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Instantons, quantum periods, and differential equations

Can the coefficient of an instanton correction be recovered by solving an ordinary differential equation? We will match one coefficient in pure SU(2)SU(2) theory, including its deformation dependence. Then we will change the boundary parameter until the coefficient diverges—and show why the differential equation itself remains well behaved.

Begin with the one-instanton calculation and planning a reproducible research calculation. The new preparation is elementary spectral perturbation theory, developed below. Neither integrable systems nor two-dimensional conformal field theory is an entry requirement.

The parent theory is four-dimensional N=2 SU(2)SU(2) Yang–Mills, with eight real supercharges and no hypermultiplets. Its generic flat-space Coulomb vacuum has an Abelian rank-one low-energy theory. The equivariant calculation retains selected supersymmetry in a rotational background; it does not preserve the full flat-space Poincaré algebra. No hypermultiplet mass, shifted or physical, occurs in this example.

The Omega parameters ϵ1,ϵ2\epsilon_1,\epsilon_2 have mass dimension one. They couple to rotations of the two coordinate planes of Euclidean four-space. Retain the instanton lesson’s conventions:

b1=b=−iα,b2=−b,q=Λ44,E=ϵ1+ϵ2.(D16.1)b_1=b=-i\alpha,\qquad b_2=-b,\qquad q=\frac{\Lambda^4}{4},\qquad E=\epsilon_1+\epsilon_2. \tag{D16.1}

Here bb is the equivariant Coulomb coordinate, qq is the dimension-four instanton parameter, and Λ\Lambda is the scale of the site’s first Seiberg–Witten curve. In the undeformed theory α=a/2\alpha=a/\sqrt2, where aa is the electric period in the fixed charge basis. This rescaling belongs to the instanton-to-curve dictionary; it does not change the allowed particle or line charges.

Write Zinst=1+qZ1+q2Z2+⋯Z_{\rm inst}=1+qZ_1+q^2Z_2+\cdots. The two one-box contributions are

Z1=1ϵ1ϵ2(2b)(E−2b)+1ϵ1ϵ2(−2b)(E+2b)=2ϵ1ϵ2(E2+4α2).(D16.2)Z_1= \frac{1}{\epsilon_1\epsilon_2(2b)(E-2b)} +\frac{1}{\epsilon_1\epsilon_2(-2b)(E+2b)} =\frac{2}{\epsilon_1\epsilon_2(E^2+4\alpha^2)}. \tag{D16.2}

The signs and finite scale factor were fixed by the previous contour calculation. In particular, copying the isolated one-instanton sign of Nekrasov’s original contour formula without its parameter translation would change this answer.

There are two distinct operations on the connected quantity log⁡Zinst\log Z_{\rm inst}:

Fcl,inst=lim⁡ϵ1,ϵ2→0ϵ1ϵ2log⁡Zinst,Winst(α,ϵ1,q)=lim⁡ϵ2→0ϵ2log⁡Zinst,FNS,inst=ϵ1Winst.(D16.3)\begin{aligned} \mathscr F_{\rm cl,inst} &=\lim_{\epsilon_1,\epsilon_2\to0} \epsilon_1\epsilon_2\log Z_{\rm inst},\\ \mathcal W_{\rm inst}(\alpha,\epsilon_1,q) &=\lim_{\epsilon_2\to0}\epsilon_2\log Z_{\rm inst},\\ \mathscr F_{\rm NS,inst}&=\epsilon_1\mathcal W_{\rm inst}. \end{aligned} \tag{D16.3}

We initially take these limits coefficient by coefficient in qq, away from poles. The first gives the ordinary instanton prepotential in this normalization. The second is the Nekrasov–Shatashvili, or NS, limit: one rotational deformation remains. W\mathcal W has dimension one and FNS\mathscr F_{\rm NS} dimension two. Their names do not make them equal to the physical prepotential with its separate 1/(2πi)1/(2\pi i) normalization. NS (3.6)–(3.8) fixes the logarithm and limit.

