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Dubrovin conjecture and the second structure connection

John Alexander Cruz Morales Departamento de matemáticas, Universidad Nacional de Colombia, sede Bogotá, Colombia School of Mathematical Sciences, University of Science and Technology of China, Hefei 230026, P.R. China [email protected]  and  Todor Milanov Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan [email protected]
Abstract.

We give a reformulation of the Dubrovin conjecture about the semisimplicity of quantum cohomology in terms of the so-called second structure connection of quantum cohomology. The key ingredient in our work is the notion of a twisted reflection vector which allows us to give an elegant description of the monodromy data of the quantum connection in terms of the monodromy data of its Laplace transform.

Key words and phrases: Gromov–Witten theory, Frobenius manifolds, Stokes multipliers

1. Introduction

1.1. Semi-simple quantum cohomology

Let XX be a smooth projective variety of complex dimension DD. The Gromov–Witten (GW) invariants of XX are defined via the intersection theory on the moduli space of stable maps ¯g,n(X,d)\overline{\mathcal{M}}_{g,n}(X,d) (see Section 3.1 for more details). The structure of the GW invariants is best understood in genus g=0g=0. Namely, the entire information is contained in a certain deformation of the classical cup product, known as the quantum cup product. Let us fix a homogeneous basis ϕi\phi_{i} (1iN1\leq i\leq N) of H(X,)H^{*}(X,\mathbb{C}). Then the quantum cup product \bullet is defined by

(ϕiϕj,ϕk)=l=0dQdl!ϕi,ϕj,ϕk,t,,t0,3+l,d,\displaystyle(\phi_{i}\bullet\phi_{j},\phi_{k})=\sum_{l=0}^{\infty}\sum_{d}\frac{Q^{d}}{l!}\langle\phi_{i},\phi_{j},\phi_{k},t,\dots,t\rangle_{0,3+l,d},

where the second sum is over all effective curve classes dH2(X,)d\in H_{2}(X,\mathbb{Z}), Q=(q1,,qr)Q=(q_{1},\dots,q_{r}) are the so-called Novikov variables, and t=i=1NtiϕiH(X,)t=\sum_{i=1}^{N}t_{i}\phi_{i}\in H^{*}(X,\mathbb{C}). The Novikov variables correspond to a choice of an ample basis p1,,prp_{1},\dots,p_{r} of H2(X,Z)H1,1(X,)H^{2}(X,Z)\cap H^{1,1}(X,\mathbb{C}) and Qd:=q1p1,dqrpr,dQ^{d}:=q_{1}^{\langle p_{1},d\rangle}\cdots q_{r}^{\langle p_{r},d\rangle}. Let us assume that ϕ1=1\phi_{1}=1 and ϕi+1=pi\phi_{i+1}=p_{i}. Then the structure constants of the quantum cup product belong to the following ring of formal power series

[[Q,t]]:=[[q1et2,,qretr+1,tr+2,,tN]],\displaystyle\mathbb{C}[\![Q,t]\!]:=\mathbb{C}[\![q_{1}e^{t_{2}},\dots,q_{r}e^{t_{r+1}},t_{r+2},\dots,t_{N}]\!],

where the fact that there is a dependence on qieti+1q_{i}e^{t_{i+1}} is a consequence of the so-called divisor equation (see [25]). The quantum cup product turns QH(X,):=H(X,[[Q,t]])QH(X,\mathbb{C}):=H^{*}(X,\mathbb{C}[\![Q,t]\!]) into a commutative associative algebra known as the big quantum cohomology of XX. We say that the quantum cohomology is semi-simple if QH(X,)QH(X,\mathbb{C}) is a semi-simple algebra, or equivalently the operators ϕ\phi\bullet of quantum multiplication by ϕH(X,)\phi\in H^{*}(X,\mathbb{C}) are not nilpotent. In the limit Q0Q\to 0, the quantum product becomes the classical cup product and since ϕ\phi\cup is always nilpotent (for ϕ1\phi\neq 1), we see that semi-simplicity is an indication that the manifold XX has sufficiently many rational curves. From that point of view it is very interesting to classify manifolds with semi-simple quantum cohomology. It is an observation of Alexey Bondal that semi-simplicity can be characterized using the language of derived categories. In his ICM talk in 1998, following Bondal’s ideas, Dubrovin was able to formulate a precise conjecture which is now known as the Dubrovin conjecture (see [9] and Conjecture 3.3.1). The goal of this paper is to answer a question which was raised by the second author in his joint work [26]. Namely, there is a conjectural description (see [26], Conjecture 1.6) of the so-called reflection vectors in quantum cohomology in terms of exceptional collections in the derived category. More precisely, Milanov–Xia were able to construct reflection vectors in the quantum cohomology of the blowup of a manifold relying only on certain vanishing results for GW invariants. The resulting formulas were very similar to the formulas for the central connection matrix conjectured by Galkin–Golyshev–Iritani in [13] and later on by Cotti–Dubrovin–Guzzetti [6]. The question is whether one can reformulate Dubrovin’s conjecture in terms of reflection vectors. As expected, the answer is yes and in this paper we would like to work out the precise relation between the reflection vectors and the monodromy data which enters the Dubrovin conjecture. Our main message is that by constructing a basis of reflection vectors in quantum cohomology one can obtain a proof of the Γ\Gamma-Conjecture II of Galkin–Golyshev–Iritani (see [13]) or equivalently the refined Dubrovin conjecture of Cotti–Dubrovin–Guzzetti (see [6], Conjecture 5.2). In the rest of this introduction we would like to formulate our results.

1.2. Quantum differential equations

From now on we are going to assume that quantum cohomology is semi-simple and convergent. The latter means that there exists a domain MH(X,)M\subseteq H^{*}(X,\mathbb{C}), such that, the formal power series representing the structure constants are convergent. Let us introduce the following two linear operators:

θ:H(X,)H(X,),θ(ϕi)=(D2deg(ϕi))ϕi\displaystyle\theta:H^{*}(X,\mathbb{C})\to H^{*}(X,\mathbb{C}),\quad\theta(\phi_{i})=\Big{(}\frac{D}{2}-\operatorname{deg}_{\mathbb{C}}(\phi_{i})\Big{)}\phi_{i}

and

ρ:H(X,)H(X,),ρ(ϕ)=c1(TX)ϕ,\displaystyle\rho:H^{*}(X,\mathbb{C})\to H^{*}(X,\mathbb{C}),\quad\rho(\phi)=c_{1}(TX)\cup\phi,

where deg(ϕ):=k\operatorname{deg}_{\mathbb{C}}(\phi):=k for ϕH2k(X,)\phi\in H^{2k}(X,\mathbb{C}) and \cup is the classical cup product. The quantum differential equations are by definition the differential equations of the following system of ODEs:

(1) ztiJ(t,z)\displaystyle z\partial_{t_{i}}J(t,z) =\displaystyle= Ai(t)J(t,z),1iN,\displaystyle A_{i}(t)J(t,z),\quad 1\leq i\leq N,
(2) (zz+E)J(t,z)\displaystyle(z\partial_{z}+E)J(t,z) =\displaystyle= θJ(t,z),\displaystyle\theta J(t,z),

where J(t,z)H(X,)J(t,z)\in H^{*}(X,\mathbb{C}), Ai(t)=ϕiA_{i}(t)=\phi_{i}\bullet is the operator of quantum multiplication by ϕi\phi_{i}, and

E=c1(X)+i=1N(1deg(ϕi))titi\displaystyle E=c_{1}(X)+\sum_{i=1}^{N}\Big{(}1-\mathrm{deg}_{\mathbb{C}}(\phi_{i})\Big{)}t_{i}\frac{\partial}{\partial t_{i}}

is the Euler vector field. The differential equations (1)–(2) can be viewed also as the equations defining the horizontal sections of a connection on the vector bundle TM×M×TM\times\mathbb{C}^{*}\to M\times\mathbb{C}^{*} which is sometimes called quantum connection or Dubrovin connection.

The differential equation with respect to zz has two singularities: regular at z=z=\infty and irregular at z=0z=0. Near z=z=\infty there is a geometric way to construct a fundamental solution. Namely, let us define S(t,z)=1+S1(t)z1+S2(t)z2+S(t,z)=1+S_{1}(t)z^{-1}+S_{2}(t)z^{-2}+\cdots where Sk(t)End(H(X,))S_{k}(t)\in\operatorname{End}(H^{*}(X,\mathbb{C})) are linear operators defined by

(Sk(t)ϕi,ϕj)=l=0dQdl!ϕiψk1,ϕj,t,,t0,2+l,d.\displaystyle(S_{k}(t)\phi_{i},\phi_{j})=\sum_{l=0}^{\infty}\sum_{d}\frac{Q^{d}}{l!}\langle\phi_{i}\psi^{k-1},\phi_{j},t,\dots,t\rangle_{0,2+l,d}.

Then S(t,z)zθzρS(t,z)z^{\theta}z^{-\rho} is a solution to the system (1)–(2).

The singularity at z=0z=0 has an interesting Stokes phenomenon. Namely, suppose that (u1,,uN)(u_{1},\dots,u_{N}) are the canonical coordinates defined in a neighborhood of some semi-simple point tMt^{\circ}\in M. By definition, the quantum product and the Poincaré pairing become diagonal:

uiuj=δijuj,(ui,uj)=δij/Δi,\displaystyle\frac{\partial}{\partial u_{i}}\bullet\frac{\partial}{\partial u_{j}}=\delta_{ij}\frac{\partial}{\partial u_{j}},\quad\Big{(}\frac{\partial}{\partial u_{i}},\frac{\partial}{\partial u_{j}}\Big{)}=\delta_{ij}/\Delta_{i},

where Δi𝒪M,t\Delta_{i}\in\mathcal{O}_{M,t^{\circ}} are some holomorphic functions. Let us define the linear map

(3) Ψ:NH(X,),Ψ(ei)=Δiui=a=1NΔitauiϕa.\Psi:\mathbb{C}^{N}\to H^{*}(X,\mathbb{C}),\quad\Psi(e_{i})=\sqrt{\Delta_{i}}\frac{\partial}{\partial u_{i}}=\sum_{a=1}^{N}\sqrt{\Delta_{i}}\frac{\partial t_{a}}{\partial u_{i}}\,\phi_{a}.

We may think of Ψ\Psi as a N×NN\times N matrix with entries Ψai=Δitaui\Psi_{ai}=\sqrt{\Delta_{i}}\frac{\partial t_{a}}{\partial u_{i}}. Let U=diag(u1,,uN)U=\operatorname{diag}(u_{1},\dots,u_{N}) be the diagonal matrix. There exists a unique formal asymptotic solution to (1)–(2) of the form ΨR(t,z)eU/z\Psi R(t,z)e^{U/z} where R(t,z)=1+R1(t)z+R2(t)z2+R(t,z)=1+R_{1}(t)z+R_{2}(t)z^{2}+\cdots, Rk(t)R_{k}(t) are N×NN\times N matrices. The matrices Rk(t)R_{k}(t) are determined uniquely by plugging in the ansatz ΨR(t,z)eU/z\Psi R(t,z)e^{U/z} into (1)–(2) and comparing the coefficients in front of the powers of zz. This gives us a recursion relation for the coefficients Rk(t)R_{k}(t) which turns out to have a unique solution. Moreover, the solution automatically satisfies R(t,z)tR(t,z)=1R(t,-z)^{t}R(t,z)=1 where t denotes the standard transposition of matrices. Suppose that the semi-simple point tt^{\circ} is generic and that the coordinate neighbourhood is so small that uiuju_{i}\neq u_{j} for iji\neq j. The rays in the zz-plane of the form 𝐢(uiuj)>0\mathbf{i}(u_{i}-u_{j})\mathbb{R}_{>0} where 𝐢:=1\mathbf{i}:=\sqrt{-1} and iji\neq j, are called the Stokes rays. Let 00\in\ell\subset\mathbb{C} be a line not parallel to any of the Stokes rays. Let us fix an orientation of \ell by choosing a unit vector e𝐢ϕe^{\mathbf{i}\phi}\in\ell, Arg(ϕ)[0,2π)\operatorname{Arg}(\phi)\in[0,2\pi). Following Dubrovin (see [10]) we will say that \ell is an admissible oriented line. The line \ell splits the zz-plane into right Πright\Pi_{\rm right} and left Πleft\Pi_{\rm left} half-planes. There exists unique solutions Xleft(t,z)X_{\rm left}(t,z) and Xright(t,z)X_{\rm right}(t,z) to (1)–(2) holomorphic respectively for zΠrightz\in\Pi_{\rm right} and zΠleftz\in\Pi_{\rm left} which are asymptotic to ΨR(t,z)eU/z\Psi R(t,z)e^{U/z} as z0z\to 0. These solutions extend analytically in zz along the positive part +\ell_{+} of \ell. In particular, we obtain 3 holomorphic solutions to (1)–(2) along the positive half +\ell_{+} of \ell which must be related as follows:

Xleft(t,z)=Xright(t,z)V+,Xleft(t,z)=S(t,z)zθzρC1,z+,\displaystyle X_{\rm left}(t,z)=X_{\rm right}(t,z)V_{+},\quad X_{\rm left}(t,z)=S(t,z)z^{\theta}z^{-\rho}C^{-1},\quad\forall z\in\ell_{+},

where V+V_{+} and C1C^{-1} are some constant matrices called respectively, the Stokes matrix and the central connection matrix. The refined Dubrovin conjecture (see [6], Conjecture 5.2) consists of 3 parts. First, the big quantum cohomology of XX is semi-simple if and only if the bounded derived category Db(X)D^{b}(X) has a full exceptional collection. The second part says that every admissible line \ell determines a full exceptional collection (E1,,EN)(E_{1},\dots,E_{N}) which determines uniquely the Stokes matrix V+V_{+} and the central connection matrix C1C^{-1}. Finally, the 3rd part of the conjecture gives very precise formulas for both V+V_{+} and CC, that is, the (i,j)(i,j)-entry of V+V_{+} is

V+,ij=χ(Ei,Ej),1i,jN\displaystyle V_{+,ij}=\chi(E_{i},E_{j}),\quad 1\leq i,j\leq N

and the ii-th column of C1C^{-1} is

C1(ei)=𝐢D¯(2π)D/2Γ^Xeπ𝐢ρCh(Ei),\displaystyle C^{-1}(e_{i})=\frac{\mathbf{i}^{\overline{D}}}{(2\pi)^{D/2}}\widehat{\Gamma}^{-}_{X}\cup e^{-\pi\mathbf{i}\rho}\cup\operatorname{Ch}(E_{i}),

where D¯{0,1}\overline{D}\in\{0,1\} is the remainder of the division of DD by 22, Γ^X=δΓ(1δ)\widehat{\Gamma}^{-}_{X}=\prod_{\delta}\Gamma(1-\delta) is the so-called gamma class of XX, and Ch(E)=ϵe2π𝐢ϵ\operatorname{Ch}(E)=\sum_{\epsilon}e^{2\pi\mathbf{i}\epsilon} is the Chern character of EE. Here the products are over the Chern roots δ\delta and ϵ\epsilon of respectively the holomorphic tangent bundle TXTX and the complex vector bundle EE. Just like in the case of Ψ\Psi, we think of C1C^{-1} as a linear map C1:NH(X,)C^{-1}:\mathbb{C}^{N}\to H^{*}(X,\mathbb{C}). We refer to Section 3.4 for more details.

The refined version of the conjecture still requires that the manifold XX is Fano. However, as it was pointed out by Arend Bayer in [3] (see also the recent work by Hiroshi Iritani [22]), by using the blowup operation we can construct many examples of non-Fano manifolds for which the first part of the Dubrovin conjecture holds. Moreover, the recent work by Milanov–Xia (see [26]) gives an indication that the blowup operation preserves the remaining two parts of the Dubrovin conjecture. Therefore, it is quite plausible that the Fano condition is redundant.

