Skip to content

Accessory Parameters and Four-Point Fuchsian Geometry

Four regular singular points introduce two freedoms that are easy to conflate. Their marked sphere has one position modulus, the cross-ratio aa. After the positions and local exponent differences are fixed, the normal-form equation still has one accessory coefficient, which we denote by cac_a. Thus aa selects the four-punctured geometry, while cac_a selects a projective connection over that geometry.

This page derives both statements directly. The result explains why the three-point hypergeometric equation is rigid, why the general Heun equation is not, and what later monodromy, isomonodromy, and spectral constructions must actually determine.

Three points are rigid; four points have a cross-ratio

Section titled “Three points are rigid; four points have a cross-ratio”

A Möbius transformation is fixed uniquely by the images of three distinct points. Given an ordered quadruple

(x0,x1,xa,x)P1,\left( x_0,x_1,x_a,x_\infty \right) \subset\mathbb P^1,

the map

m(z)=(zx0)(x1x)(zx)(x1x0)m(z) = \frac{ (z-x_0)(x_1-x_\infty) }{ (z-x_\infty)(x_1-x_0) }

sends x0,x1,xx_0,x_1,x_\infty to 0,1,0,1,\infty. The fourth image is

a=m(xa)=(xax0)(x1x)(xax)(x1x0).a=m(x_a) = \frac{ (x_a-x_0)(x_1-x_\infty) }{ (x_a-x_\infty)(x_1-x_0) }.

If one of the points is already at infinity, these formulas are understood by taking the corresponding limit. Distinctness gives

aP1{0,1,}.a\in\mathbb P^1\setminus\{0,1,\infty\}.

Consequently the moduli space of four ordered marked points on the sphere is

M0,4P1{0,1,}.\mathcal M_{0,4} \simeq \mathbb P^1\setminus\{0,1,\infty\}.

The three omitted values are collision boundary points—boundary divisors in the compactified moduli space: a0a\to0, a1a\to1, or aa\to\infty makes two marked points meet in this coordinate chart. They are boundary limits, not ordinary values of the four-distinct-point Heun equation.

The value of the cross-ratio depends on which puncture is called 00, 11, aa, or \infty. Permuting the four labels produces, generically, the six values

a,1a,1a,11a,aa1,a1a.\begin{gathered} a, \qquad 1-a, \qquad \frac1a,\\ \frac1{1-a}, \qquad \frac{a}{a-1}, \qquad \frac{a-1}{a}. \end{gathered}

The action of the permutation group S4\mathfrak S_4 on cross-ratios factors through

S4/V4S3,\mathfrak S_4/V_4\simeq\mathfrak S_3,

where V4V_4 is the Klein four subgroup that leaves a cross-ratio unchanged. The orbit has fewer than six distinct values at the harmonic points {1,12,2}\{-1,\tfrac12,2\} and at the equianharmonic points satisfying a2a+1=0a^2-a+1=0.

For an unlabeled punctured sphere, the six generic values describe the same geometry. For a differential equation, the labels also carry exponent and basis data, so a relabeling must transform those data together with aa.

Consider the normal equation

ψ(z)+T(z)ψ(z)=0.\psi''(z)+T(z)\psi(z)=0.

Under a coordinate change z=f(w)z=f(w), remove the induced first derivative by setting

ψ~(w)=(f(w))1/2ψ(f(w)).\widetilde\psi(w) = \bigl(f'(w)\bigr)^{-1/2} \psi\bigl(f(w)\bigr).

Then

ψ~(w)+T~(w)ψ~(w)=0,\widetilde\psi''(w) + \widetilde T(w)\widetilde\psi(w) =0,

with

T~(w)=(f(w))2T(f(w))+12{f,w},\widetilde T(w) = \bigl(f'(w)\bigr)^2T\bigl(f(w)\bigr) + \frac12\{f,w\},

where

{f,w}=f(w)f(w)32(f(w)f(w))2\{f,w\} = \frac{f'''(w)}{f'(w)} - \frac32 \left( \frac{f''(w)}{f'(w)} \right)^2

is the Schwarzian derivative. This inhomogeneous transformation law is what makes TT a projective connection rather than an ordinary quadratic differential. For a Möbius map, {f,w}=0\{f,w\}=0, so the coefficient transforms homogeneously.

