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Airy, Weber, and Mathieu Worked Examples

The three smallest WKB laboratories test three genuinely different pieces of the formalism. Airy is local and has no nonzero closed period. Weber is genus zero but acquires a residue cycle after its two points over infinity are removed. Mathieu lives on a periodic cylinder and produces a true genus-one pair of handle cycles.

Earlier pages built the recursion, homology, regularization, and Picard–Fuchs machinery separately. Here each model is carried from its normal-form equation to a reproducible period formula and then checked against the exact special function or elliptic integral appropriate to it. Analytic Stokes jumps and exact quantization remain outside the formal claims.

Three models isolate three kinds of geometry

Section titled “Three models isolate three kinds of geometry”

The examples should not be ordered merely by algebraic difficulty. They form a geometric ladder.

ModelCompact coverRelevant period dataExact comparison
Airy, y2=zy^2=zSphereA regularized half-contour from a simple turning pointAi\operatorname{Ai} asymptotics
Weber, y2=z2a2y^2=z^2-a^2SphereA puncture-loop action and a pole-to-pole correctionParabolic-cylinder and gamma functions
Mathieu, y2=2Λ2cos(2x)Ey^2=2\Lambda^2\cos(2x)-ETorusTwo real vanishing actions and a primitive handle basisComplete elliptic integrals and Mathieu–Floquet data

Airy relative path, Weber puncture-loop geometry, and Mathieu real vanishing cycles.

The examples separate relative-endpoint, puncture-loop, and handle data. For Mathieu, the physical cycles satisfy δδ+=2\delta_-\mathbin{\cdot}\delta_+=2 and span an index-two sublattice; a primitive basis has A=δA=\delta_- and δ+=A+2B\delta_+=A+2B.

The cover genus alone is therefore not a count of useful WKB quantities. One must also declare punctures, relative endpoints, and the differential being integrated.

Begin with the exact normal-form equation

[2z2+z]ψ=0,y2=z.\left[ -\hbar^2\partial_z^2+z \right]\psi=0, \qquad y^2=z.

The scaled coordinate

X=z2/3X=\frac{z}{\hbar^{2/3}}

turns it into ψXX=Xψ\psi_{XX}=X\psi. Thus Ai(X)\operatorname{Ai}(X) and Bi(X)\operatorname{Bi}(X) are exact solutions. The scale z=O(2/3)z=O(\hbar^{2/3}) is already a warning: an ordinary WKB series at fixed zz cannot remain uniform as the turning point is approached.

On the branch y=z1/2y=z^{1/2}, Pages 2 and 5 found

λ0=z1/2 ⁣dz,λ2=532z5/2 ⁣dz.\begin{aligned} \lambda_0 &= z^{1/2}\,\dd z, \\ \lambda_2 &= -\frac{5}{32z^{5/2}}\,\dd z. \end{aligned}

The compact cover is a sphere, so there is no nonzero closed classical period. The intrinsic half-contour prescription nevertheless gives the regularized action to a fixed ordinary point:

AAireg(z,)=23z3/2+5248z3/2+O ⁣(4z9/2).\mathcal A_{\mathrm{Ai}}^{\mathrm{reg}}(z,\hbar) = \frac23z^{3/2} + \frac{5\hbar^2}{48z^{3/2}} + O\!\left( \frac{\hbar^4}{z^{9/2}} \right).

For >0\hbar>0, take principal powers with π<argz<π-\pi<\arg z<\pi. As z/2/3|z|/\hbar^{2/3}\to\infty, uniformly for argzπδ|\arg z|\leq\pi-\delta, the standard Airy asymptotic expansion begins

Ai ⁣(z2/3)1/62πz1/4exp ⁣[2z3/23]×[1548z3/2+O ⁣(2z3)].\begin{aligned} \operatorname{Ai}\!\left( \frac{z}{\hbar^{2/3}} \right) \sim{}& \frac{\hbar^{1/6}}{2\sqrt\pi\,z^{1/4}} \exp\!\left[ -\frac{2z^{3/2}}{3\hbar} \right] \\ &\times \left[ 1- \frac{5\hbar}{48z^{3/2}} + O\!\left( \frac{\hbar^2}{z^3} \right) \right]. \end{aligned}

The decaying formal solution from Page 2 has the structure

Peven1/2exp ⁣[1AAireg].P_{\mathrm{even}}^{-1/2} \exp\!\left[ -\frac{1}{\hbar} \mathcal A_{\mathrm{Ai}}^{\mathrm{reg}} \right].

