

with the following meanings.

DatumWhat it fixes
Θ\Theta_\hbarAn \hbar-sector on which the summed solution is analytic
Lθ=eiθR+L_\theta=\ee^{\ii\theta}\mathbb R_+The ray used by the book’s Borel–Laplace integral
DDA regular spatial Stokes region, or a smaller admissible domain inside it
z^Σ^\widehat z\in\widehat\SigmaThe square-root sheet and therefore the ++/- Riccati labels
NNA regular base point or a specified singular-endpoint normalization
Γ\GammaThe lifted continuation and integration path, including its homotopy class
s\mathfrak sOrdinary or lateral Borel prescription, with an explicitly oriented detour

Three uses of sector should not be conflated.

Sector-like objectVariableBoundary selected by
Borel-summation sector\hbarLaplace decay and Borel growth
Stokes regionzzCritical horizontal trajectories of ϕθ\phi_\theta
Canonical asymptotic sector at an irregular polezz near that poleThe local exponential asymptotics there

A solution can be sectorial in the first and third senses while being defined throughout one spatial Stokes region. None of these domains is a chamber in the parameter–phase space of Page 3.

Borel summation supplies the analytic branches

Section titled “Borel summation supplies the analytic branches”

Let

Peven=P(+)P()2P_{\mathrm{even}} = \frac{P^{(+)}-P^{(-)}}{2}

be the branch-antisymmetric Riccati momentum of Chapter 8. When the potential is even in \hbar, its name also describes its literal parity. If odd powers occur, the same symbol still denotes the branch difference; it need not then be an even series.

For a regular base point or finite ramified endpoint NN, and a lifted path ΓN,z\Gamma_{N,z}, the unit formal branches are

ψ^±,N=Peven(z,)1/2×exp ⁣[±1ΓN,zPeven(ζ,) ⁣dζ].\begin{aligned} \widehat\psi_{\pm,N} ={}&P_{\mathrm{even}}(z,\hbar)^{-1/2} \\ &\times \exp\!\left[ \pm\frac{1}{\hbar} \int_{\Gamma_{N,z}} P_{\mathrm{even}}(\zeta,\hbar)\,\dd\zeta \right]. \end{aligned}

The infinite-pole analogue is defined only after the subtraction displayed below.

Factor the classical exponential before applying the ordinary shifted Borel transform of Page 1. For a regular or finite ramified endpoint, put

WN(z)=ΓN,zλ0,W_N(z) = \int_{\Gamma_{N,z}}\lambda_0,

with the half-contour interpretation when applicable. At an infinite pole, WNW_N instead denotes the separately normalized classical primitive in the endpoint-subtracted formula below; the divergent integral from the pole is never used literally. In either case write

ψ^±,N=exp ⁣(±WN)F^±,N.\widehat\psi_{\pm,N} = \exp\!\left(\pm\frac{W_N}{\hbar}\right) \widehat F_{\pm,N}.

Whenever F^±,N\widehat F_{\pm,N} is directionally summable with estimates locally uniform in zDz\in D, define

Ψ±,ND,θ(z,):=exp ⁣(±WN(z))×SθF^±,N(z,).\begin{aligned} \Psi_{\pm,N}^{D,\theta}(z,\hbar) :={}& \exp\!\left(\pm\frac{W_N(z)}{\hbar}\right) \\ &\times \mathcal S_\theta \widehat F_{\pm,N}(z,\hbar). \end{aligned}

The Laplace kernel eξ/\ee^{-\xi/\hbar} requires, more precisely, a subsector on which

Re(eiθ)>κ\operatorname{Re} \left( \frac{\ee^{\ii\theta}}{\hbar} \right) >\kappa

for the applicable Borel growth rate κ\kappa. Thus the central choice arg=θ\arg\hbar=\theta is convenient but not part of the definition of the graph. Page 3’s graph angle and the actual \hbar phase remain distinct data.

Under the analytic hypotheses of the summability theorem—rather than by formal coefficient matching alone—Ψ±,ND,θ\Psi_{\pm,N}^{D,\theta} solves the differential equation exactly. Nikolaev’s published theorem gives existence, uniqueness, and locally uniform Borel summation for the branch associated with one complete oriented WKB (θ,+)(\theta,+) or (θ,)(\theta,-) ray, under its stated analyticity and uniformity assumptions. A two-solution basis needs the hypotheses for both rays, or the generic-strip setting of its Corollary 5.6. Classical saddle-free exact-WKB frameworks instead assemble admissible paths inside Stokes regions. These are complementary theorem packages, not a license to omit the hypotheses.

The normalization endpoint changes the object

Section titled “The normalization endpoint changes the object”

If bDb\in D is regular, a value-one formal normalization is

χ^±,b(z,)=[Peven(b,)Peven(z,)]1/2×exp ⁣[±1bzPeven ⁣dζ].\begin{aligned} \widehat\chi_{\pm,b}(z,\hbar) ={}& \left[ \frac{P_{\mathrm{even}}(b,\hbar)} {P_{\mathrm{even}}(z,\hbar)} \right]^{1/2} \\ &\times \exp\!\left[ \pm\frac1\hbar \int_b^zP_{\mathrm{even}}\,\dd\zeta \right]. \end{aligned}

Then χ^±,b(b,)=1\widehat\chi_{\pm,b}(b,\hbar)=1. This pair differs from the unit WKB pair by a zz-independent scalar on each branch. It is often best for an initial-value problem, but its local Stokes multiplier is not the bare Airy constant unless the normalization factors are also transported.

Its formal ordered Wronskian is correspondingly

Wr[χ^+,b,χ^,b]=2Peven(b,).\Wr[ \widehat\chi_{+,b}, \widehat\chi_{-,b} ] = -\frac{2}{\hbar} P_{\mathrm{even}}(b,\hbar).

For an analytic summed pair, the right-hand side must be interpreted through the same multiplicative summation prescription used to build the two solutions.

Existence of such a regular-point-normalized exact solution does not, by itself, establish the existence of a turning-point-normalized one. The normalization constant needed in the singular limit may fail to exist or fail to have the required asymptotics. This distinction is explicit in rigorous existence theory and should not be hidden by the same symbol Ψ\Psi.

Let ee be an odd-order branch point of the spectral cover—a simple zero aa or, in the simple-pole framework below, a simple pole ss. The formal coefficients are singular at the base endpoint, so ezPeven ⁣dz\int_e^zP_{\mathrm{even}}\,\dd z is not an ordinary improper integral and Ψ(e)=1\Psi(e)=1 is not the normalization condition.

