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Airy, Bessel, Weber, and Hypergeometric Local Models

Four equations recur because they isolate four different pieces of linear-ODE geometry. Airy resolves a simple turning point, Bessel resolves the inverse-square normal form of a regular-singular endpoint, Weber resolves a quadratic well or two coalescing turning points, and Gauss hypergeometric resolves the complete global geometry of three regular singularities. A named function is useful only after its equation convention, scaling, basis normalization, branches, and validity region have been fixed.

This chapter asks:

The Chapter 1 case files already computed detailed Bessel, Airy, and Gauss connection data. The Chapter 2 benchmark then completed the path-labelled Gauss connection problem. Here the emphasis changes: the four models are organized as a selection atlas, Weber is added, and exact reductions are separated from leading local approximations.

Diagnostic featureCanonical equationDistinguished data
A simple zero of a normal-form potentialAiryOne recessive solution in each of three lifted sectors
An inverse-square regular-singular endpointBesselFrobenius powers at the endpoint and Hankel waves at infinity
A quadratic well or a pair of coalescing simple turning pointsWeberParabolic-cylinder solutions in four asymptotic sectors
Exactly three regular singularities on the sphereGauss hypergeometricThree Frobenius bases and rigid gamma-function connections

These rows are not merely a list of special functions. They answer different questions:

  • Airy and Weber are usually uniform local models in a small-parameter problem.
  • Bessel can be a local endpoint model or an exact equation on the whole domain.
  • Gauss is an exact global normal form for a second-order Fuchsian equation with precisely three singular points.

An equivalence to a canonical equation may use a coordinate change and a scalar gauge. Both must be retained. The coordinate selects branches and maps sectors; the gauge changes Wronskians and boundary normalizations.

Start from a Schrödinger-type normal form

2ψ(z)=Q(z)ψ(z)\hbar^2\psi''(z)=Q(z)\psi(z)

Assume that QQ is holomorphic near z0z_0, that z0z_0 is an isolated simple zero, and that 0\hbar\to0 in a fixed complex sector. Thus

Q(z0)=0,Q(z0)0.Q(z_0)=0, \qquad Q'(z_0)\neq0.

Keeping only the linear Taylor term and setting

ξ=Q(z0)1/32/3(zz0)\xi = \frac{ Q'(z_0)^{1/3} }{\hbar^{2/3}} (z-z_0)

gives

 ⁣d2ψ ⁣dξ2=ξψ.\frac{\dd^2\psi}{\dd\xi^2} = \xi\psi.

This is the Airy equation. The cube root in the scaling is part of the answer: changing it rotates the ξ\xi-plane and permutes the sectorial solutions.

For a coordinate adapted beyond leading order, choose compatible paths and branches and define an \hbar-independent Langer coordinate ζ\zeta by

23ζ(z)3/2=z0zQ(s) ⁣ds.\frac23\zeta(z)^{3/2} = \int_{z_0}^{z} \sqrt{Q(s)}\,\dd s.

Then the half-density transformation may be written in either direction as

ξ=2/3ζ,W(ζ)=ζ(z)ψ(z),ψ(z)=(ζ(z))1/2W(ζ)=(ζ(z)Q(z))1/4W(ζ).\begin{aligned} \xi&=\hbar^{-2/3}\zeta,\\ W(\zeta) &= \sqrt{\zeta'(z)}\,\psi(z),\\ \psi(z) &= \bigl(\zeta'(z)\bigr)^{-1/2}W(\zeta) = \left( \frac{\zeta(z)}{Q(z)} \right)^{1/4}W(\zeta). \end{aligned}

It gives the exact transformed equation

2 ⁣d2W ⁣dζ2=[ζ22{z,ζ}]W,\hbar^2 \frac{\dd^2W}{\dd\zeta^2} = \left[ \zeta - \frac{\hbar^2}{2} \{z,\zeta\} \right]W,

where

{z,ζ}=zζζζzζ32(zζζzζ)2\{z,\zeta\} = \frac{z_{\zeta\zeta\zeta}}{z_\zeta} - \frac32 \left( \frac{z_{\zeta\zeta}}{z_\zeta} \right)^2

is the Schwarzian derivative. The path and square-root branch determine the lift of ζ\zeta and ξ\xi. The half-density removes the first derivative generated by the coordinate change. On compact subsets of the resulting Airy neighborhood, the Schwarzian term is a controlled remainder. The reduction is not automatically the exact Airy equation.

