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Exact-WKB/GMN-Type Riemann–Hilbert Integral Equations

Page 2 inverted functional relations after choosing analytic strips and spectral divisors. This page begins from different data: Borel-summed Voros symbols, a fixed BPS chamber, and intersection-controlled jumps in the complex semiclassical-parameter plane. The result is a nonlinear Riemann–Hilbert equation whose logarithm looks TBA-like, but whose rays, kernel, discrete input, and output are not those of the ODE/IM equations.

Two normalizations must be kept separate. The full DDP-normalized GMN-type problem has paired asymptotics at ζ=0\zeta=0 and ζ=\zeta=\infty, an antipodal reality condition, and exponential damping at both ends of every BPS ray. Its conformal limit retains the exact-WKB drive exp(Zγ/)\exp(Z_\gamma/\hbar) and uses an origin-subtracted Cauchy kernel, but its far endpoint requires a new convergence hypothesis. On a distinguished Hitchin section this limit can have an oper interpretation, subject to further assumptions. Page 4 will ask when either construction can be identified with an ODE/IM TBA.

A fixed-chamber passport has independent analytic and discrete data

Section titled “A fixed-chamber passport has independent analytic and discrete data”

Let Γ\Gamma be a free abelian charge lattice equipped with an integer-valued skew pairing

γρ=ργ.\gamma\mathbin{\cdot}\rho = -\rho\mathbin{\cdot}\gamma.

The central charge is an additive map

Z:ΓC,Zγ+ρ=Zγ+Zρ.Z:\Gamma\longrightarrow\mathbb C, \qquad Z_{\gamma+\rho}=Z_\gamma+Z_\rho.

In the exact-WKB realization of Chapters 8 and 9,

Zγ=γλ0,Z_\gamma=\oint_\gamma\lambda_0,

where γ\gamma is an anti-invariant cycle on the normalized WKB cover. This period locates a possible ray; it does not by itself say that the charge is active. Activity is separate integer data

ΩBPS:ΓZ.\Omega_{\mathrm{BPS}}:\Gamma\longrightarrow\mathbb Z.

For the paired, reality-symmetric problem, assume the CPT symmetry

ΩBPS(γ)=ΩBPS(γ).\Omega_{\mathrm{BPS}}(-\gamma) = \Omega_{\mathrm{BPS}}(\gamma).

The subscript prevents confusion with the all-orders WKB form Ω()\Omega(\hbar). A regular saddle connection has the local hypermultiplet calibration ΩBPS=1\Omega_{\mathrm{BPS}}=1. A cylinder, simple-pole wall, loop, or degenerate saddle has different data and must not be inserted into the ordinary-saddle formula by analogy.

The full fixed-chamber passport is

(Γ,,Z,ΩBPS,σ,R,ϑ).\left( \Gamma,\, \mathbin{\cdot},\, Z,\, \Omega_{\mathrm{BPS}},\, \sigma,\, R,\, \vartheta \right).

Here σ:Γ{±1}\sigma:\Gamma\to\{\pm1\} is a quadratic refinement, R>0R>0 is the semiclassical size, and

ϑ:ΓR/(2πZ)\vartheta:\Gamma \longrightarrow \mathbb R/(2\pi\mathbb Z)

is additive, so ϑγ=ϑγ\vartheta_{-\gamma}=-\vartheta_\gamma modulo 2π2\pi. The refinement obeys

σ(γ)σ(ρ)=(1)γρσ(γ+ρ).\begin{aligned} \sigma(\gamma)\sigma(\rho) ={}& (-1)^{\gamma\mathbin{\cdot}\rho} \sigma(\gamma+\rho). \end{aligned}

It packages the sign relating ordinary multiplicative coordinates to intrinsic twisted-torus coordinates. Locally, an ordinary saddle is calibrated by σ(δ)=1\sigma(\delta)=-1, which turns 1σ(δ)Vδ1-\sigma(\delta)\mathcal V_\delta into 1+Vδ1+\mathcal V_\delta. One cannot set σ=1\sigma=-1 on every active charge of an arbitrary coupled spectrum without checking the quadratic-refinement identity.

For an infinite active set, two controls play different roles. A support property keeps active central charges away from zero relative to charge size,

Zδcδ,ΩBPS(δ)0,|Z_\delta|\ge c\|\delta\|, \qquad \Omega_{\mathrm{BPS}}(\delta)\ne0,

whereas a separate growth condition controls the degeneracies, for example

δΩBPS(δ)eR0Zδ<\sum_\delta \left| \Omega_{\mathrm{BPS}}(\delta) \right| \ee^{-R_0|Z_\delta|} <\infty

for some R0>0R_0>0. The first condition does not imply the second. Locally finite rays or a convergent ordered sector product are also needed. Until Page 5, assume distinct active rays, or only mutually local charges on a common ray.

