Abstract
We describe the exact WKB method from the point of view of abelianization, both for Schrödinger operators and for their higher-order analogues (opers). The main new example which we consider is the “\(T_3\) equation,” an order 3 equation on the thrice-punctured sphere, with regular singularities at the punctures. In this case the exact WKB analysis leads to consideration of a new sort of Darboux coordinate system on a moduli space of flat \({\mathrm {SL}}(3)\)-connections. We give the simplest example of such a coordinate system, and verify numerically that in these coordinates the monodromy of the \(T_3\) equation has the expected asymptotic properties. We also briefly revisit the Schrödinger equation with cubic potential and the Mathieu equation from the point of view of abelianization.
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Notes
Throughout this paper \({\mathrm {SL}}(K)\) means \({\mathrm {SL}}(K,\mathbb {C})\), and \({\mathrm {GL}}(1)\) means \({\mathrm {GL}}(1,\mathbb {C}) = \mathbb {C}^\times \).
In the main text we will distinguish several different variants of the functions \(\mathcal {X}_\gamma \). The functions \(\mathcal {X}_\gamma ^{\mathrm {intro}}\) we use in the introduction are related to those appearing in the main text by \(\mathcal {X}_\gamma ^{\mathrm {intro}}(\hbar ) = \mathcal {X}_\gamma ^{\vartheta = \arg \hbar }(\hbar )\).
Here and elsewhere in this paper, unless explicitly noted, \(\sqrt{\cdot }\) denotes the principal branch of the square root.
For a more elementary example, if a function \(x(\hbar )\) is known to be holomorphic for \(\hbar \in \mathbb {C}^\times \), \(x(\hbar ) \rightarrow c\) as \(\hbar \rightarrow 0\), and \(x(\hbar )\) is bounded as \(\hbar \rightarrow \infty \), then we can conclude \(x(\hbar ) = c\).
The family of flat connections \(\nabla _{R,\zeta }\) arises from a solution \((D,\varphi )\) of Hitchin’s equations, through the formula \(\nabla _{R,\zeta } = R \zeta ^{-1} \varphi + D + R \zeta \varphi ^\dagger \).
In comparing to the ordinary Schrödinger equation on the real line we would have \(P = 2(E-V)\).
In the important special case of \(\hbar \)-independent P, we just have \(p = P\).
In the WKB literature it is common to write the two square roots simply as \(\pm \mathrm {i}\sqrt{p}\), and label the two sheets as \(+\), − instead of i, j.
This has been a folk-theorem for some time, at least for the case of p with sufficiently generic residues, and a proof has been announced by Koike-Schäfke. See [6] for an account.
Since \(y_j = -y_i\) we could also have just written that \(\mathrm {e}^{-\mathrm {i}\vartheta } y_i\) is positive, and we could have labeled the curve just by the single index i instead of the ordered pair ij. Our redundant-looking notation is chosen with an eye toward the generalization to higher-order equations, in Sect. 5 below.
The gluing rule (2.11) should be regarded as a version of the “WKB connection formula.”
When C is a compact Riemann surface of genus g, to see that \((-1)^{\frac{1}{2}w}\) does not depend on which side we call the “inside” of \(\gamma \), we use the fact that a holomorphic quadratic differential has \(4g-4\) zeroes, which is divisible by 4.
In a generic situation the Stokes automorphisms which can occur are of the form \(\mathcal {X}_\mu \rightarrow \mathcal {X}_\mu (1 \pm \mathcal {X}_\gamma )^{\Omega (\gamma ) \langle \gamma ,\mu \rangle }\), where \(\Omega (\gamma ) = +1\) for a “flip” of the Stokes graph and \(\Omega (\gamma ) = -2\) for a “juggle” of the Stokes graph, in the terminology of [15]. The active rays corresponding to flips are typically isolated in the \(\hbar \)-plane, while juggles occur at the limit of infinite sequences of flips. A general algorithm for computing the Stokes automorphism from a Stokes graph at the BPS locus is given in [16].
In the cluster algebra literature this object is called the “Donaldson–Thomas transformation” or “DT transformation” following [60].