Choose the endpoint branch, a cut not crossing the Stokes edge in question, and a lifted contour γz\gamma_z from τ(z^)\tau(\widehat z) to z^\widehat z that passes around the branch point with the prescribed orientation. Define coefficientwise

ezPeven ⁣dζ:=12γzPeven ⁣dζ.\int_e^z P_{\mathrm{even}}\,\dd\zeta := \frac12 \int_{\gamma_z} P_{\mathrm{even}}\,\dd\zeta.

Anti-invariance under the deck involution makes this the intrinsic turning-endpoint prescription. The half-contour also applies to the simple-pole branch point in Koike’s setting, with its local theorem and coefficient hypotheses. The direction in which γz\gamma_z winds is part of the normalization.

At an infinite pole pp, the leading classical integral generally diverges. In the standard even framework one instead separates

Ω()=Peven ⁣dz,Ωreg=Ωλ0,\Omega(\hbar) = P_{\mathrm{even}}\,\dd z, \qquad \Omega^{\mathrm{reg}} = \Omega-\lambda_0,

and defines the regularized endpoint action and normalization by

Ip(z):=azλ0+pzΩreg,ψ^±,p=Peven1/2exp ⁣[±Ip(z)].\begin{aligned} \mathcal I_p(z) &:= \int_a^z\lambda_0 + \int_p^z\Omega^{\mathrm{reg}} , \\ \widehat\psi_{\pm,p} &= P_{\mathrm{even}}^{-1/2} \exp\!\left[ \pm\frac{\mathcal I_p(z)}{\hbar} \right]. \end{aligned}

Here the first term in Ip\mathcal I_p fixes a classical primitive through a chosen turning point aa, while the second uses the endpoint-subtracted quantum form. Its existence depends on the pole-order and projective correction hypotheses reviewed in Chapter 8. More general irregular normalizations may require additional polynomial or logarithmic subtractions. None is a pointwise value at pp.

Unit normalization makes the Wronskian a checksum

Section titled “Unit normalization makes the Wronskian a checksum”

For the unit formal pair, direct differentiation gives

Wr[ψ^+,N,ψ^,N]=2.\Wr[ \widehat\psi_{+,N}, \widehat\psi_{-,N} ] = -\frac2\hbar.

When both amplitudes are summed compatibly and differentiation commutes with the Borel–Laplace integral, the analytic pair inherits the exact identity

Wr[Ψ+,ND,θ,Ψ,ND,θ]=2.\Wr[ \Psi_{+,N}^{D,\theta}, \Psi_{-,N}^{D,\theta} ] = -\frac2\hbar.

The traditional exact-WKB notation uses

Soddtrad=PevenS_{\mathrm{odd}}^{\mathrm{trad}} = \frac{P_{\mathrm{even}}}{\hbar}

and the prefactor (Soddtrad)1/2(S_{\mathrm{odd}}^{\mathrm{trad}})^{-1/2}. Its solutions are \sqrt\hbar times the book’s pair and therefore have ordered Wronskian 2-2. The common scalar does not alter a local connection matrix.

If two ordered frames Fj=(fj,+,fj,)F_j=(f_{j,+},f_{j,-}) satisfy

F1=F2C,F_1=F_2C,

then

detC=Wr[f1,+,f1,]Wr[f2,+,f2,].\det C = \frac{ \Wr[f_{1,+},f_{1,-}] }{ \Wr[f_{2,+},f_{2,-}] }.

Every local matrix below has determinant one. That test catches a surprising number of transpositions and normalization errors, though it cannot determine the sign of the off-diagonal entry.

Fix a Borel direction θ\theta and its graph GθG_\theta for ϕθ=e2iθϕ0\phi_\theta=\ee^{-2\ii\theta}\phi_0. Let aa be a simple zero, and let a Stokes edge CC issuing from aa separate adjacent regions D1D_1 and D2D_2. Make the following choices and assumptions:

  1. D2D_2 is immediately counterclockwise from D1D_1 around aa.
  2. The branch cut used to label R0\sqrt{R_0} does not cross CC.
  3. Both WKB branches use the same half-contour normalization at aa.
  4. The coefficient and geometric hypotheses required for Borel summability hold—for example, the saddle-free meromorphic framework of the theorem quoted in the references.
  5. Analytic continuation is taken through a small regular point of CC, not through the singular endpoint aa.

On the chosen sheet define, along CC away from aa,

wθ,a(z)=eiθazλ0,εC:=sgnRewθ,a(z).\begin{aligned} w_{\theta,a}(z) &= \ee^{-\ii\theta} \int_a^z\lambda_0, \\ \varepsilon_C &:= \operatorname{sgn} \operatorname{Re}w_{\theta,a}(z). \end{aligned}

The real part is nonzero and has constant sign on the open edge. Put the scalar solutions into an ordered row frame

FD=(Ψ+D,ΨD).F_D = (\Psi_+^D,\Psi_-^D).

Write FD1D2F_{D_1}^{\to D_2} for the analytic continuation of the D1D_1 frame through a regular point of CC into D2D_2. In the component equations below, each left-hand D1D_1 solution is understood after that continuation.

For εC=+1\varepsilon_C=+1, the source-facing connection formula is

Ψ+D1=Ψ+D2+iΨD2,ΨD1=ΨD2.\begin{aligned} \Psi_+^{D_1} &= \Psi_+^{D_2} +\ii\Psi_-^{D_2}, \\ \Psi_-^{D_1} &= \Psi_-^{D_2}. \end{aligned}

Equivalently,

FD1D2=FD2L(i),L(s):=(10s1).F_{D_1}^{\to D_2} = F_{D_2}L(\ii), \qquad L(s) := \begin{pmatrix} 1&0\\ s&1 \end{pmatrix}.

For εC=1\varepsilon_C=-1,

Ψ+D1=Ψ+D2,ΨD1=ΨD2+iΨ+D2,\begin{aligned} \Psi_+^{D_1} &= \Psi_+^{D_2}, \\ \Psi_-^{D_1} &= \Psi_-^{D_2} +\ii\Psi_+^{D_2}, \end{aligned}

or

FD1D2=FD2U(i),U(s):=(1s01).F_{D_1}^{\to D_2} = F_{D_2}U(\ii), \qquad U(s) := \begin{pmatrix} 1&s\\ 0&1 \end{pmatrix}.

