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Stage C: Boundary Conditions and Exact Quantization

Page 5 constructed chamber-correct analytic connection coordinates. Those coordinates do not yet select a solution. A spectrum appears only after the left and right admissible solution spaces have been declared and transported into one common frame.

For a scalar second-order problem, each separated endpoint condition usually selects a line in the two-dimensional solution space. The exact quantization function is the determinant of those two transported lines. Its vanishing says that one nonzero solution satisfies both conditions. When exact WKB computes the two lines without approximation, the resulting zero condition is exact as well.

The ODE is only the first layer of the spectral problem

Section titled “The ODE is only the first layer of the spectral problem”

Retain the book’s Schrödinger convention on a real or complex contour C\mathcal C, with V=V(z;μ,)V=V(z;\mu,\hbar):

(2z2+V)ψ=Eψ.\left(-\hbar^2\partial_z^2+V\right)\psi =E\psi.

and write

R:=VE.R:=V-E.

Here EE is the spectral parameter and μ\mu denotes fixed couplings. A well-posed spectral claim needs more data than RR:

Q:=(R, C, arg, Lθ;graph chamber;cover sheet;cycle and path basis;endpoint normalizations;LL, LR;spectral sheet).\mathfrak Q := \left( \begin{gathered} R,\ \mathcal C,\ \arg\hbar,\ L_\theta; \\ \text{graph chamber};\quad \text{cover sheet}; \\ \text{cycle and path basis}; \\ \text{endpoint normalizations}; \\ \mathscr L_L,\ \mathscr L_R;\quad \text{spectral sheet} \end{gathered} \right).

The lines LL\mathscr L_L and LR\mathscr L_R are the admissible solution spaces at the two ends. The final spectral sheet is redundant for an ordinary self-adjoint bound-state problem, but indispensable for resonances and quasinormal modes.

The spectral-theory interlude explains how the function space and closed operator domain enter. This page does not recreate that operator theory. Its task is to compute the scalar boundary function after the spectral problem has been fixed.

The phrase “physical solution” must be translated into analytic data.

Boundary wordActual selectionExtra datum that must be stated
Dirichlet, Neumann, or RobinKernel of a finite endpoint covectorEndpoint coordinate and any gauge used to reach normal form
Regular at a regular singular pointA Frobenius line or a specified logarithmic combinationLocal exponent, branch, and resonance convention
Recessive or square-integrableThe decaying canonical line in a declared asymptotic sectorContour end and sector; at thresholds the line can cease to be isolated
Outgoing or ingoingA canonical oscillatory exponential on a declared sheetTime dependence, momentum branch, and continuation path
BlochAn eigenspace of one-period monodromyBloch multiplier and period orientation
Coupled system conditionAn admissible subspace of the required dimensionAnalytic frame or determinant-line convention

For example, “outgoing” changes when the time convention changes from eiωt\ee^{-\ii\omega t} to e+iωt\ee^{+\ii\omega t}. It can also change after a square-root branch is crossed. Neither choice is visible in the scalar ODE alone.

Boundary conditions are projective coefficient lines

Section titled “Boundary conditions are projective coefficient lines”

Let

F=(f+,f)F=(f_+,f_-)

be any ordered row frame of exact solutions on a regular overlap. Every solution has a coefficient column

ψ=Fc,c=(c+c).\begin{aligned} \psi&=Fc, \\ c&= \begin{pmatrix} c_+\\c_- \end{pmatrix}. \end{aligned}

A homogeneous scalar boundary condition is a line, not a normalized vector. If it is written in this frame as

Tc=0,=(+).\begin{aligned} \ell^{\mathsf T}c&=0, \\ \ell&= \begin{pmatrix} \ell_+\\\ell_- \end{pmatrix}. \end{aligned}

then one convenient spanning column is

b=(+).b= \begin{pmatrix} -\ell_-\\\ell_+ \end{pmatrix}.

Replacing bb by a nonzero scalar multiple does not change the selected solution line. If that scalar depends on EE, it must be analytic and nowhere zero to preserve the local zero divisor of a boundary function.

Finite-endpoint data can be converted mechanically

Section titled “Finite-endpoint data can be converted mechanically”

At a regular endpoint z=az=a, impose

0=αL(E)ψ(a)+βL(E)ψ(a).\begin{aligned} 0={}&\alpha_L(E)\psi(a) \\ &+\beta_L(E)\hbar\psi'(a). \end{aligned}

For the frame F=(f+,f)F=(f_+,f_-), define, for either sign,

r±:=f±(a),L,±:=αLf±(a)+βLr±.\begin{aligned} r_\pm &:=\hbar f_\pm'(a), \\ \ell_{L,\pm} &:=\alpha_Lf_\pm(a)+\beta_Lr_\pm. \end{aligned}

Then the boundary covector is

LT=(L,+L,).\ell_L^{\mathsf T} = \begin{pmatrix} \ell_{L,+} & \ell_{L,-} \end{pmatrix}.

The same construction applies at the right endpoint. It is usually safer than guessing which WKB sign a Robin condition selects. At an irregular endpoint, by contrast, the admissible line is defined by sectorial asymptotics and cannot be obtained by substituting the endpoint into a divergent WKB prefactor.