This follows from the realization of \(\lambda _j^\vartheta \) as the Borel summation of the WKB series, which implies that \(\lambda _j^\vartheta \mathrm {d}z\) is negative along \(\ell _n\), since every term of the series has this property.
The reader might wonder: what about the other solution, where \(\mathcal {X}_A = \mathcal {X}_B = \frac{1 + \sqrt{5}}{2}\)? That one turns out to be associated to a Schrödinger equation with singular potential, \(P(z) = z^3 - \frac{3}{4} \frac{\hbar ^2}{z^2}\). The specific coefficient \(-\frac{3}{4} \hbar ^2\) here ensures that the singularity at \(z=0\) is only an “apparent singularity,” with trivial monodromy; thus this equation is still associated to a flat connection \(\nabla \) in the plane, and all our discussion of abelianization applies equally well to this case. Moreover this equation still has the \(\mathbb {Z}/ 5\mathbb {Z}\) symmetry (because the two terms \(z^3\) and \(1/z^2\) differ by a factor \(z^5\)), and numerically one checks that it has \(\mathcal {X}_A = \mathcal {X}_B = \frac{1 + \sqrt{5}}{2}\). We thank Dylan Allegretti and Tom Bridgeland for several enlightening conversations about Schrödinger equations with apparent singularities.
In particular, it seems to be harder to find a solution of the integral equations (2.19) directly by iteration in this case. Instead one can start with a slightly different system of integral equations, those used in [73]; these one can solve by iteration; then one can take the limit \(R \rightarrow 0\), \(\zeta \rightarrow 0\), \(\hbar = R / \zeta \), to get solutions of (2.19).
In this context the quantity \(\frac{1}{2} Z_B\) might be called a “1-instanton action” since it corresponds to the change in the exponent of a WKB solution upon integrating along a one-way path from one branch point to another, as opposed to \(Z_B\) which is the integral over the round-trip path \(\gamma _B\).
As a check against blunders, we numerically computed the width of a few of the gaps and obtained reasonable agreement: for example, when \(\hbar = 0.2\), there is a gap extending from \(E_- \approx 1.3836418\) to \(E_+ \approx 1.3838946\), which thus has \(\delta E = \frac{1}{2}(E_+ - E_-) \approx 0.0001264\), while the estimate (4.32) gives \(\delta E \approx 0.0001278\).
Some evidence for this conjecture has been given in [76]. We thank Kohei Iwaki for pointing out this reference.
As in the order 2 case (see Sect. 2.3) this is not the only possible choice, but it is the most invariant choice.
Our conventions here differ from those of [34] by the replacement \(u \rightarrow -u\). Sorry.
In the order 2 case, some of the necessary analytic technology for dealing with wild Stokes graphs is developed in [77]. It would be exciting to develop the higher-rank analogue of this.
A useful reference on quadratic transformations is [78].
We have no great insight into why this identity is true, although we have checked it in Mathematica; it is a specialization of a “remarkable identity” originally due to Zagier, given as equation 14 in [79].
In particular this seems to be much more efficient than trying to solve the coplanarity constraints (6.3) directly.
The triangulation is made up of 2 triangles, whose interiors are \(\{|z| < 1\}\) and \(\{|z| > 1\}\).
The results of [34] show that \(\Omega (\gamma ) \ne 0\) for every primitive charge \(\gamma \), so all of the countably many phases \(\vartheta \) which could give nontrivial \(\mathbf {T}_\vartheta \) indeed do.
We thank David Ben-Zvi for explaining this point to us.