Its order-\hbar correction is exactly 5/(48z3/2)-5\hbar/(48z^{3/2}). The remaining factor 1/6/(2π)\hbar^{1/6}/(2\sqrt\pi) is an exact-solution normalization, not a period coefficient. This comparison fixes the sign and the half-contour normalization, but it does not provide a global connection formula: the displayed Airy expansion changes character when its sector boundary is crossed.

Near a generic simple turning point ztz_t, write R0(z)=c(zzt)+O((zzt)2)R_0(z)=c(z-z_t)+O((z-z_t)^2) with c0c\neq0. The local variable

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

reduces the leading equation to Airy form. Airy is therefore a local normal form for each isolated simple turning point, not a global model for a curve with several cycles.

Weber keeps closed and relative information separate

Section titled “Weber keeps closed and relative information separate”

Take the harmonic-oscillator equation

[2z2+z2]ψ=a2ψ,a>0.\left[ -\hbar^2\partial_z^2+z^2 \right]\psi = a^2\psi, \qquad a>0.

Its WKB curve is y2=z2a2y^2=z^2-a^2. The two finite turning points are z=±az=\pm a, while the two points ±\infty_\pm above infinity are unramified poles of λ0=y ⁣dz\lambda_0=y\,\dd z. Fix their sheet labels by

yz±1at ±.\frac yz\longrightarrow\pm1 \qquad \text{at }\infty_\pm.

Let δ\delta be the positively oriented lift of the cut from a-a to aa in the orientation fixed on Page 4. Residue evaluation gives

Πδ,0=iπa2.\Pi_{\delta,0} = \ii\pi a^2.

Every higher even Weber differential is residue-free. On the punctured genus-zero cover it is therefore exact, so the complete closed formal period truncates:

Πδform()=iπa2,Πδ,2k=0(k1).\Pi_\delta^{\mathrm{form}}(\hbar) = \ii\pi a^2, \qquad \Pi_{\delta,2k}=0 \quad(k\geq1).

The first exactness certificate is concrete:

λ2= ⁣d ⁣(5z24y3z24a2y).\lambda_2 = \dd\!\left( \frac{5z}{24y^3} - \frac{z}{24a^2y} \right).

Its primitive returns to the same value around δ\delta but has different finite parts at the two points over infinity.

This does not make all higher Weber data zero. For the relative path β:+\beta:\infty_-\to\infty_+ used on Page 5, define

Wβform():=1β(Ωλ0).W_\beta^{\mathrm{form}}(\hbar) := \frac1\hbar \int_\beta \left( \Omega-\lambda_0 \right).

Define the Bernoulli polynomials by

sexses1=n0Bn(x)snn!.\frac{s e^{xs}}{e^s-1} = \sum_{n\geq0} B_n(x)\frac{s^n}{n!}.

The endpoint values give the complete series

Wβform()=k1B2k(1/2)(2k1)(2k)(2a2)2k1=k1(122k1)B2k2k(2k1)2k1a4k2.\begin{aligned} W_\beta^{\mathrm{form}}(\hbar) &= \sum_{k\geq1} \frac{B_{2k}(1/2)}{(2k-1)(2k)} \left( \frac{2\hbar}{a^2} \right)^{2k-1} \\ &= \sum_{k\geq1} \frac{ \left(1-2^{2k-1}\right)B_{2k} }{ 2k(2k-1) } \frac{ \hbar^{2k-1} }{ a^{4k-2} }. \end{aligned}

Here Bn:=Bn(0)B_n:=B_n(0), and the second line uses Bn(1/2)=(21n1)BnB_n(1/2)=(2^{1-n}-1)B_n.

The first terms are

Wβform=12a2+73360a63151260a10+O(7).\begin{aligned} W_\beta^{\mathrm{form}} ={}& -\frac{\hbar}{12a^2} + \frac{7\hbar^3}{360a^6} \\ & - \frac{31\hbar^5}{1260a^{10}} + O(\hbar^7). \end{aligned}

Thus the same exact differentials that disappear on δ\delta retain nonzero endpoint constants on β\beta.

The exact special function makes the all-orders formula transparent. Put

t=a22.t=\frac{a^2}{2\hbar}.

After the scaling X=2/zX=\sqrt{2/\hbar}\,z, the equation becomes

 ⁣d2ψ ⁣dX2+(ν+12X24)ψ=0,ν=t12.\begin{aligned} \frac{\dd^2\psi}{\dd X^2} + \left( \nu+\frac12-\frac{X^2}{4} \right)\psi &=0, \\ \nu &=t-\frac12. \end{aligned}

whose standard solutions include Dν(X)D_\nu(X). Parabolic-cylinder connection coefficients contain gamma functions. Removing the elementary Stirling part gives

G(t):=logΓ ⁣(t+12)tlogt+t12log(2π),G(t)Wβform(),t,\begin{aligned} G(t) :={}& \log\Gamma\!\left(t+\frac12\right) \\ &{}-t\log t+t -\frac12\log(2\pi), \\ G(t) \sim{}& W_\beta^{\mathrm{form}}(\hbar), \qquad t\to\infty, \end{aligned}

with compatible logarithm branches and in a Stirling sector. This is an asymptotic comparison, not an assertion that a divergent formal series equals an analytic function without a summation prescription.