1.3. Reflection vectors

Suppose that the big quantum cohomology is semi-simple and convergent. The solutions to the quantum differential equations can be represented by complex oscillatory integrals of the following form:

J(t,z):=12π(z)m1/2Γeλ/zI(m)(t,λ)𝑑λ,\displaystyle J(t,z):=\frac{1}{\sqrt{2\pi}}\,(-z)^{m-1/2}\int_{\Gamma}e^{\lambda/z}I^{(m)}(t,\lambda)d\lambda,

where mm\in\mathbb{C} is a complex number and the semi-infinite integration cycle is chosen in such a way that the integral is convergent. It is easy to check that the above integral solves the quantum differential equations (1)–(2) iff the integrand I(m)(t,λ)I^{(m)}(t,\lambda) satisfies the following system of ODEs:

(4) tiI(m)(t,λ)\displaystyle\partial_{t_{i}}I^{(m)}(t,\lambda) =(λE)1(ϕi)(θm1/2)I(m)(t,λ),\displaystyle=-(\lambda-E\bullet)^{-1}(\phi_{i}\bullet)(\theta-m-1/2)\ I^{(m)}(t,\lambda),
(5) λI(m)(t,λ)\displaystyle\partial_{\lambda}I^{(m)}(t,\lambda) =(λEt)1(θm1/2)I(m)(t,λ).\displaystyle=(\lambda-E\bullet_{t})^{-1}(\theta-m-1/2)\,I^{(m)}(t,\lambda).

This is a system of differential equations for the horizontal sections of a connection (m)\nabla^{(m)} on the trivial bundle

(M×)×H(X,)(M×),\displaystyle(M\times\mathbb{C})^{\prime}\times H^{*}(X,\mathbb{C})\to(M\times\mathbb{C})^{\prime},

where

(M×)={(t,λ)|det(λEt)0}.\displaystyle(M\times\mathbb{C})^{\prime}=\{(t,\lambda)\ |\ \det(\lambda-E\bullet_{t})\neq 0\}.

The hypersurface det(λEt)=0\det(\lambda-E\bullet_{t})=0 in M×M\times\mathbb{C} is called the discriminant. The connection (m)\nabla^{(m)} is known as the second structure connection. In the case when m=0m=0 or 1-1, the connection was used by Dubrovin to define the monodromy group of a Frobenius manifold (see [8]). However, it became clear shortly afterwards that it is important to study the entire family, that is, allow mm to be any complex number (see [24] and [11]).

The space of solutions to (4)–(5) is quite interesting. In the examples of mirror symmetry the second structure connection of quantum cohomology can be identified with a Gauss–Manin connection. Therefore, the solutions to (4)–(5) should be thought as period integrals. In particular, by using (m)\nabla^{(m)} we can introduce many of the ingreidents of Picard–Lefschetz theory. This was done by Dubrovin (see [11], Section 4). He called the solutions to (4)–(5) twisted periods because their properties are very similar to the period integrals in Givental’s twisted Picard–Lefschetz theory [15]. Motivated by the work of Givental in [17], the second author introduced in [27] the following fundamental solution to (4)–(5):

(6) I(m)(t,λ)=k=0(1)kSk(t)I~(m+k)(λ),I^{(m)}(t,\lambda)=\sum_{k=0}^{\infty}(-1)^{k}S_{k}(t)\widetilde{I}^{(m+k)}(\lambda),

where

(7) I~(m)(λ)=eρλm(λθm12Γ(θm+12)).\widetilde{I}^{(m)}(\lambda)=e^{-\rho\partial_{\lambda}\partial_{m}}\Big{(}\frac{\lambda^{\theta-m-\frac{1}{2}}}{\Gamma(\theta-m+\frac{1}{2})}\Big{)}.

Note that both I(m)(t,λ)I^{(m)}(t,\lambda) and I~(m)(λ)\widetilde{I}^{(m)}(\lambda) take values in End(H(X,))\operatorname{End}(H^{*}(X,\mathbb{C})). The second structure connection has a Fuchsian singularity at infinity, therefore the series I(m)(t,λ)I^{(m)}(t,\lambda) is convergent and it defines a multi-valued analytic function in the complement to the discriminant. There are many ways to choose a fundamental solution but what makes the above choice special is the specific choice of building blocks, that is, the calibrated periods (7) while the standard approach would be monomials in λ\lambda. The existence of such decomposition follows from Givental’s formalism of quantized symplectic transformations and their actions on vertex operators (see [17], Section 5, especially Theorem 2). Although Dubrovin already knew that one can import concepts from singularity theory to quantum cohomology, somehow the above choice of a fundamental solution makes the parallel with singularity theory much more visible (at least to the authors).

Let us choose a base point tMt^{\circ}\in M, such that, Reui(t)Reuj(t)\operatorname{Re}u_{i}(t^{\circ})\neq\operatorname{Re}u_{j}(t^{\circ}) for iji\neq j. Then Reui(t)Reuj(t)\operatorname{Re}u_{i}(t)\neq\operatorname{Re}u_{j}(t) for iji\neq j for all tt sufficiently close to tt^{\circ}. Let λ\lambda^{\circ} be a positive real number, such that, λ>|ui(t)|\lambda^{\circ}>|u_{i}(t^{\circ})| for all ii. We define the mm-twisted period vectors Ia(m)(t,λ):=I(m)(t,λ)aI_{a}^{(m)}(t,\lambda):=I^{(m)}(t,\lambda)a where aH(X,)a\in H^{*}(X,\mathbb{C}) and the value depends on the choice of a reference path avoiding the discriminant from (t,λ)(t^{\circ},\lambda^{\circ}) to (t,λ)(t,\lambda). Note that at (t,λ)(t^{\circ},\lambda^{\circ}) the only ambiguity is in the choice of the value for the calibrated periods, that is, we need to specify a branch of logλ\log\lambda when λ\lambda is close to λ\lambda^{\circ}. Since λ\lambda^{\circ} is a positive real number we simply take the principal branch of the logarithm.

Let us introduce the following pairings hm:H(X,)×H(X,)h_{m}:H^{*}(X,\mathbb{C})\times H^{*}(X,\mathbb{C})\to\mathbb{C}

(8) hm(a,b):=(Ia(m)(t,λ),(λE)Ib(m)(t,λ)).h_{m}(a,b):=(I^{(m)}_{a}(t,\lambda),(\lambda-E\bullet)I^{(-m)}_{b}(t,\lambda)).

Using the differential equations of (±m)\nabla^{(\pm m)} it is easy to check that hm(a,b)h_{m}(a,b) is independent of tt and λ\lambda. It turns out that there is an explicit formula for hmh_{m} in terms of the Hodge grading operator θ\theta and the nilpotent operator ρ\rho. Let us recall the so-called Euler pairing

(9) a,b:=12π(a,eπ𝐢θeπ𝐢ρb),a,bH(X,).\langle a,b\rangle:=\frac{1}{2\pi}(a,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}b),\quad a,b\in H^{*}(X,\mathbb{C}).

As a byproduct of the proof of Theorem 2.6.1 we will get the following simple formula:

hm(a,b)=qa,b+q1b,a,\displaystyle h_{m}(a,b)=q\langle a,b\rangle+q^{-1}\langle b,a\rangle,

where q:=eπ𝐢mq:=e^{\pi\mathbf{i}m}. The above formula shows that hmh_{m} is the analogue of the [q,q1]\mathbb{Z}[q,q^{-1}]-bilinear intersection form in twisted Picard–Lefschetz theory (see [15], Section 3). Furthermore, let us fix a reference path from (t,λ)(t^{\circ},\lambda^{\circ}) to a point (t,λ)(t,\lambda) sufficiently close to a generic point bb on the discriminant. The local equation of the discriminant near bb has the form λ=ui(t)\lambda=u_{i}(t) where ui(t)u_{i}(t) is an eigenvalue of EE\bullet. It turns out that the set of all aH(X,)a\in H^{*}(X,\mathbb{C}), such that, Ia(m)(t,λ)I^{(m)}_{a}(t,\lambda) is analytic at λ=ui(t)\lambda=u_{i}(t) is a codimension 1 subspace of H(X,)H^{*}(X,\mathbb{C}). Suppose that m\nin12+m\nin\tfrac{1}{2}+\mathbb{Z}, then there is a 1-dimensional subspace of vectors βH(X,)\beta\in H^{*}(X,\mathbb{C}), such that, (λui(t))m+1/2Iβ(m)(t,λ)(\lambda-u_{i}(t))^{m+1/2}I^{(m)}_{\beta}(t,\lambda) is analytic at λ=ui(t)\lambda=u_{i}(t) and the value at λ=ui(t)\lambda=u_{i}(t) belongs to Ψ(ei)\mathbb{C}\Psi(e_{i}) where Ψ\Psi is the map (3). Therefore, for the given reference path and an arbitrary choice of log(λui(t))\log(\lambda-u_{i}(t)) there is a uniquely defined vector β=β(m)\beta=\beta(m), such that,

(10) (λui(t))m+1/2Iβ(m)(t,λ)=2πΓ(m+12)Ψ(ei)+O(λui(t)),(\lambda-u_{i}(t))^{m+1/2}I^{(m)}_{\beta}(t,\lambda)=\frac{\sqrt{2\pi}}{\Gamma(-m+\tfrac{1}{2})}\,\Psi(e_{i})+O(\lambda-u_{i}(t)),

where the coefficient in front of Ψ(ei)\Psi(e_{i}) is such that hm(β(m),β(m))=q+q1h_{m}(\beta(m),\beta(-m))=q+q^{-1}. Note that the choice of a reference path and a branch of log(λui(t))\log(\lambda-u_{i}(t)) determines β(m)\beta(m) for all m\nin12+m\nin\tfrac{1}{2}+\mathbb{Z}, that is, we have a map

β:{12+}H(X,).\displaystyle\beta:\mathbb{C}\setminus{\{\tfrac{1}{2}+\mathbb{Z}\}}\to H^{*}(X,\mathbb{C}).

Using that λI(m)(t,λ)=I(m+1)(t,λ)\partial_{\lambda}I^{(m)}(t,\lambda)=I^{(m+1)}(t,\lambda) we get that this map is periodic: β(m+1)=β(m).\beta(m+1)=\beta(m). It will follow from our results that β\beta is a trigonometric polynomial, that is, βH(X,[q2,q2])\beta\in H^{*}(X,\mathbb{C}[q^{2},q^{-2}]). If we change the value of the logarithmic branch log(λui(t))log(λui(t))+2π𝐢\log(\lambda-u_{i}(t))\mapsto\log(\lambda-u_{i}(t))+2\pi\mathbf{i}, then β(m)q2β(m)\beta(m)\mapsto-q^{-2}\beta(m). Therefore, for a fixed reference path the value of β(m)\beta(m) is fixed up to a factor in the spiral (q2)={(1)kq2k|k}(-q^{-2})^{\mathbb{Z}}=\{(-1)^{k}q^{-2k}\ |\ k\in\mathbb{Z}\}. We will say that β\beta is a twisted reflection vector corresponding to the given reference path. We usually supress the dependence on the logarithmic branch if the choice is irrelevant or it is clear from the context. The following formula for the local monodromy of (m)\nabla^{(m)} justifies our terminology:

aaq1hm(a,β(m))β(m),aH(X,),\displaystyle a\mapsto a-q^{-1}h_{m}(a,\beta(-m))\beta(m),\quad a\in H^{*}(X,\mathbb{C}),

that is, the local monodromy is a complex reflection whose fixed points locus is the hyperplane orthogonal to β(m)\beta(-m). We refer to Section 2.3 for more details and for more general settings, i.e., we can introduce twisted reflection vectors for any semi-simple Frobenius manifold.

1.4. Monodromy data and reflection vectors

We continue to work in the settings from the previous two sections. Let \ell be an admissible oriented line (see Section 1.2) with orientation e𝐢ϕe^{\mathbf{i}\phi}. By definition η=𝐢e𝐢ϕ\eta=\mathbf{i}e^{\mathbf{i}\phi} is not parallel to any of the differences ui(t)uj(t)u_{i}(t^{\circ})-u_{j}(t^{\circ}) for iji\neq j. We will refer to η\eta as an admissible direction. Our choice of a reference point (t,λ)(t^{\circ},\lambda^{\circ}) is such that the real line with its standard orientation is an admissible oriented line. The corresponding admissible direction is η:=𝐢\eta^{\circ}:=\mathbf{i}. Any other admissible direction η\eta will be equipped with a reference path to η\eta^{\circ} or equivalently, we fix an analytic branch of log\log in a neighbourhood of η\eta. Finally, we consider only tMt\in M sufficiently close to tt^{\circ}, such that, η\eta is an admissible direction for tt, that is, η\eta is not parallel to ui(t)uj(t)u_{i}(t)-u_{j}(t) for iji\neq j.

Let us construct a system of reference paths C1(η),,CN(η)C_{1}(\eta),\dots,C_{N}(\eta) corresponding to η\eta. Each Ci(η)C_{i}(\eta) starts at λ=ui\lambda=u_{i}, approaches the circle |λ|=λ|\lambda|=\lambda^{\circ} in the direction of η\eta, after hitting the circle at some point λi(η)\lambda^{i}(\eta) the path continues clockwise along the circle arc from λi(η)\lambda^{i}(\eta) to λ(η):=𝐢ηλ\lambda^{\circ}(\eta):=-\mathbf{i}\eta\lambda^{\circ}, and finally by continuously deforming the direction η\eta to η\eta^{\circ} the path connects λ(η)\lambda^{\circ}(\eta) and λ(η)=λ\lambda^{\circ}(\eta^{\circ})=\lambda^{\circ} – see Figure 1. Note that if λCi\lambda\in C_{i} is sufficiently close to uiu_{i}, then λui=sη\lambda-u_{i}=s\eta for some positive real number ss and we have a natural choice of a logarithmic branch: log(λui):=ln(s)+log(η)\log(\lambda-u_{i}):=\ln(s)+\log(\eta). Therefore, as it was explained in Section 1.3, we may choose a twisted reflection vector βi(m)\beta_{i}(m). In other words, each admissible direction determines a set of twisted reflection vectors (β1(m),,βN(m))(\beta_{1}(m),\dots,\beta_{N}(m)). Furthermore, the admissible direction determines the following order of the eigenvalues u1,,uNu_{1},\dots,u_{N} of EE\bullet: we say that ui<uju_{i}<u_{j} if uju_{j} is on the RHS of the line through uiu_{i} parallel to η\eta where RHS means that we have to stand at uiu_{i} and look in the direction η\eta. For example, for the standard admissible direction η=𝐢\eta^{\circ}=\mathbf{i}, ui<uju_{i}<u_{j} would mean that Re(ui)<Re(uj)\operatorname{Re}(u_{i})<\operatorname{Re}(u_{j}). We will refer to the order as the lexicographical order determined by η\eta. Let us assume that the enumeration of the eigenvalues u1,,uNu_{1},\dots,u_{N} is according to the lexicographical order, that is, ui<uju_{i}<u_{j} iff i<ji<j. Our main result can be stated as follows.

Theorem 1.4.1.

Let η\eta be an admissible direction and assume that the eigenvalues u1,,uNu_{1},\dots,u_{N} of the operator EE\bullet are enumerated according to the lexicographical order corresponding to η\eta. Then the following statements hold.

  1. a)

    The reflection vectors βi(m)\beta_{i}(m) (1iN1\leq i\leq N) are independent of mm and the Gram matrix of the Euler pairing (9) is upper-triangular

    βi,βj=0i>j,\displaystyle\langle\beta_{i},\beta_{j}\rangle=0\quad\forall i>j,

    with 11’s on the diagonal: βi,βi=1\langle\beta_{i},\beta_{i}\rangle=1.

  2. b)

    The pairing hmh_{m} can be computed by the following formula:

    hm(a,b)=qa,b+q1b,a,a,bH,\displaystyle h_{m}(a,b)=q\langle a,b\rangle+q^{-1}\langle b,a\rangle,\quad\forall a,b\in H,

    where ,\langle\ ,\ \rangle is the Euler pairing (9).

  3. c)

    The inverse Stokes matrix V+1V_{+}^{-1} coincides with the Gram matrix of the Euler pairing (9) in the basis βi\beta_{i} (1iN1\leq i\leq N).