The canonical entire solutions satisfy

Wr[Ai(ξ),Bi(ξ)]=1π.\Wr \left[ \operatorname{Ai}(\xi), \operatorname{Bi}(\xi) \right] = \frac1\pi.

On the principal lift, Ai(ξ)\operatorname{Ai}(\xi) is recessive in argξ<π/3|\arg\xi|<\pi/3. Its standard asymptotic expansion has

Ai(ξ)ξ1/42πexp(23ξ3/2).\operatorname{Ai}(\xi) \sim \frac{ \xi^{-1/4} }{ 2\sqrt{\pi} } \exp\left( -\frac23\xi^{3/2} \right).

The expansion is valid in the larger closed subsectors argξπδ|\arg\xi|\leq\pi-\delta for fixed δ>0\delta>0; recessiveness is the stronger statement that the displayed exponential decays.

If ω=e2πi/3\omega=\ee^{2\pi\ii/3}, the exact relation

Ai(ξ)+ωAi(ωξ)+ω2Ai(ω2ξ)=0\operatorname{Ai}(\xi) + \omega\operatorname{Ai}(\omega\xi) + \omega^2\operatorname{Ai}(\omega^2\xi) =0

packages the three sectorially recessive solutions in a two-dimensional space. It is the smallest exact laboratory for Stokes connection data. The finite turning point ξ=0\xi=0 is nevertheless an ordinary point of the Airy ODE; the irregular singularity is at infinity.

Bessel resolves an inverse-square endpoint

Section titled “Bessel resolves an inverse-square endpoint”

The Bessel equation is

z2y+zy+(z2ν2)y=0.z^2y''+zy'+(z^2-\nu^2)y=0.

Its origin is regular singular with exponents ±ν\pm\nu. A generic regular singular point is governed locally by Euler–Frobenius data; Bessel is selected when the Liouville normal form retains an inverse-square term together with the relevant constant or parameter-dependent term:

u+[k2ν214x2]u=0,k0,u(x)=xy(kx).u'' + \left[ k^2 - \frac{\nu^2-\tfrac14}{x^2} \right]u =0, \qquad k\neq0, \qquad u(x)=\sqrt{x}\,y(kx).

Thus an inverse-square coefficient determines the Bessel order, while the square root, taken on a chosen branch, is the gauge that shifts the normal-form exponents to 12±ν\tfrac12\pm\nu.

For νZ\nu\notin\mathbb Z, a unit-leading Frobenius basis on a chosen branch is

f+(z)=2νΓ(ν+1)Jν(z),f(z)=2νΓ(1ν)Jν(z),\begin{aligned} f_+(z) &= 2^\nu\Gamma(\nu+1)J_\nu(z),\\ f_-(z) &= 2^{-\nu}\Gamma(1-\nu)J_{-\nu}(z), \end{aligned}

with

f±(z)=z±ν(1+O(z2)),Wr[f+,f]=2νz.f_\pm(z)=z^{\pm\nu}\bigl(1+O(z^2)\bigr), \qquad \Wr[f_+,f_-]=-\frac{2\nu}{z}.