The exact spectrum is a benchmark, not a formal corollary

Section titled “The exact spectrum is a benchmark, not a formal corollary”

For the real-line oscillator, a solution decaying at both infinities exists precisely when ν=nZ0\nu=n\in\mathbb Z_{\geq0}. Hence

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

Equivalently, the positive mechanical action J=iΠδ,0=πa2J=-\ii\Pi_{\delta,0}=\pi a^2 obeys

J=2π(n+12).J = 2\pi\hbar \left(n+\frac12\right).

The numerical equality is exact for this quadratic potential, but its logical source is the two-ended boundary condition encoded by the parabolic-cylinder connection coefficient. The formal closed period alone does not manufacture the half-integer shift. Chapter 9 will derive how local turning-point connection data and global boundary conditions enter a quantization condition.

Mathieu turns the periodic cylinder into a torus

Section titled “Mathieu turns the periodic cylinder into a torus”

Use the periodic Schrödinger convention with Λ>0\Lambda>0:

[2x2+V(x)]ψ=Eψ,V(x)=2Λ2cos(2x).\begin{aligned} \left[ -\hbar^2\partial_x^2 +V(x) \right]\psi &=E\psi, \\ V(x) &=2\Lambda^2\cos(2x). \end{aligned}

The standard Mathieu parameters are

aM=E2,qM=Λ22.a_{\mathrm M} = \frac{E}{\hbar^2}, \qquad q_{\mathrm M} = \frac{\Lambda^2}{\hbar^2}.

Thus the semiclassical limit at fixed EE and Λ\Lambda is a correlated large-aMa_{\mathrm M}, large-qMq_{\mathrm M} limit. It is not the small-qMq_{\mathrm M} perturbation theory tabulated for weak periodic potentials.

Set w=exp(2ix)w=\exp(2\ii x). Then

R0=Λ2(w+w1)E.R_0 = \Lambda^2\left(w+w^{-1}\right)-E.

With Y=wyY=wy, the compact spectral curve and its action differential are

Y2=w(Λ2w2Ew+Λ2),λ0=Y2iw2 ⁣dw,Eλ0= ⁣dw4iY.\begin{aligned} Y^2 &= w\left( \Lambda^2w^2-Ew+\Lambda^2 \right), \\ \lambda_0 &= \frac{Y}{2\ii w^2}\,\dd w, \\ \partial_E\lambda_0 &= -\frac{\dd w}{4\ii Y}. \end{aligned}

This is a compactification of the classical curve. Substituting w=exp(2ix)w=\exp(2\ii x) directly into the quantum equation creates a first derivative; returning that equation to normal form requires the half-density and Schwarzian transformation developed on Page 8.

The four branch points are 00, \infty, and

w±=E±E24Λ42Λ2,w+w=1.w_\pm = \frac{ E\pm\sqrt{E^2-4\Lambda^4} }{2\Lambda^2}, \qquad w_+w_-=1.

For E±2Λ2E\neq\pm2\Lambda^2 they are distinct, and the compact cover has genus one. The two finite discriminant values are the minimum and maximum of the real potential. The form λ0\lambda_0 has second-kind poles at the ramification points over w=0w=0 and w=w=\infty; these are the two complex ends of the cylinder. The handle cycles used below avoid them.

Real Mathieu cycles reduce to complete elliptic integrals

Section titled “Real Mathieu cycles reduce to complete elliptic integrals”

Assume temporarily that

2Λ2<E<2Λ2-2\Lambda^2<E<2\Lambda^2

and define the elliptic parameter

m:=E+2Λ24Λ2,0<m<1.m := \frac{E+2\Lambda^2}{4\Lambda^2}, \qquad 0<m<1.

To avoid confusing a modulus with a parameter, use

K(m):=0π/2 ⁣dθ1msin2θ,E(m):=0π/21msin2θ ⁣dθ.\begin{aligned} \mathbf K(m) &:= \int_0^{\pi/2} \frac{\dd\theta}{ \sqrt{1-m\sin^2\theta}}, \\ \mathbf E(m) &:= \int_0^{\pi/2} \sqrt{1-m\sin^2\theta}\,\dd\theta. \end{aligned}

The two turning points bounding the allowed interval can be represented in the physical cell by

x±=π2±arcsinm(modπ).x_\pm = \frac\pi2 \pm\arcsin\sqrt m \pmod{\pi}.