  4. d)

    The (i,j)(i,j)-entry of the central connection matrix is related to the components of the reflection vectors by the following formula:

    Cij=12π(βi,ϕj).\displaystyle C_{ij}=\frac{1}{\sqrt{2\pi}}\,(\beta_{i},\phi_{j}).

In fact our result is more general. The above theorem can be formulated in the settings of semi-simple Frobenius manifolds. Under an additional technical assumption, i.e., we assume that the Frobenius manifold has a calibration for which the grading operator is a Hodge grading operator (see Definition 2.1.2), we prove that the conclusions of the above theorem remain true (see Theorem 2.6.1).

Using Theorem 1.4.1 we can answer the question raised in [26]. Following the analogy with singularity theory (see [1, 12]), we introduce the concept of a distinguished system of reference paths (see Definition 3.5.1). Let us recall the Iritani’s integral structure map (see [21]) ΨQ:K0(X)H(X,)\Psi_{Q}:K_{0}(X)\rightarrow H^{*}(X,\mathbb{C}) defined by

ΨQ(E):=(2π)1D2Γ^(X)ei=1rpilogqiCh(E),\displaystyle\Psi_{Q}(E):=(2\pi)^{\tfrac{1-D}{2}}\widehat{\Gamma}(X)\cup e^{-\sum_{i=1}^{r}p_{i}\log q_{i}}\cup\operatorname{Ch}(E),

where Q=(q1,,qr)Q=(q_{1},\dots,q_{r}) are the Novikov variables corresponding to an ample basis p1,,prp_{1},\dots,p_{r} of H2(X,)H1,1(X,)H^{2}(X,\mathbb{Z})\cap H^{1,1}(X,\mathbb{C}). We have the following relation:

(11) ΨQ(E),ΨQ(F)=χ(E,F),E,FK0(X)\langle\Psi_{Q}(E),\Psi_{Q}(F)\rangle=\chi(E,F),\quad E,F\in K^{0}(X)

which justifies why we refer to (9) as the Euler pairing.

Theorem 1.4.2.

Let β1,,βN\beta_{1},\dots,\beta_{N} be the reflection vectors corresponding to a distinguished system of reference paths. Parts (2) and (3) of the refined Dubrovin conjecture, i.e., Conjecture 3.4.1, hold if and only if there exists a full exceptional collection (F1,,FN)(F_{1},\dots,F_{N}), such that, βi=ΨQ(Fi)\beta_{i}=\Psi_{Q}(F_{i}) for all ii.

Theorem 1.4.2 is proved in Section 3.5 (see Theorem 3.5.1). The definition of a reflection vector is the same as the definition of a twisted reflection vector except that we require mm\in\mathbb{Z}. Since the fundamental group of {u1,,uN}\mathbb{C}\setminus{\{u_{1}^{\circ},\dots,u_{N}^{\circ}\}} is generated by simple loops corresponding to the reference paths Ci(η)C_{i}(\eta) where η\eta is an admissible direction, we have the following interesting corollary.

Corollary 1.4.1.

The set of all twisted reflection vectors is a subset of

H(X,[q2,q2])=[q2,q2]β1++[q2,q2]βN,\displaystyle H^{*}(X,\mathbb{C}[q^{2},q^{-2}])=\mathbb{C}[q^{2},q^{-2}]\beta_{1}+\cdots+\mathbb{C}[q^{2},q^{-2}]\beta_{N},

where β1,,βN\beta_{1},\dots,\beta_{N} are the reflection vectors corresponding to a distinguished system of reference paths. In addition, if the manifold XX satisfies the refined Dubrovin conjecture, then the set of twisted reflection vectors is a subset in the [q2,q2]\mathbb{Z}[q^{2},q^{-2}]-lattice [q2,q2]β1++[q2,q2]βN\mathbb{Z}[q^{2},q^{-2}]\beta_{1}+\cdots+\mathbb{Z}[q^{2},q^{-2}]\beta_{N}.

For the proof, thanks to the braid group action on the set of distinguished systems of reference paths (see Section 3.5), we may assume that β1,,βN\beta_{1},\dots,\beta_{N} are the reflection vectors corresponding to the reference paths C1(η),,CN(η)C_{1}(\eta),\dots,C_{N}(\eta) for some admissible direction η\eta. Note that every twisted reflection vector is obtained from some βi\beta_{i} by a sequence of local monodromy transformations Mj±1M_{j}^{\pm 1} (1jN1\leq j\leq N) where MjM_{j} is the monodromy transformation corresponding to the simple loop associated with Cj(η)C_{j}(\eta). According to Theorem 1.4.1, part a), the matrix of MjM_{j} (resp. Mj1M_{j}^{-1}) in the basis β1,,βN\beta_{1},\dots,\beta_{N} is upper-triangular and the only entry depending on qq is in position (j,j)(j,j), that is, it is equal to q2-q^{-2} (resp. q2-q^{2}). In addition, if the refined Dubrovin conjecture holds, then since βi,βj=χ(Fi,Fj)\langle\beta_{i},\beta_{j}\rangle=\chi(F_{i},F_{j})\in\mathbb{Z}, we get that the entries of Mj±1M_{j}^{\pm 1} belong to [q2,q2]\mathbb{Z}[q^{2},q^{-2}].

Let us point out that the full exceptional collection (F1,,FN)(F_{1},\dots,F_{N}) in Theorem 1.4.2 is not the same as the full exceptional collection (E1,,EN)(E_{1},\dots,E_{N}) in the refined Dubrovin conjecture. The reason is that the objects EiE_{i} correspond to oscillatory integrals in which the integration paths are rays with direction η-\eta while FiF_{i} correspond to reference paths going in the opposite direction η\eta. Changing the admissible direction from η\eta to η-\eta means that one has to perform a certain sequence of mutations in order to get from one exceptional collection to the other one. It turns out that the sequence of mutations that we need is well known in the theory of derived categories, i.e., this is the same sequence used to define the left Koszul dual of an exceptional collection. The precise statement is that up to a shift by DD¯2\tfrac{D-\overline{D}}{2} the exceptional collection (F1,,FN)(F_{1},\dots,F_{N}) is the left Koszul dual to (EN,,E1)(E_{N}^{\vee},\dots,E_{1}^{\vee}). The moral is that although there is some freedom in defining a Stokes matrix and a central connection matrix of the quantum connection, the statement of the refined Dubrovin conjecture is independent of the choices that we make. The different full exceptional collection that one might get due to the discrepancy of the definitions are related by mutations in the derived category. Let us point out that even Dubrovin himself did not use the definitions consistently – the central connection matrix in [10, 11] is the inverse of the central connection matrix in [6].

Finally, let us comment on the proofs. The relation between the quantum connection and its Laplace transform was studied by many people. In particular, the relation between Stokes multipliers and the monodromy data of the Laplace transform of the quantum connection is well known thanks to the work of Balsar–Jurkat–Lutz [2]. There is also a recent paper by Guzzetti (see [18]) who was able to remove some technical conditions from the main result in [2]. Although, we do not directly use any results from [2], the ideas for all proofs come from there, except for the formula for the connection matrix (see Theorem 2.6.1, part a) whose proof follows the ideas of Dubrovin (see [11], Theorem 4.19). Our results should not be very surprising to the experts. Especially, the work of Galkin–Golyshev–Iritani [13] and Dubrovin [11] contain almost all ideas and results necessary to prove Theorems 1.4.1 and 1.4.2. In some sense we could have written much shorter text. Nevertheless, in order to avoid gaps in the arguments due to misquoting results, we decided to have a self contained text independent of the results in [2, 11, 13].

1.5. Acknowledgements

We are thankful to Alexey Bondal for many useful discussions on the Dubrovin conjecture and especially for pointing out to us the notion of left and right Koszul dual of an exceptional collection. The first author also thanks Jin Chen and Mauricio Romo for many interesting discussions on the Γ\Gamma-conjectures and Dubrovin conjecture. This work is supported by the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan and by JSPS Kakenhi Grant Number JP22K03265. The first author is also supported by the President’s International Fellowship Initiative of the Chinese Academy of Sciences.

2. Twisted periods of a Frobenius manifold

As promised in the introduction, we will formulate and prove Theorem 1.4.1 more abstractly in the settings of a semi-simple Frobenius manifold. Compared to Dubrovin’s theory of twisted periods (see [11], Section 4), we introduce a fundamental solution to the second structure connection which allows us to see better the analogy with singularity theory.

2.1. Frobenius manifolds

Let MM be a complex manifold and 𝒯M\mathcal{T}_{M} be the sheaf of holomorphic vector fields on MM. Suppose that MM is equipped with the following structures:

  1. (F1)

    A non-degenerate symmetric bilinear pairing

    (,):𝒯M𝒯M𝒪M.(\,\cdot\,,\,\cdot\,):\mathcal{T}_{M}\otimes\mathcal{T}_{M}\to\mathcal{O}_{M}.
  2. (F2)

    A Frobenius multiplication: commutative associative multiplication

    :𝒯M𝒯M𝒯M,\cdot\bullet\cdot:\mathcal{T}_{M}\otimes\mathcal{T}_{M}\to\mathcal{T}_{M},

    such that (v1w,v2)=(v1,wv2)(v_{1}\bullet w,v_{2})=(v_{1},w\bullet v_{2}) v1,v2,w𝒯M\forall v_{1},v_{2},w\in\mathcal{T}_{M}.

  3. (F3)

    A unit vector field: global vector field 𝟏𝒯M(M)\mathbf{1}\in\mathcal{T}_{M}(M), such that,

    𝟏v=v,vL.C.𝟏=0,v𝒯M,\mathbf{1}\bullet v=v,\quad\nabla^{\rm L.C.}_{v}\mathbf{1}=0,\quad\forall v\in\mathcal{T}_{M},

    where L.C.\nabla^{\rm L.C.} is the Levi–Civita connection of the pairing (,)(\cdot,\cdot).

  4. (F4)

    An Euler vector field: global vector field E𝒯M(M)E\in\mathcal{T}_{M}(M), such that, there exists a constant DD\in\mathbb{C}, called conformal dimension, and

    E(v1,v2)([E,v1],v2)(v1,[E,v2])=(2D)(v1,v2)E(v_{1},v_{2})-([E,v_{1}],v_{2})-(v_{1},[E,v_{2}])=(2-D)(v_{1},v_{2})

    for all v1,v2𝒯Mv_{1},v_{2}\in\mathcal{T}_{M}.

Note that the complex manifold TM×TM\times\mathbb{C}^{*} has a structure of a holomorphic vector bundle with base M×M\times\mathbb{C}^{*}: the fiber over (t,z)M×(t,z)\in M\times\mathbb{C}^{*} is TtM×{z}TtMT_{t}M\times\{z\}\cong T_{t}M which has a natural structure of a vector space. Given the data (F1)-(F4), we define the so called Dubrovin connection on the vector bundle TM×TM\times\mathbb{C}^{*}

v\displaystyle\nabla_{v} :=vL.C.z1v,v𝒯M,\displaystyle:=\nabla^{\rm L.C.}_{v}-z^{-1}v\bullet,\quad v\in\mathcal{T}_{M},
/z\displaystyle\nabla_{\partial/\partial z} :=zz1θ+z2E,\displaystyle:=\frac{\partial}{\partial z}-z^{-1}\theta+z^{-2}E\bullet,

where zz is the standard coordinate on ={0}\mathbb{C}^{*}=\mathbb{C}\setminus{\{0\}}, where vv\bullet is an endomorphism of 𝒯M\mathcal{T}_{M} defined by the Frobenius multiplication by the vector field vv, and where θ:𝒯M𝒯M\theta:\mathcal{T}_{M}\to\mathcal{T}_{M} is an 𝒪M\mathcal{O}_{M}-modules morphism defined by

θ(v):=vL.C.(E)(1D2)v.\theta(v):=\nabla^{\rm L.C.}_{v}(E)-\Big{(}1-\frac{D}{2}\Big{)}v.
Definition 2.1.1.

The data ((,),,𝟏,E)((\cdot,\cdot),\bullet,\mathbf{1},E), satisfying the properties (F1)(F4)(F1)-(F4), is said to be a Frobenius structure of conformal dimension DD if the corresponding Dubrovin connection is flat, that is, if (t1,,tN)(t_{1},\dots,t_{N}) are holomorphic local coordinates on MM, then the set of N+1N+1 differential operators /ti(1iN)\nabla_{\partial/\partial t_{i}}\ (1\leq i\leq N), /z\nabla_{\partial/\partial z} pairwise commute. ∎

Near z=z=\infty the Dubrovin connection has a fundamental solution of the following form:

(12) X(t,z)=S(t,z)zδzρ,X(t,z)=S(t,z)z^{\delta}z^{-\rho},

where δ\delta is a diagonalizable operator, ρ\rho is a nilpotent operator, and the operator-valued series S(t,z)=1+S1(t)z1+S(t,z)=1+S_{1}(t)z^{-1}+\cdots, SkEnd(𝒯M)S_{k}\in\operatorname{End}(\mathcal{T}_{M}) satisfies the symplectic condition S(t,z)S(t,z)T=1S(t,z)S(t,-z)^{T}=1, where T is transposition with respect to the Frobenius pairing. It can be proved that δ\delta coincides with the semi-simple part θs\theta_{s} of the grading operator θ\theta in the Jordan–Chevalley decomposition θ=θs+θn\theta=\theta_{s}+\theta_{n}, where the operators θs\theta_{s} and θn\theta_{n} are uniquely determined by the following 3 conditions:

  1. (i)

    Commutativity: [θs,θn]=0[\theta_{s},\theta_{n}]=0.

  2. (ii)

    The operator θs\theta_{s} is diagonalizable.

  3. (iii)

    The operator θn\theta_{n} is nilpotent.

Moreover, the operator ρ=θn+l=1ρl\rho=-\theta_{n}+\sum_{l=1}^{\infty}\rho_{l} where ρl0\rho_{l}\neq 0 for finitely many ll and [δ,ρl]=lρl[\delta,\rho_{l}]=-l\rho_{l}. For more details we refer to [28], Section 1.3.1. Following Givental [16] we will refer to the pair (S(t,z),ρ)(S(t,z),\rho) as calibration of MM. Sometimes we will drop ρ\rho from the notation and say that S(t,z)S(t,z) is the calibration.

Remark 2.1.1.

The pair (S(t,z),ρ)(S(t,z),\rho) is not uniquely determined from the Frobenius structure and in general there is no canonical choice. More precisely, one can prove that there exists a unipotent Lie group acting faithfully and transitively on the set of such pairs – see [28], Section 1.3.1. ∎

Definition 2.1.2.

Let S(t,z)S(t,z) be a calibration of MM and ρ\rho be the corresponding nilpotent operator. The grading operator θ\theta is said to be a Hodge grading operator for the calibration (S(t,z),ρ)(S(t,z),\rho) if

  1. (i)

    The operator θ\theta is diagonalizable.

  2. (ii)

    The following commutation relation holds: [θ,ρ]=ρ.[\theta,\rho]=-\rho.

Note that if θ\theta is a Hodge grading operator, then δ=θ\delta=\theta and ρl=0\rho_{l}=0 for all l1l\neq 1. The fundamental solution takes the form X(t,z)=S(t,z)zθzρX(t,z)=S(t,z)z^{\theta}z^{-\rho}. From now on we will consider only Frobenius manifolds with a fixed calibration, such that, θ\theta is a Hodge grading operator. The problem that we will be interested in is local, so we will further assume that MM has a global flat coordinate system (t1,,tN)(t_{1},\dots,t_{N}).

Let us fix a base point tMt^{\circ}\in M. Put ϕi:=/ti|t\phi_{i}:=\partial/\partial t_{i}|_{t^{\circ}} (1iN)(1\leq i\leq N), then {ϕi}i=1N\{\phi_{i}\}_{i=1}^{N} is a basis of the reference tangent space H:=TtMH:=T_{t^{\circ}}M. The flat vector fields /ti\partial/\partial t_{i} (1iN1\leq i\leq N) provide a trivialization of the tangent bundle TMM×HTM\cong M\times H. This allows us to identify the Frobenius multiplication \bullet with a family of associative commutative multiplications t:HHH\bullet_{t}:H\otimes H\to H depending analytically on tMt\in M. The operator θ:𝒯M𝒯M\theta:\mathcal{T}_{M}\to\mathcal{T}_{M} defined above preserves the subspace of flat vector fields. It induces a linear operator on HH, known to be skew symmetric with respect to the Frobenius pairing (,)(\ ,\ ).