For each γ\gamma, the RH unknown is a nonzero function Vγ(ζ)\mathcal V_\gamma(\zeta), holomorphic on C×\mathbb C^\times minus the active rays and admitting boundary values on both banks. “Riemann–Hilbert” means that these functions are reconstructed from their prescribed multiplicative jumps together with endpoint asymptotics, a character law, and reality data.

The contrast with Page 2 is structural:

ODE/IM inversionExact-WKB/GMN reconstruction
Baxter divisor or finite fusion nodesCharge lattice and active BPS classes
Multiplicative qq-shiftsRays in the ζ\zeta-plane
Fusion incidence matrixSkew intersection pairing
Fourier or Wiener–Hopf inverseCauchy or Plemelj inverse
Determinant or pseudoenergyResummed period or Darboux coordinate

Central charges determine decay rays, not spatial Stokes curves

Section titled “Central charges determine decay rays, not spatial Stokes curves”

For an oriented active charge δ\delta, define its BPS ray by

δ={ζ:ZδζR<0}=ZδR>0.\begin{aligned} \ell_\delta &= \left\{ \zeta: \frac{Z_\delta}{\zeta}\in\mathbb R_{<0} \right\} \\ &= -Z_\delta\mathbb R_{>0}. \end{aligned}

This ray lies in the complex ζ\zeta-plane. It is not a Stokes curve drawn in the ODE’s spatial zz-plane. Orient δ\ell_\delta outward, from 00 to \infty, and define

  • the ++ boundary as the left, counterclockwise bank;
  • the - boundary as the right, clockwise bank.

After rotating a ray to the positive real axis, these are exactly the upper and lower banks used in Chapter 9. The 2010 GMN paper instead calls the right bank ++ and the left bank -, so

V+book=XGMN10,Vbook=X+GMN10.\mathcal V_+^{\mathrm{book}} = \mathcal X_-^{\mathrm{GMN10}}, \qquad \mathcal V_-^{\mathrm{book}} = \mathcal X_+^{\mathrm{GMN10}}.

At fixed geometric pairing, the original interaction coefficient is

ΩBPS(δ)(γδ)4πi=+ΩBPS(δ)(δγ)4πi,-\frac{ \Omega_{\mathrm{BPS}}(\delta) (\gamma\mathbin{\cdot}\delta) }{ 4\pi\ii } = +\frac{ \Omega_{\mathrm{BPS}}(\delta) (\delta\mathbin{\cdot}\gamma) }{ 4\pi\ii },

which is opposite to the coefficient below. Original GMN imposes the clockwise value as a KS transform of the counterclockwise value; Chapter 9 DDP imposes the counterclockwise value as the transform of the clockwise value.

This page also follows the inverse, later-GMN/DDP phase-jump convention; GMN’s 2013 WKB paper explicitly notes the sign change from the earlier paper. Thus the jump is inverted as well as the banks being relabeled. The coefficient below is derived directly from the book’s DDP jump and Plemelj, not copied from the 2010 formula.

Write

Zδ=Zδeiϕδ,ζ=eiϕδt,t>0.Z_\delta = |Z_\delta|\ee^{\ii\phi_\delta}, \qquad \zeta' = -\ee^{\ii\phi_\delta}t, \quad t>0.

The semiflat coordinate is the jump-free reference coordinate carrying the prescribed endpoint asymptotics. It is

Vγsf(ζ)=exp ⁣[πR(Zγζ+Zγζ)+iϑγ].\begin{aligned} \mathcal V_\gamma^{\mathrm{sf}}(\zeta) = \exp\!\left[ \pi R \left( \frac{Z_\gamma}{\zeta} +\overline{Z_\gamma}\zeta \right) +\ii\vartheta_\gamma \right]. \end{aligned}

On its own ray, the active coordinate has modulus

Vδsf(ζ)=exp ⁣[πRZδ(t+t1)].\left| \mathcal V_\delta^{\mathrm{sf}}(\zeta') \right| = \exp\!\left[ -\pi R|Z_\delta| \left( t+t^{-1} \right) \right].

It therefore decays exponentially as t0t\to0 and as tt\to\infty. The first decay is the exact-WKB choice Re(Zδ/ζ)<0\operatorname{Re}(Z_\delta/\zeta')<0; the second comes from the conjugate term and is lost in the conformal limit.

Two intersecting WKB cycles map through their central charges to oriented BPS rays in the complex semiclassical-parameter plane; logarithmic jump data on those rays feed an off-ray coordinate through a Cauchy kernel.

Fixed-chamber Riemann–Hilbert reconstruction. Intersection data decide which ray logarithm acts on each coordinate. The orientation Zδ/ζ<0Z_\delta/\zeta'<0 makes the active symbol small near the origin, while the full semiflat term also damps the far endpoint. No Baxter divisor, fusion graph, or ODE/IM Fourier kernel enters this construction.