First keep the two physical real contours distinct from a canonical basis. Let δ\delta_- be the doubled allowed interval around the minimum at x=π/2x=\pi/2, and let δ+\delta_+ be the doubled forbidden interval across the maximum at x=0x=0. In the convention y2=VEy^2=V-E, orient them so that

Πδ,0=iJ,Πδ+,0=J+.\begin{aligned} \Pi_{\delta_-,0} &= \ii J_-, \\ \Pi_{\delta_+,0} &= J_+. \end{aligned}

The positive real actions are

J=8Λ[E(m)(1m)K(m)],J+=8Λ[E(1m)mK(1m)].\begin{aligned} J_- &= 8\Lambda \left[ \mathbf E(m) -(1-m)\mathbf K(m) \right], \\ J_+ &= 8\Lambda \left[ \mathbf E(1-m) -m\mathbf K(1-m) \right]. \end{aligned}

Both δ\delta_- and δ+\delta_+ are primitive, but they are not a symplectic pair. After their common branch-point endpoints are resolved, the two crossings have the same sign. Choose the global cycle orientations so that this sign is positive. Each resolved crossing then contributes +1+1, giving

δδ+=+2.\delta_-\mathbin{\cdot}\delta_+=+2.

Equivalently, the complementary base arcs join to a loop around the branch point w=0w=0. This is the cylinder’s two-ended topology made visible on the double cover. A primitive integral basis can be chosen so that

A=δ,δ+=A+2B,AB=+1.\begin{aligned} A &=\delta_- , \\ \delta_+ &=A+2B, \\ A\mathbin{\cdot}B &=+1. \end{aligned}

Consequently, the corresponding primitive-basis periods are

ΠA,0=iJ,ΠB,0=J+iJ2.\Pi_{A,0}=\ii J_- , \qquad \Pi_{B,0} = \frac{J_+-\ii J_-}{2}.

Although the last expression contains 1/21/2, BB is an integral cycle: the two real vanishing cycles represent the same class modulo 22 on this four-branch-point cover.

The derivative check is particularly simple for the physical actions:

EJ=K(m)Λ,EJ+=K(1m)Λ.\partial_EJ_- = \frac{\mathbf K(m)}{\Lambda}, \qquad \partial_EJ_+ = -\frac{\mathbf K(1-m)}{\Lambda}.

In the primitive basis this implies

EΠA,0=iK(m)Λ,EΠB,0=K(1m)+iK(m)2Λ.\begin{aligned} \partial_E\Pi_{A,0} &= \frac{\ii\mathbf K(m)}{\Lambda}, \\ \partial_E\Pi_{B,0} &= -\frac{ \mathbf K(1-m)+\ii\mathbf K(m) }{2\Lambda}. \end{aligned}

The resulting elliptic ratio is a useful orientation check:

τ:=EΠB,0EΠA,0=12+iK(1m)2K(m),Imτ>0.\begin{aligned} \tau :={}& \frac{\partial_E\Pi_{B,0}}{ \partial_E\Pi_{A,0}} \\ &= -\frac12 + \frac{\ii\mathbf K(1-m)}{2\mathbf K(m)}, \\ \operatorname{Im}\tau &>0. \end{aligned}

As E2Λ2E\to-2\Lambda^2, δ=A\delta_-=A collapses around the potential minimum. As E+2Λ2E\to+2\Lambda^2, δ+=A+2B\delta_+=A+2B collapses around the maximum. Analytic continuation away from the real chamber transports the integral cycle lattice; it does not preserve the labels “allowed” and “forbidden.”

One operator computes both Mathieu quantum periods

Section titled “One operator computes both Mathieu quantum periods”

Let

R0(x;E)=2Λ2cos(2x)E,y2=R0.R_0(x;E) = 2\Lambda^2\cos(2x)-E, \qquad y^2=R_0.

The action form has the exact Picard–Fuchs certificate

[(E24Λ4)E2+14]λ0= ⁣dx ⁣[Λ2sin(2x)2y].\begin{aligned} &\left[ \left(E^2-4\Lambda^4\right)\partial_E^2 + \frac14 \right]\lambda_0 \\ &\qquad= \dd_x\!\left[ \frac{\Lambda^2\sin(2x)}{2y} \right]. \end{aligned}

Therefore every flat closed period satisfies

[(E24Λ4)E2+14]Πγ,0=0.\left[ \left(E^2-4\Lambda^4\right)\partial_E^2 + \frac14 \right] \Pi_{\gamma,0} =0.