There are two flat connections that one can associate with the Frobenius structure. The first one is the Dubrovin connection – defined above. The Dubrovin connection in flat coordinates takes the following form:

/ti\displaystyle\nabla_{\partial/\partial t_{i}} =\displaystyle= tiz1ϕi,\displaystyle\frac{\partial}{\partial t_{i}}-z^{-1}\phi_{i}\bullet\ ,
/z\displaystyle\nabla_{\partial/\partial z} =\displaystyle= zz1θ+z2E,\displaystyle\frac{\partial}{\partial z}-z^{-1}\theta+z^{-2}E\bullet\ ,

where zz is the standard coordinate on ={0}\mathbb{C}^{*}=\mathbb{C}-\{0\} and for vΓ(M,𝒯M)v\in\Gamma(M,\mathcal{T}_{M}) we denote by v:HHv\bullet:H\to H the linear operator of Frobenius multiplication by vv.

We will be interested also in the second structure connection

(13) /ti(m)\displaystyle\nabla^{(m)}_{\partial/\partial t_{i}} =ti+(λEt)1(ϕit)(θm1/2),\displaystyle=\frac{\partial}{\partial t_{i}}+(\lambda-E\bullet_{t})^{-1}(\phi_{i}\bullet_{t})(\theta-m-1/2)\ ,
(14) /λ(m)\displaystyle\nabla^{(m)}_{\partial/\partial\lambda} =λ(λEt)1(θm1/2),\displaystyle=\frac{\partial}{\partial\lambda}-(\lambda-E\bullet_{t})^{-1}(\theta-m-1/2)\ ,

where mm\in\mathbb{C} is a complex parameter. This is a connection on the trivial bundle

(M×)×H(M×),\displaystyle(M\times\mathbb{C})^{\prime}\times H\to(M\times\mathbb{C})^{\prime},

where

(M×)={(t,λ)|det(λEt)0}.\displaystyle(M\times\mathbb{C})^{\prime}=\{(t,\lambda)\ |\ \det(\lambda-E\bullet_{t})\neq 0\}.

The hypersurface det(λEt)=0\det(\lambda-E\bullet_{t})=0 in M×M\times\mathbb{C} is called the discriminant.

2.2. Twisted periods

Let mm\in\mathbb{C} be any complex number.

Definition 2.2.1.

By a mm-twisted period of the Frobenius manifold MM we mean a sequence I(m+k)I^{(m+k)} (k)(k\in\mathbb{Z}) satisfying the following two properties:

  1. (i)

    Flatness: I(m+k)I^{(m+k)} is a horizontal section for (m+k)\nabla^{(m+k)}.

  2. (ii)

    Translation invariance: λI(m+k)=I(m+k+1)\partial_{\lambda}I^{(m+k)}=I^{(m+k+1)}.∎

The set of all mm-twisted periods has a natural structure of a vector space. Note that if k>0k>0 is sufficiently large, then the mm-twisted period sequence is uniquely determined from I(mk)I^{(m-k)} only. Indeed, by translation invariance, we have I(mk+i)=λiI(mk)I^{(m-k+i)}=\partial_{\lambda}^{i}I^{(m-k)} for all i0i\geq 0. Using (14)

(λE)I(mk)=(θm+k1/2)I(mk1).\displaystyle(\lambda-E\bullet)I^{(m-k)}=(\theta-m+k-1/2)I^{(m-k-1)}.

We get that as long as θm+k12\theta-m+k-\tfrac{1}{2} is invertible we can express I(mk1)I^{(m-k-1)} in terms of I(mk)I^{(m-k)}. Let us choose kk so large that mk+12m-k+\tfrac{1}{2} is smaller than the real parts of all eigenvalues of θ\theta. Then, it is clear that all I(mk1),I(mk2),I^{(m-k-1)},I^{(m-k-2)},\dots can be expressed in terms of I(mk)I^{(m-k)}.

Suppose now that (S(t,z),ρ)(S(t,z),\rho) is a calibration. We will construct an isomorphism between HH and the space of all mm-twisted periods. Let us fix a reference point (t,λ)(M×)(t^{\circ},\lambda^{\circ})\in(M\times\mathbb{C})^{\prime} such that λ\lambda^{\circ} is a sufficiently large positive real number. It is easy to check that the following function is a solution to the second structure connection (m)\nabla^{(m)}

(15) I(m)(t,λ)=k=0(1)kSk(t)I~(m+k)(λ),I^{(m)}(t,\lambda)=\sum_{k=0}^{\infty}(-1)^{k}S_{k}(t)\widetilde{I}^{(m+k)}(\lambda),

where

(16) I~(m)(λ)=eρλm(λθm12Γ(θm+12)).\widetilde{I}^{(m)}(\lambda)=e^{-\rho\partial_{\lambda}\partial_{m}}\Big{(}\frac{\lambda^{\theta-m-\frac{1}{2}}}{\Gamma(\theta-m+\frac{1}{2})}\Big{)}.

Note that both I(m)(t,λ)I^{(m)}(t,\lambda) and I~(m)(λ)\widetilde{I}^{(m)}(\lambda) take values in End(H)\operatorname{End}(H). The second structure connection has a Fuchsian singularity at infinity, therefore the series I(m)(t,λ)I^{(m)}(t,\lambda) is convergent for all (t,λ)(t,\lambda) sufficiently close to (t,λ)(t^{\circ},\lambda^{\circ}). Using the differential equations (13)–(14) we extend I(m)I^{(m)} to a multi-valued analytic function on (M×)(M\times\mathbb{C})^{\prime} taking values in End(H)\operatorname{End}(H). We define the following multi-valued functions taking values in HH:

(17) Ia(m)(t,λ):=I(m)(t,λ)a,aH,m.I^{(m)}_{a}(t,\lambda):=I^{(m)}(t,\lambda)\,a,\quad a\in H,\quad m\in\mathbb{C}.

Clearly, for each fixed aHa\in H, the sequence Ia(m+k)(t,λ)I^{(m+k)}_{a}(t,\lambda) (kk\in\mathbb{Z}) is a period vector in the sence of Definition 2.2.1. Moreover, if kk\in\mathbb{Z} is sufficiently negative, then I(m+k)(t,λ)I^{(m+k)}(t,\lambda) is an invertible operator. Therefore, all mm-twisted period vectors of MM have the form Ia(m+k)(t,λ)I_{a}^{(m+k)}(t,\lambda) (k)(k\in\mathbb{Z}) for some aHa\in H. Note that the analytic continuation along a closed loop around the discriminant leaves the space of mm-twisted periods invariant. Therefore, for each m/m\in\mathbb{C}/\mathbb{Z} we have a monodromy representation

(18) π1((M×),(t,λ))GL(H).\pi_{1}((M\times\mathbb{C})^{\prime},(t^{\circ},\lambda^{\circ}))\to\operatorname{GL}(H).
Remark 2.2.1.

If mm\in\mathbb{Z}, then the representation (18) defines the monodromy group of the Frobenius manifold. Put q=eπ𝐢mq=e^{\pi\mathbf{i}m}, then (18) defines a qq-deformation of the monodromy group of the Frobenius manifold.∎

2.3. Local monodromy

Recall that a point tMt\in M is said to be semi-simple if there are local coordinates (u1,,uN)(u_{1},\dots,u_{N}) near tt, called canonical coordinates, such that, the multiplication and the Frobenius pairing take the following form:

uiuj=δijuj,(ui,uj)=δijΔj,\displaystyle\frac{\partial}{\partial u_{i}}\bullet\frac{\partial}{\partial u_{j}}=\delta_{ij}\frac{\partial}{\partial u_{j}},\quad\Big{(}\frac{\partial}{\partial u_{i}},\frac{\partial}{\partial u_{j}}\Big{)}=\frac{\delta_{ij}}{\Delta_{j}},

where Δj𝒪M,t\Delta_{j}\in\mathcal{O}_{M,t} (1jN1\leq j\leq N) are holomorphic functions that do not vanish at tt. The Frobenius manifold MM is said to be semi-simple if it has at least one semi-simple point. The subset 𝒦M\mathcal{K}\subset M of points that are not semi-simple is called the caustic. If MM is semi-simple, then the caustic is either the empty set or an analytic hypersurface.

From now on we will assume that MM is a semi-simple Frobenius manifold. Let us choose the base point tt^{\circ}, such that, Reui(t)Reuj(t)\operatorname{Re}u_{i}(t^{\circ})\neq\operatorname{Re}u_{j}(t^{\circ}) for iji\neq j. Then Reui(t)Reuj(t)\operatorname{Re}u_{i}(t)\neq\operatorname{Re}u_{j}(t) for iji\neq j for all tt sufficiently close to tt^{\circ}. We would like to describe the space of horizontal sections of (m)\nabla^{(m)} locally in a neighbourhood of λ=ui(t)\lambda=u_{i}(t). There is a distinguished solution which can be constructed similarly to (15) but by using Givental’s R-matrix instead of the calibration SS. Let us recall the definition of Givental’s R-matrix (see [16]). Let U(t)=diag(u1(t),,uN(t))U(t)=\operatorname{diag}(u_{1}(t),\dots,u_{N}(t)) and let Ψ(t)\Psi(t) be the N×NN\times N matrix whose (a,i)(a,i) entry is Ψai(t):=Δitaui\Psi_{ai}(t):=\sqrt{\Delta_{i}}\tfrac{\partial t_{a}}{\partial u_{i}}. In other words, Ψ(t)\Psi(t) is the matrix of the linear isomorphism NTtM\mathbb{C}^{N}\cong T_{t}M, eiΔi/uie_{i}\mapsto\sqrt{\Delta_{i}}\partial/\partial u_{i} with respect to the standard basis {ei}i=1N\{e_{i}\}_{i=1}^{N} of N\mathbb{C}^{N} and the flat basis {/ta}a=1N\{\partial/\partial t_{a}\}_{a=1}^{N} of TtMT_{t}M. According to Givental, there exists a unique operator-valued formal series R(t,z)=1+R1(t)z+R2(t)z2+R(t,z)=1+R_{1}(t)z+R_{2}(t)z^{2}+\cdots, such that, the Dubrovin connection has a formal asymptotic solution at z=0z=0 of the form Ψ(t)R(t,z)eU(t)/z\Psi(t)R(t,z)e^{U(t)/z}. Moreover, the matrix series R(t,z)R(t,z) satisfies the symplectic condition R(t,z)tR(t,z)=1R(t,-z)^{t}R(t,z)=1 where t is the standard transposition operation for matrices. It is straightforward to check that the following Laurent series is a solution to (m)\nabla^{(m)}:

(19) Ii(m)(t,λ):=2πk=0(1)kΨ(t)Rk(t)ei(λui)km1/2Γ(km+1/2).I_{i}^{(m)}(t,\lambda):=\sqrt{2\pi}\,\sum_{k=0}^{\infty}(-1)^{k}\,\Psi(t)R_{k}(t)e_{i}\,\frac{(\lambda-u_{i})^{k-m-1/2}}{\Gamma(k-m+1/2)}.

The following proposition is straightforward to prove (see [28], Section 3.2.2)

Proposition 2.3.1.

Suppose that m12\ninm-\tfrac{1}{2}\nin\mathbb{Z}. In a neighbourhood of λ=ui(t)\lambda=u_{i}(t), the space of holomorphic solutions of (m)\nabla^{(m)} is a subspace of co-dimension 1 in the space of all solutions.

From now on we will assume that m12\ninm-\tfrac{1}{2}\nin\mathbb{Z}. Under this condition every solution to (m)\nabla^{(m)}, locally near λ=ui(t)\lambda=u_{i}(t) is a sum of a holomorphic solution and cIi(m)(t,λ)cI^{(m)}_{i}(t,\lambda) for some constant cc. In particular, we can easily describe the local monodromy of (m)\nabla^{(m)} near λ=ui(t)\lambda=u_{i}(t). The analytic continuation along a simple counter-clockwise loop around λ=ui(t)\lambda=u_{i}(t) transforms Ii(m)(t,λ)q2Ii(m)(t,λ)I_{i}^{(m)}(t,\lambda)\mapsto-q^{-2}I_{i}^{(m)}(t,\lambda) where q:=eπ𝐢mq:=e^{\pi\mathbf{i}m}. Note that locally near λ=ui(t)\lambda=u_{i}(t) the holomorphic solutions are precisely the monodromy invariant ones.

Remark 2.3.1.

In the case when m12m-\tfrac{1}{2}\in\mathbb{Z} there might be solutions involving log(λui(t))\log(\lambda-u_{i}(t)).

Let us introduce the following pairings hm:H×Hh_{m}:H\times H\to\mathbb{C}

(20) hm(a,b):=(Ia(m)(t,λ),(λE)Iβ(m)(t,λ)).h_{m}(a,b):=(I^{(m)}_{a}(t,\lambda),(\lambda-E\bullet)I^{(-m)}_{\beta}(t,\lambda)).

Using the differential equations of (±m)\nabla^{(\pm m)} it is easy to check that hm(a,b)h_{m}(a,b) is independent of tt and λ\lambda. In particular, it is a monodromy invariant pairing between the space of mm-twisted and (m)(-m)-twisted periods. Note that we also have the following symmetry:

hm(a,b)=hm(b,a),a,bH.\displaystyle h_{m}(a,b)=h_{-m}(b,a),\quad\forall a,b\in H.

It turns out that there is an explicit formula for hmh_{m} in terms of the Hodge grading operator θ\theta and the nilpotent operator ρ\rho. Let us recall the so-called Euler pairing

(21) a,b:=12π(a,eπ𝐢θeπ𝐢ρb),a,bH.\langle a,b\rangle:=\frac{1}{2\pi}(a,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}b),\quad a,b\in H.

As a byproduct of the proof of Theorem 2.6.1 we will get the following simple formula:

hm(a,b)=qa,b+q1b,a,\displaystyle h_{m}(a,b)=q\langle a,b\rangle+q^{-1}\langle b,a\rangle,

where q:=eπ𝐢mq:=e^{\pi\mathbf{i}m}. Given a reference path (avoiding the discriminant) from (t,λ)(t^{\circ},\lambda^{\circ}) to (t,ui(t))(t,u_{i}(t)), there exists a vector βi(m)\beta_{i}(m), such that, the period vector Iβi(m)(m)(t,λ)=Ii(m)(t,λ)I^{(m)}_{\beta_{i}(m)}(t,\lambda)=I^{(m)}_{i}(t,\lambda). Since the series in (19) involves fractional powers of λui\lambda-u_{i}, the value of βi(m)\beta_{i}(m) depends not only on the reference path but also on the choice of a branch for log(λui)\log(\lambda-u_{i}). In other words, the value of βi(m)\beta_{i}(m) is unique up to a factor in the spiral (q2)(-q^{-2})^{\mathbb{Z}}. Note that fixing the reference path and the branch of log(λui)\log(\lambda-u_{i}) determines βi(m)\beta_{i}(m) for all m{12+}m\in\mathbb{C}\setminus{\{\tfrac{1}{2}+\mathbb{Z}\}}. We will refer to βi(m)\beta_{i}(m) as the mm-twisted reflection vector corresponding to the reference path.

Lemma 2.3.1.

a) We have hm(βi(m),βi(m))=q+q1h_{m}(\beta_{i}(m),\beta_{i}(-m))=q+q^{-1}.

b) If aHa\in H is such that Ia(m)(t,λ)I^{(m)}_{a}(t,\lambda) is holomorphic at λ=ui(t)\lambda=u_{i}(t), then hm(a,βi(m))=0h_{m}(a,\beta_{i}(-m))=0.

Proof.

The proof is obtained by substituting formula (19) into the definition (20) and extracting the leading order term in the Laurent series expansion at λ=ui\lambda=u_{i}. If we do this for the pairing in part a) we will get

2πΓ(m+12)Γ(m+12)=2sinπ(m+12)=2cos(πm)=q+q1.\displaystyle\frac{2\pi}{\Gamma(-m+\tfrac{1}{2})\Gamma(m+\tfrac{1}{2})}=2\sin\pi(m+\tfrac{1}{2})=2\cos(\pi m)=q+q^{-1}.