Here is a heuristic way to understand why \(L_\gamma \) can be wrapped supersymmetrically around the circle. Suppose \(\hbar \) is real. We imagine lifting the 4-dimensional theory to a 5-dimensional theory on an \(\mathbb {R}^4\) bundle over \(S^1\), where the \(S^1\) base has length \(\rho \), and the \(x_2\)-\(x_3\) plane in the fiber is rotated by an angle \(\rho \hbar \) as we go around the \(S^1\) base. In the limit \(\rho \rightarrow 0\) this gives rise to an effectively 4-dimensional theory, which can be identified with the \(\Omega \)-background deformation of the original theory. On the other hand, this 5-dimensional background is locally Euclidean space, and in the 5-dimensional theory, we can put the line defect \(L_\gamma \) supersymmetrically on any straight line. We choose a straight line in the \(x_4\) direction, beginning at some point \((x_0,x_1,x_2,x_3,x_4 = 0)\). After going around the \(S^1\) fiber this line will return to \((x_0,x_1,x'_2,x'_3,x_4 = 0)\) where \((x'_2,x'_3)\) is the image of \((x_2,x_3)\) under rotation by an angle \(\rho \hbar \). If \(\rho \hbar = \frac{2\pi }{N}\), then after going around N times, the line closes up to a loop, which pierces the \(\mathbb {R}^4\) fiber in N points arranged around a circle in the \(x_2\)-\(x_3\) plane. In the limit as \(\rho \rightarrow 0\) ie \(N \rightarrow \infty \), these N points just look like a line wrapped around the circle.
By a change of variable introduced in [81], \(\mathcal {M}(\mathfrak {g},C,\hbar )\) can be identified with the moduli space of the theory without \(\Omega \)-background, compactified on a circle of radius \(R = |\hbar |^{-1}\). This moduli space is hyperkähler, with complex structures labeled by \(\zeta \in \mathbb {CP}^1\); the boundary condition we get preserves the subalgebra labeled by \(\zeta = \frac{\hbar }{|\hbar |}\).
In conformal theories \(\widetilde{\mathcal {F}}\) depends only on the \(\widetilde{Z}_{A_i}\) and not on \(\hbar \). In non-conformal theories there are complex parameters \(m_i\) with the dimension of mass, and then \(\widetilde{\mathcal {F}}\) depends on \(\hbar \) through the combinations \(m_i / \hbar \).
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Acknowledgements
We thank Dylan Allegretti, Tom Bridgeland, Gerald Dunne, Dan Freed, Marco Gualtieri, Kohei Iwaki, Saebyeok Jeong, Anton Leykin, Marcos Mariño, Nikita Nikolaev, Shinji Sasaki, Bernd Sturmfels and Joerg Teschner for useful and enlightening discussions. LH’s work is supported by a Royal Society Dorothy Hodgkin Fellowship. AN’s work on this paper was supported by NSF grant DMS-1711692 and by a Simons Fellowship in Mathematics.
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A Computations of Spectral Coordinates
A Computations of Spectral Coordinates
In this appendix we give some computations omitted from the main text.
1.1 A.1 Computations for the cubic potential
Computation of (3.3). We will only describe the computation for \(\mathcal {X}_A\); that for \(\mathcal {X}_B\) is similar.
We need to compute the parallel transport of \(\nabla ^\mathrm {ab}\) along a path in the homology class \(\gamma _A\). To compute concretely it is convenient to work relative to bases of \(\nabla ^\mathrm {ab}\)-flat sections in each domain. Each local \(\nabla ^\mathrm {ab}\)-flat section corresponds to a local \(\nabla \)-flat section, and by continuation we can think of all these local flat sections as lying in a single 2-dimensional vector space V, the space of global \(\nabla \)-flat sections over the plane. See Fig. 18.
Relative to these local bases, the parallel transport within each domain is just represented by 1, and the only nontrivial part is the gluing factor from (2.11):
-
When we cross a single wall of type ij on sheet i, from side L to side R, we get a factor
$$\begin{aligned} \frac{[\psi _i^L, \psi _j^L]}{[\psi _i^R, \psi _j^L]}. \end{aligned}$$(A.1) -
When we cross a single wall of type ij on sheet j, we also get a gluing factor, but this factor is just 1 if \(\psi _j^L = \psi _j^R\), which it always is in this example.
The representative of \(\gamma _A\) shown in Fig. 18 crosses six walls; multiplying the factors for these six crossings, starting from the eastmost region, gives
matching (3.3) as desired.
1.2 A.2 Computations for the Mathieu equation
Computation of (4.5). We need to compute the parallel transport of \(\nabla ^\mathrm {ab}\) along a path in the homology class \(\gamma _B\). We use the path given in Fig. 6.
As above, it is convenient to work relative to bases of \(\nabla ^\mathrm {ab}\)-flat sections in each domain. See Fig. 19. Again by continuation we think of all these local flat sections as lying in a single 2-dimensional vector space V. In this case there is an added technical difficulty: the monodromy around \(z = 0\) means there are no global \(\nabla \)-flat sections. Instead we identify V as the space of \(\nabla \)-flat sections on the complement of the blue dashed line (“monodromy cut”).