Transport both admissible lines into one frame

Section titled “Transport both admissible lines into one frame”

Choose a regular matching point mm and a unit-normalized Borel-summed WKB frame

Fm:=(Ψm,+,Ψm,),Wm:=Wr[Ψm,+,Ψm,],Wm=2.\begin{aligned} F_m &:=(\Psi_{m,+},\Psi_{m,-}), \\ W_m &:=\Wr[\Psi_{m,+},\Psi_{m,-}], \\ W_m&=-\frac2\hbar. \end{aligned}

Let FLF_L and FRF_R be local frames in which the endpoint lines are represented by nonzero columns bLb_L and bRb_R. Continue each frame to the matching region using the convention of Page 4:

FLm=FmTL,FRm=FmTR.\begin{aligned} F_L^{\to m}&=F_mT_L, \\ F_R^{\to m}&=F_mT_R. \end{aligned}

The continued admissible solutions are therefore

ψL=FmTLbL,ψR=FmTRbR.\begin{aligned} \psi_L&=F_mT_Lb_L, \\ \psi_R&=F_mT_Rb_R. \end{aligned}

Put

cL=TLbL,cR=TRbR.\begin{aligned} c_L&=T_Lb_L, \\ c_R&=T_Rb_R. \end{aligned}

Since the Wronskian is alternating and bilinear,

Wr[ψL,ψR]=det(cL,cR)Wm=2det(cL,cR).\begin{aligned} \Wr[\psi_L,\psi_R] &=\det(c_L,c_R)W_m \\ &=-\frac2\hbar\det(c_L,c_R). \end{aligned}

Hence the coefficient determinant

ΔWKB:=det(cL,cR),=det(TLbL,TRbR).\begin{aligned} \Delta_{\mathrm{WKB}} &:=\det(c_L,c_R), \\ &=\det(T_Lb_L,T_Rb_R). \end{aligned}

vanishes precisely when the two endpoint lines coincide. This is the same boundary-Wronskian construction introduced in Chapter 2, now evaluated through exact-WKB connection data.

For an equation still written as y+p(z,E)y+q(z,E)y=0y''+p(z,E)y'+q(z,E)y=0, the raw Wronskian is not constant. On a fixed path use the Abel-normalized function

A(z,E):=exp ⁣(zzp(s,E) ⁣ds),ΔA(z,E):=A(z,E)Wr[yL,yR](z,E).\begin{aligned} A(z,E) &:=\exp\!\left(\int_{z_*}^{z}p(s,E)\,\dd s\right), \\ \Delta_A(z,E) &:=A(z,E)\Wr[y_L,y_R](z,E). \end{aligned}

It is independent of the regular matching point. Passing to Schrödinger normal form builds this Abel factor into the gauge transformation.

Left and right admissible solution lines are transported through exact-WKB connection factors into one matching frame, where their wedge determinant is tested.

Boundary-to-frame assembly. Each endpoint chooses a projective line; the ordered products TLT_L and TRT_R transport those lines through local shears, diagonal Voros transport, sheet exchange, and formal monodromy. Quantization is the vanishing of their wedge in one common frame.

Suppose a route encounters NN frame changes and Page 4’s source-facing relations are

Fj1j=FjCj,j=1,,N.F_{j-1}^{\to j}=F_jC_j, \qquad j=1,\ldots,N.

If c0c_0 is the initial coefficient column, then

cj=Cjcj1.c_j=C_jc_{j-1}.

Consequently,

T=CNCN1C1.T=C_NC_{N-1}\cdots C_1.

The first encountered factor acts first on the column and therefore sits furthest to the right in the final product. Reversing this order is one of the most common sources of an apparently plausible but wrong spectral equation.

This TT is a source-to-match coefficient transport. If one instead uses Chapter 2’s endpoint relation FR=FLCLRF_R=F_LC_{LR}, then Page 4’s source-facing local relations must be inverted when inserted into CLRC_{LR}. Mixing these two matrix directions silently reverses the local shears.

The elementary factors have distinct origins:

L(s)=(10s1),U(s)=(1s01),D(V)=(dV00dV1),dV:=eV/2,J=(0110).\begin{aligned} L(s) &= \begin{pmatrix} 1&0\\s&1 \end{pmatrix}, \\ U(s) &= \begin{pmatrix} 1&s\\0&1 \end{pmatrix}, \\ D(V) &= \begin{pmatrix} d_V&0\\0&d_V^{-1} \end{pmatrix}, \\ d_V &:=\ee^{V/2}, \\ J &= \begin{pmatrix} 0&1\\1&0 \end{pmatrix}. \end{aligned}
  • A simple-zero edge supplies L(±i)L(\pm\ii) or U(±i)U(\pm\ii) after the crossing orientation and source-facing convention are fixed.
  • A simple-pole edge replaces the Airy multiplier by its exponent-dependent Koike multiplier under the restricted theorem’s hypotheses.
  • D(V)D(V) changes a normalization endpoint; VV is a regularized and directionally summed open or closed Voros exponent.
  • JJ exchanges sheets and branch labels. It is not a Stokes crossing.
  • Formal monodromy and singular-endpoint matrices must be inserted when a route winds around a pole or changes an asymptotic sector at infinity.

The entries of TLT_L and TRT_R are therefore functions of summed Voros symbols, not merely products of the constants ±i\pm\ii.

The exact-WKB passport turns the determinant into a theorem

Section titled “The exact-WKB passport turns the determinant into a theorem”

The algebra above is unconditional once exact frames and exact connection matrices have been supplied. Exact WKB supplies them only after the following hypotheses have been checked on the routes actually used.