Chapter 9 fixed the active cycle as the first argument of the intersection pairing. In the local ordinary-saddle calibration, the analytic jump across δ\ell_\delta is

Vγ,+=Vγ,×(1+Vδ,)ΩBPS(δ)δγ.\begin{aligned} \mathcal V_{\gamma,+} ={}& \mathcal V_{\gamma,-} \\ &\times \left( 1+\mathcal V_{\delta,-} \right)^{ -\Omega_{\mathrm{BPS}}(\delta)\, \delta\mathbin{\cdot}\gamma }. \end{aligned}

For ΩBPS(δ)=1\Omega_{\mathrm{BPS}}(\delta)=1, this is precisely the DDP formula already proved in its stated scope. The active coordinate is unchanged because δδ=0\delta\mathbin{\cdot}\delta=0.

The refinement-aware jump is obtained by replacing the logarithmic factor with

Log ⁣(1σ(δ)Vδ,).\Log\!\left( 1-\sigma(\delta)\mathcal V_{\delta,-} \right).

Thus the logarithmic boundary difference is

LogVγ,+LogVγ,=ΩBPS(δ)(δγ)×Log ⁣(1σ(δ)Vδ,).\begin{aligned} \Log\mathcal V_{\gamma,+} -\Log\mathcal V_{\gamma,-} ={}& -\Omega_{\mathrm{BPS}}(\delta) \left( \delta\mathbin{\cdot}\gamma \right) \\ &\times \Log\!\left( 1-\sigma(\delta)\mathcal V_{\delta,-} \right). \end{aligned}

The branch is continued from a ray endpoint where the active coordinate is small. If 1σ(δ)Vδ1-\sigma(\delta)\mathcal V_\delta vanishes on the contour, that branch prescription fails: the contour must be deformed or supplied with source terms. Those are Page 5 operations.

Phase alignment is not enough to assert this jump. A saddle connection, cylinder, or other justified BPS state must actually realize the charge, and its index must be known. Likewise, aligned noncommuting charges require an ordered product of jump factors rather than one scalar logarithm.

A residue-two Cauchy kernel reconstructs the full coordinate

Section titled “A residue-two Cauchy kernel reconstructs the full coordinate”

Introduce the symmetric one-form

K(ζ,ζ)= ⁣dζζζ+ζζζ.K(\zeta,\zeta') = \frac{\dd\zeta'}{\zeta'} \frac{\zeta'+\zeta}{\zeta'-\zeta}.

Near the target point,

K(ζ,ζ)=2 ⁣dζζζ+regular.K(\zeta,\zeta') = 2\frac{\dd\zeta'}{\zeta'-\zeta} +\text{regular}.

Because the residue is 22, the Plemelj coefficient is 1/(4πi)1/(4\pi\ii), not 1/(2πi)1/(2\pi\ii). With every ray oriented 00\to\infty, the book-normalized equation is

LogVγ(ζ)=LogVγsf(ζ)14πiδΩBPS(δ)(δγ)×δ0 ⁣dζζζ+ζζζ×Log ⁣(1σ(δ)Vδ(ζ)).\begin{aligned} \Log\mathcal V_\gamma(\zeta) ={}& \Log\mathcal V_\gamma^{\mathrm{sf}}(\zeta) \\ &- \frac{1}{4\pi\ii} \sum_\delta \Omega_{\mathrm{BPS}}(\delta) \left( \delta\mathbin{\cdot}\gamma \right) \\ &\quad\times \int_{\ell_\delta}^{0\to\infty} \frac{\dd\zeta'}{\zeta'} \frac{\zeta'+\zeta}{\zeta'-\zeta} \\ &\quad\times \Log\!\left( 1-\sigma(\delta) \mathcal V_\delta(\zeta') \right). \end{aligned}

For a local ordinary saddle, put σ(δ)=1\sigma(\delta)=-1. Taking the left-minus-right boundary value of its integral gives

ΩBPS(δ)(δγ)Log(1+Vδ),-\Omega_{\mathrm{BPS}}(\delta) \left( \delta\mathbin{\cdot}\gamma \right) \Log(1+\mathcal V_\delta),

which is exactly the declared DDP jump. This one-line residue check is the safest way to translate between sources with different bank labels. When the target lies on a ray, the integral means a principal value plus the appropriate half-residue boundary term.