Again the only nontrivial part of the parallel transport is the gluing factors appearing in (2.11), (2.12), When we cross a double wall on sheet i, from side L to side R, we get a factor
and when we cross a single wall of type ij on sheet i, from side L to side R, we get a factor
We can further simplify these factors by choosing bases with \([\psi _1, \psi _2] = 1\), \([\psi '_1 , \psi '_2] = 1\), \([\psi ''_1, \psi ''_2] = 1\). Then starting from the southwest corner, the gluing factors we encounter are
Using \(M \psi ''_1 = \mu \psi ''_1\), \(M \psi ''_2 = \mu ^{-1} \psi _2\), and \(M \psi _1 = \psi _2\), \(M \psi '_1 = \psi '_2\), this reduces to
which matches the desired (4.5).
Computation of (4.21). Just as above, all we need to compute are the gluing factors along the paths \(\gamma _A\) and \(\gamma _B\), with respect to the bases shown in Fig. 20.
We can choose \([\psi , \psi '] = 1\) to simplify. In going around \(\gamma _A\) we only meet one wall, with the gluing factor
To fix the branch we would need to carefully implement the WKB prescription from Sect. 2.3, which we do not do here.
For \(\gamma _B\) the product of gluing factors, starting from the southeast, is
The results (A.7), (A.8) match the desired (4.21).
1.3 A.3 Computations for the \(T_3\) equation
Abelianizations and adapted bases. Suppose we have a \(\mathcal {W}\)-abelianization of the \(T_3\) equation. Then we can choose bases compatible with the \(\mathcal {W}\)-abelianization in the various domains of Fig. 21, as shown.
In writing the form of these bases we began by labeling the basis in the middle as \((\psi _1,\psi _2,\psi _3)\) and then used the facts that:
-
According to (5.6) the k-th projective basis element does not change when we cross a wall of type ij and ji (this implies e.g. that the first basis element in the northeast region must be \(\psi _1\)),
-
Crossing a branch cut of the covering \(\Sigma \rightarrow C\) (orange in Fig. 21) permutes the projective basis elements,
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The projective bases on the two sides of a monodromy cut (blue in Fig. 21) differ by the monodromy (\(\mathbf {A}\), \(\mathbf {B}\) or \(\mathbf {C}\)) attached to the cut.
One key fact remains to be used: again by (5.6), for a wall of type ij and ji, the plane spanned by the i-th and j-th basis elements is the same on both sides of the wall. Applying this to the northeast wall, which is of type 23 and 32, leads to the condition that
which is (6.3b); doing similarly for the other two walls gives the other two parts of (6.3). Thus, the basis \((\psi _1, \psi _2, \psi _3)\) is indeed a basis in special position. Conversely, given a basis \((\psi _1, \psi _2, \psi _3)\) in special position, the local bases shown in Fig. 21 give a \(\mathcal {W}\)-abelianization. This shows the claimed identification between \(\mathcal {W}\)-abelianizations and bases in special position.
Computation of (6.18). As above, all we need to compute are the gluing factors along the paths representing \(\gamma _A\) and \(\gamma _B\) shown in Fig. 13. These factors are given by (5.6): for a wall of type ij and ji, and a path on sheet i, the factor is
Since all the walls are double, we will not need to use (5.5) anywhere.
For \(\gamma _A\) the computation is particularly simple: only two of the four crossings give a nontrivial factor, namely the places where the path crosses the 23–32 wall. This gives directly
matching (6.18a) as desired. The computation giving \(\mathcal {X}_B\) is similar but a little longer since three of the four crossings give nontrivial factors: thus we have altogether 6 factors in numerator and denominator; one common factor cancels, leaving the desired (6.18b).
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Hollands, L., Neitzke, A. Exact WKB and Abelianization for the \(T_3\) Equation. Commun. Math. Phys. 380, 131–186 (2020). https://doi.org/10.1007/s00220-020-03875-1
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DOI: https://doi.org/10.1007/s00220-020-03875-1