Since log⁡Zinst=qZ1+O(q2)\log Z_{\rm inst}=qZ_1+O(q^2),

FNS,inst=2q4α2+ϵ12+O(q2),Fcl,inst=q2α2+O(q2).(D16.4)\mathscr F_{\rm NS,inst} =\frac{2q}{4\alpha^2+\epsilon_1^2}+O(q^2), \qquad \mathscr F_{\rm cl,inst} =\frac{q}{2\alpha^2}+O(q^2). \tag{D16.4}

Keeping ϵ1\epsilon_1 finite and simply renaming the first expression “the Seiberg–Witten answer” loses a physical deformation.

Why an energy involves a derivative of the logarithm

Section titled “Why an energy involves a derivative of the logarithm”

The spectral quantity to compare is a quadratic scalar observable, not the prepotential itself. Its relation to the logarithm is often called a deformed Matone relation. We can see its normalization directly.

In the NS fixed-point description, let xu,j0=bu+(j−1)ϵ1x^0_{u,j}=b_u+(j-1)\epsilon_1 label the empty columns of the Young diagrams used in instanton counting. A column with many boxes has a finite rescaled length λu,j\lambda_{u,j} as ϵ2→0\epsilon_2\to0, and endpoint xu,j=xu,j0+λu,jx_{u,j}=x^0_{u,j}+\lambda_{u,j}. The source input is

q∂qWinst=∑u,jλu,j,⟨Tr⁡2Φeq 2⟩=∑ubu2−∑u,j[(xu,j+ϵ1)2−(xu,j0+ϵ1)2−xu,j2+(xu,j0)2].(D16.5)\begin{aligned} q\partial_q\mathcal W_{\rm inst}&=\sum_{u,j}\lambda_{u,j},\\ \left\langle\operatorname{Tr}_2\Phi_{\rm eq}^{\,2}\right\rangle &=\sum_u b_u^2-\sum_{u,j} \left[(x_{u,j}+\epsilon_1)^2 -(x^0_{u,j}+\epsilon_1)^2-x_{u,j}^2+(x^0_{u,j})^2\right]. \end{aligned} \tag{D16.5}

These are the box-counting and scalar-observable formulas in Poghossian (23), (29), (31), with W\mathcal W normalized as in (D16.3). The trace is the ordinary fundamental trace. The critical-column construction is a localization input; we do not derive its full saddle here.

Each square bracket is 2ϵ1λu,j2\epsilon_1\lambda_{u,j}. Also ∑bu2=−2α2\sum b_u^2=-2\alpha^2. Define the continued, normalized observable uNS=−⟨Tr⁡2Φeq 2⟩/2u_{\rm NS}=-\langle\operatorname{Tr}_2\Phi_{\rm eq}^{\,2}\rangle/2. Therefore

uNS=α2+q∂qFNS,inst.(D16.6)u_{\rm NS}=\alpha^2+q\partial_q\mathscr F_{\rm NS,inst}. \tag{D16.6}

The definition fixes the additive convention by uNS(q=0)=α2u_{\rm NS}(q=0)=\alpha^2; no extra ϵ12\epsilon_1^2 constant is inserted. At instanton order qkq^k, the derivative multiplies the connected coefficient by kk. Thus equality of an energy coefficient and a prepotential coefficient at first order is special. At second order they differ by a factor of two.

Choose the differential equation and its boundary condition

Section titled “Choose the differential equation and its boundary condition”

For a self-adjoint circle problem, take q>0q>0, ℏ>0\hbar>0, and the explicit analytic continuation

ϵ1=iℏ,α∈R.(D16.7)\epsilon_1=i\hbar,\qquad \alpha\in\mathbb R. \tag{D16.7}

ℏ\hbar has mass dimension one; it is not a dimensionless copy of the usual laboratory Planck constant. Then the gauge calculation predicts uNS=α2+2q/(4α2−ℏ2)+O(q2)u_{\rm NS}=\alpha^2+2q/(4\alpha^2-\hbar^2)+O(q^2).