These equations state the theorem in exactly the orientation printed in the standard source: the analytic continuation of the D1D_1 solution is re-expanded in the D2D_2 basis. If a transfer algorithm instead replaces that continued source frame by the canonical destination frame, it inverts the matrix:

FD2=FD1D2{L(i),εC=+1,U(i),εC=1.F_{D_2} = F_{D_1}^{\to D_2} \begin{cases} L(-\ii),&\varepsilon_C=+1,\\ U(-\ii),&\varepsilon_C=-1. \end{cases}

Thus “counterclockwise gives +i+\ii” is incomplete. It gives +i+\ii in FD1D2=FD2CF_{D_1}^{\to D_2}=F_{D_2}C and i-\ii in the canonical-frame replacement FD2=FD1D2C1F_{D_2}=F_{D_1}^{\to D_2}C^{-1}. Analytic continuation itself is encoded by the first relation, not by C1C^{-1}.

What the triangular matrix actually changes

Section titled “What the triangular matrix actually changes”

On the central \hbar ray arg=θ\arg\hbar=\theta,

Ψ+Ψexp ⁣[2Rewθ,a].\left| \frac{\Psi_+}{\Psi_-} \right| \asymp \exp\!\left[ \frac{2\operatorname{Re}w_{\theta,a}} {|\hbar|} \right].

When εC=+1\varepsilon_C=+1, Ψ+\Psi_+ is dominant and the theorem changes that basis element by a multiple of the unchanged subdominant one. For εC=1\varepsilon_C=-1, the roles are reversed. If ϑ=argθ\vartheta=\arg\hbar\neq\theta, actual magnitude is instead governed by

Re[eiϑWa(z)],\operatorname{Re} \left[ \ee^{-\ii\vartheta}W_a(z) \right],

and on the edge this equals Rewθ,acos(θϑ)\operatorname{Re}w_{\theta,a}\cos(\theta-\vartheta). Consequently the graph sign still agrees with dominance throughout the compatible Laplace half-plane ϑθ<π/2|\vartheta-\theta|<\pi/2. It can reverse only after continuation beyond that half-plane; the formula above, not the central-ray mnemonic, remains the general test.

Continue a fixed solution across CC and write its expansions before and after the crossing as

ψ=FDjcj,cj=(AjBj).\psi=F_{D_j}c_j, \qquad c_j= \begin{pmatrix} A_j\\B_j \end{pmatrix}.

From FD1D2=FD2CF_{D_1}^{\to D_2}=F_{D_2}C one obtains

c2=Cc1.c_2=Cc_1.

For εC=+1\varepsilon_C=+1 this says

A2=A1,B2=B1+iA1.A_2=A_1, \qquad B_2=B_1+\ii A_1.

The dominant basis function changes, while the subdominant coefficient changes. Both familiar descriptions of the Stokes rule are therefore correct, but they refer to dual objects.

The deck transformation exchanges the branch labels. With

J=(0110),J= \begin{pmatrix} 0&1\\1&0 \end{pmatrix},

one has

JL(i)J=U(i).JL(\ii)J=U(\ii).

Reversing the spatial crossing gives

L(i)1=L(i),U(i)1=U(i).L(\ii)^{-1}=L(-\ii), \qquad U(\ii)^{-1}=U(-\ii).

Changing a sheet, reversing a path, transposing a basis convention, and inverting a crossing are four different operations. A sign table should record which one has actually been performed.

Suppose a new row frame is related to the endpoint-normalized one by

F~D=FDDD,\widetilde F_D=F_DD_D,

where DDD_D is diagonal and may itself be a Borel-summed open-action factor. Then

F~D1=F~D2C~,C~=DD21CDD1.\widetilde F_{D_1} = \widetilde F_{D_2}\widetilde C, \qquad \widetilde C = D_{D_2}^{-1}CD_{D_1}.

If the same diagonal matrix DD is used on both sides,

C~=D1CD.\widetilde C=D^{-1}CD.

For example,

D=diag(d+,d),D1L(i)D=(10id+/d1).\begin{aligned} D &=\operatorname{diag}(d_+,d_-), \\ D^{-1}L(\ii)D &= \begin{pmatrix} 1&0\\ \ii d_+/d_-&1 \end{pmatrix}. \end{aligned}

The bare i\ii is therefore universal only in the local endpoint normalization. Regular-basepoint normalizations dress it by an open exponential, whose Borel sum and lateral behavior are Voros data.

Exact Airy functions fix the sign and scale

Section titled “Exact Airy functions fix the sign and scale”

Consider the equation

2ψ=zψ,>0,X=z2/3,ω=e2πi/3.\begin{aligned} \hbar^2\psi''&=z\psi, & \hbar&>0, \\ X&=\frac{z}{\hbar^{2/3}}, & \omega&=\ee^{2\pi\ii/3}. \end{aligned}

Take the positive Stokes edge, let DD_\downarrow lie just below it, and let DD_\uparrow lie just above it. Thus DD_\uparrow follows DD_\downarrow counterclockwise around the turning point. On the positive edge,

w0,0(z)=23z3/2>0,w_{0,0}(z) = \frac23z^{3/2}>0,

so the growing branch is labelled ++ and the recessive branch is labelled -. Define the exact solutions

A(z,)=2π1/6\Ai(X),G(z,)=2π1/6eiπ/6\Ai(ωX),G(z,)=2π1/6eiπ/6\Ai(ω2X).\begin{aligned} A(z,\hbar) &= 2\sqrt\pi\,\hbar^{-1/6}\Ai(X), \\ G_\downarrow(z,\hbar) &= 2\sqrt\pi\,\hbar^{-1/6} \ee^{\ii\pi/6}\Ai(\omega X), \\ G_\uparrow(z,\hbar) &= 2\sqrt\pi\,\hbar^{-1/6} \ee^{-\ii\pi/6}\Ai(\omega^2X). \end{aligned}

Equivalently,

G=π1/6[\Bi(X)+i\Ai(X)],G=π1/6[\Bi(X)i\Ai(X)].\begin{aligned} G_\downarrow &= \sqrt\pi\,\hbar^{-1/6} \bigl[\Bi(X)+\ii\Ai(X)\bigr], \\ G_\uparrow &= \sqrt\pi\,\hbar^{-1/6} \bigl[\Bi(X)-\ii\Ai(X)\bigr]. \end{aligned}

The sectorial Airy asymptotics give precisely the book’s unit leading WKB amplitudes:

Az1/4exp ⁣(2z3/23),G,z1/4exp ⁣(+2z3/23)\begin{aligned} A &\sim z^{-1/4} \exp\!\left(-\frac{2z^{3/2}}{3\hbar}\right), \\ G_{\downarrow,\uparrow} &\sim z^{-1/4} \exp\!\left(+\frac{2z^{3/2}}{3\hbar}\right) \end{aligned}

on their respective sides of the ray. The exact rotated-Airy identity

\Ai(X)+ω2\Ai(ω2X)+ω\Ai(ωX)=0\Ai(X) +\omega^2\Ai(\omega^2X) +\omega\Ai(\omega X) =0

is equivalent to

G=G+iA.G_\downarrow = G_\uparrow+\ii A.