The equation is posed with the character law

Vγ+ρ=VγVρ,Vγ=Vγ1,\mathcal V_{\gamma+\rho} = \mathcal V_\gamma\mathcal V_\rho, \qquad \mathcal V_{-\gamma} = \mathcal V_\gamma^{-1},

With the even BPS spectrum, σ(δ)=σ(δ)\sigma(-\delta)=\sigma(\delta), and logarithm branches paired by antipodal conjugation, the equation also obeys the reality condition

Vγ(ζ)=Vγ(1ζ),\mathcal V_\gamma(\zeta) = \overline{ \mathcal V_{-\gamma} \left( -\frac1{\overline\zeta} \right) },

and the paired asymptotic orders

LogVγ(ζ)=πRZγζ+O(1),ζ0,LogVγ(ζ)=πRZγζ+O(1),ζ.\begin{aligned} \Log\mathcal V_\gamma(\zeta) &= \frac{\pi RZ_\gamma}{\zeta} +O(1), && \zeta\to0, \\ \Log\mathcal V_\gamma(\zeta) &= \pi R\overline{Z_\gamma}\zeta +O(1), && \zeta\to\infty. \end{aligned}

The bounded zero mode is part of the normalization. In particular, the symmetric kernel approaches a nonzero constant as ζ0\zeta\to0; one should not silently strengthen the first line to Vγ/Vγsf1\mathcal V_\gamma/\mathcal V_\gamma^{\mathrm{sf}}\to1.

For a finite spectrum, the semiflat estimate gives endpoint convergence if the nonlinear solution remains controlled relative to the semiflat seed and the logarithm has no contour zero. For an infinite spectrum, charge sums, ray integrals, and limits may be interchanged only under uniform domination. GMN’s large-RR Appendix C gives a contraction argument only after its weighted multicover and convergence assumptions, together with the needed uniform bounds, supplement the support estimate. The rigorous theorems cited here cover restricted settings; they do not prove a pole-free global solution for every such spectrum, or at arbitrary small RR.

The conformal equation changes both the drive and the endpoint problem

Section titled “The conformal equation changes both the drive and the endpoint problem”

To compare the full coordinate with the book’s exact-WKB symbol, set

ζ=πR.\zeta=\pi R\hbar.

Then the semiflat exponent becomes

πR(Zγζ+Zγζ)=Zγ+π2R2Zγ.\begin{aligned} \pi R \left( \frac{Z_\gamma}{\zeta} +\overline{Z_\gamma}\zeta \right) ={}& \frac{Z_\gamma}{\hbar} \\ &+ \pi^2R^2 \overline{Z_\gamma}\hbar. \end{aligned}

The formal conformal scaling

R0,ζ0,=ζπRfixedR\to0, \qquad \zeta\to0, \qquad \hbar=\frac{\zeta}{\pi R} \quad\text{fixed}

therefore retains the exact-WKB factor exp(Zγ/)\exp(Z_\gamma/\hbar) and removes the conjugate drive. But it also removes the large-|\hbar'| damping along every integration ray. The limit cannot generally be passed under the integral sign.

The kernel identity

14 ⁣dζζζ+ζζζ=14 ⁣dζζ+12ζ ⁣dζζ(ζζ)\begin{aligned} & \frac14 \frac{\dd\zeta'}{\zeta'} \frac{\zeta'+\zeta}{\zeta'-\zeta} \\ &\qquad= \frac14\frac{\dd\zeta'}{\zeta'} + \frac12 \frac{\zeta\,\dd\zeta'}{ \zeta'(\zeta'-\zeta) } \end{aligned}

separates a target-independent constant from an origin-normalized Cauchy transform. If the constant is absorbed into a declared zero mode cγc_\gamma, and if the limiting integral converges, one obtains

LogVγconf()=Zγ+cγ2πiδΩBPS(δ)(δγ)×δ ⁣d()×Log ⁣(1σ(δ)Vδconf()).\begin{aligned} \Log\mathcal V_\gamma^{\mathrm{conf}}(\hbar) ={}& \frac{Z_\gamma}{\hbar} +c_\gamma \\ &- \frac{\hbar}{2\pi\ii} \sum_\delta \Omega_{\mathrm{BPS}}(\delta) \left( \delta\mathbin{\cdot}\gamma \right) \\ &\quad\times \int_{\ell_\delta} \frac{\dd\hbar'}{ \hbar'(\hbar'-\hbar) } \\ &\quad\times \Log\!\left( 1-\sigma(\delta) \mathcal V_\delta^{\mathrm{conf}}(\hbar') \right). \end{aligned}

Indeed,

()=11,\frac{\hbar}{ \hbar'(\hbar'-\hbar) } = \frac1{\hbar'-\hbar} -\frac1{\hbar'},

so the second term fixes the origin normalization while leaving the jump unchanged. Matching a regularized exact-WKB cycle symbol usually selects cγ=0c_\gamma=0, but only when this book explicitly chooses a regularization whose quantum correction tends to zero. That is normalization data, not a consequence of Plemelj. The zero modes are not independent: the character law requires

cγ+ρ=cγ+cρ(mod2πi)c_{\gamma+\rho} = c_\gamma+c_\rho \pmod{2\pi\ii}

on the declared logarithm branches, with cγ=cγc_{-\gamma}=-c_\gamma modulo the same branch period. Any real section must also impose its inherited conjugation condition.