At infinity, Hν(1)H_\nu^{(1)} and Hν(2)H_\nu^{(2)} select outgoing and incoming oscillatory branches only after a time convention, a sector, and a branch of z1/2z^{1/2} have been specified. With time dependence eiωt\ee^{-\ii\omega t}, Hν(1)H_\nu^{(1)} is outgoing on the positive real ray; reversing the time convention swaps that interpretation. Their raw Wronskian is

Wr[Hν(1)(z),Hν(2)(z)]=4iπz.\Wr \left[ H_\nu^{(1)}(z), H_\nu^{(2)}(z) \right] = -\frac{4\ii}{\pi z}.

The exceptional set is instructive. Frobenius resonance occurs when 2νZ2\nu\in\mathbb Z, but a logarithm is not forced at every resonant value. For ν=nZ\nu=n\in\mathbb Z, the pair Jν,JνJ_\nu,J_{-\nu} collapses and YnY_n supplies a logarithmic solution. For νZ+12\nu\in\mathbb Z+\tfrac12, the exponent difference is still integral, yet JνJ_\nu and JνJ_{-\nu} remain independent.

Use the parabolic-cylinder convention

y+(ν+12z24)y=0.y''+ \left( \nu+\frac12-\frac{z^2}{4} \right)y=0.

Every finite point is ordinary. The DLMF notations are related by

Dν(z)=U(ν12,z),D_\nu(z) = U\left( -\nu-\frac12,z \right),

where this two-argument UU is a parabolic-cylinder function, not Tricomi’s confluent hypergeometric U(a,b,z)U(a,b,z).

Put

E=ν+12,Q(z)=z24E.E=\nu+\frac12, \qquad Q(z)=\frac{z^2}{4}-E.

Then the equation is y=Qyy''=Qy. For E0E\neq0, its turning points

z±=±2Ez_\pm=\pm2\sqrt E

are simple on a chosen square-root branch. They coalesce into one double turning point at E=0E=0.

For positive E, the Weber potential is negative between two simple turning points and positive outside them; at E equal to zero, the two points merge into a double turning point.

The Weber potential Q(z)=z2/4EQ(z)=z^2/4-E has two simple turning points for E>0E>0; they merge at E=0E=0. Along the real axis, solutions are oscillatory where Q<0Q<0 and exponential where Q>0Q>0.

When the ++ turning point is well separated, choose E1/6E^{1/6} compatibly with E\sqrt E, so that (E1/6)3=E(E^{1/6})^3=\sqrt E, and set

s=E1/6(z2E).s = E^{1/6} \left( z-2\sqrt E \right).

On the same branches, direct substitution gives

 ⁣d2y ⁣ds2=[s+s24E2/3]y.\frac{\dd^2y}{\dd s^2} = \left[ s+\frac{s^2}{4E^{2/3}} \right]y.

Thus either separated Weber turning point has an Airy neighborhood, while the Weber equation retains both points in one global scaled model. The Airy approximation above is accurate on bounded ss-sets as E|E|\to\infty in a fixed parameter sector; it is not uniform across both turning points.

The solution Dν(z)D_\nu(z) is normalized by

Dν(z)zνez2/4,argz3π4δ,D_\nu(z) \sim z^\nu\ee^{-z^2/4}, \qquad |\arg z| \leq \frac{3\pi}{4}-\delta,

uniformly on every such closed subsector, for fixed δ>0\delta>0, and on the chosen branch of zνz^\nu. The two formal exponential factors at infinity are ez2/4\ee^{-z^2/4} and ez2/4\ee^{z^2/4}; infinity is an unramified irregular singularity of formal slope two, hence of minimal Poincaré rank two. Their equal-magnitude rays obey

Re(z2)=0,argz=π4+kπ2.\operatorname{Re}(z^2)=0, \qquad \arg z=\frac{\pi}{4}+\frac{k\pi}{2}.

This phase condition is safer than relying on inconsistent “Stokes” versus “anti-Stokes” terminology.

The right- and left-recessive solutions on the real line are

uR(z,ν)=Dν(z),uL(z,ν)=Dν(z).u_R(z,\nu)=D_\nu(z), \qquad u_L(z,\nu)=D_\nu(-z).