Therefore

(G,A)=(G,A)L(i),(G_\downarrow,A) = (G_\uparrow,A)L(\ii),

which is exactly the εC=+1\varepsilon_C=+1 theorem with D1=DD_1=D_\downarrow and D2=DD_2=D_\uparrow. Solving instead for the canonical upper basis gives the replacement rule

(G,A)=(G,A)L(i).(G_\uparrow,A) = (G_\downarrow,A)L(-\ii).

The Wronskian fixes the remaining normalization. Since z=2/3X\partial_z=\hbar^{-2/3}\partial_X and WrX[\Ai,\Bi]=1/π\Wr_X[\Ai,\Bi]=1/\pi,

Wrz[G,A]=Wrz[G,A]=2.\Wr_z[G_\downarrow,A] = \Wr_z[G_\uparrow,A] = -\frac2\hbar.

This one model simultaneously calibrates the side ordering, row-frame convention, +i+\ii in the analytic-continuation relation, i-\ii in the canonical-frame replacement, and the book’s 2/-2/\hbar Wronskian.

One circuit is not three matrices equal to the identity

Section titled “One circuit is not three matrices equal to the identity”

Successive canonical-frame replacements around the three Airy edges alternate lower and upper inverse shears. Their product is

L(i)U(i)L(i)=(0ii0)=iJ.L(-\ii)U(-\ii)L(-\ii) = \begin{pmatrix} 0&-\ii\\ -\ii&0 \end{pmatrix} = -\ii J.

This is not a contradiction with the fact that Airy functions are entire. A circuit around the simple branch point also sends

R0R0,R01/4iR01/4,\sqrt{R_0}\longmapsto-\sqrt{R_0}, \qquad R_0^{-1/4}\longmapsto-\ii R_0^{-1/4},

and hence relabels the formal WKB frame by the same matrix iJ-\ii J. The analytic local monodromy is trivial only after this formal sheet and prefactor transport is included:

L(i)U(i)L(i)(iJ)1=I.L(-\ii)U(-\ii)L(-\ii)(-\ii J)^{-1}=I.

The Langer coordinate explains universality, but does not prove it

Section titled “The Langer coordinate explains universality, but does not prove it”

Near a general simple zero aa, choose a sheet and set

ζ(z)=[32azR0(t) ⁣dt]2/3.\zeta(z) = \left[ \frac32 \int_a^z\sqrt{R_0(t)}\,\dd t \right]^{2/3}.

Then

ζ(ζ)2=R0.\zeta(\zeta')^2=R_0.

With

ψ(z)=(ζ(z))1/2Y(ζ),\psi(z) = (\zeta'(z))^{-1/2}Y(\zeta),

the transformed equation is

2Yζζ=[R(z,)(ζ)2+22(ζ)2{ζ,z}]Y,\hbar^2Y_{\zeta\zeta} = \left[ \frac{R(z,\hbar)}{(\zeta')^2} + \frac{\hbar^2}{2(\zeta')^2} \{\zeta,z\} \right]Y,

where

{ζ,z}=ζζ32(ζζ)2\{\zeta,z\} = \frac{\zeta'''}{\zeta'} -\frac32 \left(\frac{\zeta''}{\zeta'}\right)^2

is the Schwarzian derivative. Its leading term is the Airy equation 2Yζζ=ζY\hbar^2Y_{\zeta\zeta}=\zeta Y. For the exactly linear potential R0=c(za)R_0=c(z-a), the scaled variable

X=c1/3(za)2/3X = \frac{c^{1/3}(z-a)}{\hbar^{2/3}}

reduces the equation to Airy exactly, and all three unit-normalized solutions acquire the common factor c1/6c^{-1/6}.

For a nonlinear R0R_0 or a nonzero subleading potential, the Schwarzian and subleading terms remain. The universal multiplier then follows from the exact local transformation and Borel analysis in the connection theorem—not from discarding those corrections in a leading Airy approximation.

An oriented simple-zero connection, its exact Airy calibration, and the distinct simple-pole multiplier.

Local connection passport. Left: D2D_2 follows D1D_1 counterclockwise, so the analytically continued source frame obeys FD1D2=FD2L(i)F_{D_1}^{\to D_2}=F_{D_2}L(\ii); the figure abbreviates the continuation superscript. Center: rotated Airy functions fix that sign and the ordered Wronskian exactly. Right: a simple-pole branch point has one prong and remembers the Frobenius exponent difference νs\nu_s, replacing i\ii by 2icos(πνs)2\ii\cos(\pi\nu_s).

A simple-pole branch point is a different local problem

Section titled “A simple-pole branch point is a different local problem”

The Airy formula applies to a simple zero of R0R_0. A simple pole of the leading quadratic differential is also a ramification point of the spectral cover and emits one Stokes prong, but its exact local connection remembers subleading regular-singular data.

Use the restricted meromorphic framework

R(z,)=R0(z)+2R2(z).R(z,\hbar) = R_0(z)+\hbar^2R_2(z).

Near a simple pole ss, in a local Schrödinger coordinate, write

R0(z)=aszs+O(1),R2(z)=bs(zs)2+O ⁣((zs)1).\begin{aligned} R_0(z) &= \frac{a_s}{z-s}+O(1), \\ R_2(z) &= \frac{b_s}{(z-s)^2} +O\!\left((z-s)^{-1}\right). \end{aligned}

Define

νs=1+4bs,ts=eπiνs,κs=ts+ts1=2cos(πνs),ms=iκs=2icos(πνs).\begin{aligned} \nu_s &= \sqrt{1+4b_s}, \\ t_s &= \ee^{\pi\ii\nu_s}, \\ \kappa_s &= t_s+t_s^{-1} = 2\cos(\pi\nu_s), \\ m_s &= \ii\kappa_s = 2\ii\cos(\pi\nu_s). \end{aligned}

This notation separates the symmetric trace-like quantity κs\kappa_s from the full off-diagonal multiplier msm_s.