The leading coefficient vanishes at exactly the two finite discriminant values. The elliptic formulas above solve this equation with different cycle data.

For the source-free equation, direct substitution in the Page 6 formula for λ2\lambda_2 gives the pointwise identity

λ2=[14E3EE253(E24Λ4)E3]λ0.\begin{aligned} \lambda_2 ={}& \left[ -\frac14\partial_E -3E\partial_E^2 \right. \\ &\left. \qquad -\frac53 \left(E^2-4\Lambda^4\right) \partial_E^3 \right] \lambda_0. \end{aligned}

Reducing the third derivative by the Picard–Fuchs equation gives, for every flat closed cycle γ\gamma,

Πγ,2=[16E+E3E2]Πγ,0=[16EE12(E24Λ4)]Πγ,0.\begin{aligned} \Pi_{\gamma,2} &= \left[ \frac16\partial_E + \frac E3\partial_E^2 \right] \Pi_{\gamma,0} \\ &= \left[ \frac16\partial_E - \frac{E}{ 12\left(E^2-4\Lambda^4\right) } \right] \Pi_{\gamma,0}. \end{aligned}

The second representative is valid only off the discriminant. Acting first on the two physical real periods gives

Πδ,2=iJ,2,Πδ+,2=J+,2.\begin{aligned} \Pi_{\delta_-,2} &= \ii J_{-,2}, \\ \Pi_{\delta_+,2} &= J_{+,2}. \end{aligned}

Here

J,2:=K(m)12Λm+(2m1)E(m)12Λm(1m),J+,2:=K(1m)12Λ(1m)+(2m1)E(1m)12Λm(1m).\begin{aligned} J_{-,2} &:= \frac{\mathbf K(m)}{12\Lambda m} \\ &\quad+ \frac{ (2m-1)\mathbf E(m) }{12\Lambda m(1-m)}, \\ J_{+,2} &:= -\frac{\mathbf K(1-m)}{12\Lambda(1-m)} \\ &\quad+ \frac{ (2m-1)\mathbf E(1-m) }{12\Lambda m(1-m)}. \end{aligned}

Linearity then preserves the integral normalization:

ΠA,2=iJ,2,ΠB,2=J+,2iJ,22.\Pi_{A,2} = \ii J_{-,2}, \qquad \Pi_{B,2} = \frac{J_{+,2}-\ii J_{-,2}}{2}.

These are formal coefficients, not Borel sums. As a cycle degeneration is approached, the first correction has a finite one-sided limit while the corresponding classical action vanishes:

m0:J2πΛm,J,2π16Λ,m1:J+2πΛ(1m),J+,2π16Λ.\begin{aligned} m\to0: \quad J_- &\sim2\pi\Lambda m, \\ J_{-,2} &\to\frac{\pi}{16\Lambda}, \\ m\to1: \quad J_+ &\sim2\pi\Lambda(1-m), \\ J_{+,2} &\to-\frac{\pi}{16\Lambda}. \end{aligned}

Thus 2J±,2\hbar^2J_{\pm,2} is no longer a small correction relative to J±J_\pm; fixed-energy WKB is nonuniform there. For example, near the minimum put x=π/2+ux=\pi/2+u and E=2Λ2+ϵE=-2\Lambda^2+\epsilon. Then

2Λ2cos(2x)E=4Λ2u2ϵ+O(u4),2\Lambda^2\cos(2x)-E = 4\Lambda^2u^2-\epsilon +O(u^4),

so a correlated local scaling produces the Weber problem. At an isolated turning point away from the collision, the local model is Airy. The three examples are therefore nested rather than unrelated.

Mathieu’s exact solutions may be normalized by

ψ(x+π)=exp(iπν)ψ(x),\psi(x+\pi) = \exp(\ii\pi\nu)\psi(x),

where ν\nu is the characteristic exponent. Periodic and antiperiodic band edges correspond to integral ν\nu. The formal AA- and BB-periods are ingredients in semiclassical descriptions of this monodromy, but the equation above is an exact statement about an analytic solution. Converting the formal periods into its exact Hill discriminant requires a summation chamber, Stokes data, and a global connection formula. Those enter Chapter 9; the band spectrum is developed in Chapter 14.

The Airy–Weber–Mathieu check verifies:

  • the Airy scaling, first even WKB correction, and asymptotic coefficient;
  • Weber closed residues and several terms of the Bernoulli formula;
  • the Weber gamma-tail coefficients and parabolic-cylinder parameter;
  • the Mathieu algebraic curve, discriminant, Picard–Fuchs certificate, and first quantum operator;
  • the real JJ_- and J+J_+ actions against direct quadrature, followed by the primitive-basis conversion.