For each source ray, a direct sufficient endpoint contract is

0εLog(1σ(δ)Vδconf) ⁣d<,ALog(1σ(δ)Vδconf)2 ⁣d<.\begin{aligned} & \int_0^\varepsilon \frac{ \left| \Log(1-\sigma(\delta)\mathcal V_\delta^{\mathrm{conf}}) \right| }{ |\hbar'| } \,|\dd\hbar'| <\infty, \\ & \int_A^\infty \frac{ \left| \Log(1-\sigma(\delta)\mathcal V_\delta^{\mathrm{conf}}) \right| }{ |\hbar'|^2 } \,|\dd\hbar'| <\infty. \end{aligned}

for some ε>0\varepsilon>0 and A>0A>0 along the ray. The semiclassical exponential controls the first integral. A bounded far-end logarithm already controls the second, so decay is sufficient but not necessary.

Gaiotto’s published conformal equation inherits the original GMN crossing direction and therefore has the opposite interaction sign at fixed geometric pairing. The equation above is its DDP-normalized inverse-jump analogue.

Gaiotto’s conformal scaling assumes that the limit exists and has controlled large-\hbar behavior. Its oper interpretation further restricts to the distinguished section with vanishing Wilson-line angles, up to canonical refinement signs; the general identification of the limiting Lagrangian with the oper locus is conjectural.

Allegretti proves that Borel sums of Voros symbols equal Fock–Goncharov coordinates in the stated complete saddle-free setting, but that theorem alone does not say that they solve the nonlinear equation displayed here. Iwaki–Kidwai give an actual model-specific BPS-RH solution for hypergeometric-type quantum curves and almost-doubled uncoupled BPS structures. Outside such settings, a matching leading exponential and matching jump factor establish a strong analogy—not equality of analytic functions.

Rapidity reveals a phase-shifted Cauchy kernel

Section titled “Rapidity reveals a phase-shifted Cauchy kernel”

The conformal equation can be written in a TBA-like form without turning it into the Page 2 TBA. Put

Za=maeiϕa,a(θ)=eiϕaθ,Z_a=m_a\ee^{\ii\phi_a}, \qquad \hbar_a(\theta) = -\ee^{\ii\phi_a-\theta},

and define a boundary pseudoenergy by

Va(θ)=Vγa,conf(a(θ))=eεa(θ).\mathcal V_a(\theta) = \mathcal V_{\gamma_a,-}^{\mathrm{conf}} \bigl( \hbar_a(\theta) \bigr) = \ee^{-\varepsilon_a(\theta)}.

Then Za/a=maeθZ_a/\hbar_a=-m_a\ee^\theta. Parameterizing the source ray in the same way gives

a(θ)b(θ)a(θ)=1exp[θθ+i(ϕbϕa)]1.\begin{aligned} \frac{\hbar_a(\theta)}{ \hbar_b(\theta')-\hbar_a(\theta) } = \frac1{ \exp[ \theta-\theta' +\ii(\phi_b-\phi_a) ]-1 }. \end{aligned}

Thus the origin-normalized equation has the schematic form

εa(θ)=maeθca+12πibΩBPS(γb)(γbγa)×RLb(θ) ⁣dθeθθ+i(ϕbϕa)1,\begin{aligned} \varepsilon_a(\theta) ={}& m_a\ee^\theta-c_a \\ &+ \frac1{2\pi\ii} \sum_b \Omega_{\mathrm{BPS}}(\gamma_b) \left( \gamma_b\mathbin{\cdot}\gamma_a \right) \\ &\quad\times \int_{\mathbb R} \frac{ L_b(\theta')\,\dd\theta' }{ \ee^{ \theta-\theta' +\ii(\phi_b-\phi_a) }-1 }, \end{aligned}

with

Lb=Log ⁣(1σ(γb)eεb).L_b = \Log\!\left( 1-\sigma(\gamma_b) \ee^{-\varepsilon_b} \right).

The kernel comes from relative ray phases. A pole reaches the real integration line when two interacting rays coincide, precisely where the simple fixed-ray factorization ceases to be sufficient. By contrast, Page 2’s kernels came from qq-shift multipliers and a fusion incidence matrix. Combining antipodal rays can turn the Cauchy kernel into familiar hyperbolic kernels in special models; Page 4 audits the extra identifications required.