Normalize both branches at ss by the contour prescription described above. With the same region ordering and sign εC=sgnRewθ,s\varepsilon_C=\operatorname{sgn}\operatorname{Re}w_{\theta,s}, the simple-pole connection theorem is

FD1=FD2{L(ms),εC=+1,U(ms),εC=1.F_{D_1} = F_{D_2} \begin{cases} L(m_s),&\varepsilon_C=+1,\\ U(m_s),&\varepsilon_C=-1. \end{cases}

Replacing the continued D1D_1 frame by the canonical D2D_2 frame again uses the inverse and hence ms-m_s. The theorem imposes no extra nonresonance condition on νs\nu_s; the formula is invariant under νsνs\nu_s\mapsto-\nu_s. At

νsZ+12,\nu_s\in\mathbb Z+\frac12,

the multiplier vanishes even though the geometric one-prong edge remains.

The modified-Bessel model exposes the exponent difference

Section titled “The modified-Bessel model exposes the exponent difference”

Take the exactly solvable model

2ψ=(ax+2bx2)ψ,a>0,x>0,>0.\begin{aligned} \hbar^2\psi'' &= \left( \frac{a}{x} + \frac{\hbar^2b}{x^2} \right)\psi, \\ a&>0, &x&>0, &\hbar&>0. \end{aligned}

Set

X=2ax,ψ(x)=xu(X),ν2=1+4b.\begin{aligned} X&=\frac{2\sqrt{ax}}{\hbar}, \\ \psi(x)&=\sqrt{x}\,u(X), \\ \nu^2&=1+4b. \end{aligned}

Direct substitution gives the modified-Bessel equation

X2uXX+XuX(X2+ν2)u=0.X^2u_{XX} +Xu_X -(X^2+\nu^2)u =0.

The exact pair

Ψ+I=2πxIν(X),ΨK=2πxKν(X)\begin{aligned} \Psi_+^{I} &= 2\sqrt{\frac{\pi}{\hbar}}\, \sqrt{x}\,I_\nu(X), \\ \Psi_-^{K} &= \frac{2}{\sqrt{\pi\hbar}}\, \sqrt{x}\,K_\nu(X) \end{aligned}

has the unit WKB leading behavior

Ψ±(ax)1/4e±X\Psi_\pm \sim \left(\frac{a}{x}\right)^{-1/4} \ee^{\pm X}

and, using WrX[Kν,Iν]=1/X\Wr_X[K_\nu,I_\nu]=1/X,

Wrx[Ψ+I,ΨK]=2.\Wr_x[\Psi_+^{I},\Psi_-^{K}] = -\frac2\hbar.

Two continuations of the growing solution across the relevant cut can be normalized as

G=2iπxKν(eπiX),G=2iπxKν(eπiX).\begin{aligned} G_\downarrow &= \frac{2\ii}{\sqrt{\pi\hbar}}\, \sqrt{x}\, K_\nu(\ee^{\pi\ii}X), \\ G_\uparrow &= -\frac{2\ii}{\sqrt{\pi\hbar}}\, \sqrt{x}\, K_\nu(\ee^{-\pi\ii}X). \end{aligned}

For X>0X>0, the standard continuation identities

Kν(eπiX)=eπiνKν(X)πiIν(X),Kν(eπiX)=eπiνKν(X)+πiIν(X)\begin{aligned} K_\nu(\ee^{\pi\ii}X) &= \ee^{-\pi\ii\nu}K_\nu(X) -\pi\ii I_\nu(X), \\ K_\nu(\ee^{-\pi\ii}X) &= \ee^{\pi\ii\nu}K_\nu(X) +\pi\ii I_\nu(X) \end{aligned}

give

GG=2icos(πν)ΨK.G_\downarrow-G_\uparrow = 2\ii\cos(\pi\nu)\,\Psi_-^{K}.

Moreover,

Wrx[G,ΨK]=Wrx[G,ΨK]=2.\Wr_x[G_\downarrow,\Psi_-^{K}] = \Wr_x[G_\uparrow,\Psi_-^{K}] = -\frac2\hbar.

The model thus reproduces both the Koike multiplier and its unit-normalized Wronskian. The theorem for a general admissible simple pole additionally requires the exact local reduction and summability argument.

Near x=0x=0, the indicial equation is

ρ(ρ1)=b.\rho(\rho-1)=b.

Thus

ρ±=1±ν2,e2πiρ±=e±πiν.\rho_\pm = \frac{1\pm\nu}{2}, \qquad \ee^{2\pi\ii\rho_\pm} = -\ee^{\pm\pi\ii\nu}.

If MsM_s denotes the local Frobenius monodromy, then

trMs=2cos(πν),ms=itrMs.\operatorname{tr}M_s = -2\cos(\pi\nu), \qquad m_s = -\ii\,\operatorname{tr}M_s.

At resonant integer ν\nu, the trace formula remains valid even when a logarithm makes the monodromy nondiagonalizable. The connection multiplier depends on the exponent difference, or equivalently on bsb_s. It does not depend on asa_s, and it is not a residue of λ0\lambda_0: on the spectral cover, λ0\lambda_0 is regular and nonzero above a simple pole.

Compute bsb_s only after putting the equation into Schrödinger, or projective, normal form. A first-derivative removal contributes to the double-pole coefficient and can therefore change νs\nu_s.

Section titled “Spatial crossing and lateral summation are related, not identical”

The local theorem above fixes θ\theta and compares two spatial regions. Both regional solutions use the same Borel ray:

D1D2,z varies, Lθ fixed.D_1\longleftrightarrow D_2, \qquad \text{$z$ varies, $L_\theta$ fixed}.

A lateral Stokes discontinuity instead fixes a regular spatial point and compares rays immediately above and below a singular Borel direction:

Sθ+Sθ.\mathcal S_{\theta+} \longleftrightarrow \mathcal S_{\theta-}.

Here zz is fixed and the Borel contour varies.

The book uses ++ for the contour above the oriented Borel ray and - for the contour below it. Fix a small ϵ>0\epsilon>0. For a simple-zero edge, assume that every graph throughout the closed phase interval [θϵ,θ+ϵ][\theta-\epsilon,\theta+\epsilon] is saddle-free, and that the fixed spatial point lies on the graph only at the central phase θ\theta. Let Fθ+F_{\theta+} and FθF_{\theta-} denote the two lateral sums of the same endpoint-normalized formal row frame at that point, with the sheet, lifted normalization path, and branch labels held fixed. The phase-rotation form of the ordinary connection theorem then translates to

Fθ+=Fθ{L(i),εC=+1,U(i),εC=1.F_{\theta+} = F_{\theta-} \begin{cases} L(\ii),&\varepsilon_C=+1,\\ U(\ii),&\varepsilon_C=-1. \end{cases}

This equality is the translated simple-zero corollary, with its own uniformity hypotheses; it is not the definition of the spatial connection. A simple-pole analogue would replace i\ii by msm_s and requires the restricted simple-pole framework and a uniformly controlled graph family. It is not being folded into the displayed ordinary formula. In particular, the ++/- notation in Iwaki–Nakanishi’s later wall-crossing sections is opposite to this book’s above/below convention after argη=arg\arg\eta=-\arg\hbar is translated. Importing only the symbols would reverse the jump.