With the book’s Wronskian convention,

Wr[Dν(z),Dν(z)]=2πΓ(ν).\Wr \left[ D_\nu(z), D_\nu(-z) \right] = \frac{\sqrt{2\pi}}{\Gamma(-\nu)}.

Consequently, the left-to-right boundary Wronskian is

F(ν)=Wr[uL,uR]=2πΓ(ν).F(\nu) = \Wr[u_L,u_R] = -\frac{\sqrt{2\pi}}{\Gamma(-\nu)}.

The sign records the ordering, while the zero set records when the two selected solution lines coincide.

For example, scale the harmonic oscillator

[2 ⁣d2 ⁣dx2+α2x2]ψ=Eψ,,α>0,\left[ -\hbar^2\frac{\dd^2}{\dd x^2} + \alpha^2x^2 \right]\psi = \mathcal E\psi, \qquad \hbar,\alpha>0,

by

z=2αx,ν+12=E2α.z=\sqrt{\frac{2\alpha}{\hbar}}\,x, \qquad \nu+\frac12 = \frac{\mathcal E}{2\alpha\hbar}.

Take the standard self-adjoint realization on L2(R, ⁣dx)L^2(\mathbb R,\dd x) associated with the closed quadratic form

q[ψ]=R(2ψ(x)2+α2x2ψ(x)2) ⁣dx,D(q)=H1(R)L2(R,x2 ⁣dx).\begin{aligned} \mathfrak q[\psi] &= \int_{\mathbb R} \left( \hbar^2|\psi'(x)|^2 + \alpha^2x^2|\psi(x)|^2 \right)\dd x,\\ \mathcal D(\mathfrak q) &= H^1(\mathbb R) \cap L^2(\mathbb R,x^2\dd x). \end{aligned}

The scaling produces the displayed Weber equation. Square integrability at both real infinities is equivalent to the Wronskian condition

1Γ(ν)=0.\frac1{\Gamma(-\nu)}=0.

Because gamma has poles at the nonpositive integers,

ν=nZ0,En=(2n+1)α.\nu=n\in\mathbb Z_{\ge0}, \qquad \mathcal E_n=(2n+1)\alpha\hbar.

At those values,

Dn(z)=2n/2ez2/4Hn(z2),D_n(z) = 2^{-n/2} \ee^{-z^2/4} H_n\left( \frac{z}{\sqrt2} \right),

where HnH_n is the physicists’ Hermite polynomial, and Dn(z)=(1)nDn(z)D_n(-z)=(-1)^nD_n(z). Here an asymptotic connection Wronskian is also a spectral boundary function because the Hilbert space and self-adjoint realization have been declared.

More generally, consider an analytic parameter family whose potential has a nondegenerate double zero with a generic unfolding into two simple zeros. If no competing singularity lies nearby and the parameter remains in a fixed sector, a parameter-dependent Liouville transformation produces a Weber approximant with a controlled remainder across the pair. The quadratic Taylor model suggests the canonical equation; the transformation and remainder estimate establish uniformity. The exact harmonic oscillator is special because its reduction has no remainder.

Gauss resolves three regular singularities

Section titled “Gauss resolves three regular singularities”

The Gauss equation in this book is

z(1z)y+[c(a+b+1)z]yaby=0.z(1-z)y'' + \left[ c-(a+b+1)z \right]y' -ab\,y=0.

Its Riemann scheme is

P ⁣{0100a1ccabb;z}.P\!\left\{ \begin{matrix} 0&1&\infty\\ 0&0&a\\ 1-c&c-a-b&b \end{matrix} ;z \right\}.

The sum of all six exponents is

(1c)+(cab)+(a+b)=1,(1-c)+(c-a-b)+(a+b)=1,

the second-order Fuchs relation on the sphere. The exponent differences

θ0=1c,θ1=cab,θ=ab\theta_0=1-c, \qquad \theta_1=c-a-b, \qquad \theta_\infty=a-b

are convenient gauge-invariant local parameters.