The double-pole term nevertheless feeds into the transformed simple-pole residue. If zi=f(wi)z_i=f(w_i) and both coordinates are finite, then

c~i=f(wi)ci+Δif(wi)f(wi).\widetilde c_i = f'(w_i)c_i + \Delta_i \frac{f''(w_i)}{f'(w_i)}.

Thus an individual accessory residue transforms affinely, not as a scalar. If a puncture crosses infinity, the same statement must be applied in its local chart.

There is a second way to see the same structure. For two independent solutions, the developing ratio

F(z)=ψ1(z)ψ2(z)F(z)=\frac{\psi_1(z)}{\psi_2(z)}

satisfies

{F,z}=2T(z).\{F,z\}=2T(z).

Analytic continuation changes the basis (ψ1,ψ2)(\psi_1,\psi_2) linearly and therefore changes FF by a Möbius transformation. The coefficient TT packages the corresponding projective monodromy problem.

Infinity leaves n − 3 accessory coefficients

Section titled “Infinity leaves n − 3 accessory coefficients”

Place one of n3n\geq3 regular singular points at infinity and denote the other n1n-1 positions by z1,,zn1z_1,\ldots,z_{n-1}. With the centered local coefficients

Δj=1θj24\Delta_j = \frac{1-\theta_j^2}{4}

fixed, the most general rational normal-form coefficient with no other finite poles is

T(z)=j=1n1[Δj(zzj)2+cjzzj].T(z) = \sum_{j=1}^{n-1} \left[ \frac{\Delta_j}{(z-z_j)^2} + \frac{c_j}{z-z_j} \right].

The Δj\Delta_j determine the two local powers. The simple-pole residues cjc_j are the candidate accessory coefficients. Expanding at infinity gives

T(z)=1zj=1n1cj+1z2j=1n1(Δj+zjcj)+O(z3).\begin{aligned} T(z) &= \frac1z\sum_{j=1}^{n-1}c_j\\ &\quad+ \frac1{z^2} \sum_{j=1}^{n-1} \left( \Delta_j+z_jc_j \right) + O(z^{-3}). \end{aligned}

For infinity to be regular singular with prescribed coefficient Δ\Delta_\infty, the residues must obey

j=1n1cj=0,\sum_{j=1}^{n-1}c_j=0,

and

j=1n1(Δj+zjcj)=Δ.\sum_{j=1}^{n-1} \left( \Delta_j+z_jc_j \right) = \Delta_\infty.

The next Laurent coefficient is not constrained to vanish. In the local coordinate w=1/zw=1/z, it is the simple-pole residue at infinity:

c=j=1n1(2zjΔj+zj2cj).c_\infty = \sum_{j=1}^{n-1} \left( 2z_j\Delta_j+z_j^2c_j \right).

These are two independent linear constraints on n1n-1 residues. Therefore the number of free accessory coefficients is

(n1)2=n3.(n-1)-2=n-3.

This count holds with the singular positions and exponent differences fixed:

Number of regular singular pointsPosition moduliAccessory coefficientsGeneric scalar model
330000Gauss hypergeometric
441111General Heun
n3n\geq3n3n-3n3n-3General second-order Fuchsian

The first n3n-3 comes from marked-sphere geometry; the second comes from the coefficient of the projective connection. Equal dimensions do not make these two kinds of data interchangeable.

Now specialize to

(z0,z1,za,z)=(0,1,a,).(z_0,z_1,z_a,z_\infty) = (0,1,a,\infty).