Keep these five operations distinct.

  • Continue and re-expand. Keep the Borel ray LθL_\theta fixed, change the spatial region, and use FD1D2=FD2CF_{D_1}^{\to D_2}=F_{D_2}C.
  • Replace by the destination frame. Keep the continued solution space fixed, change the canonical basis, and use FD2=FD1D2C1F_{D_2}=F_{D_1}^{\to D_2}C^{-1}.
  • Compare lateral Borel sums. Keep a regular zz fixed, move the contour above or below LθL_\theta, and invoke the translated lateral theorem.
  • Exchange sheets. Keep the base point zz fixed, change its lift on Σ^\widehat\Sigma, conjugate by JJ, and relabel the signs.
  • Reverse a path. Keep its endpoints, reverse its orientation, and invert the associated transport.

Local matrices need diagonal transport before they become global

Section titled “Local matrices need diagonal transport before they become global”

Suppose β\beta is an oriented lifted path from a ramified endpoint aa to another ramified endpoint bb, and define the closed anti-invariant cycle

γ=βτβ.\gamma = \beta-\tau_*\beta.

With the orientation just declared,

γPeven ⁣dz=2abPeven ⁣dz.\oint_\gamma P_{\mathrm{even}}\,\dd z = 2\int_a^b P_{\mathrm{even}}\,\dd z.

Introduce the total formal Voros exponent

V^γtot:=1γPeven ⁣dz.\widehat V_\gamma^{\mathrm{tot}} := \frac1\hbar \oint_\gamma P_{\mathrm{even}}\,\dd z.

The two endpoint-normalized formal frames satisfy

F^a=F^b(exp(V^γtot/2)00exp(V^γtot/2)).\widehat F_a = \widehat F_b \begin{pmatrix} \exp(\widehat V_\gamma^{\mathrm{tot}}/2)&0\\ 0&\exp(-\widehat V_\gamma^{\mathrm{tot}}/2) \end{pmatrix}.

This identity is formal until the open or closed exponent is regularized and Borel-summed with its complete path and lateral passport. If a route crosses an edge emitted by bb while the current frame is normalized at aa, the bare L(i)L(\ii) or U(i)U(\ii) must be conjugated by this diagonal transport. At a simple pole, replace the local i\ii by msm_s but keep the same normalization logic.

A single edge therefore contributes a universal local shear. A global connection calculation alternates such shears with diagonal open-path transports, branch-cut relabellings, formal monodromy factors, and possibly singular-endpoint matrices. Page 5 constructs the required Voros symbols and derives how their Borel sums change when a saddle wall is crossed.

For a concrete equation, use the following order.

  1. Put the equation in Schrödinger normal form and record how the dependent variable changed.
  2. Fix θ\theta, the compatible \hbar-sector, the phased quadratic differential, and a square-root sheet.
  3. Construct the Stokes graph and verify the summability hypotheses on the regions and paths actually used.
  4. Classify the emitting critical point: simple zero, simple pole, higher-order zero, or another singularity.
  5. Draw the cut away from the selected edge and specify the endpoint half-contour or pole subtraction.
  6. Order D1,D2D_1,D_2 counterclockwise and compute εC=sgnRewθ,e\varepsilon_C=\operatorname{sgn}\operatorname{Re}w_{\theta,e}.
  7. Write the source-facing matrix FD1D2=FD2CF_{D_1}^{\to D_2}=F_{D_2}C. Invert it only when replacing the continued source frame by the canonical destination frame.
  8. Conjugate by any change of endpoint or scalar normalization.
  9. Check the determinant and ordered Wronskian.
  10. Multiply local and transport factors in path order, keeping sheet relabellings explicit.

This workflow is deliberately more verbose than the mnemonic “dominant picks up subdominant.” The extra ledger is what makes the answer reproducible.

The companion script audits the convention-sensitive algebra and the two exactly solvable models. It verifies:

  • Airy scaling, rotated identities, unit amplitudes, and the 2/-2/\hbar Wronskians;
  • the lower and upper triangular matrices, their inverses, determinant, sheet conjugation, and three-edge closure;
  • diagonal normalization conjugation;
  • the simple-pole substitution into the modified-Bessel equation;
  • the normalized IνI_\nuKνK_\nu Wronskian and two continuation identities;
  • the multiplier 2icos(πν)2\ii\cos(\pi\nu), its branch invariance, and its half-integer zeros.

Download the canonical-sectorial connection checker

Run it from the project root:

Terminal window
python3 public/code/advanced-ode/canonical-sectorial-connection-check.py

The script checks identities and representative high-precision special-function values. It does not prove Borel summability, the general exact reduction theorem, or a global monodromy formula.

Calling a branch canonical without its passport. A formal sign is not a canonical analytic solution. Record the \hbar-sector, Borel ray, spatial region, sheet, endpoint, path, lateral prescription, and scalar normalization.

Treating a ramified endpoint as an initial value. The formula azPeven ⁣dz\int_a^zP_{\mathrm{even}}\dd z at a simple zero or simple pole is a half-contour on the cover. It does not mean that the singular formal expression has been evaluated at aa.

Mixing a row basis with a coefficient column. Right multiplication changes basis functions, whereas the coefficients of a fixed solution obey the dual relation. Transposing one convention without transposing the other changes which entry jumps.

Calling i\ii basis-independent. It is universal in the declared unit endpoint normalization. A diagonal change of normalization conjugates the triangular matrix and dresses its off-diagonal entry.

Applying Airy at a simple pole. A simple pole has one prong, not three, and its exact multiplier depends on the Frobenius exponent difference. The ordinary Airy formula also does not cover a higher-order or merging turning point.

Computing the pole parameter before removing the first derivative. The Liouville transformation can alter the double-pole coefficient. Koike’s bsb_s belongs to Schrödinger normal form.