For this ordering of the exponent pairs, the inverse map is

c=1θ0,a=1θ0θ1+θ2,b=1θ0θ1θ2.\begin{aligned} c&=1-\theta_0,\\ a&= \frac{ 1-\theta_0-\theta_1+\theta_\infty }{2},\\ b&= \frac{ 1-\theta_0-\theta_1-\theta_\infty }{2}. \end{aligned}

Swapping the two exponents at a puncture flips the corresponding θj\theta_j. It can change the displayed (a,b,c)(a,b,c) even when the unordered local conjugacy data are unchanged.

Every second-order Fuchsian equation on the sphere with exactly three distinct singular points can be moved to 0,1,0,1,\infty by a Möbius transformation and reduced to this form by a scalar gauge. Once the three local exponent pairs are fixed, no accessory parameter remains. This is why the generic Gauss monodromy problem is rigid and why its connection coefficients reduce to gamma quotients.

The full normalized bases, lateral phases at infinity, gamma connection matrices, monodromy products, resonant limits, and Jacobi spectrum are worked out on the hypergeometric benchmark. The next page adds a fourth regular singular point. Its position supplies a cross-ratio and its coefficient data contain an accessory parameter, so local exponents no longer determine the global equation.

Before importing a special-function identity, classify the reduction:

ClaimWhat must be shown
Exact equivalenceAn invertible coordinate and gauge transform the full equation, including all parameters
Leading local modelA scaled equation converges on a stated bounded scaled domain
Uniform approximationThe error is controlled across a turning-point or endpoint region
Formal normal formEquality holds only as a formal asymptotic series
Spectral equivalenceThe transform also maps the Hilbert space, domain, and boundary conditions

The distinction matters. A local Airy reduction predicts the transition through one turning point but does not by itself determine a two-end spectrum. A Weber reduction can be uniform across two merging turning points without making the original potential globally quadratic. A Liouville transform can preserve the solution space while changing its natural measure and endpoint domain.

Given a new scalar equation:

  1. Put it in Liouville normal form and retain the scalar gauge.
  2. Locate poles and zeros of the normal-form coefficient.
  3. Choose Airy for one simple zero, Bessel for an inverse-square endpoint, Weber for a quadratic well or coalescing pair, and Gauss for three regular singularities.
  4. Derive the scaled variable instead of guessing it from notation.
  5. Declare the exact local or asymptotic bases, their branches, and their sectors.
  6. Check a Wronskian and one overlap, differential-equation, or monodromy identity.
  7. Record resonant, polynomial, and degenerate parameter loci before taking limits.

This workflow selects the smallest model that retains the feature being studied. It also makes clear when the general or confluent Heun equation is genuinely needed.

PageNew question
Canonical Local ModelsWhich local geometry selects Airy, Bessel, Weber, or Gauss?
The General Heun EquationHow are the standard and normal forms normalized?
Accessory Parameters and Four-Point GeometryWhat global freedom appears at four regular singularities?
The Confluence HierarchyHow do HeunG, HeunC, HeunD, HeunB, and HeunT differ?
Canonical Local and Asymptotic BasesWhich basis belongs to each singular point or sector?
Möbius, Gauge, Discrete, and Confluence TransformationsWhich operations preserve the equation class, and which are singular limits?
Parameter Crosswalks among Common ConventionsHow do mathematical, physical, and software conventions translate?
Polynomial, Algebraic, and Quasi-Exactly Solvable SectorsWhen do polynomial, algebraic, or quasi-exact solutions occur?

Calling a turning point singular. A zero of a normal-form potential is where a WKB basis fails, not necessarily where the exact ODE coefficients are singular. Airy’s finite turning point is ordinary.

Naming a function without its convention. Weber functions alone have several parameter conventions, and a symbol such as U(a,z)U(a,z) is not the same parameterization as Dν(z)D_\nu(z). State the differential equation first.