This proves a). The proof of b) is similar.∎

Proposition 2.3.2.

Let σi\sigma_{i} be the local monodromy transformation of (m)\nabla^{(m)} corresponding to a simple counter-clockwise loop around λ=ui(t)\lambda=u_{i}(t). Then

σi(a)=aq1hm(a,βi(m))βi(m),aH,\displaystyle\sigma_{i}(a)=a-q^{-1}h_{m}(a,\beta_{i}(-m))\,\beta_{i}(m),\quad a\in H,

where βi(±m)H\beta_{i}(\pm m)\in H are ±m\pm m-twisted reflection vectors corresponding to the simple loop.

Proof.

According to Proposition 2.3.1 there exists a decomposition a=a+kβi(m)a=a^{\prime}+k\beta_{i}(m), such that, Ia(m)(t,λ)I^{(m)}_{a^{\prime}}(t,\lambda) is analytic at λ=ui(t)\lambda=u_{i}(t). We have

σi(a)=akq2βi(m)=a(1+q2)kβi(m).\displaystyle\sigma_{i}(a)=a^{\prime}-kq^{-2}\beta_{i}(m)=a-(1+q^{-2})k\beta_{i}(m).

On the other hand, recalling Lemma 2.3.1 we have hm(a,βi(m))=k(q+q1)=k(1+q2)qh_{m}(a,\beta_{i}(-m))=k(q+q^{-1})=k(1+q^{-2})q. Therefore, k(1+q2)=q1hm(a,βi(m))k(1+q^{-2})=q^{-1}h_{m}(a,\beta_{i}(-m)) which yields the formula that we had to prove. ∎

2.4. Asymptotic expansions and Stokes matrices

Let us assume that the base point tt^{\circ} is such that Re(ui(t))Re(uj(t))\operatorname{Re}(u_{i}(t))\neq\operatorname{Re}(u_{j}(t)) for iji\neq j for all tMt\in M sufficiently close to tt^{\circ}. We write uiu_{i} for ui(t)u_{i}(t) for simplicity.

ην\eta_{\nu}η\etaην+1\eta_{\nu+1}uiu_{i}Γi(η)\Gamma_{i}(\eta)λi(η)\lambda^{i}(\eta)λ(η)\lambda^{\circ}(\eta)Ci(η)C_{i}(\eta)λ(η)\lambda^{\circ}(-\eta)λi(η)\lambda^{i}(-\eta)Ci(η)C_{i}(-\eta)
Figure 1. Reference paths and admissible directions

Let 𝕊1={η||η|=1}\mathbb{S}^{1}=\{\eta\in\mathbb{C}\ |\ |\eta|=1\} be the unit circle. A point η𝕊1\eta\in\mathbb{S}^{1} is said to be an admissible direction if the ray Γi(η):={ui+ηs|s0}\Gamma_{i}(\eta):=\{u_{i}+\eta s\ |\ s\in\mathbb{R}_{\geq 0}\} does not pass through uju_{j} for jij\neq i. A direction which is not admissible is said to be critical. If η𝕊1\eta\in\mathbb{S}^{1} is a critical direction, then η-\eta is also critical. Therefore, the number of all critical directions is even, say 2μ2\mu for some μ\mu\in\mathbb{Z}. Following [2] we order the critical directions in a clockwise order η0,η1,,η2μ1\eta_{0},\eta_{1},\dots,\eta_{2\mu-1} in such a way that

π2<Arg(η2μ1)<<Arg(η0)3π2.\displaystyle-\tfrac{\pi}{2}<\operatorname{Arg}(\eta_{2\mu-1})<\cdots<\operatorname{Arg}(\eta_{0})\leq\tfrac{3\pi}{2}.

Let us assume that λ>|ui|\lambda^{\circ}>|u_{i}| for all ii. Our assumption for tt^{\circ} implies that 𝐢=1\mathbf{i}=\sqrt{-1} is an admissible direction. This is going to be our default admissible direction. It will be convenient to introduce an auxiliary reference point λ(η):=𝐢ηλ\lambda^{\circ}(\eta):=-\mathbf{i}\eta\lambda^{\circ}. Note that if we continuously change the admissible direction from 𝐢\mathbf{i} to η\eta, then we will obtain a path connecting λ=λ(𝐢)\lambda^{\circ}=\lambda^{\circ}(\mathbf{i}) and λ(η)\lambda^{\circ}(\eta).

Suppose that η\eta is an admissible direction. Let us consider the following oscillatory integrals:

(22) Xi(η,t,z)=12π(z)m1/2Γi(η)eλ/zIi(m)(t,λ)𝑑λ,X_{i}(\eta,t,z)=\frac{1}{\sqrt{2\pi}}\,(-z)^{m-1/2}\int_{\Gamma_{i}(\eta)}e^{\lambda/z}I_{i}^{(m)}(t,\lambda)d\lambda,

where mm\in\mathbb{C} is a complex number, such that, Re(m)<0\operatorname{Re}(m)<0. The integral is absolutely convergent for all zz in the half-plane

Hη:={z|Re(η/z)<0}={z|Re(ηz¯)<0},\displaystyle H_{\eta}:=\{z\in\mathbb{C}\ |\ \operatorname{Re}(\eta/z)<0\}=\{z\in\mathbb{C}\ |\ \operatorname{Re}(\eta\,\overline{z})<0\},

where z¯\overline{z} is the complex conjugate of zz. Note that if zi=xi+𝐢yiz_{i}=x_{i}+\mathbf{i}y_{i} (i=1,2i=1,2), then Re(z1z¯2)=x1x2+y1y2\operatorname{Re}(z_{1}\,\overline{z}_{2})=x_{1}x_{2}+y_{1}y_{2} is the standard Euclidean pairing. Therefore, HηH_{\eta} is the half-plane in \mathbb{C} whose boundary is the line orthogonal to η\eta and which does not contain η\eta. The definition of (22) requires also a choice of log(z)\log(-z) and log(λui)\log(\lambda-u_{i}) in order to be able to define fractional powers of z-z and (λui)(\lambda-u_{i}). Since the admissible direction η\eta is obtained after a continuous deformation from 𝐢\mathbf{i}, we may fix logη=𝐢Arg(η)+2kπ𝐢\log\eta=\mathbf{i}\operatorname{Arg}(\eta)+2k\pi\mathbf{i} by continuity and by choosing log𝐢:=π𝐢/2\log\mathbf{i}:=\pi\mathbf{i}/2. Since ηHη\eta\in H_{-\eta} the choice of log\log at η\eta uniquely determines a holomorphic branch of log\log defined on the entire half-plane HηH_{-\eta}. Note that when λΓi(η)\lambda\in\Gamma_{i}(\eta) we have λuiHη\lambda-u_{i}\in H_{-\eta}. Moreover, for the convergence of the integral (22) we have to require that zHη-z\in H_{-\eta}. Therefore, both z-z and (λui)(\lambda-u_{i}) belong to HηH_{-\eta} and we have a natural choice of the value of log\log. We get that Xi(η,t,z)X_{i}(\eta,t,z) is a holomorphic function for zHηz\in H_{\eta}. Put λui=sz\lambda-u_{i}=-sz and note that for zη>0z\in-\eta\mathbb{R}_{>0} we have

Γi(η)eλ/z(λui)km12Γ(km+12)𝑑λ=eui/z(z)km+12.\displaystyle\int_{\Gamma_{i}(\eta)}e^{\lambda/z}\frac{(\lambda-u_{i})^{k-m-\tfrac{1}{2}}}{\Gamma(k-m+\tfrac{1}{2})}d\lambda=e^{u_{i}/z}\,(-z)^{k-m+\tfrac{1}{2}}.

Recalling the stationary phase asymptotic method and using the expansion (19) we get that

(23) Xi(η,t,z)Ψ(t)R(t,z)eieui/z,z0 in Hη.X_{i}(\eta,t,z)\ \sim\ \Psi(t)R(t,z)e_{i}e^{u_{i}/z},\quad z\to 0\mbox{ in }H_{\eta}.

Suppose that η\eta^{\prime} and η′′\eta^{\prime\prime} are two admissible directions, such that, η\eta^{\prime} and η′′\eta^{\prime\prime} belong to the same clockwise arc from ην\eta_{\nu} to ην+1\eta_{\nu+1},i.e., the arc bounded by two adjacent critical directions. By definition, the sector between the rays Γi(η)\Gamma_{i}(\eta^{\prime}) and Γi(η′′)\Gamma_{i}(\eta^{\prime\prime}) does not contain uju_{j} for jij\neq i. This implies that Ii(m)(t,λ)I^{(m)}_{i}(t,\lambda) extends to a holomorphic function in that sector. Using the Cauchy residue theorem, it is easy to prove that Xi(η,t,z)=Xi(η′′,t,z)X_{i}(\eta^{\prime},t,z)=X_{i}(\eta^{\prime\prime},t,z) for all zHηHη′′z\in H_{\eta^{\prime}}\cap H_{\eta^{\prime\prime}}. We get that for every admissible direction η\eta, the oscillatory integral (22) extends analytically in zz for all zHηνHην+1z\in H_{\eta_{\nu}}\cup H_{\eta_{\nu+1}} where ην\eta_{\nu} and ην+1\eta_{\nu+1} are the two critical directions adjacent to η\eta.

η\etaην\eta_{\nu}ην+1\eta_{\nu+1}HηνHην+1H_{-\eta_{\nu}}\cap H_{\eta_{\nu+1}}HηνHην+1H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}
Figure 2. Domains of analyticity in zz

Figure (2) might help visualize the domains of analyticity. Let us denote by X(η,t,z)X(\eta,t,z) the matrix of size N×NN\times N whose ii-th column is Xi(η,t,z)X_{i}(\eta,t,z). Since both X(η,t,z)X(-\eta,t,z) and X(η,t,z)X(\eta,t,z) are solutions to the Dubrovin connection for zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}, there exists a matrix V+(η)V_{+}(\eta), such that,

(24) X(η,t,z)=X(η,t,z)V+(η),zHηνHην+1.X(-\eta,t,z)=X(\eta,t,z)\,V_{+}(\eta),\quad\forall z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}.

Similarly, there exists a matrix V(η)V_{-}(\eta), such that,

(25) X(η,t,z)=X(η,t,z)V(η),zHηνHην+1.X(-\eta,t,z)=X(\eta,t,z)\,V_{-}(\eta),\quad\forall z\in H_{-\eta_{\nu}}\cap H_{\eta_{\nu+1}}.

In both formulas (24) and (25) we define η-\eta by continuously rotating η\eta on 180180^{\circ} in clockwise direction. The matrices V+V_{+} and VV_{-} are called Stokes matrices. There is a simple relation between V+V_{+} and VV_{-} (see [8], Proposition 3.10).

Proposition 2.4.1.

We have V+=VtV_{+}=V_{-}^{t} where t is the usual transposition operation of matrices.

Proof.

Let gab=(/ta,/tb)g_{ab}=(\partial/\partial t_{a},\partial/\partial t_{b}) be the matrix of the Frobenius pairing. Note that ΨtgΨ=1\Psi^{t}g\Psi=1. We claim that X(η,t,z)tgX(η,t,z)=1X(-\eta,t,-z)^{t}gX(\eta,t,z)=1. First of all, using that X(±η,t,z)X(\pm\eta,t,z) is a solution to the Dubrovin connection we get that A:=X(η,t,z)tgX(η,t,z)A:=X(\eta,t,-z)^{t}gX(\eta,t,z) is a constant independent of tt and zz. Let us recall the asymptotic expansions X(η,t,z)Ψ(t)R(t,z)eU/zX(\eta,t,z)\sim\Psi(t)R(t,z)e^{U/z} and X(η,t,z)Ψ(t)R(t,z)eU/zX(-\eta,t,-z)\sim\Psi(t)R(t,-z)e^{-U/z} where z0z\to 0 and zHηz\in H_{\eta}. In particular, we have that both X(η,t,z)eU/zX(\eta,t,z)e^{-U/z} and X(η,t,z)eU/zX(-\eta,t,-z)e^{U/z} have limit when z0z\to 0 and zHηz\in H_{\eta} which must be Ψ\Psi (in both cases). Therefore, eU/zAeU/zΨtgΨ=1e^{U/z}Ae^{-U/z}\to\Psi^{t}g\Psi=1 when z0z\to 0 in the half-plane HηH_{\eta}. This implies that the diagonal entries of AA must be 1. For iji\neq j, since η\eta is an admissible direction, we can find z0Hηz_{0}\in H_{\eta}, such that, Re((uiuj)/z0)>0\operatorname{Re}((u_{i}-u_{j})/z_{0})>0. If Aij0A_{ij}\neq 0, then the (i,j)(i,j) entry of eU/zAeU/ze^{U/z}Ae^{-U/z}, that is, e(uiuj)/zAije^{(u_{i}-u_{j})/z}A_{ij} has an exponential growth as z0z\to 0 in the direction of z0z_{0} – contradiction. This completes the proof of our claim.

Suppose that zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}. Then we have X(η,t,z)=X(η,t,z)V+1X(\eta,t,z)=X(-\eta,t,z)V_{+}^{-1} and X(η,t,z)=X(η,t,z)VX(-\eta,t,-z)=X(\eta,t,-z)V_{-} because zHηνHην+1-z\in H_{-\eta_{\nu}}\cap H_{\eta_{\nu+1}}. We get

1=X(η,t,z)tgX(η,t,z)=VtX(η,t,z)tgX(η,t,z)V+1=VtV+1.\displaystyle 1=X(-\eta,t,-z)^{t}gX(\eta,t,z)=V_{-}^{t}\,X(\eta,t,-z)^{t}gX(-\eta,t,z)V_{+}^{-1}=V_{-}^{t}\,V_{+}^{-1}.\qed

The following proposition is well known (see [8], Proposition 3.10).

Proposition 2.4.2.

Let V+,ijV_{+,ij} be the (i,j)(i,j)-entry of the Stokes matrix V+V_{+}. Suppose that zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}. Then

  1. (a)

    The diagonal entries V+,ii=1V_{+,ii}=1 for all 1iN1\leq i\leq N.

  2. (b)

    If Re((uiuj)/z)>0\operatorname{Re}((u_{i}-u_{j})/z)>0, then V+,ij=0V_{+,ij}=0.

Proof.

Using the asymptotic expansion (23) and the identity (24) we get that eU/(sz)V+eU/(sz)e^{U/(sz)}V_{+}e^{-U/(sz)}, where s>0s\in\mathbb{R}_{>0} and zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}, has a limit when s0s\to 0 which must be the identity matrix. Part (a) follows immediately from this observation. For part (b) we need only to notice that if Re((uiuj)/z)>0\operatorname{Re}((u_{i}-u_{j})/z)>0, then e(uiuj)/(sz)e^{(u_{i}-u_{j})/(sz)} has an exponential growth as s0s\to 0. Therefore, the limit of e(uiuj)/(sz)V+,ije^{(u_{i}-u_{j})/(sz)}V_{+,ij} exists only if V+,ij=0V_{+,ij}=0. ∎

Remark 2.4.1.

Note that the condition Re((uiuj)/z)>0\operatorname{Re}((u_{i}-u_{j})/z)>0 in (b) is independent of the choice of zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}, otherwise the direction of uiuju_{i}-u_{j} or ujuiu_{j}-u_{i} must belong to the cone spanned by ην\eta_{\nu} and ην+1\eta_{\nu+1} contradicting the fact that there are no critical directions between ην\eta_{\nu} and ην+1\eta_{\nu+1}. ∎

Recalling Proposition 2.4.1 we get the following corollary.

Corollary 2.4.1.

Let V,ijV_{-,ij} be the (i,j)(i,j)-entry of the Stokes matrix VV_{-}. Suppose that zHηνHην+1z\in H_{-\eta_{\nu}}\cap H_{\eta_{\nu+1}}. Then

  1. (a)

    The diagonal entries V,ii=1V_{-,ii}=1 for all 1iN1\leq i\leq N.