Write

T(z)=Δ0z2+Δ1(z1)2+Δa(za)2+c0z+c1z1+caza.\begin{aligned} T(z) &= \frac{\Delta_0}{z^2} + \frac{\Delta_1}{(z-1)^2} + \frac{\Delta_a}{(z-a)^2}\\ &\quad+ \frac{c_0}{z} + \frac{c_1}{z-1} + \frac{c_a}{z-a}. \end{aligned}

The two conditions at infinity are

c0+c1+ca=0c_0+c_1+c_a=0

and

Δ0+Δ1+Δa+c1+aca=Δ.\Delta_0+\Delta_1+\Delta_a + c_1+ac_a = \Delta_\infty.

Define

Λ=ΔΔ0Δ1Δa.\Lambda = \Delta_\infty-\Delta_0-\Delta_1-\Delta_a.

Choosing cac_a as the free coordinate gives

c0=Λ+(a1)ca,c1=Λaca.\begin{aligned} c_0&=-\Lambda+(a-1)c_a,\\ c_1&=\Lambda-ac_a. \end{aligned}

Substitution recovers the compact form from the previous page:

T(z)=Δ0z2+Δ1(z1)2+Δa(za)2+Λz(z1)+a(a1)caz(z1)(za).\begin{aligned} T(z) &= \frac{\Delta_0}{z^2} + \frac{\Delta_1}{(z-1)^2} + \frac{\Delta_a}{(z-a)^2}\\ &\quad+ \frac{\Lambda}{z(z-1)} + \frac{a(a-1)c_a}{z(z-1)(z-a)}. \end{aligned}

The standard Heun coordinate qq, the shifted compact coordinate κH\kappa_{\mathrm H}, and the residue cac_a are related by

κH=qγ2(aδ+ϵ),\kappa_{\mathrm H} = q-\frac{\gamma}{2} \left( a\delta+\epsilon \right),

and

ca=aΛκHa(a1).c_a = \frac{a\Lambda-\kappa_{\mathrm H}}{a(a-1)}.

The constrained residues may equivalently be read from κH\kappa_{\mathrm H}:

c0=κHa,c1=ΛκH1a.c_0=-\frac{\kappa_{\mathrm H}}a, \qquad c_1 = \frac{\Lambda-\kappa_{\mathrm H}}{1-a}.

Equivalently,

q=γ2(aδ+ϵ)+aΛa(a1)ca.q = \frac{\gamma}{2} \left( a\delta+\epsilon \right) + a\Lambda-a(a-1)c_a.

All three are legitimate accessory coordinates after a convention is fixed. They are not numerically interchangeable: changing the scalar gauge or the chosen partial-fraction basis shifts and rescales the displayed coordinate.

Fix aa and all four Δj\Delta_j. If the accessory residue changes by η\eta, then

(Tca+ηTca)dz2=ηωa,ωa=a(a1)dz2z(z1)(za).\begin{aligned} \left( T_{c_a+\eta}-T_{c_a} \right)dz^2 &= \eta\,\omega_a,\\ \omega_a &= \frac{ a(a-1)\,dz^2 }{ z(z-1)(z-a) }. \end{aligned}

The quadratic differential ωa\omega_a has at most a simple pole at each of 0,1,a,0,1,a,\infty. It is the unique such differential up to scale. More generally, if D\mathscr D is the divisor of nn marked points and KP1K_{\mathbb P^1} is the canonical bundle, then

H0(P1,KP12(D))H^0 \left( \mathbb P^1, K_{\mathbb P^1}^{\otimes2}(\mathscr D) \right)

has dimension n3n-3. The projective connections with fixed double-pole data form an affine space modeled on this vector space.

“Affine” matters. The difference of two such connections is an honest quadratic differential, but an individual projective connection has no preferred zero until a reference convention is chosen. This is the geometric reason that one source’s accessory parameter can differ from another’s by an exponent-dependent shift.