Dropping the scaling gauge. A coordinate change normally generates a first derivative. The compensating half-density affects Wronskians and boundary normalization.

Turning a local model into a global spectrum. Local decay or recessiveness becomes a spectral condition only after both endpoint conditions, the operator domain, and the parameter map have been supplied.

Let

2ψ(z)=[κ(zz0)+β(zz0)2]ψ(z),κ0.\hbar^2\psi''(z) = \left[ \kappa(z-z_0) + \beta(z-z_0)^2 \right]\psi(z), \qquad \kappa\neq0.

Find the scaled coordinate that makes the linear term exactly Airy, and determine the order of the quadratic correction for bounded scaled coordinate as 0\hbar\to0.

Solution

Set

ξ=κ1/3zz02/3,zz0=2/3κ1/3ξ.\xi = \kappa^{1/3} \frac{z-z_0}{\hbar^{2/3}}, \qquad z-z_0 = \hbar^{2/3}\kappa^{-1/3}\xi.

Since

 ⁣d2 ⁣dz2=κ2/34/3 ⁣d2 ⁣dξ2,\frac{\dd^2}{\dd z^2} = \kappa^{2/3}\hbar^{-4/3} \frac{\dd^2}{\dd\xi^2},

division by κ2/32/3\kappa^{2/3}\hbar^{2/3} gives

 ⁣d2ψ ⁣dξ2=[ξ+2/3βκ4/3ξ2]ψ.\frac{\dd^2\psi}{\dd\xi^2} = \left[ \xi + \hbar^{2/3} \frac{\beta}{\kappa^{4/3}} \xi^2 \right]\psi.

Thus the correction is O(2/3)O(\hbar^{2/3}) on bounded ξ\xi-sets. The branch of κ1/3\kappa^{1/3} fixes the rotation of the Airy sectors.

Starting from Bessel’s equation, set u(z)=z1/2y(z)u(z)=z^{1/2}y(z). Derive the normal-form equation and recover the exponents of uu at zero. For real ν0\nu\geq0, determine when both local branches belong to L2((0,ε), ⁣dz)L^2((0,\varepsilon),\dd z).

Solution

The standard Liouville substitution for y+z1y+(1ν2z2)y=0y''+z^{-1}y'+(1-\nu^2z^{-2})y=0 is u=exp(12z1 ⁣dz)y=z1/2yu=\exp(\tfrac12\int z^{-1}\dd z)y=z^{1/2}y. Direct substitution gives

u+[1ν214z2]u=0.u'' + \left[ 1-\frac{\nu^2-\tfrac14}{z^2} \right]u =0.

Its indicial equation is

ρ(ρ1)(ν214)=0,\rho(\rho-1) -\left( \nu^2-\frac14 \right) =0,

so

ρ±=12±ν.\rho_\pm=\frac12\pm\nu.

The shift by 1/21/2 is exactly the exponent carried by the square-root gauge. For ν>0\nu>0 the two branches behave as z1/2+νz^{1/2+\nu} and z1/2νz^{1/2-\nu}. The first is always square-integrable, whereas the second is square-integrable exactly when

12ν>1,that is,ν<1.1-2\nu>-1, \qquad\text{that is,}\qquad \nu<1.

At ν=0\nu=0, both z1/2z^{1/2} and the resonant branch z1/2logzz^{1/2}\log z are square-integrable. Thus the endpoint is limit-circle for 0ν<10\leq\nu<1 and limit-point for ν1\nu\geq1.

Use

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\bigl((1-\nu)/2\bigr) },\\ D_\nu'(0) &= -\frac{ 2^{(\nu+1)/2}\sqrt{\pi} }{ \Gamma(-\nu/2) } \end{aligned}

to compute Wr[Dν(z),Dν(z)]\Wr[D_\nu(z),D_\nu(-z)]. Then recover the two-sided oscillator quantization condition.