Rank two separates exact solvability from nonlinear coupling

Section titled “Rank two separates exact solvability from nonlinear coupling”

First take

Γ=ZδZβ,δβ=1,\Gamma = \mathbb Z\delta\oplus\mathbb Z\beta, \qquad \delta\mathbin{\cdot}\beta=1,

with only ±δ\pm\delta active and ΩBPS(±δ)=1\Omega_{\mathrm{BPS}}(\pm\delta)=1. Choose σ(δ)=σ(δ)=1\sigma(\delta)=\sigma(-\delta)=-1. The active spectrum is uncoupled because its active charges pair trivially with one another. Consequently,

V±δ=V±δsf.\mathcal V_{\pm\delta} = \mathcal V_{\pm\delta}^{\mathrm{sf}}.

The probe coordinate is nevertheless nontrivial:

LogVβVβsf=14πiδK(ζ,ζ)Log(1+Vδsf)+14πiδK(ζ,ζ)Log(1+Vδsf).\begin{aligned} \Log \frac{\mathcal V_\beta}{ \mathcal V_\beta^{\mathrm{sf}} } ={}& -\frac1{4\pi\ii} \int_{\ell_\delta} K(\zeta,\zeta') \Log(1+\mathcal V_\delta^{\mathrm{sf}}) \\ &+ \frac1{4\pi\ii} \int_{\ell_{-\delta}} K(\zeta,\zeta') \Log(1+\mathcal V_{-\delta}^{\mathrm{sf}}). \end{aligned}

Both integrals converge exponentially, and V±δsf<1|\mathcal V_{\pm\delta}^{\mathrm{sf}}|<1 on their own rays, so the principal logarithms meet no zero. This is the elementary calibration of an exact finite mutually local solution of the displayed two-ended equation. Bridgeland’s finite uncoupled theorem is a separate result in his one-ended DT normalization and assumes a constant term equal to one on every active class.

Now choose two charges with

γ1γ2=1,ΩBPS(γ1)=ΩBPS(γ2)=1.\gamma_1\mathbin{\cdot}\gamma_2=1, \qquad \Omega_{\mathrm{BPS}}(\gamma_1) = \Omega_{\mathrm{BPS}}(\gamma_2) =1.

In one ray half-plane, write [ΔaLogVb]a[\Delta_a\Log\mathcal V_b]_{\ell_a} for the contribution from a\ell_a alone; the antipodal rays must still be added in the full reality-symmetric problem. The ordinary-saddle source terms are

[Δ2LogV1]2=14πi2KLog(1+V2),[Δ1LogV2]1=14πi1KLog(1+V1).\begin{aligned} [\Delta_2\Log\mathcal V_1]_{\ell_2} &= \frac1{4\pi\ii} \int_{\ell_2} K\Log(1+\mathcal V_2), \\ [\Delta_1\Log\mathcal V_2]_{\ell_1} &= - \frac1{4\pi\ii} \int_{\ell_1} K\Log(1+\mathcal V_1). \end{aligned}

The opposite signs are forced by antisymmetry. Iterating these equations produces powers such as exp(nZγa/ζ)\exp(nZ_{\gamma_a}/\zeta) from the Taylor series of Log(1+Vγa)\Log(1+\mathcal V_{\gamma_a}). They are composite action grades; they do not declare that every multiple nγan\gamma_a has a nonzero BPS index.

Plemelj equivalence is not a general existence theorem

Section titled “Plemelj equivalence is not a general existence theorem”

Under the stated trace and convergence hypotheses, taking boundary values of the integral equation reproduces the jump. Conversely, suppose an RH solution with the declared functional jump law and normalization already exists. Its boundary traces determine actual additive discontinuity functions. Subtract the Cauchy reconstruction of those fixed functions. The logarithmic difference has no jumps, is removable at the two endpoints under the normalization bounds, and vanishes after the zero mode has been fixed. A Liouville argument on the compactified plane then makes the difference zero.

That proves reversibility for an existing solution. It does not prove that the nonlinear fixed-point problem has a solution, that Picard iteration converges, or that no extra poles appear. GMN’s Appendix C gives an argument under additional weighted multicover and convergence assumptions; Garza proves a theorem for a restricted local rank-two setting. General coupled or small-RR existence and uniqueness remain model-dependent.

Finally, an RH solution gives resummed cycle or transport coordinates, not an ODE spectrum by itself. A boundary determinant or exact quantization condition must still turn those coordinates into spectral zeros. Page 4 asks when the RH coordinates and the ODE/IM unknowns describe the same analytic objects; Page 5 changes rays, contours, and chamber data.

Confusing spatial and parameter-space rays. A Stokes curve lives in the ODE’s zz-plane. A BPS integration ray lives in the ζ\zeta- or \hbar-plane and is fixed by a central charge.