The inherited classical curve is w+q/w=X2−uw+q/w=X^2-u, with differential X dw/wX\,dw/w. On w=q eiθw=\sqrt q\,e^{i\theta} it becomes X2=u+2qcos⁡θX^2=u+2\sqrt q\cos\theta, and the electric action is (2π)−1∫02πX dθ(2\pi)^{-1}\int_0^{2\pi}X\,d\theta. Quantize XX as −iℏ∂θ-i\hbar\partial_\theta. Our chosen spectral problem is consequently

[−ℏ2d2dθ2−2qcos⁡θ]ψ=uψ,(ψψ′)(θ+2π)=e2πiα/ℏ(ψψ′)(θ).(D16.8)\left[-\hbar^2\frac{d^2}{d\theta^2} -2\sqrt q\cos\theta\right]\psi=u\psi, \qquad \begin{pmatrix}\psi\\\psi'\end{pmatrix}(\theta+2\pi) =e^{2\pi i\alpha/\hbar} \begin{pmatrix}\psi\\\psi'\end{pmatrix}(\theta). \tag{D16.8}

The boundary multiplier is a Floquet multiplier: a wave may return with a phase after one cell. Both conditions are needed to cancel the integration-by-parts boundary term and obtain a self-adjoint operator. The multiplier knows α\alpha only modulo ℏ\hbar; specifying the branch that approaches u=α2u=\alpha^2 as q→0q\to0 also specifies which free mode is being continued.

The NS correspondence motivates this quantization; quantizing a classical curve alone does not prove the correspondence to all instanton orders. NS section 5.1.3 explicitly distinguishes the quasi-periodic Mathieu problem from the square-integrable modified-Mathieu problem on a line. Our circle boundary condition is the former. For comparison with Başar–Dunne (2.1), divide our equation by two and shift θ\theta by π\pi: their potential scale squared is q\sqrt q, their eigenvalue is u/2u/2, and their ℏ\hbar is ours. No coefficient is compared before this translation.

Use orthonormal free waves ∣n⟩=(2π)−1/2ei(α/ℏ+n)θ|n\rangle=(2\pi)^{-1/2}e^{i(\alpha/\hbar+n)\theta}, n∈Zn\in\mathbb Z. Their energies are dn=(α+nℏ)2d_n=(\alpha+n\hbar)^2. The potential connects only neighboring modes, with matrix element −q-\sqrt q. We continue ∣0⟩|0\rangle.

Write ψ=∣0⟩+c1∣1⟩+c−1∣−1⟩+⋯\psi=|0\rangle+c_1|1\rangle+c_{-1}|-1\rangle+\cdots. To first order in q\sqrt q, the equations for the neighboring coefficients give c±1=q/(d±1−d0)c_{\pm1}=\sqrt q/(d_{\pm1}-d_0). The n=0n=0 equation then gives

u−α2=−q(c1+c−1)+O(q2)=q[1α2−(α+ℏ)2+1α2−(α−ℏ)2]+O(q2)=2q4α2−ℏ2+O(q2).(D16.9)\begin{aligned} u-\alpha^2 &=-\sqrt q(c_1+c_{-1})+O(q^2)\\ &=q\left[\frac{1}{\alpha^2-(\alpha+\hbar)^2} +\frac{1}{\alpha^2-(\alpha-\hbar)^2}\right]+O(q^2)\\ &=\frac{2q}{4\alpha^2-\hbar^2}+O(q^2). \end{aligned} \tag{D16.9}

This is the promised match, including sign, denominator and scale. Odd powers of q\sqrt q vanish on an isolated branch because changing q\sqrt q to −q-\sqrt q is the unitary translation θ↦θ+π\theta\mapsto\theta+\pi.

For ordinary nondegenerate perturbation theory require 2α/ℏ∉Z2\alpha/\hbar\notin\mathbb Z and a small potential relative to the relevant free-level separations. The first displayed coefficient sees the resonances 2α=±ℏ2\alpha=\pm\hbar; higher orders see further mode collisions.