  1. Normal form and parameter domain. The dependent-variable gauge, contour, open set in EE, and sector in nonzero \hbar are fixed. Turning points do not coalesce there unless a uniform local model is included.
  2. Borel direction. The oriented ray LθL_\theta and, when singular, its above/below lateral prescription are fixed using the convention of Page 1.
  3. Graph chamber. The phased quadratic differential and its Stokes graph are known throughout the continuation. A saddle-free theorem, a lateral resolution, or a stated wall-crossing theorem covers every segment.
  4. Cover data. The square-root sheet, branch cuts, lifted paths, closed cycles, and their orientations are fixed.
  5. Critical-point hypotheses. Every local shear is justified by the appropriate simple-zero, simple-pole, higher-turning-point, or uniform connection theorem.
  6. Endpoint regularization. Turning-point half-contours and pole subtractions are specified. No singular endpoint is treated as an ordinary value-one base point.
  7. Summability and uniformity. The WKB series and every quantum part of a Voros exponent used in the product are Borel summable in the chosen direction, uniformly enough for continuation and differentiation.
  8. Boundary identification. The summed WKB line is proved to equal the desired regular, recessive, incoming, or outgoing analytic line at each endpoint.
  9. Analytic continuation. The finite product follows the declared contour without crossing an unrecorded singularity or changing the spectral sheet.

Under these conditions, the summed WKB frame solves the original ODE, the local and transport matrices are identities between its exact solutions, and ΔWKB\Delta_{\mathrm{WKB}} equals an exact boundary Wronskian up to a nowhere-vanishing analytic factor. Its zeros, with multiplicity, are then exact in the stated parameter domain.

As EE varies, the turning points and cycles move. The parameter domain must therefore support a consistent Gauss–Manin transport and avoid discriminants, thresholds, and graph walls not covered by the declared continuation theorem. One printed formula need not extend through all of them.

One finite cycle gives a Bohr–Sommerfeld form only after factorization

Section titled “One finite cycle gives a Bohr–Sommerfeld form only after factorization”

Consider a real analytic confining potential with two simple real turning points x(E)<x+(E)x_-(E)<x_+(E) and

p(x,E):=EV(x)p(x,E):=\sqrt{E-V(x)}

between them; choose the positive square root. Define the half-action and positive classical action by

I0(E):=xx+p(x,E) ⁣dx,J0(E):=2I0(E).\begin{aligned} I_0(E) &:=\int_{x_-}^{x_+}p(x,E)\,\dd x, \\ J_0(E)&:=2I_0(E). \end{aligned}

Orient the finite WKB cycle γ\gamma so that

Πγ,0=iJ0.\Pi_{\gamma,0}=\ii J_0.

Using Page 5’s separation of the classical transmonomial from the quantum power series, first define the chamber-correct quantum correction and resummed period by

Vγ,θq:=SθV^γq,Πγ,θsum:=Zγ+Vγ,θq,Jθ:=iΠγ,θsum.\begin{aligned} V_{\gamma,\theta}^{\mathrm q} &:=\mathcal S_\theta\widehat V_\gamma^{\mathrm q}, \\ \Pi_{\gamma,\theta}^{\mathrm{sum}} &:=Z_\gamma+\hbar V_{\gamma,\theta}^{\mathrm q}, \\ \mathcal J_\theta &:=-\ii\Pi_{\gamma,\theta}^{\mathrm{sum}}. \end{aligned}

At a singular Borel direction, replace Sθ\mathcal S_\theta by the declared lateral sum throughout.

Suppose—not merely guess—that the boundary determinant has the factorization

ΔWKB(E,)=g(E,)(1+Vγ,θ),\Delta_{\mathrm{WKB}}(E,\hbar) = g(E,\hbar) \left( 1+\mathcal V_{\gamma,\theta} \right),

where gg is analytic and nowhere zero on the spectral domain. Since

Vγ,θ=exp ⁣(iJθ),\mathcal V_{\gamma,\theta} = \exp\!\left( \frac{\ii\mathcal J_\theta}{\hbar} \right),

the boundary condition becomes

Jθ(E,)=2π(n+12),nZ,\mathcal J_\theta(E,\hbar) = 2\pi\hbar \left( n+\frac12 \right), \qquad n\in\mathbb Z,

after a continuous logarithm branch has been chosen. The allowed range of nn still comes from the spectral domain and boundary problem.

The simplest two-turning-point topology makes the assumed factorization visible. Choose endpoint frames whose first columns are the left- and right-recessive solutions. Convert Page 4’s source-facing formulae to the endpoint convention FR=FLCwellF_R=F_LC_{\mathrm{well}}, and include the sheet relabeling that puts both Airy crossings into the same lower-triangular form. The audited connection word is then, up to zero-free endpoint normalizations,

Cwell=L(i)DvL(i),Dv=(v1/200v1/2),v=Vγ,θ.\begin{aligned} C_{\mathrm{well}} &= L(-\ii)D_vL(-\ii), \\ D_v &= \begin{pmatrix} v^{1/2}&0\\ 0&v^{-1/2} \end{pmatrix}, \\ v &= \mathcal V_{\gamma,\theta}. \end{aligned}

The boundary function is the lower-left entry:

(Cwell)21=i(v1/2+v1/2)=iv1/2(1+v).\begin{aligned} (C_{\mathrm{well}})_{21} &= -\ii \left( v^{1/2}+v^{-1/2} \right) \\ &= -\ii v^{-1/2}(1+v). \end{aligned}

The square-root branch affects the nonzero prefactor but not the zero condition. Other frame directions may transpose, conjugate, or invert this word; the invariant calculation is always the wedge of the two admissible lines.