Demanding identity from three bare Airy shears. A circuit also exchanges sheets and rotates the fourth-root prefactor. The product of the three canonical-frame replacement shears is iJ-\ii J, exactly the missing formal-frame transport.

Multiplying local matrices with incompatible endpoints. The bare Airy and simple-pole constants assume normalization at the edge’s emitting critical point. Changing that endpoint inserts a diagonal Voros transport before the next local shear.

Expand

F1=F2L(κ),F1=F2U(κ)F_1=F_2L(\kappa), \qquad F_1=F_2U(\kappa)

into component relations. Derive the inverse canonical-frame replacement rules and the coefficient transformation for a fixed solution.

Solution

For Fj=(Ψ+j,Ψj)F_j=(\Psi_+^j,\Psi_-^j),

F1=F2L(κ)F_1=F_2L(\kappa)

means

Ψ+1=Ψ+2+κΨ2,Ψ1=Ψ2.\Psi_+^1 = \Psi_+^2+\kappa\Psi_-^2, \qquad \Psi_-^1 = \Psi_-^2.

Similarly,

F1=F2U(κ)F_1=F_2U(\kappa)

means

Ψ+1=Ψ+2,Ψ1=Ψ2+κΨ+2.\Psi_+^1 = \Psi_+^2, \qquad \Psi_-^1 = \Psi_-^2+\kappa\Psi_+^2.

Because

L(κ)1=L(κ),U(κ)1=U(κ),L(\kappa)^{-1}=L(-\kappa), \qquad U(\kappa)^{-1}=U(-\kappa),

write F12F_1^{\to2} for the continued source frame. The two canonical-frame replacements are

F2=F12L(κ),F2=F12U(κ).F_2 = F_1^{\to2}L(-\kappa), \qquad F_2 = F_1^{\to2}U(-\kappa).

If ψ=Fjcj\psi=F_jc_j is fixed and F12=F2CF_1^{\to2}=F_2C, then

c2=Cc1.c_2=Cc_1.

Thus for a lower shear,

A2=A1,B2=B1+κA1.\begin{aligned} A_2&=A_1, \\ B_2&=B_1+\kappa A_1. \end{aligned}

For an upper shear,

A2=A1+κB1,B2=B1.\begin{aligned} A_2&=A_1+\kappa B_1, \\ B_2&=B_1. \end{aligned}

2. Recover every Airy normalization constant

Section titled “2. Recover every Airy normalization constant”

Starting from

\Ai(X)X1/42πe2X3/2/3,\Bi(X)X1/4πe2X3/2/3.\begin{aligned} \Ai(X) &\sim \frac{X^{-1/4}}{2\sqrt\pi} \ee^{-2X^{3/2}/3}, \\ \Bi(X) &\sim \frac{X^{-1/4}}{\sqrt\pi} \ee^{2X^{3/2}/3}. \end{aligned}

derive the factors in AA, GG_\downarrow, and GG_\uparrow. Then prove their connection identity and ordered Wronskians.

Solution

Because X=z/2/3X=z/\hbar^{2/3},

1/6X1/4=z1/4.\hbar^{-1/6}X^{-1/4}=z^{-1/4}.

Multiplying \Ai\Ai by 2π1/62\sqrt\pi\,\hbar^{-1/6} therefore gives the unit recessive WKB amplitude. Multiplying \Bi\Bi by π1/6\sqrt\pi\,\hbar^{-1/6} gives the unit growing amplitude. The combinations

G,=π1/6(\Bi±i\Ai)G_{\downarrow,\uparrow} = \sqrt\pi\,\hbar^{-1/6} (\Bi\pm\ii\Ai)

have that same leading growing term on their respective sides. The rotated-Airy connection identities fix the remaining phases:

\Bi(X)+i\Ai(X)=2eiπ/6\Ai(ωX),\Bi(X)i\Ai(X)=2eiπ/6\Ai(ω2X).\begin{aligned} \Bi(X)+\ii\Ai(X) &= 2\ee^{\ii\pi/6}\Ai(\omega X), \\ \Bi(X)-\ii\Ai(X) &= 2\ee^{-\ii\pi/6}\Ai(\omega^2X). \end{aligned}

Thus the constants in all three exact definitions are recovered. Their difference is

GG=2iπ1/6\Ai=iA.G_\downarrow-G_\uparrow = 2\ii\sqrt\pi\,\hbar^{-1/6}\Ai = \ii A.

Finally,

Wrz[G,,A]=2π1WrX[\Bi,\Ai]=2.\begin{aligned} \Wr_z[G_{\downarrow,\uparrow},A] &= 2\pi\hbar^{-1} \Wr_X[\Bi,\Ai] \\ &= -\frac2\hbar. \end{aligned}

Here the normalization and variable-change factors combine as 1/32/3=1\hbar^{-1/3}\hbar^{-2/3}=\hbar^{-1}, and the added multiples of \Ai\Ai do not change this Wronskian.

3. Advanced: derive the Langer transformation

Section titled “3. Advanced: derive the Langer transformation”

Show that

ζ=(32azR0 ⁣dt)2/3\zeta = \left(\frac32\int_a^z\sqrt{R_0}\,\dd t\right)^{2/3}

satisfies ζ(ζ)2=R0\zeta(\zeta')^2=R_0. For ψ=(ζ)1/2Y(ζ)\psi=(\zeta')^{-1/2}Y(\zeta), derive the Schwarzian term in the transformed equation.

Solution

Raising the definition to the power 3/23/2 and differentiating gives

32ζ1/2ζ=32R0.\frac32\zeta^{1/2}\zeta' = \frac32\sqrt{R_0}.

Squaring yields ζ(ζ)2=R0\zeta(\zeta')^2=R_0. Put A=(ζ)1/2A=(\zeta')^{-1/2}. Then

2Aζ+Aζ=02A'\zeta'+A\zeta''=0

and

AA=12ζζ+34(ζζ)2=12{ζ,z}.\frac{A''}{A} = -\frac12\frac{\zeta'''}{\zeta'} +\frac34 \left(\frac{\zeta''}{\zeta'}\right)^2 = -\frac12\{\zeta,z\}.

Consequently,

ψ=A(ζ)2Yζζ12A{ζ,z}Y.\psi'' = A(\zeta')^2Y_{\zeta\zeta} -\frac12A\{\zeta,z\}Y.

Substitution into 2ψ=Rψ\hbar^2\psi''=R\psi and division by A(ζ)2A(\zeta')^2 gives

2Yζζ=[R(ζ)2+22(ζ)2{ζ,z}]Y.\hbar^2Y_{\zeta\zeta} = \left[ \frac{R}{(\zeta')^2} + \frac{\hbar^2}{2(\zeta')^2} \{\zeta,z\} \right]Y.