The cross-ratio a parametrizes the four-punctured sphere, while a vertical affine fiber parametrized by c_a selects projective connections with the same local exponent data.

The position modulus aM0,4a\in\mathcal M_{0,4} labels the four-punctured sphere. With the local exponent differences fixed, cac_a moves along the one-dimensional affine fiber of projective connections above that point. The axes are schematic: both coordinates are complex, and the drawing does not assume 0<a<10<a<1.

This picture is kinematic. Holding cac_a fixed while aa moves generally changes holonomy, while one scalar monodromy or spectral condition may select nonlinear branches ca(a)c_a(a).

For a nonresonant normal-form singularity with exponent difference θj\theta_j, the local powers are

(zzj)(1±θj)/2.(z-z_j)^{(1\pm\theta_j)/2}.

The lift naturally induced by these normal-form powers has eigenvalues

e±πiθj-\ee^{\pm\pi\ii\theta_j}

and trace

trMj=2cos(πθj).\operatorname{tr}M_j = -2\cos(\pi\theta_j).

These local conjugacy data depend on θj\theta_j, not on cac_a. By contrast, relative data such as

tr(M0M1),tr(M1Ma),tr(MaM0)\operatorname{tr}(M_0M_1), \qquad \operatorname{tr}(M_1M_a), \qquad \operatorname{tr}(M_aM_0)

are global and generally vary with the accessory coefficient.

With the ordered relation

M0MaM1M=I,M_0M_aM_1M_\infty=I,

the generic fixed-local-class character variety is a complex surface. At fixed aa, the one-dimensional accessory line generically maps by holonomy to a curve on that surface. Allowing both aa and cac_a to vary gives a two-dimensional coefficient family. This dimension match does not imply that the holonomy map is globally one-to-one or onto.

Resonance can expose the accessory locally

Section titled “Resonance can expose the accessory locally”

The simple-pole residue never enters the indicial equation, but at an integer exponent difference it can enter the later compatibility condition that decides whether a logarithm occurs. A concrete Heun family makes this visible. Take

a=2,α=β=1,γ=δ=2,ϵ=1.a=2, \qquad \alpha=\beta=1, \qquad \gamma=\delta=2, \qquad \epsilon=-1.

The Fuchs relation holds, and

y+(2z+2z11z2)y+zqz(z1)(z2)y=0.\begin{aligned} y'' &+ \left( \frac2z+\frac2{z-1}-\frac1{z-2} \right)y'\\ &+ \frac{z-q}{z(z-1)(z-2)}y =0. \end{aligned}

At z=2z=2 the exponents are 00 and 22. Put t=z2t=z-2. The two coefficient functions have expansions

p(t)=1t+3+O(t)p(t) = -\frac1t+3+O(t)

and

r(t)=2q2t+3q44+O(t).r(t) = \frac{2-q}{2t} + \frac{3q-4}{4} + O(t).

For y=b0+b1t+b2t2+y=b_0+b_1t+b_2t^2+\cdots, the coefficient of t1t^{-1} gives

b1=2q2b0.b_1=\frac{2-q}{2}b_0.

At the resonant step the b2b_2 terms cancel. The remaining compatibility condition is

(q3)(q4)4b0=0.\frac{(q-3)(q-4)}4\,b_0=0.

Therefore q=3q=3 and q=4q=4 make the puncture apparent: both standard-form solutions are holomorphic and its local monodromy is II. For every other qq, a logarithm occurs and the local monodromy has a nontrivial unipotent part.

The same conclusion in normal-form coordinates is especially instructive:

(Δ0,Δ1,Δa,Δ)=(0,0,34,14),Λ=1,κH=q3,ca=5q2.\begin{gathered} \left( \Delta_0,\Delta_1,\Delta_a,\Delta_\infty \right) = \left( 0,0,-\frac34,\frac14 \right),\\ \Lambda=1, \qquad \kappa_{\mathrm H}=q-3, \qquad c_a=\frac{5-q}{2}. \end{gathered}

Apparency occurs at ca=1c_a=1 or ca=1/2c_a=1/2. By contrast, ca=0c_a=0 occurs at q=5q=5 and is not apparent. The puncture is not ordinary either: its double pole remains. In the normal determinant-one lift the log-free local monodromy is I-I; the Liouville gauge converts it to II in standard form, and both are projectively trivial.