Run

Terminal window
python3 public/code/advanced-ode/airy-weber-mathieu-check.py

The script checks formal identities and a high-precision classical quadrature. It does not Borel-sum a series, determine a Stokes chamber, or solve a Mathieu band problem.

Dropping the imaginary unit in an allowed region. With y2=VEy^2=V-E, the chosen momentum is imaginary where E>VE>V. Convert to the positive mechanical action only after fixing the sheet and cycle orientation.

Treating Airy asymptotics as one global formula. The exact Airy function is entire, but each displayed asymptotic representation has a sector. Continuing the exact function and continuing one formal expansion are not the same operation.

Calling every Weber correction zero. Higher closed periods vanish, whereas the pole-to-pole correction has a nontrivial Bernoulli series. The difference is absolute versus relative data, not a contradiction.

Deriving the Maslov shift from a classical integral alone. The closed Weber action happens to reproduce the exact energies after a half-integer condition is supplied. The shift comes from analytic turning-point and boundary data.

Confusing Mathieu’s parameter with the cylinder coordinate. The standard parameter is qM=Λ2/2q_{\mathrm M}=\Lambda^2/\hbar^2; the algebraic coordinate used above is w=exp(2ix)w=\exp(2\ii x). They play unrelated roles.

Substituting a discriminant value into a regular-family operator. At E=±2Λ2E=\pm2\Lambda^2, a cycle degenerates and the fixed-energy WKB expansion is nonuniform. Coefficientwise endpoint limits can diagnose the failure, but spectral conclusions at the colliding pair require a Weber scaling. Airy applies while an individual turning point remains isolated.

Starting from the regularized Airy action, expand

z1/4exp ⁣[1AAireg]z^{-1/4} \exp\!\left[ -\frac1\hbar \mathcal A_{\mathrm{Ai}}^{\mathrm{reg}} \right]

through relative order \hbar. Compare it with the first correction in the asymptotic expansion of Ai(z/2/3)\operatorname{Ai}(z/\hbar^{2/3}).

Solution

Substitution gives

z1/4exp ⁣[2z3/23548z3/2+O(3)]=z1/4exp ⁣[2z3/23]×[1548z3/2+O(2)].\begin{aligned} &z^{-1/4} \exp\!\left[ -\frac{2z^{3/2}}{3\hbar} - \frac{5\hbar}{48z^{3/2}} +O(\hbar^3) \right] \\ &\qquad= z^{-1/4} \exp\!\left[ -\frac{2z^{3/2}}{3\hbar} \right] \\ &\qquad\quad\times \left[ 1- \frac{5\hbar}{48z^{3/2}} +O(\hbar^2) \right]. \end{aligned}

This is the first Airy coefficient. The exact normalization 1/6/(2π)\hbar^{1/6}/(2\sqrt\pi) is independent of zz and is not fixed by the phase integral.

2. Reduce Weber to parabolic-cylinder form

Section titled “2. Reduce Weber to parabolic-cylinder form”

Apply X=2/zX=\sqrt{2/\hbar}\,z to the Weber equation and derive ν=a2/(2)1/2\nu=a^2/(2\hbar)-1/2. Explain why decay at both real infinities forces ν\nu to be a nonnegative integer.

Solution

Since z2=(2/)X2\partial_z^2=(2/\hbar)\partial_X^2, division by 22\hbar gives

 ⁣d2ψ ⁣dX2+[a22X24]ψ=0.\frac{\dd^2\psi}{\dd X^2} + \left[ \frac{a^2}{2\hbar} - \frac{X^2}{4} \right]\psi =0.

Comparison with the standard equation identifies ν+1/2=a2/(2)\nu+1/2=a^2/(2\hbar). The solution Dν(X)D_\nu(X) decays for X+X\to+\infty. Its connection formula at -\infty contains a growing component proportional to 1/Γ(ν)1/\Gamma(-\nu). That coefficient vanishes exactly for ν=nZ0\nu=n\in\mathbb Z_{\geq0}, giving an2=(2n+1)a_n^2=(2n+1)\hbar.

3. Recover the Weber Bernoulli coefficients

Section titled “3. Recover the Weber Bernoulli coefficients”

Use the shifted Stirling expansion of logΓ(t+1/2)\log\Gamma(t+1/2) to compute the first three inverse powers in G(t)G(t). Substitute t=a2/(2)t=a^2/(2\hbar).