Solution

Because

 ⁣d ⁣dzDν(z)=Dν(z),\frac{\dd}{\dd z}D_\nu(-z) = -D_\nu'(-z),

evaluation at zero gives

Wr[Dν(z),Dν(z)]z=0=2Dν(0)Dν(0).\Wr \left[ D_\nu(z),D_\nu(-z) \right]_{z=0} = -2D_\nu(0)D_\nu'(0).

Substitution of the two special values and the duplication formula for gamma yield

Wr[Dν(z),Dν(z)]=2πΓ(ν).\Wr \left[ D_\nu(z),D_\nu(-z) \right] = \frac{\sqrt{2\pi}}{\Gamma(-\nu)}.

The Wronskian is constant because the Weber equation has no first-derivative term. It vanishes precisely when ν-\nu is a nonpositive integer:

ν=nZ0.\nu=n\in\mathbb Z_{\ge0}.

Using ν+12=E/(2α)\nu+\tfrac12=\mathcal E/(2\alpha\hbar) gives

En=(2n+1)α.\mathcal E_n=(2n+1)\alpha\hbar.

Let E0E\neq0 in y=(z2/4E)yy''=(z^2/4-E)y and choose branches with (E1/6)3=E(E^{1/6})^3=\sqrt E. Near z+=2Ez_+=2\sqrt E, set

s=E1/6(zz+).s=E^{1/6}(z-z_+).

Derive the scaled equation and explain why this Airy reduction does not cover both turning points uniformly.

Solution

Write z=2E+E1/6sz=2\sqrt E+E^{-1/6}s. Then

z24E=E1/3s+14E1/3s2,\frac{z^2}{4}-E = E^{1/3}s + \frac14E^{-1/3}s^2,

while  ⁣d2/ ⁣dz2=E1/3 ⁣d2/ ⁣ds2\dd^2/\dd z^2=E^{1/3}\dd^2/\dd s^2. Therefore

 ⁣d2y ⁣ds2=[s+s24E2/3]y.\frac{\dd^2y}{\dd s^2} = \left[ s+\frac{s^2}{4E^{2/3}} \right]y.

For bounded ss and large E|E| in a fixed parameter sector, the second term is small and the leading equation is Airy. The other turning point is at z=2Ez_-=-2\sqrt E, whose distance from z+z_+ is 4E4\sqrt E; it escapes to infinite ss-distance in this local scaling. Weber, rather than one Airy chart, is the uniform model that retains the pair.

Derive the exponents of the Gauss equation at 00, 11, and \infty, and verify the Fuchs relation. Then reconstruct (a,b,c)(a,b,c) from

(θ0,θ1,θ)=(13,14,15)\left( \theta_0,\theta_1,\theta_\infty \right) = \left( \frac13,\frac14,\frac15 \right)

using the exponent ordering on this page.

Solution

At zero, substituting yzρy\sim z^\rho gives

ρ(ρ+c1)=0,\rho(\rho+c-1)=0,

so the exponents are 00 and 1c1-c. At one, put t=1zt=1-z and obtain

ρ(ρ+a+bc)=0,\rho(\rho+a+b-c)=0,

so the exponents are 00 and cabc-a-b.

At infinity, substitute yzρy\sim z^{-\rho}. The leading balance gives

(ρa)(ρb)=0,(\rho-a)(\rho-b)=0,

so the exponents in the local coordinate 1/z1/z are aa and bb. Their sum is

(1c)+(cab)+a+b=1,(1-c)+(c-a-b)+a+b=1,

as required for a second-order Fuchsian equation with three singular points on the sphere.