DatumWhat fixes it?
Marked-sphere geometryThe cross-ratio aa, up to relabeling
Local monodromy eigenvaluesThe exponent differences θj\theta_j
Resonant logarithm or apparencyA compatibility condition that can involve the accessory coordinate
Scalar differential equation with those dataOne accessory coordinate, such as cac_a or qq
Global monodromy representationAnalytic continuation of that equation
Distinguished or spectral accessory valuesAdditional monodromy, regularity, apparency, or boundary conditions

Here cac_a labels the full affine family of projective connections with the stated polar data. In the uniformization literature, “the accessory parameter problem” often means selecting the special value whose projective monodromy is Fuchsian. Isomonodromic, conformal-block, and spectral problems impose different global selection rules, developed in later chapters.

The accessory parameter is therefore not “the monodromy.” It is a coefficient coordinate whose dependence on monodromy is nonlinear; an inverse monodromy problem may also have several branches. At resonance, the exponent difference fixes the eigenvalues but not by itself the logarithmic or Jordan data.

Confusing the base with the fiber. The cross-ratio aa moves a puncture; cac_a changes the equation while the punctures stay fixed. Both are global data, but they answer different questions.

Calling zero accessory canonical. The equation ca=0c_a=0 depends on the chosen coordinate and reference projective connection. It neither removes the fourth puncture nor implies trivial monodromy.

Calling an apparent point ordinary. In this book, an apparent point has two holomorphic scalar solutions and local monodromy II in the stated standard-form gauge. After the multivalued Liouville gauge, the natural normal-form lift may instead be I-I; its projective monodromy is still trivial. An ordinary point additionally requires the coefficient poles to disappear in the chosen scalar gauge.

Forgetting that punctures are labeled. The six anharmonic values describe one generic unlabeled configuration, but exponent and basis labels must be permuted with the points.

Using the wrong number of constraints at infinity. A marked regular singularity at infinity imposes two conditions on the finite residues. An ordinary infinity imposes three.

Equating local traces with global monodromy. Fixed local exponents fix individual conjugacy classes only in the nonresonant generic setting. Products of monodromy matrices and connection data still depend on the accessory coefficient.

Verify that

m(z)=(zx0)(x1x)(zx)(x1x0)m(z) = \frac{ (z-x_0)(x_1-x_\infty) }{ (z-x_\infty)(x_1-x_0) }

sends (x0,x1,x)(x_0,x_1,x_\infty) to (0,1,)(0,1,\infty). Compute a=m(xa)a=m(x_a) for

(x0,x1,xa,x)=(0,2,3,).(x_0,x_1,x_a,x_\infty)=(0,2,3,\infty).
Solution

Substitution gives m(x0)=0m(x_0)=0. At z=x1z=x_1, numerator and denominator are the same product, so m(x1)=1m(x_1)=1. The denominator vanishes at xx_\infty, while the numerator is nonzero because the points are distinct, so m(x)=m(x_\infty)=\infty.

When x=x_\infty=\infty, divide the factors involving xx_\infty before taking the limit:

limxx1xzx=1.\lim_{x_\infty\to\infty} \frac{x_1-x_\infty}{z-x_\infty} =1.

Therefore the example has

m(z)=z2,a=m(3)=32.m(z)=\frac z2, \qquad a=m(3)=\frac32.

2. Count and reconstruct the accessory residues

Section titled “2. Count and reconstruct the accessory residues”

For n3n\geq3 regular singularities with n1n-1 finite positions, expand the normal-form coefficient at infinity and count the free residues. Then specialize to 00, 11, aa, and \infty, solve for c0,c1c_0,c_1 in terms of cac_a, and recover the compact simple-pole term.