Expanding only formally gives

Jθ(E,)J0(E)+2J2(E)+4J4(E)+.\begin{aligned} \mathcal J_\theta(E,\hbar) \sim{}& J_0(E) + \hbar^2J_2(E) \\ &+ \hbar^4J_4(E) +\cdots. \end{aligned}

Keeping just J0J_0 yields the familiar leading rule

J0(E)=2π(n+12).J_0(E) = 2\pi\hbar \left( n+\frac12 \right).

The half-integer shift comes from the two turning-point connection matrices, equivalently from the minus sign in Vγ=1\mathcal V_\gamma=-1. It should not be inserted a second time into the definition of the closed quantum period.

The factorization can fail or acquire more terms when

  • additional real wells contribute independent admissible routes;
  • complex turning points create active cycles in the chosen direction;
  • a barrier or double turning point requires a uniform Weber-type local model;
  • a pole changes the local multiplier;
  • the boundary conditions are periodic, outgoing, or coupled rather than two-ended recessive;
  • a graph wall changes the coordinate chart and the boundary vectors have not been transformed with it.

Page 7 will treat the first nonperturbative corrections and their transseries interpretation. Page 8 will remove the assumption that the important turning points lie on the real axis.

Weber proves the determinant and the cycle equation coincide

Section titled “Weber proves the determinant and the cycle equation coincide”

Take the real-line oscillator already calibrated in Chapter 8,

[2z2+z2]ψ=a2ψ,>0,a2>0.\begin{gathered} \left[ -\hbar^2\partial_z^2+z^2 \right]\psi = a^2\psi, \\ \hbar>0, \qquad a^2>0. \end{gathered}

Set

X=2z,ν=a2212.X=\sqrt{\frac2\hbar}\,z, \qquad \nu=\frac{a^2}{2\hbar}-\frac12.

Then

 ⁣d2ψ ⁣dX2+(ν+12X24)ψ=0.\frac{\dd^2\psi}{\dd X^2} + \left( \nu+\frac12-\frac{X^2}{4} \right)\psi =0.

For real XX, the right- and left-recessive solutions may be chosen as

ψR(z)=Dν(X),ψL(z)=Dν(X).\psi_R(z)=D_\nu(X), \qquad \psi_L(z)=D_\nu(-X).

The parabolic-cylinder Wronskian is

WrX[Dν(X),Dν(X)]=2πΓ(ν).\Wr_X[D_\nu(X),D_\nu(-X)] = \frac{\sqrt{2\pi}}{\Gamma(-\nu)}.

Reversing the ordered pair and using  ⁣dX/ ⁣dz=2/\dd X/\dd z=\sqrt{2/\hbar} gives

Wrz[ψL,ψR]=2π/Γ(ν).\Wr_z[\psi_L,\psi_R] = -\frac{2\sqrt{\pi/\hbar}}{\Gamma(-\nu)}.

Normalize away the harmless constant:

ΔW(ν):=4πWrz[ψL,ψR]=1Γ(ν).\Delta_{\mathrm W}(\nu) := -\sqrt{\frac{\hbar}{4\pi}} \Wr_z[\psi_L,\psi_R] = \frac1{\Gamma(-\nu)}.

Because the reciprocal gamma function is entire, the boundary determinant vanishes exactly at

ν=n,n=0,1,2,.\nu=n, \qquad n=0,1,2,\ldots.

Therefore

an2=(2n+1).a_n^2 = (2n+1)\hbar.

No semiclassical truncation has entered this calculation. The two-end decay condition and the exact connection coefficient produced the spectrum.

For the cut cycle δ\delta oriented as in Chapter 8,

Πδ=iπa2,\Pi_\delta = \ii\pi a^2,

and every higher closed Weber period vanishes. Hence

Vδ=exp ⁣(iπa2)=e2πiν.\begin{aligned} \mathcal V_\delta &= \exp\!\left( \frac{\ii\pi a^2}{\hbar} \right) \\ &= -\ee^{2\pi\ii\nu}. \end{aligned}

Euler’s reflection formula gives the exact factorization

ΔW(ν)=Γ(ν+1)eπiν2πi×(1+Vδ).\begin{aligned} \Delta_{\mathrm W}(\nu) ={}& \frac{ \Gamma(\nu+1)\ee^{-\pi\ii\nu} }{2\pi\ii} \\ &\times \left( 1+\mathcal V_\delta \right). \end{aligned}

On the physical domain a2>0a^2>0, equivalently ν>1/2\nu>-1/2, the prefactor is analytic and nowhere zero. Thus

ΔW=01+Vδ=0\Delta_{\mathrm W}=0 \quad\Longleftrightarrow\quad 1+\mathcal V_\delta=0

there. This is a proof that the simple cycle equation is an exact quantization condition for this boundary problem.

Outside that domain, 1+Vδ1+\mathcal V_\delta also vanishes at negative integers. Those apparent roots are canceled by poles of Γ(ν+1)\Gamma(\nu+1) in the full boundary determinant. The example makes Page 5’s warning concrete: a Voros factor by itself does not know the admissible spectral domain or endpoint normalization.

The cycle here is Chapter 8’s δcut\delta_{\mathrm{cut}}. It is not Page 5’s oppositely oriented active wall class at θ=π/2\theta=\pi/2.