The inverse parameter map gives

c=23,a=12(11314+15)=37120,b=12(1131415)=13120.\begin{aligned} c&=\frac23,\\ a&= \frac12 \left( 1-\frac13-\frac14+\frac15 \right) = \frac{37}{120},\\ b&= \frac12 \left( 1-\frac13-\frac14-\frac15 \right) = \frac{13}{120}. \end{aligned}

Here each prefactor 12\tfrac12 multiplies the following parenthesis. Reordering a local exponent pair flips the corresponding θj\theta_j and therefore changes this displayed parameterization.

6. Show that the oscillator zeros are simple

Section titled “6. Show that the oscillator zeros are simple”

Let

F(ν)=2πΓ(ν).F(\nu) = -\frac{\sqrt{2\pi}}{\Gamma(-\nu)}.

Show that each zero ν=nZ0\nu=n\in\mathbb Z_{\geq0} is simple and compute F(n)F'(n).

Solution

The residue of gamma at z=nz=-n is (1)n/n!(-1)^n/n!, so

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

Therefore

1Γ(ν)(1)n+1n!(νn),\frac1{\Gamma(-\nu)} \sim (-1)^{n+1}n!(\nu-n),

and hence

F(n)=(1)n2πn!0.F'(n) = (-1)^n\sqrt{2\pi}\,n! \neq0.

The reciprocal-gamma quantization zeros are all simple. In operator language, this agrees with the simplicity of the one-dimensional harmonic oscillator spectrum.

Choose the first canonical model to test in each situation:

  1. one simple zero of Q(z)Q(z) in 2y=Qy\hbar^2y''=Qy;

  2. a radial endpoint satisfying

    u=[ν214r2+O(1)]u;u'' = \left[ \frac{\nu^2-\tfrac14}{r^2} + O(1) \right]u;
  3. two turning points whose separation tends to zero;

  4. four distinct regular singularities on the sphere.

Solution
  1. Airy captures the simple turning point after an 2/3\hbar^{2/3} scaling.
  2. Bessel captures the inverse-square endpoint and its two Frobenius powers.
  3. Weber is the uniform quadratic model for a coalescing pair.
  4. None of the four models on this page is generically sufficient. Three regular singularities are Gauss-rigid, but the fourth introduces a cross-ratio and an accessory parameter. The general Heun equation is the next model.

In every case, “first model” means the smallest equation retaining the local or global datum of interest. Establishing an exact equivalence requires checking the full transformed equation, not only its leading singular term.

  • NIST DLMF §9.2 and §9.7 give the Airy equation, Wronskians, connection formulae, and asymptotics; §2.8(iii), (vi) treats simple and coalescing turning points, and §12.16 develops parabolic-cylinder uniform approximations.
  • NIST DLMF §10.2, §10.4, §10.5, and §10.8 give the Bessel definitions, connection identities, Wronskians, and logarithmic limiting cases; §10.17 gives the large-argument bases.
  • NIST DLMF §12.2, §12.7, and §12.9 fix the parabolic-cylinder conventions, special values, Hermite specialization, and sectorial asymptotics; §2.7(ii) fixes the irregular-rank convention.
  • NIST DLMF §18.39(i) gives the harmonic oscillator’s L2L^2 realization and spectrum; §1.18 reviews self-adjoint second-order differential operators and endpoint classification.
  • NIST DLMF §15.10 gives the Gauss equation, local bases, and connection formulae; §15.11 gives the reduction of a three-singularity Fuchsian equation to Gauss form.
  • NIST DLMF §31.2(i) identifies the singularity and accessory parameters of the four-point Heun equation.
  • F. W. J. Olver, Asymptotics and Special Functions, A K Peters, 1997, develops turning-point transformations and uniform Airy and parabolic-cylinder approximations.
  • N. M. Temme, Special Functions: An Introduction to the Classical Functions of Mathematical Physics, Wiley, 1996, provides a normalization-conscious account of the four model families.
  • K. Iwasaki, H. Kimura, S. Shimomura, and M. Yoshida, From Gauss to Painlevé, Vieweg, 1991, develops the rigid three-point equation and the transition to accessory-parameter and monodromy-deformation problems.