Solution

Use

1zzj=1z+zjz2+O(z3)\frac1{z-z_j} = \frac1z+\frac{z_j}{z^2}+O(z^{-3})

and

1(zzj)2=1z2+O(z3).\frac1{(z-z_j)^2} = \frac1{z^2}+O(z^{-3}).

Then

T(z)=1zjcj+1z2j(Δj+zjcj)+O(z3).\begin{aligned} T(z) &= \frac1z\sum_jc_j\\ &\quad+ \frac1{z^2} \sum_j \left( \Delta_j+z_jc_j \right) + O(z^{-3}). \end{aligned}

Prescribing a regular singularity at infinity gives

jcj=0,j(Δj+zjcj)=Δ.\sum_jc_j=0, \qquad \sum_j \left( \Delta_j+z_jc_j \right) = \Delta_\infty.

Thus n1n-1 residues obey two independent constraints, leaving n3n-3. For finite positions 0,1,a0,1,a, these equations become

c0+c1+ca=0c_0+c_1+c_a=0

and

c1+aca=ΔΔ0Δ1Δa=Λ.c_1+ac_a = \Delta_\infty-\Delta_0-\Delta_1-\Delta_a = \Lambda.

Therefore

c1=Λaca,c0=Λ+(a1)ca.c_1=\Lambda-ac_a, \qquad c_0=-\Lambda+(a-1)c_a.

Finally,

c0z+c1z1+caza=Λz(z1)+a(a1)caz(z1)(za).\begin{aligned} \frac{c_0}{z} + \frac{c_1}{z-1} + \frac{c_a}{z-a} &= \frac{\Lambda}{z(z-1)}\\ &\quad+ \frac{a(a-1)c_a}{z(z-1)(z-a)}. \end{aligned}

At fixed aa and exponent data, start from

ca=aΛκHa(a1),κH=qγ2(aδ+ϵ).c_a = \frac{a\Lambda-\kappa_{\mathrm H}}{a(a-1)}, \qquad \kappa_{\mathrm H} = q-\frac{\gamma}{2}(a\delta+\epsilon).

Derive ca/q\partial c_a/\partial q, reconstruct qq from cac_a, and compute T/q\partial T/\partial q.

Solution

Only κH\kappa_{\mathrm H} depends on qq, with unit derivative. Hence

caq=1a(a1).\frac{\partial c_a}{\partial q} = -\frac1{a(a-1)}.

Solving the affine relation for qq gives

q=γ2(aδ+ϵ)+aΛa(a1)ca.q = \frac{\gamma}{2} \left( a\delta+\epsilon \right) + a\Lambda-a(a-1)c_a.

The qq-dependent part of the normal coefficient is

T(z)κHz(z1)(za).T(z) \supset \frac{-\kappa_{\mathrm H}}{z(z-1)(z-a)}.

Therefore

Tq=1z(z1)(za).\frac{\partial T}{\partial q} = -\frac1{z(z-1)(z-a)}.

This derivative is invariant under exponent-dependent affine shifts of the chosen accessory origin, but its normalization still depends on the coordinate convention.

Starting from the two normal-form powers

(zzj)(1±θj)/2,(z-z_j)^{(1\pm\theta_j)/2},

derive the eigenvalues and trace of the determinant-one local monodromy lift. Explain why nonintegral θj\theta_j fixes its semisimple conjugacy class, whereas integral θj\theta_j does not determine the logarithmic Jordan part.

Solution

One counterclockwise turn multiplies the two powers by

exp[2πi1±θj2]=e±πiθj.\exp \left[ 2\pi\ii\frac{1\pm\theta_j}{2} \right] = -\ee^{\pm\pi\ii\theta_j}.

Their product is one, so this is a determinant-one lift. Its trace is

trMj=2cos(πθj).\operatorname{tr}M_j = -2\cos(\pi\theta_j).