Near ν=n0\nu=n\geq0,

ΔW(ν)=(1)n+1n!(νn)+O ⁣((νn)2).\begin{aligned} \Delta_{\mathrm W}(\nu) ={}& (-1)^{n+1}n! (\nu-n) \\ &+ O\!\left((\nu-n)^2\right). \end{aligned}

Therefore

ΔWa2a2=(2n+1)=(1)n+1n!20.\left. \frac{\partial\Delta_{\mathrm W}}{\partial a^2} \right|_{a^2=(2n+1)\hbar} = \frac{(-1)^{n+1}n!}{2\hbar} \neq0.

The determinant detects not only the root locations but their simplicity. Multiplying it by a zero-free analytic factor changes the derivative’s value, but not whether the derivative vanishes at a root.

The same equation has two different half-line spectra

Section titled “The same equation has two different half-line spectra”

On z0z\geq0, the right-recessive solution is still Dν(X)D_\nu(X). Dirichlet and Neumann conditions at the regular endpoint use the exact values below, where the prime differentiates with respect to XX:

Dν(0)=2ν/2πΓ ⁣((1ν)/2),Dν(0)=2(ν+1)/2πΓ(ν/2).\begin{aligned} D_\nu(0) &= \frac{ 2^{\nu/2}\sqrt\pi }{ \Gamma\!\left((1-\nu)/2\right) }, \\ D_\nu'(0) &= -\frac{ 2^{(\nu+1)/2}\sqrt\pi }{ \Gamma(-\nu/2) }. \end{aligned}

After removing nonzero factors, the two boundary functions are

ΔD(ν)=1Γ ⁣((1ν)/2),ΔN(ν)=1Γ(ν/2).\begin{aligned} \Delta_D(\nu) &= \frac1{ \Gamma\!\left((1-\nu)/2\right) }, \\ \Delta_N(\nu) &= \frac1{ \Gamma(-\nu/2) }. \end{aligned}

Their roots give

condition at 0νa2Dirichlet2m+1(4m+3)Neumann2m(4m+1)\begin{array}{c|c|c} \text{condition at }0 &\nu &a^2 \\ \hline \text{Dirichlet} &2m+1 &(4m+3)\hbar \\ \text{Neumann} &2m &(4m+1)\hbar \end{array}

for m0m\geq0. The two sequences are the odd and even full-line states. The differential equation and recessive condition at ++\infty are the same; changing the condition at 00 changes the spectrum.

Other boundary problems change the scalar equation

Section titled “Other boundary problems change the scalar equation”

The transported-line construction is not restricted to bound states.

A connection entry for separated endpoint lines

Section titled “A connection entry for separated endpoint lines”

Suppose local ordered frames have their first columns equal to the selected endpoint solutions and

FR=FLCLR.F_R=F_LC_{LR}.

Then the right selected solution is

ψR=(CLR)11ψL+(CLR)21ψ~L.\psi_R = (C_{LR})_{11}\psi_L + (C_{LR})_{21}\widetilde\psi_L.

The spectral condition is

(CLR)21=0.(C_{LR})_{21}=0.

Reordering either basis changes the vanishing entry. The invariant statement is that the selected lines intersect, or equivalently that their Wronskian vanishes.

Bloch conditions use monodromy, not two recessive lines

Section titled “Bloch conditions use monodromy, not two recessive lines”

Let M(E,)M(E,\hbar) be the exact one-period monodromy in an ordered frame and let μB\mu_B be the declared Bloch multiplier. A Bloch solution exists when

ΔμB(E,):=det ⁣(M(E,)μBI)=0.\Delta_{\mu_B}(E,\hbar) := \det\!\left( M(E,\hbar)-\mu_BI \right) =0.

If MSL(2,C)M\in SL(2,\mathbb C), then

ΔμB=μB2μBtrM+1.\Delta_{\mu_B} = \mu_B^2 - \mu_B\operatorname{tr}M +1.

For μB=eikL\mu_B=\ee^{\ii kL} this becomes

trM=2cos(kL).\operatorname{tr}M = 2\cos(kL).

The exact-WKB task is now to compute the monodromy product, including formal monodromy and every Stokes/Voros factor. At periodic and antiperiodic band edges, μB=+1\mu_B=+1 and 1-1 respectively.

The equality trM=±2\operatorname{tr}M=\pm2 guarantees a periodic or antiperiodic eigenline. It does not by itself imply that M=±IM=\pm I, that two independent Bloch solutions exist, or that the band edge is simple.

Resonances use outgoing lines on a continued sheet

Section titled “Resonances use outgoing lines on a continued sheet”

For a resonance or quasinormal problem, choose the outgoing or ingoing canonical line at each contour end and continue both on the declared spectral sheet. Their Wronskian again supplies a scalar condition. Its zeros are generally complex, and the identification of those zeros with poles of a continued resolvent is an additional theorem from spectral theory.

Nothing in the determinant algebra forces self-adjointness, reality, or stability. Those properties come from the operator domain, symmetries, and sheet structure.

Chamber changes act on the whole boundary problem

Section titled “Chamber changes act on the whole boundary problem”

Let two WKB frames on opposite lateral determinations satisfy

Fm+=FmG,F_m^+=F_m^-G,

where GG is the relevant Stokes or wall-crossing matrix. A fixed exact solution has coefficients related by

c+=G1c.c^+=G^{-1}c^-.

Therefore

det(cL+,cR+)=det(G1)det(cL,cR).\det(c_L^+,c_R^+) = \det(G^{-1}) \det(c_L^-,c_R^-).