As a numerical example, choose mass units with ℏ=1\hbar=1, α=1/3\alpha=1/3, q=10−4q=10^{-4}. The free value is 1/91/9 and the first correction is −3.6×10−4-3.6\times10^{-4}. Direct diagonalization of the Fourier operator gives

u=0.11075141308533925847…,∣u−(19−0.00036)∣≃3.02×10−7.(D16.10)u=0.11075141308533925847\ldots, \qquad \left|u-\left(\frac19-0.00036\right)\right| \simeq3.02\times10^{-7}. \tag{D16.10}

The negative shift is expected: this free mode lies below its coupled neighbors. It is not a negative instanton probability; the connected holomorphic coefficient is not a probability distribution.

A separate check integrates the original second-order ODE over one cell. Its fundamental matrix has determinant one because the Wronskian is constant. At the eigenvalue its trace must be 2cos⁡(2πα/ℏ)2\cos(2\pi\alpha/\hbar). This checks the boundary phase independently of the Fourier matrix. Successive step sizes give the expected fourth-order convergence; numerical precision alone is not an estimate of integration error.

Recover a classical period without changing the question

Section titled “Recover a classical period without changing the question”

Set ψ=exp⁡[(i/ℏ)∫P dθ]\psi=\exp[(i/\hbar)\int P\,d\theta]. Substitution into (D16.8) gives

P2−iℏP′=u+2qcos⁡θ.(D16.11)P^2-i\hbar P'=u+2\sqrt q\cos\theta. \tag{D16.11}

This is a first-order nonlinear equation for the logarithmic derivative of the wave. A WKB expansion means solving it in powers of ℏ\hbar. Its leading term is P0=u+2qcos⁡θP_0=\sqrt{u+2\sqrt q\cos\theta}, on a chosen branch. The next term is P1=iP0′/(2P0)P_1=iP_0'/(2P_0); its integral vanishes on a rotation contour with no zero or winding of P0P_0.

For u>2qu>2\sqrt q, expand the leading period:

αcl=12π∫02πP0 dθ=u(1−q4u2−15q264u4+⋯ ).(D16.12)\alpha_{\rm cl} =\frac1{2\pi}\int_0^{2\pi}P_0\,d\theta =\sqrt u\left(1-\frac{q}{4u^2} -\frac{15q^2}{64u^4}+\cdots\right). \tag{D16.12}

The linear cosine averages to zero; its square averages to 1/21/2. Inversion begins with u=αcl2+q/(2αcl2)+⋯u=\alpha_{\rm cl}^2+q/(2\alpha_{\rm cl}^2)+\cdots, agreeing with (D16.9) as ℏ→0\hbar\to0 coefficient by coefficient.

At finite ℏ\hbar, the continued α\alpha is a quantum action/Floquet coordinate. It must not simply be substituted for the undeformed physical period in a four-dimensional BPS mass formula. Nor does the coefficientwise limit prove uniform convergence of a chosen eigenvalue branch: the conditions 2α/ℏ∈Z2\alpha/\hbar\in\mathbb Z accumulate as ℏ→0\hbar\to0 at fixed α\alpha.

A controlled variation: resolve the first resonance

Section titled “A controlled variation: resolve the first resonance”

Let α=ℏ/2+δ\alpha=\hbar/2+\delta, with ∣δ∣≪ℏ|\delta|\ll\hbar. The free modes 00 and −1-1 are now close. Keeping their mixing exactly gives

Hpair=((ℏ/2+δ)2−q−q(−ℏ/2+δ)2),u±pair=ℏ24+δ2±ℏ2δ2+q.(D16.13)H_{\rm pair}= \begin{pmatrix} (\hbar/2+\delta)^2&-\sqrt q\\ -\sqrt q&(-\hbar/2+\delta)^2 \end{pmatrix}, \qquad u_\pm^{\rm pair} =\frac{\hbar^2}{4}+\delta^2 \pm\sqrt{\hbar^2\delta^2+q}. \tag{D16.13}

The other free modes are separated by order ℏ2\hbar^2. For q≪ℏ2\sqrt q\ll\hbar^2 their leading effect is of order q/ℏ2q/\hbar^2. At exact resonance the leading gap is 2q2\sqrt q, and both eigenvalues remain finite. The expansion in integer powers of qq has failed because it divided by the splitting of two states that had to be diagonalized together.