If θjZ\theta_j\notin\mathbb Z, the eigenvalues are distinct, so they determine a semisimple SL(2,C)SL(2,\mathbb C) conjugacy class. If θjZ\theta_j\in\mathbb Z, the eigenvalues coincide. A log-free basis gives Mj=±IM_j=\pm I in this lift, whereas a logarithmic solution gives a nontrivial Jordan matrix with the same trace. The exponent difference alone cannot distinguish these cases.

In the general Heun equation, set ϵ=1\epsilon=-1 and define

A=aαβq.A=a\alpha\beta-q.

Put t=zat=z-a and y=b0+b1t+b2t2+y=b_0+b_1t+b_2t^2+\cdots. Show that the no-log compatibility condition at the exponent difference 22 is

0=A2+[γ(a1)+δa(2a1)]A+αβa(a1).\begin{aligned} 0 ={}& A^2\\ &+ \left[ \gamma(a-1)+\delta a-(2a-1) \right]A\\ &+ \alpha\beta a(a-1). \end{aligned}

Then recover the apparent values for a=2a=2, α=β=1\alpha=\beta=1, and γ=δ=2\gamma=\delta=2.

Solution

Write

D0=a(a1),D1=2a1.D_0=a(a-1), \qquad D_1=2a-1.

The coefficient functions have the local expansions

p(t)=1t+(γa+δa1)+O(t)p(t) = -\frac1t + \left( \frac\gamma a+\frac\delta{a-1} \right) + O(t)

and

r(t)=AD0t+αβD0AD1D02+O(t).r(t) = \frac{A}{D_0t} + \frac{\alpha\beta}{D_0} - \frac{AD_1}{D_0^2} + O(t).

The coefficient of t1t^{-1} in the differential equation gives

b1+AD0b0=0,-b_1+\frac{A}{D_0}b_0=0,

so b1=Ab0/D0b_1=Ab_0/D_0. At order t0t^0, the two contributions containing b2b_2 cancel. Dividing by b0b_0 and multiplying by D02D_0^2 gives

0=A2+[γ(a1)+δaD1]A+αβD0,\begin{aligned} 0 ={}& A^2\\ &+ \left[ \gamma(a-1)+\delta a-D_1 \right]A\\ &+ \alpha\beta D_0, \end{aligned}

which is the required condition. For the stated specialization, A=2qA=2-q, D0=2D_0=2, and the coefficient of AA is 33. Hence

(2q)2+3(2q)+2=(q3)(q4)=0.(2-q)^2+3(2-q)+2 = (q-3)(q-4) =0.

Thus q=3q=3 and q=4q=4 are exactly the apparent values. In either case the smaller-exponent solution is holomorphic, and the larger-exponent Frobenius solution is already holomorphic.

For the same resonant family, compare:

  1. the apparent values;
  2. the value at which ca=0c_a=0;
  3. the condition for the pole at z=az=a to disappear from the standard Heun equation.

Explain why these are different notions.

Solution

For this family,

ca=5q2.c_a=\frac{5-q}{2}.

The apparent values q=3q=3 and q=4q=4 therefore correspond to

ca=1andca=12.c_a=1 \qquad\text{and}\qquad c_a=\frac12.

By contrast, ca=0c_a=0 occurs at q=5q=5. The resonant obstruction there is

(53)(54)4=120,\frac{(5-3)(5-4)}4=\frac12\ne0,

so a logarithm is present.

For a general Heun equation, removing the pole at z=az=a from the standard-form coefficients requires both

ϵ=0andq=aαβ.\epsilon=0 \qquad\text{and}\qquad q=a\alpha\beta.

The present family has ϵ=1\epsilon=-1, so the pole never disappears. In the book’s standard-form convention, apparency means two holomorphic scalar solutions and local monodromy II even though coefficient poles may remain. The equation ca=0c_a=0 merely removes one simple-pole residue in a chosen normal-form decomposition; an ordinary point requires the coefficient poles themselves to vanish.