Solution

The shifted expansion is

G(t)124t+72880t33140320t5+O(t7).\begin{aligned} G(t) \sim{}& -\frac{1}{24t} + \frac{7}{2880t^3} \\ & - \frac{31}{40320t^5} + O(t^{-7}). \end{aligned}

Since t(2k1)=(2/a2)2k1t^{-(2k-1)}=(2\hbar/a^2)^{2k-1}, this becomes

12a2+73360a63151260a10+O(7),-\frac{\hbar}{12a^2} + \frac{7\hbar^3}{360a^6} - \frac{31\hbar^5}{1260a^{10}} + O(\hbar^7),

which is the pole-to-pole series. It says nothing about the higher closed periods, which vanish separately.

For 2Λ2<E<2Λ2-2\Lambda^2<E<2\Lambda^2, derive JJ_- by writing x=π/2+ux=\pi/2+u and then setting sinu=msinθ\sin u=\sqrt m\sin\theta. Obtain J+J_+ by the complementary substitution around x=0x=0.

Solution

Around the minimum,

E2Λ2cos(2x)=4Λ2(msin2u).E-2\Lambda^2\cos(2x) = 4\Lambda^2 \left( m-\sin^2u \right).

The doubled allowed action is therefore

J=8Λ0arcsinmmsin2u ⁣du.J_- = 8\Lambda \int_0^{\arcsin\sqrt m} \sqrt{m-\sin^2u}\,\dd u.

The stated substitution reduces the integral to E(m)(1m)K(m)\mathbf E(m)-(1-m)\mathbf K(m). Around the maximum,

2Λ2cos(2x)E=4Λ2(1msin2x),2\Lambda^2\cos(2x)-E = 4\Lambda^2 \left( 1-m-\sin^2x \right),

and the same calculation with m1mm\mapsto1-m gives J+=8Λ[E(1m)mK(1m)]J_+=8\Lambda[\mathbf E(1-m)-m\mathbf K(1-m)].

Suppose the oriented real vanishing cycles obey δδ+=2\delta_-\mathbin{\cdot}\delta_+=2 and choose A=δA=\delta_-, δ+=A+2B\delta_+=A+2B. Verify the intersection of AA and BB, and express their classical periods in terms of JJ_- and J+J_+.

Solution

Skew-symmetry gives AA=0A\mathbin{\cdot}A=0, so

2=δδ+=A(A+2B)=2AB.2 = \delta_-\mathbin{\cdot}\delta_+ = A\mathbin{\cdot}(A+2B) = 2A\mathbin{\cdot}B.

Hence AB=1A\mathbin{\cdot}B=1. Periods are linear in homology, and the chosen real-cycle orientations give

ΠA,0=iJ,ΠB,0=J+iJ2.\Pi_{A,0}=\ii J_- , \qquad \Pi_{B,0} = \frac{J_+-\ii J_-}{2}.

The division by two occurs in a change between integral bases; it does not license arbitrary half-integral cycles.

6. Verify the Mathieu Picard–Fuchs certificate

Section titled “6. Verify the Mathieu Picard–Fuchs certificate”

For R0=2Λ2cos(2x)ER_0=2\Lambda^2\cos(2x)-E, prove the exact-form identity in the text and integrate it over a flat closed cycle.

Solution

Because E2λ0= ⁣dx/(4y3)\partial_E^2\lambda_0=-\dd x/(4y^3), the left-hand side has coefficient

E24Λ44y3+y4.-\frac{E^2-4\Lambda^4}{4y^3} + \frac y4.

Use y2=2Λ2cos(2x)Ey^2=2\Lambda^2\cos(2x)-E to put this over y3y^3. Differentiating Λ2sin(2x)/(2y)\Lambda^2\sin(2x)/(2y) gives the same numerator. The primitive is single-valued meromorphic on the spectral cover, so its integral over a closed cycle vanishes.

Starting from the third-order pointwise operator for λ2\lambda_2, differentiate the Picard–Fuchs equation once and derive the second-order period operator.

Solution

Let D=E24Λ4D=E^2-4\Lambda^4 and let ff be a classical period. Then

Df+14f=0,Df+2Ef+14f=0.\begin{aligned} Df''+\frac14f &=0, \\ Df'''+2Ef''+\frac14f' &=0. \end{aligned}

Substitution in

14f3Ef53Df-\frac14f' -3Ef'' -\frac53Df'''

gives

16f+E3f.\frac16f' + \frac E3f''.

Using the first Picard–Fuchs equation once more yields the equivalent first-order representative

16fE12Df.\frac16f' - \frac{E}{12D}f.

Its discriminant pole is introduced by derivative-order reduction.

Expand the potential near x=π/2x=\pi/2 and x=0x=0. Which local equation appears when the energy approaches the corresponding extremum? What model applies at one isolated turning point before the collision?

Solution

With x=π/2+ux=\pi/2+u,

2Λ2cos(2x)=2Λ2+4Λ2u2+O(u4).2\Lambda^2\cos(2x) = -2\Lambda^2+4\Lambda^2u^2+O(u^4).