For the unit-Wronskian shears of Pages 4–5, detG=1\det G=1, so the determinant is unchanged. More general analytic frame renormalizations multiply it by a nowhere-zero factor. In either case, the consistently continued zero divisor is invariant.

By contrast, applying the DDP substitution to a Voros symbol while leaving the endpoint vectors or the rest of the route product in the old chamber mixes two coordinate charts. The resulting scalar need not represent the same boundary problem and may acquire spurious zeros.

On an actually singular Borel ray, the two lateral determinants are distinct prescribed objects until a theorem identifies their physical completion. The covariance calculation does not, by itself, prove median summability or ambiguity cancellation; Page 7 supplies that extra layer.

Assume Δ(E)\Delta(E) is analytic near an isolated root EE_* and is not identically zero. The root multiplicity is

m=ordEΔ.m = \operatorname{ord}_{E_*}\Delta.

Equivalently, for a small positively oriented circle CC_* containing no other zero,

m=12πiCΔ(E)Δ(E) ⁣dE.m = \frac{1}{2\pi\ii} \oint_{C_*} \frac{\Delta'(E)}{\Delta(E)} \,\dd E.

This contour count is invariant under ΔgΔ\Delta\mapsto g\Delta with gg analytic and nowhere zero. A simple root has Δ(E)0\Delta'(E_*)\neq0; a multiple root requires further derivatives.

For a holomorphic Fredholm pencil of index zero, a suitably normalized characteristic function can encode algebraic multiplicity. Without those operator hypotheses, the order of a chosen scalar boundary function should not automatically be called the algebraic multiplicity of an operator eigenvalue.

Likewise, a boundary Wronskian is not automatically a Fredholm determinant, a zeta-regularized determinant, or a canonical product. Chapter 2 states the additional hypotheses and comparison theorems for those objects.

For the real Schrödinger problem, differentiation gives the useful local identity

 ⁣d ⁣dxWr[ψ,Eψ]=ψ22.\frac{\dd}{\dd x} \Wr[\psi,\partial_E\psi] = -\frac{\psi^2}{\hbar^2}.

If the endpoint conditions and normalizations are EE-independent in the required Lagrange-bracket sense, and ψR=κψL=κψ\psi_R=\kappa\psi_L=\kappa\psi at an eigenvalue, integration yields

Δ(En)=κ2xLxRψ(x)2 ⁣dx\Delta'(E_n) = \frac{\kappa}{\hbar^2} \int_{x_L}^{x_R}\psi(x)^2\,\dd x

for the corresponding raw boundary Wronskian. There is no complex conjugation in this analytic identity. In a real self-adjoint problem the integral proves simplicity; in a nonselfadjoint problem the proper derivative test generally involves an adjoint mode.

Numerically, three checks are especially valuable:

  1. evaluate the Wronskian at several regular matching points;
  2. compare two independent normalizations and verify that their ratio is nonzero near the root;
  3. use a contour count or derivative test rather than relying only on a small plotted value of Δ|\Delta|.

A reproducible boundary-to-spectrum workflow

Section titled “A reproducible boundary-to-spectrum workflow”

For a concrete exact-WKB spectral calculation, proceed in this order.

  1. State the differential expression, contour, function space or radiation problem, and spectral parameter domain.
  2. Fix the time convention and spectral sheet when outgoing or ingoing conditions are used.
  3. Put the equation in Schrödinger normal form and retain the inverse gauge map for the original boundary data.
  4. Fix arg\arg\hbar, the Borel ray LθL_\theta, the graph chamber, and any lateral prescription.
  5. Draw the phased Stokes graph and choose the cover sheet, cuts, cycles, lifted paths, and orientations.
  6. Identify the exact analytic line selected at each endpoint. Do not use a formal decay mnemonic at a threshold or singular endpoint.
  7. Choose local WKB frames and represent the endpoint lines by coefficient columns bLb_L and bRb_R.
  8. Choose one matching frame and record every source-facing relation Fj1j=FjCjF_{j-1}^{\to j}=F_jC_j.
  9. Assemble TLT_L and TRT_R in path order, including local shears, diagonal Voros transports, sheet exchanges, and formal monodromy.
  10. Form ΔWKB=det(TLbL,TRbR)\Delta_{\mathrm{WKB}}=\det(T_Lb_L,T_Rb_R) and verify its Wronskian normalization.
  11. Prove that the summed frames and matrices satisfy the analytic passport; label the result conditional if any theorem hypothesis remains open.
  12. Solve the scalar equation with controlled summation, truncation, and root-finding error, then check it against an independent method.

This sequence separates a geometry error, a matrix-order error, a boundary error, and a numerical error before they can compensate accidentally.

The companion script exact-quantization-check.py checks the finite-dimensional identities and the Weber calibration. It verifies

  • the determinant–Wronskian relation for a general coefficient pair;
  • source-facing route order and determinant-one covariance;
  • the two-shear factor 1+V1+\mathcal V;
  • the parabolic-cylinder Wronskian at several regular points;
  • the reciprocal-gamma/Voros factorization at real and complex ν\nu;
  • the first seven Weber roots, their derivatives, and the cancellation of negative-integer cycle roots;
  • the half-line Dirichlet/Neumann parity split and Hermite states;
  • the SL(2)SL(2) Bloch characteristic polynomial.

These tests do not prove Borel summability, endpoint admissibility, graph completeness, or the applicability of a local connection theorem to a new potential.