  2. (b)

    If Re((uiuj)/z)>0\operatorname{Re}((u_{i}-u_{j})/z)>0, then V,ij=0V_{-,ij}=0. ∎

2.5. Stokes matrices and the intersection pairing

Let us continue to work in the settings of the previous subsection. We would like to construct a system of reference paths CiC_{i} and express the entries of the Stokes matrix V+V_{+} in terms of the Euler pairing and the reflection vectors corresponding to the reference paths. Let λi(η)\lambda^{i}(\eta) be the intersection of the ray Γi(η)\Gamma_{i}(\eta) and the circle |λ|=λ|\lambda|=\lambda^{\circ} (see Figure 1). Recall that we fixed an auxiliary reference point λ(η)=𝐢ηλ\lambda^{\circ}(\eta)=-\mathbf{i}\eta\lambda^{\circ} which is connected to λ\lambda^{\circ} by contuniously deforming the direction from 𝐢\mathbf{i} to η\eta. We define the path Ci(η)C_{i}(\eta) to be the composition of the counter-clockwise oriented arc from λ(η)\lambda^{\circ}(\eta) to λi(η)\lambda^{i}(\eta) and the line segment from λi(η)\lambda^{i}(\eta) to uiu_{i} (see the blue paths on Figure 1). Let βi(m)H\beta_{i}(m)\in H be the reflection vector corresponding to the path Ci(η)C_{i}(\eta), that is, Ii(m)(t,λ)=Iβi(m)(m)(t,λ)I^{(m)}_{i}(t,\lambda)=I^{(m)}_{\beta_{i}(m)}(t,\lambda). Following [2], let us introduce the vectors βi(m)\beta_{i}^{*}(m) (1iN1\leq i\leq N), such that, hm(βi(m),βj(m))=δijh_{m}(\beta_{i}^{*}(m),\beta_{j}(-m))=\delta_{ij}. The pairing hmh_{m} is non-degenerate except for finitely many mm\in\mathbb{C}. The definition of βi(m)\beta_{i}^{*}(m) makes sense except for finitely many values of mm. The properties of the corresponding period vectors can be summarized as follows (compare with [2], Proposition 1 and Theorem 2’).

Proposition 2.5.1.

a) The period vector Iβi(m)(m)(t,λ)I^{(m)}_{\beta_{i}^{*}(m)}(t,\lambda) is analytic at λ=uj\lambda=u_{j} for jij\neq i, where the value of the period is specified via the reference path Cj(η)C_{j}(\eta).

b) The following formula holds:

βi(m)=(q+q1)βi(m)+j:jihm(βi(m),βj(m))βj(m).\displaystyle\beta_{i}(m)=(q+q^{-1})\,\beta_{i}^{*}(m)+\sum_{j:j\neq i}h_{m}(\beta_{i}(m),\beta_{j}(-m))\beta_{j}^{*}(m).

c) Let γi(η)\gamma_{i}(-\eta)\subset\mathbb{C} be a contour starting at λ=\lambda=\infty, approaching λ=ui\lambda=u_{i} along the ray Γi(η)\Gamma_{i}(-\eta), making a small loop around λ=ui\lambda=u_{i}, and finally returning back to λ=\lambda=\infty along Γi(η)\Gamma_{i}(-\eta). Put

Xi(η,t,z)=q(z)m1/22πγi(η)eλ/zIβi(m)(t,λ)𝑑λ,\displaystyle X_{i}^{*}(-\eta,t,z)=-q\,\frac{(-z)^{m-1/2}}{\sqrt{2\pi}}\,\int_{\gamma_{i}(-\eta)}e^{\lambda/z}I^{(m)}_{\beta_{i}^{*}}(t,\lambda)d\lambda,

where the value of Iβi(m)(t,λ)I^{(m)}_{\beta_{i}^{*}}(t,\lambda) is determined by the reference path Ci(η)C_{i}(\eta) as follows: first we fix the value at the intersection of γi(η)\gamma_{i}(-\eta) and Ci(η)C_{i}(\eta), then we extend by continuity to the remaining points of γi(η)\gamma_{i}(-\eta). Then Xi(η,t,z)X_{i}^{*}(-\eta,t,z) coincides with Xi(η,t,z)X_{i}(-\eta,t,z) for all zHηz\in H_{-\eta} where in order to specify the value of Xi(η,t,z)X_{i}(-\eta,t,z) and of log(z)\log(-z) we take a clockwise rotation from η\eta to η-\eta.

Proof.

a) Using Proposition 2.3.2 we get that σj(βi)=βiq1hm(βi(m),βj(m))βj(m)=βi\sigma_{j}(\beta_{i}^{*})=\beta_{i}^{*}-q^{-1}h_{m}(\beta_{i}^{*}(m),\beta_{j}(-m))\,\beta_{j}(m)=\beta_{i}^{*} where we use that for iji\neq j the pairing hm(βi(m),βj(m))=0h_{m}(\beta_{i}^{*}(m),\beta_{j}(-m))=0. Therefore, the period Iβi(m)(m)(t,λ)I^{(m)}_{\beta_{i}^{*}(m)}(t,\lambda) is single-valued in a neighborhood of λ=uj\lambda=u_{j} which is possible only if it is holomorphic.

b) This is obvious from the definition of βi(m)\beta_{i}^{*}(m).

c) According to parts a) and b), the difference (q+q1)Iβi(m)(t,λ)Iβi(m)(t,λ)(q+q^{-1})I^{(m)}_{\beta_{i}^{*}}(t,\lambda)-I^{(m)}_{\beta_{i}}(t,\lambda) is holomorphic at λ=ui\lambda=u_{i}. Moreover, the periods being solutions to a Fuchsian differential equation, have at most polynomial growth at λ=\lambda=\infty. Recalling the Cauchy residue theorem we get

(26) γi(η)eλ/z((q+q1)Iβi(m)(t,λ)Iβi(m)(t,λ))𝑑λ=0.\int_{\gamma_{i}(-\eta)}e^{\lambda/z}((q+q^{-1})\,I^{(m)}_{\beta_{i}^{*}}(t,\lambda)-I^{(m)}_{\beta_{i}}(t,\lambda))d\lambda=0.

Using integration by parts, it is easy to check that XiX_{i}^{*} is invariant under the shift mm+1m\mapsto m+1. Therefore, we may assume that Re(m)<0\operatorname{Re}(m)<0. Note that

(27) γi(η)eλ/zIβi(m)(t,λ)𝑑λ=(Γi(η)q2Γi(η))eλ/zIβi(m)(t,λ)dλ.\int_{\gamma_{i}(-\eta)}e^{\lambda/z}I^{(m)}_{\beta_{i}}(t,\lambda)d\lambda=\Big{(}-\int_{\Gamma_{i}(-\eta)}-q^{-2}\int_{\Gamma_{i}(-\eta)}\Big{)}e^{\lambda/z}I^{(m)}_{\beta_{i}}(t,\lambda)d\lambda.

Indeed, let us split the integration contour γi(η)\gamma_{i}(-\eta) into 3 pieces: Γi(η)[ui,uiϵη]-\Gamma_{i}(-\eta)\setminus{[u_{i},u_{i}-\epsilon\eta]} going from η-\infty\eta to uiϵηu_{i}-\epsilon\eta, an ϵ\epsilon-loop around λ=ui\lambda=u_{i} starting and ending at uiϵηu_{i}-\epsilon\eta, and the ray Γi(η)[ui,uiϵη]\Gamma_{i}(-\eta)\setminus{[u_{i},u_{i}-\epsilon\eta]} from uiϵηu_{i}-\epsilon\eta to η-\infty\eta . Recalling the Laurent series expansion (19), we get that under the analytic continuation along the ϵ\epsilon-loop, the integrand Iβi(m)(t,λ)I^{(m)}_{\beta_{i}}(t,\lambda) gains a factor of q2-q^{-2}. Since the orientations of the first and the third contours are opposite, we get that the corresponding integrals differ by a factor of q2q^{-2}. Furthermore, since m<0m<0, the integral along the loop has a contribution which vanishes in the limit ϵ0\epsilon\to 0. This completes the proof of formula (27). Using formulas (26) and (27) we get

γi(η)eλ/zIβi(m)(t,λ)=1+q2q+q1Γi(η)eλ/zIβi(m)(t,λ))dλ=q1Γi(η)eλ/zIβi(m)(t,λ))dλ.\displaystyle\int_{\gamma_{i}(-\eta)}e^{\lambda/z}\,I^{(m)}_{\beta_{i}^{*}}(t,\lambda)=-\frac{1+q^{-2}}{q+q^{-1}}\,\int_{\Gamma_{i}(-\eta)}e^{\lambda/z}\,I^{(m)}_{\beta_{i}}(t,\lambda))d\lambda=-q^{-1}\int_{\Gamma_{i}(-\eta)}e^{\lambda/z}\,I^{(m)}_{\beta_{i}}(t,\lambda))d\lambda.

The statement in part c) follows from the above formula. ∎

Suppose now that η~\widetilde{\eta} is another admissible direction, such that, ην<η~<ην1\eta_{\nu}<\widetilde{\eta}<\eta_{\nu-1}. In other words, η~\widetilde{\eta} is obtained from η\eta by crossing the critical direction ην\eta_{\nu}. Let β~i\widetilde{\beta}_{i} and β~i\widetilde{\beta}_{i}^{*} be the vectors corresponding to the reference paths Ci(η~)C_{i}(\widetilde{\eta}). We would like to express β~i\widetilde{\beta}_{i} and β~i\widetilde{\beta}_{i}^{*} in terms of βi\beta_{i} and βi\beta_{i}^{*}. Let us split the points u1,,uNu_{1},\dots,u_{N} into groups, such that, each group belongs to a ray with direction ην\eta_{\nu} and the rays of different groups are different. Let (uj1,,ujk)(u_{j_{1}},\dots,u_{j_{k}}) be one such group whose elements are ordered in such a way that uja=ujk+saηνu_{j_{a}}=u_{j_{k}}+s_{a}\eta_{\nu} for some real numbers s1>s2>>sk=0s_{1}>s_{2}>\cdots>s_{k}=0. We will refer to such a sequence (uj1,,ujk)(u_{j_{1}},\dots,u_{j_{k}}) as ην\eta_{\nu}-sequence. Clearly this splitting is uniquely determined by the critical direction ην\eta_{\nu}.

ujku_{j_{k}}λjk(η)\lambda^{j_{k}}(\eta)Cjk(η)C_{j_{k}}(\eta)λjk(η~)\lambda^{j_{k}}(\widetilde{\eta})Cjk(η~)C_{j_{k}}(\widetilde{\eta})uj3u_{j_{3}}uj2u_{j_{2}}uj1u_{j_{1}}
Figure 3. ην\eta_{\nu}-sequence
Proposition 2.5.2.

Suppose that (uj1,,ujk)(u_{j_{1}},\dots,u_{j_{k}}) is a ην\eta_{\nu}-sequence. Then

β~j1=βj1,β~jt=σj11σjt11(βjt)(2tk)\displaystyle\widetilde{\beta}_{j_{1}}=\beta_{j_{1}},\quad\widetilde{\beta}_{j_{t}}=\sigma^{-1}_{j_{1}}\cdots\sigma^{-1}_{j_{t-1}}(\beta_{j_{t}})\quad(2\leq t\leq k)

and

β~jk=βjk,β~jt=βjt+a=t+1kq1hm(βjt(m),βja(m))βja(1tk1).\displaystyle\widetilde{\beta}_{j_{k}}^{*}=\beta_{j_{k}}^{*},\quad\widetilde{\beta}_{j_{t}}^{*}=\beta_{j_{t}}^{*}+\sum_{a=t+1}^{k}q^{-1}\,h_{m}(\beta_{j_{t}}(m),\beta_{j_{a}}(-m))\beta_{j_{a}}^{*}\quad(1\leq t\leq k-1).
Proof.

For part a), let us look at figure (3). By definition, the period Ijk(m)(t,λ)I^{(m)}_{j_{k}}(t,\lambda) defined in a neighbourhood of λ=ujk\lambda=u_{j_{k}} is obtained from Iβjk(m)(t,λ)I^{(m)}_{\beta_{j_{k}}}(t,\lambda) via the analytic continuation along the reference path Cjk(η)C_{j_{k}}(\eta). On the other hand, the analytic continuation of Ijk(m)(t,λ)I^{(m)}_{j_{k}}(t,\lambda) along the inverse of the reference path Cjk(η~)C_{j_{k}}(\widetilde{\eta}) yields Iβ~jk(m)(t,λ)I^{(m)}_{\widetilde{\beta}_{j_{k}}}(t,\lambda). The conclusion is that the cycle β~jk\widetilde{\beta}_{j_{k}} is obtained from βjk\beta_{j_{k}} after a monodromy transformation along a small modification of the loop consisting of the following 3 pieces: the line segment from λjk(η)\lambda^{j_{k}}(\eta) to ujku_{j_{k}}, the line segment from ujku_{j_{k}} to λjk(η~)\lambda^{j_{k}}(\widetilde{\eta}), and the arc from λjk(η~)\lambda^{j_{k}}(\widetilde{\eta}) to λjk(η)\lambda^{j_{k}}(\eta). The small modification, necessary to avoid the singularity ujku_{j_{k}}, is taken as follows: when we approach ujku_{j_{k}} along Cjk(η)C_{j_{k}}(\eta) we have to stop slightly before hitting ujku_{j_{k}}, make an anti-clockwise rotation along ujku_{j_{k}} until we hit Cjk(η~)C_{j_{k}}(\widetilde{\eta}) and then continue along the old contour. The reason why we have to make anti-clockwise rotation, and not clockwise, is that the value of log(λujk)\log(\lambda-u_{j_{k}}), needed to define Ijk(m)(t,λ)I^{(m)}_{j_{k}}(t,\lambda), is determined by logη\log\eta (resp. logη~\log\widetilde{\eta}) when λCjk(η)\lambda\in C_{j_{k}}(\eta) (resp. λCjk(η~)\lambda\in C_{j_{k}}(\widetilde{\eta})). Since η~\widetilde{\eta} is obtained from η\eta by anti-clockwise rotation, we have to go around ujku_{j_{k}} anti-clockwise. Clearly, the loop decomposes into simple loops going successively clockwise around the points ujk1,,uj1u_{j_{k-1}},\dots,u_{j_{1}} in the given order, i.e., first around ujk1u_{j_{k-1}}, then ujk2u_{j_{k-2}}, etc., finally uj1u_{j_{1}}. After this discussion the first formula that we have to prove should be clear.

For the second formula, let us argue by induction. The fact that β~jk=βjk\widetilde{\beta}_{j_{k}}^{*}=\beta_{j_{k}}^{*} follows immediately from the first part of the proposition which implies that β~jt\widetilde{\beta}_{j_{t}} is a sum of βjt\beta_{j_{t}} and a linear combination of βj1,,βjt1\beta_{j_{1}},\dots,\beta_{j_{t-1}}. Suppose that the formula is proved for all t>st>s. Let us find coefficients bs+1,,bkb_{s+1},\dots,b_{k}, such that

B:=βjs+bs+1βjs+1++bkβjk\displaystyle B:=\beta_{j_{s}}^{*}+b_{s+1}\beta_{j_{s+1}}^{*}+\cdots+b_{k}\beta_{j_{k}}^{*}

satisfies the defining equations of β~js\widetilde{\beta}^{*}_{j_{s}}. Note that hm(B,β~ja)=δjs,jah_{m}(B,\widetilde{\beta}_{j_{a}})=\delta_{j_{s},j_{a}} for all asa\leq s. Therefore, we have to solve the equations hm(B,β~ja)=0h_{m}(B,\widetilde{\beta}_{j_{a}})=0 (a=s+1,,ka=s+1,\dots,k) for bs+1,,bkb_{s+1},\dots,b_{k}. For a=s+1a=s+1, we get

(28) hm(B,β~js+1)=hm(σjsσj1(B),βjs+1)=hm(σjs(βjs)+bs+1βjs+1,βjs+1),h_{m}(B,\widetilde{\beta}_{j_{s+1}})=h_{m}(\sigma_{j_{s}}\cdots\sigma_{j_{1}}(B),\beta_{j_{s+1}})=h_{m}(\sigma_{j_{s}}(\beta_{j_{s}}^{*})+b_{s+1}\beta_{j_{s+1}}^{*},\beta_{j_{s+1}}),

where we used that the pairing hmh_{m} is monodromy invariant and we dropped from BB all terms that do not contribute. Note that by Proposition 2.3.2 we have

σjs(βjs)=βjsq1hm(βjs,βjs)βjs=βjsq1βjs.\displaystyle\sigma_{j_{s}}(\beta_{j_{s}}^{*})=\beta_{j_{s}}^{*}-q^{-1}h_{m}(\beta_{j_{s}}^{*},\beta_{j_{s}})\beta_{j_{s}}=\beta_{j_{s}}^{*}-q^{-1}\,\beta_{j_{s}}.