Near x=0x=0,

2Λ2cos(2x)=2Λ24Λ2x2+O(x4).2\Lambda^2\cos(2x) = 2\Lambda^2-4\Lambda^2x^2+O(x^4).

The lower collision is an ordinary Weber oscillator and the upper collision is its inverted continuation. Away from either collision, each individual simple turning point has an Airy scaling. The elliptic expansion must be reorganized in the correlated local limit: a finite coefficientwise endpoint limit does not make the fixed-energy WKB hierarchy uniform there.

  • NIST Digital Library of Mathematical Functions, §9.2 and §9.7(ii), equation (9.7.5). Defines the Airy equation and gives the sectorial Poincaré expansion used for the normalization check.
  • NIST Digital Library of Mathematical Functions, equation (12.2.4), equation (12.2.5), §12.2(v), equation (12.7.2), and §12.9(i). Defines DνD_\nu, records the connection formulas, identifies the Hermite-polynomial cases, and supplies the large-variable asymptotics used in the oscillator benchmark.
  • NIST Digital Library of Mathematical Functions, §5.11(i). Gives Stirling expansions and their sector conditions for the gamma-function comparison.
  • K. Iwaki, T. Koike, and Y.-M. Takei, “Voros Coefficients for the Hypergeometric Differential Equations and Eynard–Orantin’s Topological Recursion, Part I: For the Weber Equation”, Annales Henri Poincaré 24 (2023), 1305–1353, §4, especially Theorem 4.10. Derives the complete Weber Voros coefficient in terms of Bernoulli polynomials. Its normalization maps to this page by xIKT=2zx_{\mathrm{IKT}}=2z, IKT=2\hbar_{\mathrm{IKT}}=2\hbar, λIKT=a2\lambda_{\mathrm{IKT}}=a^2, and νIKT=0\nu_{\mathrm{IKT}}=0; its rational-cover path 00\to\infty represents the oriented path +\infty_-\to\infty_+ used here.
  • NIST Digital Library of Mathematical Functions, §28.2(i), equations (28.2.1)–(28.2.3), §28.2(iii), equations (28.2.14)–(28.2.16), and §28.2(v), especially Table 28.2.1. Fixes the standard Mathieu parameters, algebraic forms, and Floquet normalization, including the periodic and antiperiodic integral characteristic exponents.
  • NIST Digital Library of Mathematical Functions, §19.2(ii) and §19.4(i). Defines the complete elliptic integrals and records the derivative identities used for JJ_- and J+J_+; the DLMF modulus satisfies k2=mk^2=m here.
  • K. Imaizumi, “Exact WKB Analysis and TBA Equations for the Mathieu Equation”, Physics Letters B 806 (2020), 135500, §§2–3, especially equations (2.1)–(2.12) and (3.16)–(3.18). Gives the two Mathieu cycle sectors and the first quantum-period operator; Figure 2.1 and equations (2.13)–(2.14) also display the two same-sign crossings behind the physical-cycle factor 22. Its variables translate by q=2xq=2x, there=2\hbar_{\mathrm{there}}=2\hbar, and Λthere2=2Λ2\Lambda_{\mathrm{there}}^2=2\Lambda^2, with uthere=Eu_{\mathrm{there}}=E and pthere2=EV=y2p_{\mathrm{there}}^2=E-V=-y^2. On the selected sheet its period is athere=2iΠherea_{\mathrm{there}}=-2\ii\Pi_{\mathrm{here}}, and the first operator rescales as Dhere=4D1,there\mathcal D_{\mathrm{here}}=4\mathcal D_{1,\mathrm{there}}, giving 16E+E3E2\frac16\partial_E+\frac E3\partial_E^2. Imaizumi draws the cycles on qq+4πq\sim q+4\pi; the degree-two quotient to qq+2πq\sim q+2\pi, equivalently this page’s xx+πx\sim x+\pi, identifies his equal-period forbidden cycles β\beta and β~\widetilde\beta while retaining their two same-sign crossings.
  • A.-K. Kashani-Poor and J. Troost, “Pure N=2\mathcal N=2 Super Yang–Mills and Exact WKB”, Journal of High Energy Physics 08 (2015), 160, §2.1. Uses an intersection-one homology basis for the same elliptic curve–Mathieu correspondence, providing the primitive-basis side of the cycle normalization used here.
  • J. L. Dunham, “The Wentzel–Brillouin–Kramers Method of Solving the Wave Equation”, Physical Review 41 (1932), 713–720. Classical source for the all-orders closed-contour expansion and oscillator benchmark.