Inferring activity from phase alone. The phase of ZδZ_\delta locates a possible ray. A realized saddle class or other justified BPS input is needed to set ΩBPS(δ)\Omega_{\mathrm{BPS}}(\delta).

Reversing an intersection or a bank. The book puts the active class first in δγ\delta\mathbin{\cdot}\gamma and calls the left bank ++. Reversing either convention reverses the exponent; copying a source formula without translating both can hide two sign changes.

Putting a plus sign on every charge. The factor 1+Vδ1+\mathcal V_\delta is the local σ(δ)=1\sigma(\delta)=-1 ordinary-saddle calibration. A coupled spectrum must satisfy one coherent quadratic-refinement convention.

Taking the conformal limit under the integral sign. Removing the conjugate drive removes far-end damping. A subtraction changes the normalization, not the missing endpoint estimate.

Calling a fixed-point equation a solution theorem. Plemelj fixes the jump and, with a vanishing condition, its reconstruction. Global nonlinear existence needs a separate contraction, explicit formula, or model-specific theorem.

Recognizing a familiar hyperbolic kernel. Combining antipodal Cauchy rays can produce 1/cosh1/\cosh-type kernels. That resemblance does not identify the nodes, masses, unknowns, or observable with ODE/IM; Page 4 requires the complete dictionary.

Changing chamber data inside the equation. The active indices, ray ordering, and refinement package are fixed on this page. Reordering noncommuting rays or changing indices is the wall-crossing problem of Page 5.

Let Zδ=ZδeiϕZ_\delta=|Z_\delta|\ee^{\ii\phi} and ζ=eiϕt\zeta'=-\ee^{\ii\phi}t. Evaluate the two terms in the semiflat exponent.

Solution

Direct substitution gives

Zδζ=Zδt,Zδζ=Zδt.\frac{Z_\delta}{\zeta'} = -\frac{|Z_\delta|}{t}, \qquad \overline{Z_\delta}\zeta' = -|Z_\delta|t.

Therefore

Vδsf(ζ)=eπRZδ(t+t1).\left| \mathcal V_\delta^{\mathrm{sf}}(\zeta') \right| = \ee^{-\pi R|Z_\delta|(t+t^{-1})}.

It decays faster than any power at both endpoints against the measure  ⁣dt/t\dd t/t. The conformal limit deletes the term proportional to tt.

Expand K(ζ,ζ)K(\zeta,\zeta') near ζ=ζ\zeta'=\zeta and derive the left-minus-right jump produced by one source charge.

Solution

Since ζ/ζ=1\zeta'/\zeta'=1 at the pole,

K(ζ,ζ)=2 ⁣dζζζ+O(1) ⁣dζ.K(\zeta,\zeta') = 2\frac{\dd\zeta'}{\zeta'-\zeta} +O(1)\dd\zeta'.

The oriented Plemelj formula assigns jump ff to (2πi)1f(ζ) ⁣dζ/(ζζ)(2\pi\ii)^{-1}\int f(\zeta')\dd\zeta'/(\zeta'-\zeta). Hence

A4πiKL-\frac{A}{4\pi\ii} \int K\,L

has left-minus-right jump AL-A L. Taking A=ΩBPS(δ)(δγ)A=\Omega_{\mathrm{BPS}}(\delta) (\delta\mathbin{\cdot}\gamma) reproduces the DDP exponent.

Show that the symmetric and origin-normalized kernel one-forms have the same pole and differ by a target-independent term.

Solution

Algebra gives

12 ⁣dζζζ+ζζζζ ⁣dζζ(ζζ)= ⁣dζ2ζ.\begin{aligned} & \frac12 \frac{\dd\zeta'}{\zeta'} \frac{\zeta'+\zeta}{\zeta'-\zeta} - \frac{\zeta\,\dd\zeta'}{ \zeta'(\zeta'-\zeta) } \\ &\qquad= \frac{\dd\zeta'}{2\zeta'}. \end{aligned}

The difference has no target ζ\zeta, so both kernels encode the same Plemelj jump. Their integrals differ by a bounded zero mode, which must be included in the RH normalization.

Assume γ1γ2=1\gamma_1\mathbin{\cdot}\gamma_2=1. Determine the contribution of 2\ell_2 to LogV1\Log\mathcal V_1 and of 1\ell_1 to LogV2\Log\mathcal V_2.

Solution

For target γ1\gamma_1, the active-first pairing is

γ2γ1=1,\gamma_2\mathbin{\cdot}\gamma_1=-1,

so the minus sign in front of the Cauchy sum makes the contribution positive. For target γ2\gamma_2, γ1γ2=1\gamma_1\mathbin{\cdot}\gamma_2=1, so the contribution is negative. Self-couplings vanish by skew-symmetry.