Quantizing the printed ODE. An ODE has a two-dimensional solution space, not a preferred spectrum. State the operator domain or radiation problem before solving a scalar equation.

Setting one Voros factor to 1-1 by pattern recognition. The equation 1+Vγ=01+\mathcal V_\gamma=0 is spectral only after the transported boundary determinant is shown to have that factor with a zero-free remainder. Weber shows both why the rule works and how it can acquire spurious roots outside the declared domain.

Multiplying matrices in drawing order. With row frames and coefficient columns, the first encountered source-facing matrix is the rightmost factor in the final product. Derive the update cj=Cjcj1c_j=C_jc_{j-1} before coding.

Using a formal period as an analytic number. A divergent all-orders period must be summed in a specified direction and chamber. Optimal truncation or Borel–Padé is a numerical approximation, not the definition of the exact symbol.

Changing the frame but not the boundary vector. Coefficients transform contragrediently. A Stokes or wall-crossing transformation applied to only one part of the determinant mixes conventions and can move its zeros.

Reading multiplicity from a normalization-dependent slope. A zero-free factor changes Δ(E)\Delta'(E_*). It preserves the order of the zero, which is the invariant datum.

1. Prove the determinant–Wronskian identity

Section titled “1. Prove the determinant–Wronskian identity”

Let F=(f+,f)F=(f_+,f_-) and u=Fcu=Fc, v=Fdv=Fd. Show that

Wr[u,v]=det(c,d)Wr[f+,f].\Wr[u,v] = \det(c,d)\Wr[f_+,f_-].

Specialize to the unit WKB normalization.

Solution

Write u=c+f++cfu=c_+f_++c_-f_- and v=d+f++dfv=d_+f_++d_-f_-. Bilinearity and antisymmetry leave only the two cross terms:

Wr[u,v]=c+dWr[f+,f]+cd+Wr[f,f+]=(c+dcd+)Wr[f+,f].\begin{aligned} \Wr[u,v] &= c_+d_-\Wr[f_+,f_-] \\ &\quad+ c_-d_+\Wr[f_-,f_+] \\ &= (c_+d_--c_-d_+) \Wr[f_+,f_-]. \end{aligned}

The coefficient in parentheses is det(c,d)\det(c,d). For Wr[f+,f]=2/\Wr[f_+,f_-]=-2/\hbar,

det(c,d)=2Wr[u,v].\det(c,d) = -\frac\hbar2\Wr[u,v].

For F=(f+,f)F=(f_+,f_-) at z=az=a, impose

αψ(a)+βψ(a)=0.\alpha\psi(a)+\beta\hbar\psi'(a)=0.

Find a coefficient column spanning the admissible line.

Solution

Define

+=αf+(a)+βf+(a),=αf(a)+βf(a).\begin{aligned} \ell_+ &= \alpha f_+(a)+\beta\hbar f_+'(a), \\ \ell_- &= \alpha f_-(a)+\beta\hbar f_-'(a). \end{aligned}

The boundary condition is +c++c=0\ell_+c_++\ell_-c_-=0, so one spanning column is

b=(+).b= \begin{pmatrix} -\ell_-\\\ell_+ \end{pmatrix}.

Indeed Tb=0\ell^{\mathsf T}b=0. Any nonzero scalar multiple represents the same projective line.

Suppose

F01=F1C1,F12=F2C2,F23=F3C3.\begin{aligned} F_0^{\to1} &=F_1C_1, \\ F_1^{\to2} &=F_2C_2, \\ F_2^{\to3} &=F_3C_3. \end{aligned}

If ψ=F0c0\psi=F_0c_0, find its coefficient column in F3F_3.

Solution

At the first step,

ψ=F1C1c0,\psi=F_1C_1c_0,

so c1=C1c0c_1=C_1c_0. Repeating the argument gives

c2=C2C1c0,c3=C3C2C1c0.c_2=C_2C_1c_0, \qquad c_3=C_3C_2C_1c_0.

Thus the first encountered matrix is the rightmost factor.

Let Fm+=FmGF_m^+=F_m^-G with GG invertible. Derive the transformation of the two coefficient columns and their determinant.

Solution

For a fixed solution,

Fmc=Fm+c+=FmGc+.F_m^-c^- = F_m^+c^+ = F_m^-Gc^+.

Hence c+=G1cc^+=G^{-1}c^-. Applying this to both endpoint lines gives

det(cL+,cR+)=det(G1)det(cL,cR).\det(c_L^+,c_R^+) = \det(G^{-1}) \det(c_L^-,c_R^-).

If GSL(2)G\in SL(2), the determinant is unchanged. For a general analytic frame change it is multiplied by a nowhere-zero factor.

Use

Dν(X)=U ⁣(ν12,X)D_\nu(X)=U\!\left(-\nu-\frac12,X\right)

and

WrX[U(A,X),U(A,X)]=2πΓ(A+1/2)\Wr_X[U(A,X),U(A,-X)] = \frac{\sqrt{2\pi}}{\Gamma(A+1/2)}

to compute Wrz[Dν(X),Dν(X)]\Wr_z[D_\nu(-X),D_\nu(X)] for X=2/zX=\sqrt{2/\hbar}\,z.

Solution

Set A=ν1/2A=-\nu-1/2. Then

WrX[Dν(X),Dν(X)]=2πΓ(ν).\Wr_X[D_\nu(X),D_\nu(-X)] = \frac{\sqrt{2\pi}}{\Gamma(-\nu)}.