Substituting this formula in (28) we get bs+1=q1hm(βjs,βjs+1)b_{s+1}=q^{-1}h_{m}(\beta_{j_{s}},\beta_{j_{s+1}}). Suppose that we proved that bs+i=q1hm(βjs,βjs+i)b_{s+i}=q^{-1}\,h_{m}(\beta_{j_{s}},\beta_{j_{s+i}}) for i=1,,li=1,\dots,l. In order to determine bs+l+1b_{s+l+1}, let us consider the equation hm(B,β~js+l+1)=0h_{m}(B,\widetilde{\beta}_{j_{s+l+1}})=0. We get

hm(σjs+lσjs(B),βjs+l+1)=0.\displaystyle h_{m}(\sigma_{j_{s+l}}\cdots\sigma_{j_{s}}(B),\beta_{j_{s+l+1}})=0.

Recalling the ansatz for BB we get that in σjs+lσjs(B)\sigma_{j_{s+l}}\cdots\sigma_{j_{s}}(B) only the following terms will contribute:

σjs+lσjs+1(σjs(βjs))+bs+1σjs+lσjs+2(σjs+1(βjs+1))++bs+lσjs+l(βjs+l)+bs+l+1βjs+l+1.\displaystyle\sigma_{j_{s+l}}\cdots\sigma_{j_{s+1}}(\sigma_{j_{s}}(\beta_{j_{s}}^{*}))+b_{s+1}\sigma_{j_{s+l}}\cdots\sigma_{j_{s+2}}(\sigma_{j_{s+1}}(\beta_{j_{s+1}}^{*}))+\cdots+b_{s+l}\sigma_{j_{s+l}}(\beta_{j_{s+l}}^{*})+b_{s+l+1}\beta_{j_{s+l+1}}^{*}.

We have σjt(βjt)=βjtq1βjt\sigma_{j_{t}}(\beta_{j_{t}}^{*})=\beta_{j_{t}}^{*}-q^{-1}\beta_{j_{t}} for t=s,s+1,,s+lt=s,s+1,\dots,s+l. Note that βjt\beta_{j_{t}}^{*} is fixed by σjt+1,,σjs+l\sigma_{j_{t+1}},\dots,\sigma_{j_{s+l}} and that hm(βjt,βjs+l+1)=0h_{m}(\beta_{j_{t}}^{*},\beta_{j_{s+l+1}})=0. Therefore, we may replace the above expression with

(29) σjs+lσjs+1(q1βjs)+bs+1σjs+lσjs+2(q1βjs+1)++bs+l(q1βjs+l)+bs+l+1βjs+l+1.\sigma_{j_{s+l}}\cdots\sigma_{j_{s+1}}(-q^{-1}\beta_{j_{s}})+b_{s+1}\sigma_{j_{s+l}}\cdots\sigma_{j_{s+2}}(-q^{-1}\beta_{j_{s+1}})+\cdots+b_{s+l}(-q^{-1}\beta_{j_{s+l}})+b_{s+l+1}\beta_{j_{s+l+1}}^{*}.

Let us add the first two terms. After pulling out the common expression q1σjs+lσjs+2-q^{-1}\,\sigma_{j_{s+l}}\cdots\sigma_{j_{s+2}} we are left with

σjs+1(βjs)+bs+1βjs+1=βjsq1hm(βjs,βjs+1)βjs+1+bs+1βjs+1=βjs,\displaystyle\sigma_{j_{s+1}}(\beta_{j_{s}})+b_{s+1}\beta_{j_{s+1}}=\beta_{j_{s}}-q^{-1}\,h_{m}(\beta_{j_{s}},\beta_{j_{s+1}})\beta_{j_{s+1}}+b_{s+1}\beta_{j_{s+1}}=\beta_{j_{s}},

where we used the formula for bs+1b_{s+1}. Therefore, after adding up the first two terms in (29) we get

σjs+lσjs+2(q1βjs)+bs+2σjs+lσjs+3(q1βjs+2)++bs+l(q1βjs+l)+bs+l+1βjs+l+1.\displaystyle\sigma_{j_{s+l}}\cdots\sigma_{j_{s+2}}(-q^{-1}\beta_{j_{s}})+b_{s+2}\sigma_{j_{s+l}}\cdots\sigma_{j_{s+3}}(-q^{-1}\beta_{j_{s+2}})+\cdots+b_{s+l}(-q^{-1}\beta_{j_{s+l}})+b_{s+l+1}\beta_{j_{s+l+1}}^{*}.

Clearly we can continue adding up the first two terms until we reach

σjs+l(q1βjs)+bs+l(q1βjs+l)+bs+l+1βjs+l+1=qβjs+bs+l+1βjs+l+1.\displaystyle\sigma_{j_{s+l}}(-q^{-1}\beta_{j_{s}})+b_{s+l}(-q^{-1}\beta_{j_{s+l}})+b_{s+l+1}\beta_{j_{s+l+1}}^{*}=-q\beta_{j_{s}}+b_{s+l+1}\beta_{j_{s+l+1}}^{*}.

The hmh_{m}-pairing of the above expression with βjs+l+1\beta_{j_{s+l+1}} must be 0. We get bs+l+1=q1hm(βjs,βjs+l+1)b_{s+l+1}=q^{-1}h_{m}(\beta_{j_{s}},\beta_{j_{s+l+1}}). This completes the proof. ∎

Let us denote by WνW_{\nu} the matrix whose (i,j)(i,j)-entry is

Wν,ij:={q1hm(βi(m),βj(m)) if uiΓj(ην),1 if i=j,0 otherwise.\displaystyle W_{\nu,ij}:=\begin{cases}q^{-1}\,h_{m}(\beta_{i}(m),\beta_{j}(-m))&\mbox{ if }u_{i}\in\Gamma_{j}(\eta_{\nu}),\\ 1&\mbox{ if }i=j,\\ 0&\mbox{ otherwise.}\end{cases}
Proposition 2.5.3.

Suppose that η\eta and η~\widetilde{\eta} are admissible directions separated by a single critical direction ην\eta_{\nu}. Then

Xj(η~,t,z)=i=1NXi(η,t,z)Wν,jizHηHη~.\displaystyle X_{j}(-\widetilde{\eta},t,z)=\sum_{i=1}^{N}X_{i}(-\eta,t,z)\,W_{\nu,ji}\quad\forall z\in H_{-\eta}\cap H_{-\widetilde{\eta}}.
Proof.

The 2nd formula in Proposition 2.5.2 implies that

(30) Iβ~j(m)(t,λ)=k=1NIβk(m)(t,λ)Wν,jk,1jN.I^{(m)}_{\widetilde{\beta}_{j}^{*}}(t,\lambda)=\sum_{k=1}^{N}I^{(m)}_{\beta_{k}^{*}}(t,\lambda)\,W_{\nu,jk},\quad 1\leq j\leq N.

Recalling Proposition 2.5.1, c), we get that in order to complete the proof it would be sufficient to deform the integration contours γj(η~)\gamma_{j}(-\widetilde{\eta}) and γk(η)\gamma_{k}(-\eta) (k:ujΓk(ην)k:\ u_{j}\in\Gamma_{k}(\eta_{\nu})) to a common contour without changing the values of the corresponding oscillatory integrals. This would be possible thanks to our special choice of reference paths.

Let uiu_{i} be the last entry of the ην\eta_{\nu}-sequence containing uju_{j}. We pick a contour γi(η~,η)\gamma_{i}(-\widetilde{\eta},-\eta) consisting of 3 parts: the ray Γi(η~)[ui,uiϵη~)\Gamma_{i}(-\widetilde{\eta})\setminus{[u_{i},u_{i}-\epsilon\widetilde{\eta})} with orientation from λ=η~\lambda=-\infty\,\widetilde{\eta} to λ=uiϵη~\lambda=u_{i}-\epsilon\widetilde{\eta}, the counter-clockwise arc from uiϵη~u_{i}-\epsilon\widetilde{\eta} to uiϵηu_{i}-\epsilon\eta, and finally the ray Γi(η)[ui,uiϵη)\Gamma_{i}(-\eta)\setminus{[u_{i},u_{i}-\epsilon\eta)} (see Figure 4).

uiu_{i}γi(η~,η)\gamma_{i}(-\widetilde{\eta},-\eta)η\etaη~\widetilde{\eta}ην\eta_{\nu}uku_{k}uj\ u_{j}γj(η~)\gamma_{j}(-\widetilde{\eta})γk(η)\gamma_{k}(-\eta)
Figure 4. Contour deformation

Let uku_{k} be a point in the ην\eta_{\nu}-sequence preceding uju_{j}. We claim that

(31) γi(η~,η)eλ/zIβk(m)(t,λ)𝑑λ=γk(η)eλ/zIβk(m)(t,λ)𝑑λ\int_{\gamma_{i}(-\widetilde{\eta},-\eta)}e^{\lambda/z}I^{(m)}_{\beta_{k}^{*}}(t,\lambda)d\lambda=\int_{\gamma_{k}(-\eta)}e^{\lambda/z}I^{(m)}_{\beta_{k}^{*}}(t,\lambda)d\lambda

and

(32) γi(η~,η)eλ/zIβ~j(m)(t,λ)𝑑λ=γj(η~)eλ/zIβ~j(m)(t,λ)𝑑λ.\int_{\gamma_{i}(-\widetilde{\eta},-\eta)}e^{\lambda/z}I^{(m)}_{\widetilde{\beta}_{j}^{*}}(t,\lambda)d\lambda=\int_{\gamma_{j}(-\widetilde{\eta})}e^{\lambda/z}I^{(m)}_{\widetilde{\beta}_{j}^{*}}(t,\lambda)d\lambda.

Let us justify the first identity. The argument for the second one is similar. To begin with, note that βk\beta_{k}^{*} is invariant under the monodromy transformations σl\sigma_{l} (the monodromy transformation corresponding to the simple loop Cl(η)C_{l}(\eta)) for lkl\neq k. Thanks to our special choice of the reference paths, i.e., the reference paths Cl(η)C_{l}(\eta) (lk)(l\neq k) do not intersect the ray Γk(η)\Gamma_{k}(-\eta), the fundamental group of Γk(η)\mathbb{C}\setminus{\Gamma_{k}(-\eta)} is generated by the simple loops corresponding to the paths Cl(η)C_{l}(\eta) with lkl\neq k. Therefore, the period integral Iβk(m)(t,λ)I^{(m)}_{\beta_{k}^{*}}(t,\lambda) extends to a holomorphic function in λ\lambda for all λΓk(η)\lambda\in\mathbb{C}\setminus{\Gamma_{k}(-\eta)}. In particular, Iβk(m)(t,λ)I^{(m)}_{\beta_{k}^{*}}(t,\lambda) extends to a holomorphic function in the domain DD bounded by the contours γi(η~,η)\gamma_{i}(-\widetilde{\eta},-\eta) and γk(η)\gamma_{k}(-\eta). Furthermore, for zHη~Hηz\in H_{-\widetilde{\eta}}\cap H_{-\eta} the integrand eλ/zIβk(m)(t,λ)e^{\lambda/z}I^{(m)}_{\beta_{k}^{*}}(t,\lambda) will have an exponential decay at infinity in DD. Therefore, the identity follows from the Cauchy residue theorem. Finally, the formula that we have to prove follows from Proposition 2.5.1, c) and formulas (30), (31), and (32). ∎

Now we can express the Stokes matrix V+(η)V_{+}(\eta) in terms of the reflection vectors. Let us first extend the definition of the critical directions ην\eta_{\nu} (0ν2μ10\leq\nu\leq 2\mu-1) by allowing arbitrary ν\nu\in\mathbb{Z} so that ην+2μ=ην\eta_{\nu+2\mu}=\eta_{\nu}. More precisely, ην+2μ\eta_{\nu+2\mu} is obtained from ην\eta_{\nu} by clockwise rotation on angle 2π.2\pi. Such an extension is clearly unique. Note that we have the following symmetry:

(33) ην=ηνμ=ην+μ,ν.-\eta_{\nu}=\eta_{\nu-\mu}=\eta_{\nu+\mu},\quad\forall\nu\in\mathbb{Z}.

Recall that X(η,t,z)X(\eta,t,z) is the matrix with columns Xi(η,t,z)X_{i}(\eta,t,z). We proved that X(η~,t,z)=X(η,t,z)WνtX(-\widetilde{\eta},t,z)=X(-\eta,t,z)\,W_{\nu}^{t} where η~\widetilde{\eta} is an admissible direction obtained from η\eta by crossing the critical direction ην\eta_{\nu} and zHηHη~z\in H_{-\eta}\cap H_{-\widetilde{\eta}}. Note that η-\eta is obtained from η~-\widetilde{\eta} by a clockwise rotation. If η~\widetilde{\eta} is rotated across ην1\eta_{\nu-1} to η~~\widetilde{{\widetilde{\eta}}}, then we get

X(η~~,t,z)=X(η~,t,z)Wν1t=X(η,t,z)WνtWν1t,zHηHη~~,\displaystyle X(-\widetilde{{\widetilde{\eta}}},t,z)=X(-\widetilde{\eta},t,z)W_{\nu-1}^{t}=X(-\eta,t,z)\,W_{\nu}^{t}\,W_{\nu-1}^{t},\quad z\in H_{-\eta}\cap H_{-\widetilde{{\widetilde{\eta}}}},

where again η-\eta is obtained from η~~-\widetilde{{\widetilde{\eta}}} via a clockwise rotation. Continuing in this way, i.e., rotating η\eta clockwise until it crosses all the critical directions ην,ην1,,ην(μ1)=ην+1\eta_{\nu},\eta_{\nu-1},\dots,\eta_{\nu-(\mu-1)}=-\eta_{\nu+1}, we get

X(η,t,z)=X(η,t,z)WνtWν1tWν(μ1)t,\displaystyle X(\eta,t,z)=X(-\eta,t,z)W_{\nu}^{t}\,W_{\nu-1}^{t}\,\cdots\,W_{\nu-(\mu-1)}^{t},

where we may take zHηνHην+1z\in H_{-\eta_{\nu}}\cap H_{\eta_{\nu+1}} because we can start with η\eta sufficiently close to ην\eta_{\nu} and at the end cross ην(μ1)=ην+1\eta_{\nu-(\mu-1)}=-\eta_{\nu+1} and stay sufficiently close to ην+1-\eta_{\nu+1}. Recalling the definition of the Stokes matrix V(η)V_{-}(\eta) we get

(34) V(η)=(WνtWν1tWν(μ1)t)1,V_{-}(\eta)=(W_{\nu}^{t}\,W_{\nu-1}^{t}\,\cdots\,W_{\nu-(\mu-1)}^{t})^{-1},

where η\eta is an admissible direction whose adjacent critical directions are ην\eta_{\nu} and ην+1\eta_{\nu+1}. Recalling the relation V+=VtV_{+}=V_{-}^{t} (see Proposition 2.4.1) we get

V+(η)=(Wν(μ1)Wν(μ2)Wν)1.\displaystyle V_{+}(\eta)=(W_{\nu-(\mu-1)}\,W_{\nu-(\mu-2)}\,\cdots\,W_{\nu})^{-1}.