Let D\mathscr D be the divisor of n3n\geq3 distinct points on P1\mathbb P^1. Use the genus-zero Riemann–Roch formula to compute

dimH0(P1,KP12(D)).\dim H^0 \left( \mathbb P^1, K_{\mathbb P^1}^{\otimes2}(\mathscr D) \right).

For n=4n=4, verify directly that ωa\omega_a has at most simple poles at all four punctures.

Solution

On P1\mathbb P^1,

degKP1=2.\deg K_{\mathbb P^1}=-2.

Therefore

deg[KP12(D)]=4+n.\deg \left[ K_{\mathbb P^1}^{\otimes2}(\mathscr D) \right] = -4+n.

For a line bundle of degree dd on P1\mathbb P^1,

h0=max{d+1,0}.h^0=\max\{d+1,0\}.

Hence, for n3n\geq3,

h0=n3.h^0=n-3.

For four points,

ωa=a(a1)dz2z(z1)(za)\omega_a = \frac{ a(a-1)\,dz^2 }{ z(z-1)(z-a) }

plainly has simple finite poles at 00, 11, and aa. Near infinity, set w=1/zw=1/z. Since dz2=w4dw2dz^2=w^{-4}dw^2 and the rational coefficient is a(a1)z3+O(z4)a(a-1)z^{-3}+O(z^{-4}), one obtains

ωa=[a(a1)w+O(1)]dw2.\omega_a = \left[ \frac{a(a-1)}w+O(1) \right]dw^2.

Thus infinity is also only a simple pole. The one-dimensional space is spanned by ωa\omega_a.

  • NIST Digital Library of Mathematical Functions, §1.13(iv) gives the Liouville–Schwarzian coordinate law; §31.14(i), equations 31.14.1–31.14.5, gives the general second-order Fuchsian equation and its accessory-parameter count; and §31.2(i)–(ii), equations 31.2.1–31.2.4, identifies aa and qq as the singularity and accessory parameters of the general Heun equation.
  • F. C. S. Brown, “Multiple zeta values and periods of moduli spaces M0,n\mathcal M_{0,n}, Annales scientifiques de l’École Normale Supérieure 42 (2009), 371–489, §2.1, pp. 381–382, equations (2.1)–(2.3), defines labeled pointed-sphere moduli, cross-ratio coordinates, and the effective anharmonic action.
  • R. S. Maier, “The 192 solutions of the Heun equation”, Mathematics of Computation 76 (2007), 811–843, Introduction and §2, equations (2.1)–(2.3), and §3, gives the n3n-3 accessory count and the Heun cross-ratio orbit in a normalized Fuchsian convention.
  • K. Iwasaki, H. Kimura, S. Shimomura, and M. Yoshida, From Gauss to Painlevé: A Modern Theory of Special Functions, Vieweg, 1991, develops Fuchsian equations, monodromy, and deformation geometry from the rigid hypergeometric case onward.
  • H. M. Farkas and I. Kra, Riemann Surfaces, 2nd ed., Springer, 1992, supplies the Möbius, cross-ratio, divisor, and Riemann–Roch background used here.
  • L. A. Takhtajan and P. G. Zograf, “Hyperbolic 2-spheres with conical singularities, accessory parameters and Kähler metrics on M0,n\mathcal M_{0,n}, Transactions of the American Mathematical Society 355 (2003), 1857–1867, Lemma 1, equations (5)–(7), relates Fuchsian accessory parameters to pointed-sphere moduli. Its equation uses u+12Tφu=0u''+\tfrac12T_\varphi u=0, so its printed residues differ by a factor of two from this page’s convention.
  • A. Ronveaux (ed.), Heun’s Differential Equations, Oxford University Press, 1995, Part A, records the canonical Heun equation, its transformations, and accessory-parameter conventions.