Reversing the pair changes the sign, and changing variables contributes  ⁣dX/ ⁣dz=2/\dd X/\dd z=\sqrt{2/\hbar}. Therefore

Wrz[Dν(X),Dν(X)]=2π/Γ(ν).\Wr_z[D_\nu(-X),D_\nu(X)] = -\frac{2\sqrt{\pi/\hbar}}{\Gamma(-\nu)}.

Multiplication by /(4π)-\sqrt{\hbar/(4\pi)} gives ΔW=1/Γ(ν)\Delta_{\mathrm W}=1/\Gamma(-\nu).

6. Factor the Weber determinant through its cycle symbol

Section titled “6. Factor the Weber determinant through its cycle symbol”

Starting from Euler’s reflection formula and Vδ=e2πiν\mathcal V_\delta=-\ee^{2\pi\ii\nu}, prove

1Γ(ν)=Γ(ν+1)eπiν2πi(1+Vδ).\frac1{\Gamma(-\nu)} = \frac{ \Gamma(\nu+1)\ee^{-\pi\ii\nu} }{2\pi\ii} \left( 1+\mathcal V_\delta \right).

Why is the equivalence of zero sets restricted to a domain?

Solution

Reflection gives

1Γ(ν)=Γ(ν+1)sin(πν)π.\frac1{\Gamma(-\nu)} = -\frac{\Gamma(\nu+1)\sin(\pi\nu)}{\pi}.

Also,

1+Vδ=1e2πiν=2ieπiνsin(πν).1+\mathcal V_\delta = 1-\ee^{2\pi\ii\nu} = -2\ii\ee^{\pi\ii\nu} \sin(\pi\nu).

Combining the two identities proves the formula. The prefactor is analytic and nonzero on ν>1/2\nu>-1/2, but has poles at negative integers. Globally those poles cancel the additional zeros of 1+Vδ1+\mathcal V_\delta, so the two factors do not have the same zero divisor on the whole plane.

Show that

 ⁣d ⁣dν1Γ(ν)ν=n=(1)n+1n!\left. \frac{\dd}{\dd\nu} \frac1{\Gamma(-\nu)} \right|_{\nu=n} = (-1)^{n+1}n!

for n0n\geq0.

Solution

Near z=nz=-n, gamma has the simple pole

Γ(z)=(1)nn!(z+n)+O(1).\Gamma(z) = \frac{(-1)^n}{n!(z+n)} +O(1).

Put z=νz=-\nu and ν=n+ε\nu=n+\varepsilon. Then z+n=εz+n=-\varepsilon, so

1Γ(ν)=(1)n+1n!ε+O(ε2).\frac1{\Gamma(-\nu)} = (-1)^{n+1}n!\,\varepsilon +O(\varepsilon^2).

The stated derivative follows and is nonzero.

Let MSL(2,C)M\in SL(2,\mathbb C). Show that

det(MμI)=μ2μtrM+1.\det(M-\mu I) = \mu^2-\mu\operatorname{tr}M+1.

Set μ=eikL\mu=\ee^{\ii kL}.

Solution

For a 2×22\times2 matrix,

det(MμI)=μ2μtrM+detM.\det(M-\mu I) = \mu^2-\mu\operatorname{tr}M+\det M.

Since detM=1\det M=1, the displayed polynomial follows. Dividing its zero condition by μ0\mu\neq0 gives

trM=μ+μ1=2cos(kL).\operatorname{tr}M = \mu+\mu^{-1} = 2\cos(kL).

9. Preview the first instanton displacement

Section titled “9. Preview the first instanton displacement”

Suppose a chamber-labelled boundary function has the formal action-graded form

Q(E,)=Q0(E,)+σeA/Q1(E,)+,\begin{aligned} \mathcal Q(E,\hbar) ={}& \mathcal Q_0(E,\hbar) \\ &+ \sigma\ee^{-A/\hbar} \mathcal Q_1(E,\hbar) +\cdots, \end{aligned}

and Q0(E0,)=0\mathcal Q_0(E_0,\hbar)=0 with EQ0(E0,)0\partial_E\mathcal Q_0(E_0,\hbar)\neq0. Find the first displacement of the root.

Solution

Put E=E0+δEE=E_0+\delta E and expand to first order in the instanton monomial. Then

0=EQ0(E0,)δE+σeA/Q1(E0,)+.\begin{aligned} 0 ={}& \partial_E\mathcal Q_0(E_0,\hbar) \,\delta E \\ &+ \sigma\ee^{-A/\hbar} \mathcal Q_1(E_0,\hbar) +\cdots. \end{aligned}

Therefore

δE=σeA/Q1(E0,)EQ0(E0,)+.\delta E = -\sigma\ee^{-A/\hbar} \frac{ \mathcal Q_1(E_0,\hbar) }{ \partial_E\mathcal Q_0(E_0,\hbar) } +\cdots.

This is only the first formal displacement. The lateral dependence of σ\sigma, higher sectors, logarithms, and ambiguity cancellation are the subject of Page 7.

This page treated the boundary determinant as the primary object and showed when it reduces to a one-cycle equation. In a multiwell problem or near a graph wall, the determinant contains exponentially small symbols from additional cycles. Solving it then shifts a perturbative root by an instanton series; lateral ambiguities of the perturbative sector must cancel those of the nonperturbative sectors.

Page 7 derives that mechanism from the determinant rather than appending an instanton term by hand.