For ℏ=1\hbar=1, q=10−4q=10^{-4}, the full Fourier problem gives a gap 0.0199995000153…0.0199995000153\ldots, close to 0.020.02. The midpoint is 0.2499499995834…0.2499499995834\ldots, rather than exactly 1/41/4: remote modes also contribute. Halving q\sqrt q tests both the leading gap and the correction scaling.

This is a bounded research-training extension, not a newly discovered spectrum. A useful deliverable is a table over the dimensionless ratio ℏδ/q\hbar\delta/\sqrt q at fixed ℏ\hbar comparing (i) ordinary one-instanton order, (ii) the two-state approximation, and (iii) a converged ODE or Fourier calculation. Record the free gap, the cutoff residual and the numerical step error separately. Agreement only away from δ=0\delta=0 diagnoses nonuniform perturbation theory, rather than a failure of the differential equation or a new singularity of the undeformed Coulomb branch.

1. Continue one more order without claiming two instantons

Section titled “1. Continue one more order without claiming two instantons”

For the same circle problem, normalize the Fourier coefficient c0=1c_0=1 and use (dn−u)cn=q(cn−1+cn+1)(d_n-u)c_n=\sqrt q(c_{n-1}+c_{n+1}). Find the coefficient of q2q^2 in uu. Determine the connected NS coefficient that a future two-instanton calculation would have to reproduce, and check the classical limit.

Hint 1

The n=±2n=\pm2 modes first enter at order qq. Retain the order-qq shift of uu in the denominators for c±1c_{\pm1}.

Hint 2

Let Dn=dn−d0D_n=d_n-d_0 and A=2/(4α2−ℏ2)A=2/(4\alpha^2-\hbar^2). The coefficient is −∑η=±1[A/Dη2+1/(Dη2D2η)]-\sum_{\eta=\pm1}[A/D_\eta^2+1/(D_\eta^2D_{2\eta})].

Solution

Writing g=qg=\sqrt q, the recurrence gives cη=g/Dη+g3[A/Dη2+1/(Dη2D2η)]+O(g5)c_\eta=g/D_\eta+g^3[A/D_\eta^2+1/(D_\eta^2D_{2\eta})]+O(g^5). Here the second term comes from c2η=g2/(DηD2η)+O(g4)c_{2\eta}=g^2/(D_\eta D_{2\eta})+O(g^4) and from expanding Dη−(u−d0)D_\eta-(u-d_0). Use u−d0=−g(c−1+c1)u-d_0=-g(c_{-1}+c_1) to obtain

u=α2+2q4α2−ℏ2+2(20α2+7ℏ2)q2(4α2−ℏ2)3(4α2−4ℏ2)+O(q3).u=\alpha^2+\frac{2q}{4\alpha^2-\hbar^2} +\frac{2(20\alpha^2+7\hbar^2)q^2} {(4\alpha^2-\hbar^2)^3(4\alpha^2-4\hbar^2)} +O(q^3).

The required q2q^2 coefficient of FNS,inst\mathscr F_{\rm NS,inst} is half the displayed coefficient, by (D16.6). We have derived an ODE prediction, not performed the two-instanton fixed-point sum. As ℏ→0\hbar\to0, the energy coefficient becomes 5/(32α6)5/(32\alpha^6). Squaring (D16.12) gives αcl2=u−q/(2u)−13q2/(32u3)+⋯\alpha_{\rm cl}^2=u-q/(2u)-13q^2/(32u^3)+\cdots; inversion reproduces the same 5/325/32. The poles at α=±ℏ\alpha=\pm\hbar mark new free-mode degeneracies relevant at this order.

2. Estimate the contribution of the remote modes

Section titled “2. Estimate the contribution of the remote modes”

At α=ℏ/2\alpha=\hbar/2, derive the leading common shift of the two resonant levels from the modes n=1,−2n=1,-2. Explain why this correction changes the midpoint before it changes the leading gap. Compare its value with the numerical example.

Hint 1

The pair eigenvectors are (∣0⟩±∣−1⟩)/2(|0\rangle\pm|-1\rangle)/\sqrt2. Each remote mode couples to only one component.