The leading coefficient is R0/(ζ)2=ζR_0/(\zeta')^2=\zeta.

Compute

L(i)U(i)L(i)L(-\ii)U(-\ii)L(-\ii)

and explain why the result is not II even though the Airy equation has no singularity at the turning point.

Solution

Direct multiplication gives

L(i)U(i)L(i)=(0ii0)=iJ.L(-\ii)U(-\ii)L(-\ii) = \begin{pmatrix} 0&-\ii\\ -\ii&0 \end{pmatrix} = -\ii J.

The Airy solutions themselves are entire, but the WKB frame is ramified. One positive circuit changes z\sqrt z to z-\sqrt z, exchanges the exponential labels, and changes z1/4z^{-1/4} by i-\ii. Its formal transport is therefore iJ-\ii J. Removing that relabelling gives

(iJ)(iJ)1=I,(-\ii J)(-\ii J)^{-1}=I,

as required for the analytic monodromy.

Let

D=diag(a,b),F~=FD.D=\operatorname{diag}(a,b), \qquad \widetilde F=FD.

Find the transformed lower and upper multipliers. Can a Wronskian-preserving rescaling change the printed multiplier?

Solution

The connection matrix becomes C~=D1CD\widetilde C=D^{-1}CD. Hence

D1L(κ)D=L ⁣(κab),D1U(κ)D=U ⁣(κba).\begin{aligned} D^{-1}L(\kappa)D &= L\!\left(\kappa\frac ab\right), \\ D^{-1}U(\kappa)D &= U\!\left(\kappa\frac ba\right). \end{aligned}

The ordered Wronskian is multiplied by detD=ab\det D=ab. Even if ab=1ab=1, one can take a=ca=c and b=c1b=c^{-1}, changing the lower multiplier to κc2\kappa c^2 and the upper multiplier to κc2\kappa c^{-2}. Wronskian normalization alone therefore does not fix the off-diagonal constant.

6. Reduce the simple-pole model to Bessel form

Section titled “6. Reduce the simple-pole model to Bessel form”

For

2ψ=(ax+2bx2)ψ,\hbar^2\psi'' = \left(\frac a x+\frac{\hbar^2b}{x^2}\right)\psi,

use X=2ax/X=2\sqrt{ax}/\hbar and ψ=xu(X)\psi=\sqrt{x}\,u(X) to derive the modified-Bessel equation. Verify the normalized IνI_\nuKνK_\nu Wronskian.

Solution

Since X=X/(2x)X'=X/(2x), direct differentiation gives

ψ=x3/24(X2uXX+XuXu).\psi'' = \frac{x^{-3/2}}4 \left( X^2u_{XX}+Xu_X-u \right).

Also ax/2=X2/4ax/\hbar^2=X^2/4. The differential equation becomes

X2uXX+XuX(X2+1+4b)u=0,X^2u_{XX} +Xu_X -(X^2+1+4b)u =0,

so ν2=1+4b\nu^2=1+4b. For any two functions f(X),g(X)f(X),g(X),

Wrx[xf,xg]=xXWrX[f,g],=X2WrX[f,g].\begin{aligned} \Wr_x[\sqrt{x}f,\sqrt{x}g] &= xX'\Wr_X[f,g], \\ &= \frac X2\Wr_X[f,g]. \end{aligned}

Because WrX[Iν,Kν]=1/X\Wr_X[I_\nu,K_\nu]=-1/X, the unscaled Wronskian is 1/2-1/2. The product of the two displayed normalization constants is 4/4/\hbar, so

Wrx[Ψ+I,ΨK]=2.\Wr_x[\Psi_+^I,\Psi_-^K] = -\frac2\hbar.

7. Read the pole multiplier from Frobenius data

Section titled “7. Read the pole multiplier from Frobenius data”

Compute the exponent difference and multiplier for the simple-pole model. Evaluate it for b=0b=0, b=3/16b=-3/16, and b=2b=2.

Solution

The indicial roots obey

ρ(ρ1)=b,ρ±=1±1+4b2.\rho(\rho-1)=b, \qquad \rho_\pm=\frac{1\pm\sqrt{1+4b}}2.

Thus ν=1+4b\nu=\sqrt{1+4b} and

m=2icos(πν).m=2\ii\cos(\pi\nu).

For b=0b=0, ν=1\nu=1 and m=2im=-2\ii, already different from the Airy multiplier. For b=3/16b=-3/16, ν=1/2\nu=1/2 and m=0m=0. For b=2b=2, ν=3\nu=3 and m=2im=-2\ii. The last case is resonant: the trace and connection multiplier remain defined, but the trace alone does not decide whether the Frobenius monodromy is diagonalizable.

8. Audit eligibility and the missing global factor

Section titled “8. Audit eligibility and the missing global factor”

Decide which local theorem applies to each leading behavior:

R0=z,R0=z2,R=1z+2bz2,R=1z+R1(z).\begin{aligned} R_0&=z, \\ R_0&=z^2, \\ R&=\frac1z+\frac{\hbar^2b}{z^2}, \\ R&=\frac1z+\hbar R_1(z). \end{aligned}

Then let β:ab\beta:a\to b join two ramified endpoints and derive the normalization transport between FaF_a and FbF_b.

Solution

R0=zR_0=z has a simple zero and uses the ordinary Airy connection theorem. The double zero R0=z2R_0=z^2 is not covered by that theorem. The third equation has the stated simple-pole form and is eligible for Koike’s local theorem when the remaining global and summability hypotheses hold. The fourth has an arbitrary odd \hbar term and is not covered by the quoted simple-pole theorem.

For

γ=βτβ,\gamma=\beta-\tau_*\beta,

anti-invariance gives

γPeven ⁣dz=2abPeven ⁣dz.\oint_\gamma P_{\mathrm{even}}\,\dd z = 2\int_a^bP_{\mathrm{even}}\,\dd z.

Since az=ab+bz\int_a^z=\int_a^b+\int_b^z,

Fa=Fbdiag ⁣(eV^γtot/2,eV^γtot/2).F_a = F_b \operatorname{diag}\!\left( \ee^{\widehat V_\gamma^{\mathrm{tot}}/2}, \ee^{-\widehat V_\gamma^{\mathrm{tot}}/2} \right).

Its Borel-summed version conjugates the next local triangular factor. This is the missing nonlocal factor in a product of bare connection matrices.