In the uncoupled example, determine the jumps of Vβ\mathcal V_\beta on δ\ell_\delta and δ\ell_{-\delta}.

Solution

Because δβ=1\delta\mathbin{\cdot}\beta=1,

Vβ,+=Vβ,1+Vδon δ.\mathcal V_{\beta,+} = \frac{\mathcal V_{\beta,-}}{ 1+\mathcal V_\delta } \qquad\text{on }\ell_\delta.

But (δ)β=1(-\delta)\mathbin{\cdot}\beta=-1, so

Vβ,+=Vβ,(1+Vδ)on δ.\mathcal V_{\beta,+} = \mathcal V_{\beta,-} \left( 1+\mathcal V_{-\delta} \right) \qquad\text{on }\ell_{-\delta}.

These are exactly the two boundary jumps of the explicit probe Cauchy transform.

6. Derive the phase-shifted rapidity kernel

Section titled “6. Derive the phase-shifted rapidity kernel”

Substitute a=eiϕaθ\hbar_a=-\ee^{\ii\phi_a-\theta} and b=eiϕbθ\hbar_b'=-\ee^{\ii\phi_b-\theta'} into the origin-normalized Cauchy kernel. Determine when its pole lies on the real θ\theta'-contour.

Solution

The ratio in the kernel is

aba=1eθθ+i(ϕbϕa)1=:Kab(θθ).\begin{aligned} \frac{\hbar_a}{ \hbar_b'-\hbar_a } &= \frac1{ \ee^{ \theta-\theta' +\ii(\phi_b-\phi_a) }-1 } \\ &=: K_{ab}(\theta-\theta'). \end{aligned}

The parameterization reverses the ray limits, while  ⁣db/b= ⁣dθ\dd\hbar_b'/\hbar_b'=-\dd\theta', so the two signs cancel. A pole on the real contour requires

θθ+i(ϕbϕa)=2πin.\theta-\theta' +\ii(\phi_b-\phi_a) = 2\pi\ii n.

For real θ,θ\theta,\theta', this occurs precisely when ϕbϕa=0\phi_b-\phi_a=0 modulo 2π2\pi: the two interacting rays coincide. The ordered-product treatment then belongs to Page 5.

As an optional large-RR check, let a>0a>0, ξ=1|\xi|=1, and define K0K_0 as the modified Bessel function of the second kind. Expanding the logarithm gives

0 ⁣dttLog ⁣(1+ξea(t+t1))=2n=1(1)n+1ξnnK0(2an).\begin{aligned} & \int_0^\infty \frac{\dd t}{t} \Log\!\left( 1+\xi\ee^{-a(t+t^{-1})} \right) \\ &\qquad= 2\sum_{n=1}^\infty \frac{(-1)^{n+1}\xi^n}{n} K_0(2an). \end{aligned}

Indeed, t+t12t+t^{-1}\ge2 makes the logarithmic expansion uniformly dominated, and

0 ⁣dttean(t+t1)=2K0(2an).\int_0^\infty \frac{\dd t}{t} \ee^{-an(t+t^{-1})} = 2K_0(2an).

This also quantifies the large-RR exponential suppression.

Use ζ=πR\zeta=\pi R\hbar to find the limiting drive and explain why the unsubtracted ray integral can diverge.

Solution

The drive is

Zγ+π2R2Zγ,\frac{Z_\gamma}{\hbar} + \pi^2R^2\overline{Z_\gamma}\hbar,

so only Zγ/Z_\gamma/\hbar remains as R0R\to0. Along a source ray, the second term had supplied decay as |\hbar'|\to\infty. Without it, the active coordinate need not tend to zero; the logarithm can approach a nonzero constant, and an unsubtracted  ⁣d/\dd\hbar'/\hbar' integral then diverges logarithmically. The origin subtraction changes the far-end weight to  ⁣d/()2\dd\hbar'/(\hbar')^2, for which a bounded logarithm is already integrable. It still requires the displayed weighted endpoint bound; far-end decay is sufficient but not necessary.

8. Prove uniqueness of a fixed Cauchy reconstruction

Section titled “8. Prove uniqueness of a fixed Cauchy reconstruction”

Suppose two logarithmic functions have identical actual additive discontinuity functions and zero-mode normalization, and their difference is removable at 00 and \infty. Show that their Cauchy reconstructions coincide.

Solution

The difference has zero boundary jump on every ray, so analytic continuation glues it to a holomorphic function on C×\mathbb C^\times. The endpoint hypotheses extend it across 00 and \infty, giving a holomorphic function on the Riemann sphere. It is constant, and the common zero-mode normalization makes that constant zero.

This proves uniqueness after the actual discontinuity functions are fixed. It does not prove uniqueness for the nonlinear RH problem: two solutions satisfying the same functional jump law could have different source traces. It also supplies no existence theorem.

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