Hint 2

To leading order in qq, both energy denominators are ℏ2/4−9ℏ2/4=−2ℏ2\hbar^2/4-9\hbar^2/4=-2\hbar^2.

Solution

Each coupling has squared modulus q/2q/2. Summing over the two remote modes gives 2(q/2)/(−2ℏ2)=−q/(2ℏ2)2(q/2)/(-2\hbar^2)=-q/(2\hbar^2) for either pair state. Thus

u±=ℏ24±q−q2ℏ2+O(q3/2/ℏ4).u_\pm=\frac{\hbar^2}{4}\pm\sqrt q-\frac{q}{2\hbar^2} +O(q^{3/2}/\hbar^4).

The common shift cancels in the gap, leaving 2q2\sqrt q at leading order. For ℏ=1\hbar=1, q=10−4q=10^{-4} the predicted midpoint is 0.249950.24995, in agreement with 0.2499499995834…0.2499499995834\ldots. The remaining gap correction is smaller by a relative factor of order q/ℏ4q/\hbar^4. This calculation requires q/ℏ2≪1\sqrt q/\hbar^2\ll1; it does not authorize using the two-state matrix at arbitrary potential strength.

3. A change of phase and a change of spectral problem

Section titled “3. A change of phase and a change of spectral problem”

Replace cos⁡θ\cos\theta by cos⁡(θ+φ)\cos(\theta+\varphi) for real φ\varphi. Determine whether the eigenvalues and Floquet multiplier change. Then explain why replacing the circle by a real line with a cosh⁡x\cosh x potential is a different problem, even though the potentials are related by analytic continuation.

Hint 1

Translate the coordinate, or multiply Fourier coefficient cnc_n by a phase. Check the boundary condition as well as the differential expression.

Hint 2

For the line problem, ask what replaces the return phase after one period.

Solution

The translation operator ψ(θ)↦ψ(θ+φ)\psi(\theta)\mapsto\psi(\theta+\varphi) is unitary on the same quasi-periodic domain. It preserves the derivative seam and multiplier. Equivalently the two neighboring Fourier entries gain conjugate factors e±iφe^{\pm i\varphi}, removable by a diagonal unitary matrix. Every eigenvalue is unchanged.

Analytically continuing θ\theta to an imaginary coordinate changes the real contour, kinetic sign and admissible wavefunctions. For a confining positive cosh⁡x\cosh x problem on R\mathbb R, square integrability requires decay at both ends; there is no circle multiplier to hold fixed. An analytic continuation of a differential expression alone does not establish a unitary equivalence of these domains. One must translate scales and specify a connection or quantization condition. This is the type A/type B distinction in NS, rather than a new choice of four-dimensional electric charge unit.

The literature check for this dossier is dated 20 October 2026. Nekrasov supplies the instanton construction; NS identifies the retained-deformation limit and distinguishes its spectral problems. Poghossian supplies the scalar-observable relation used above. Başar and Dunne analyze why perturbative periods and nonperturbative band or gap information must be distinguished. Our one-coefficient and two-state calculations reproduce established structures; neither is a novelty claim.

The later François–Grassi study, published June 2026, constructs entire off-shell eigenfunctions in a different spectral/topological-string setting and studies modified-Mathieu limits. “Off-shell” there concerns an eigenvalue parameter before spectral quantization. It does not turn our circle calculation into a proof of that construction.

There is also a separate conformal-block branch: AGT section 4 connects the four-flavor SU(2)SU(2) problem to Liouville four-point data, distinguishing the instanton block from the full correlator. That continuation needs a mass/momentum map, the Abelian prefactor and a dimensionless coupling; our dimension-four qq cannot be substituted for its cross-ratio.

The next achievable task is to calculate the actual two-instanton connected term and compare it with Exercise 1, at generic α,ℏ\alpha,\hbar before approaching resonance. A discrepancy by two suggests confusion between the logarithm and the quadratic observable; a wrong denominator sign suggests a lost ϵ1=iℏ\epsilon_1=i\hbar continuation. Agreement establishes a further local coefficient. It does not establish all-order equality, a unique nonperturbative completion, or a spectrum without boundary conditions.