Slightly modifying the above argument we will obtain a simpler formula for the Stokes matrices (see [2], Proposition 5). To begin with, we need an analogue of Proposition 2.5.2. If necessary let us change the enumeration of the points u1,,uNu_{1},\dots,u_{N} so that the following property holds: if we draw a line at uiu_{i} parallel to η\eta and we stand at uiu_{i} looking towards infinity in the direction η\eta, then all points uju_{j} with i<ji<j (resp. j<ij<i) will be in the RHS (resp. LHS) half-plane. Note that i<ji<j is equivalent to Re(uiuj)/z<0\operatorname{Re}(u_{i}-u_{j})/z<0 for all zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}. Therefore, recalling Proposition 2.4.2 we get that V+,ij=0V_{+,ij}=0 for i>ji>j, that is, V+V_{+} is an upper-triangular matrix with ones on the diagonal.

Let β~i(m)\widetilde{\beta}_{i}(m) be the reflection vector corresponding to the reference path obtained by composing Ci(η)C_{i}(-\eta) and the counter-clockwise oriented arc from λ(η)\lambda^{\circ}(\eta) to λ(η)\lambda^{\circ}(-\eta) (see Figure 1). Note that thanks to our choice of the indexes of u1,,uNu_{1},\dots,u_{N} we have

(35) β~1=β1,β~t=σ11σ21σt11(βt)2tN.\widetilde{\beta}_{1}=\beta_{1},\quad\widetilde{\beta}_{t}=\sigma^{-1}_{1}\sigma^{-1}_{2}\cdots\sigma^{-1}_{t-1}(\beta_{t})\quad 2\leq t\leq N.

Note that the formulas about β~j\widetilde{\beta}_{j}^{*} (1jN1\leq j\leq N) in Proposition 2.5.2 were derived in a purely algebraic way from the relations between β~j\widetilde{\beta}_{j} (1jN1\leq j\leq N) and βj\beta_{j} (1jN1\leq j\leq N). Therefore, in the current settings we must have

(36) β~N=βN,β~k=βk+a=k+1Nq1hm(βk(m),βa(m))βa.\widetilde{\beta}_{N}^{*}=\beta_{N}^{*},\quad\widetilde{\beta}_{k}^{*}=\beta_{k}^{*}+\sum_{a=k+1}^{N}q^{-1}h_{m}(\beta_{k}(m),\beta_{a}(-m))\beta_{a}^{*}.

Let us define the matrix W+W_{+} of size N×NN\times N whose (i,j)(i,j) entry is

(37) W+,ij={q1hm(βi(m),βj(m)) if i<j,1 if i=j,0 otherwise .W_{+,ij}=\begin{cases}q^{-1}h_{m}(\beta_{i}(m),\beta_{j}(-m))&\mbox{ if }i<j,\\ 1&\mbox{ if }i=j,\\ 0&\mbox{ otherwise }.\end{cases}

Arguing in the same way as in the proof of Proposition 2.5.3 we get X(η,t,z)=X(η,t,z)W+tX(\eta,t,z)=X(-\eta,t,z)W_{+}^{t} for all zHηνHην+1z\in H_{-\eta_{\nu}}\cap H_{\eta_{\nu+1}}. Recalling the definition of the Stokes matrix V(η)V_{-}(\eta) we get that V(η)=(W+t)1V_{-}(\eta)=(W_{+}^{t})^{-1} and hence V+(η)=W+1V_{+}(\eta)=W_{+}^{-1}, that is, formulas (37) give the entries of the inverse Stokes matrix V+(η)1V_{+}(\eta)^{-1}.

Finally, we will finish this section by proving that the Stokes matrices V+V_{+} and VV_{-} are independent of mm. More precisely, we will express the pairings hm(βk(m),βj(m))h_{m}(\beta_{k}(m),\beta_{j}(-m)) in terms of the intersection pairing (|)(\ |\ ). We follow the idea from the proof of Lemma 2’ in [2].

Lemma 2.5.1.

Let mm\in\mathbb{C} be a complex number with Re(m)<0\operatorname{Re}(m)<0. Let us fix a negative integer ll, such that, the real part of α=m1+l\alpha=-m-1+l is positive. Then

Iβi(m)(m)(t,λ)=uiλ(λs)αΓ(α+1)Iβi(l)(t,s)𝑑s.\displaystyle I^{(m)}_{\beta_{i}(m)}(t,\lambda)=\int_{u_{i}}^{\lambda}\frac{(\lambda-s)^{\alpha}}{\Gamma(\alpha+1)}\,I^{(l)}_{\beta_{i}}(t,s)ds.
Proof.

It is sufficient to prove the formula locally near λ=ui\lambda=u_{i}. We have a Laurent series expansion

Iβi(l)(t,s)=2πk=0ΨRkei(sui)kl1/2Γ(kl+1/2).\displaystyle I^{(l)}_{\beta_{i}}(t,s)=\sqrt{2\pi}\sum_{k=0}^{\infty}\Psi R_{k}e_{i}\,\frac{(s-u_{i})^{k-l-1/2}}{\Gamma(k-l+1/2)}.

Using the substitution x=λsλuix=\frac{\lambda-s}{\lambda-u_{i}} and the standard formulas for the Euler β\beta-integral we get

uiλ(λs)αΓ(α+1)(sui)kl1/2Γ(kl+1/2)𝑑s=01xα(1x)kl1/2𝑑x(λui)α+kl+1/2Γ(α+1)Γ(kl+1/2)=(λui)α+kl+1/2Γ(α+kl+3/2).\displaystyle\int_{u_{i}}^{\lambda}\frac{(\lambda-s)^{\alpha}}{\Gamma(\alpha+1)}\frac{(s-u_{i})^{k-l-1/2}}{\Gamma(k-l+1/2)}\,ds=\int_{0}^{1}x^{\alpha}(1-x)^{k-l-1/2}dx\,\frac{(\lambda-u_{i})^{\alpha+k-l+1/2}}{\Gamma(\alpha+1)\Gamma(k-l+1/2)}=\frac{(\lambda-u_{i})^{\alpha+k-l+1/2}}{\Gamma(\alpha+k-l+3/2)}.

It remains only to note that αl+1=m\alpha-l+1=-m, that is, substituting the Laurent series expansion of Iβi(l)(t,s)I^{(l)}_{\beta_{i}}(t,s) and termwise integrating in ss yields precisely the Laurent series of Iβi(m)(m)(t,λ)I^{(m)}_{\beta_{i}(m)}(t,\lambda). ∎

Proposition 2.5.4.

The pairing hmh_{m} takes the following form in the basis of reflection vectors βi(m)\beta_{i}(m) (1iN1\leq i\leq N) corresponding to the reference paths Ci(η)C_{i}(\eta) (1iN1\leq i\leq N) :

hm(βk(m),βj(m))={q(βk|βj) if k<j,q+q1 if k=j,q1(βk|βj) if k>j.\displaystyle h_{m}(\beta_{k}(m),\beta_{j}(-m))=\begin{cases}q(\beta_{k}|\beta_{j})&\mbox{ if }k<j,\\ q+q^{-1}&\mbox{ if }k=j,\\ q^{-1}(\beta_{k}|\beta_{j})&\mbox{ if }k>j.\end{cases}
Proof.

Let λ0Γj(η)\lambda_{0}\in\Gamma_{j}(-\eta) be a point sufficiently close to uju_{j}. Let us choose mm, such that, its real part is sufficiently negative. Let us consider the following difference

(38) Iβk+(m)(t,λ0)Iβk(m)(t,λ0),I^{(m)}_{\beta_{k}^{+}}(t,\lambda_{0})-I^{(m)}_{\beta_{k}^{-}}(t,\lambda_{0}),

where βk+\beta_{k}^{+} (resp. βk\beta_{k}^{-}) means that the value of the period is obtained from Iβk(m)(t,λ)I^{(m)}_{\beta_{k}}(t,\lambda) via analytic continuation along a path which approaches uju_{j} along Cj(η)C_{j}(\eta), makes a small counter-clockwise (resp. clockwise) arc around uju_{j}, and continues towards λ0\lambda_{0} along Γj(η)\Gamma_{j}(-\eta). We would like to compute (38) in two different ways. First, by definition βk+=σj(βk)=βkq1hm(βk(m),βj(m))βj\beta_{k}^{+}=\sigma_{j}(\beta_{k}^{-})=\beta_{k}^{-}-q^{-1}h_{m}(\beta_{k}(m),\beta_{j}(-m))\beta_{j}^{-} where we put a sign βj\beta_{j}^{-} to emphasize that the reference path should contain the clockwise arc around uju_{j}. We get that the difference (38) coincides with

(39) q1hm(βk(m),βj(m))Iβj(m)(t,λ0).-q^{-1}h_{m}(\beta_{k}(m),\beta_{j}(-m))\,I^{(m)}_{\beta_{j}^{-}}(t,\lambda_{0}).

On the other hand, the analytic continuation can be computed using the integral formula from Lemma 2.5.1. Namely,

(40) Iβk±(m)(t,λ0)=ukλ0(λ0s)αΓ(α+1)Ik(l)(t,s)𝑑s,I^{(m)}_{\beta_{k}^{\pm}}(t,\lambda_{0})=\int_{u_{k}}^{\lambda_{0}}\frac{(\lambda_{0}-s)^{\alpha}}{\Gamma(\alpha+1)}\,I^{(-l)}_{k}(t,s)ds,

where the integration path is from uku_{k} to λk(η)\lambda^{k}(\eta) (see Figure 1), the arc from λk(η)\lambda^{k}(\eta) to λj(η)\lambda^{j}(\eta) (clockwise for k<jk<j and anti-clockwise for k>jk>j), the line segment approaching uju_{j} along Γj(η)\Gamma_{j}(\eta), a small clockwise (for βk\beta_{k}^{-}) or anti-clockwise (for βk+\beta_{k}^{+}) arc around uju_{j}, and finally a straight line segment to λ0\lambda_{0}. Note that the integral splits into two

ukuj(λ0s)αΓ(α+1)Ik(l)(t,s)𝑑s+ujλ0(λ0s)αΓ(α+1)Iβk±(l)(t,s)𝑑s,\displaystyle\int_{u_{k}}^{u_{j}}\frac{(\lambda_{0}-s)^{\alpha}}{\Gamma(\alpha+1)}\,I^{(-l)}_{k}(t,s)ds+\int_{u_{j}}^{\lambda_{0}}\frac{(\lambda_{0}-s)^{\alpha}}{\Gamma(\alpha+1)}\,I^{(-l)}_{\beta_{k}^{\pm}}(t,s)ds,

where the first integral does not depend on the choice of an arc around uju_{j}. Since ll is an integer, we have βk+(l)βk(l)=(βk|βj)βj(l).\beta_{k}^{+}(-l)-\beta_{k}^{-}(-l)=-(\beta_{k}|\beta_{j})\beta_{j}^{-}(-l). Therefore, the difference (38) takes the following form:

(41) (βk|βj)ujλ0(λ0s)αΓ(α+1)Iβj(l)(t,s)𝑑s.-(\beta_{k}|\beta_{j})\,\int_{u_{j}}^{\lambda_{0}}\frac{(\lambda_{0}-s)^{\alpha}}{\Gamma(\alpha+1)}\,I^{(-l)}_{\beta_{j}^{-}}(t,s)ds.

Note that Arg(λ0s)\operatorname{Arg}(\lambda_{0}-s) in the above formula is obtained by continuously varying a small line segment [s,λ0][s,\lambda_{0}] along the integration path in (40). The starting value of the argument is Arg(η)\operatorname{Arg}(\eta). If k>jk>j, then the segment [s,λ0][s,\lambda_{0}] will be rotated anti-clockwise on angle π\pi, so the final value of Arg(λ0s)\operatorname{Arg}(\lambda_{0}-s) will be Arg(η)+π\operatorname{Arg}(\eta)+\pi. If k<jk<j, then the segment will be rotated clockwise and the value of Arg(λ0s)\operatorname{Arg}(\lambda_{0}-s) will eventually become Arg(η)π\operatorname{Arg}(\eta)-\pi. Recalling Lemma 2.5.1 we have

Iβj(m)(t,λ0)=ujλ0(λ0s)αΓ(α+1)Iβj(l)(t,s)𝑑s,\displaystyle I^{(m)}_{\beta_{j}^{-}}(t,\lambda_{0})=\int_{u_{j}}^{\lambda_{0}}\frac{(\lambda_{0}-s)^{\alpha}}{\Gamma(\alpha+1)}\,I^{(-l)}_{\beta_{j}^{-}}(t,s)ds,

where Arg(λ0s)\operatorname{Arg}(\lambda_{0}-s) should be Arg(η)π\operatorname{Arg}(\eta)-\pi. The conclusion is that the expression (41), that is the difference (38), coincides with e2π𝐢α(βk|βj)Iβj(m)(t,λ0)-e^{2\pi\mathbf{i}\alpha}(\beta_{k}|\beta_{j})\,I^{(m)}_{\beta_{j}^{-}}(t,\lambda_{0}) for k>jk>j and with (βk|βj)Iβj(m)(t,λ0)-(\beta_{k}|\beta_{j})\,I^{(m)}_{\beta_{j}^{-}}(t,\lambda_{0}) for k<jk<j. Note that e2π𝐢α=e2π𝐢m=q2e^{2\pi\mathbf{i}\alpha}=e^{-2\pi\mathbf{i}m}=q^{-2}. Comparing with our previous formula (39) we get the statement of the proposition for the case when kjk\neq j. The case k=jk=j was already considered (see Lemma 2.3.1). ∎

2.6. The central connection matrix

Let us start by introducing Figure 5 which might be helpful in visualizing the constructions and following the arguments in this section. Let us identify =2\mathbb{C}=\mathbb{R}^{2} in the standard way. There are two kinds of objects on Figure 5: points and vectors. We think of the points as elements of the λ\lambda-plane and of vectors as elements of the zz-plane. For example, when we talk about the sector HηνHην+1H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}} then one can think about the vectors in the shaded region on Figure 5.

Suppose that η\eta is an admissible direction and let X(η,t,z)X(\eta,t,z) be the matrix whose columns Xi(η,t,z)X_{i}(\eta,t,z) are defined by the oscillatory integrals (22). Similarly, let us introduce also X(η,t,z)X(-\eta,t,z) where the admissible direction η-\eta is obtained from η\eta by a clock-wise rotation. Then we have X(η,t,z)ΨReU/zX(\eta,t,z)\sim\Psi Re^{U/z} as z0z\to 0 and zHηz\in H_{\eta} and X(η,t,z)ΨReU/zX(-\eta,t,z)\sim\Psi Re^{U/z} as z0z\to 0 and zHηz\in H_{-\eta}.

η\etaη-\etaz-zzz𝐢η-\mathbf{i}\eta𝐢ην-\mathbf{i}\eta_{\nu}𝐢ην+1-\mathbf{i}\eta_{\nu+1}γi(η)\gamma_{i}(-\eta)LiL_{i}uiu_{i}HηH_{-\eta}HηH_{\eta}
Figure 5. Points in the λ\lambda-plane and vectors in the zz-plane

Recall that the definition of Xi(±η,t,z)X_{i}(\pm\eta,t,z) requires a choice of log(z)\log(-z), that is we need to define an analytic branch of log\log on both HηH_{\eta} and HηH_{-\eta}. Since ηHη\eta\in H_{-\eta} and by definition η\eta is continuously connected to the default admissible direction 𝐢\mathbf{i}, we have a natural choice of a branch of log\log on HηH_{-\eta}. Using the clock-wise arc from η\eta to η-\eta we can extend analytically log:Hη\log:H_{-\eta}\to\mathbb{C} across the ray 𝐢η>0-\mathbf{i}\eta\mathbb{R}_{>0} (see Figure 5) to the entire half-plane HηH_{\eta}. Recall that both X(η,t,z)X(\eta,t,z) and X(η,t,z)X(-\eta,t,z) extend analytically in zHηνHην+1z\in H_{\eta_{\nu}}\cup H_{-\eta_{\nu+1}} by deforming the integration contour of XiX_{i} (see Section 2.4). We get that X(η,t,z)X(\eta,t,z), X(η,t,z)X(-\eta,t,z), and S(t,z)zθzρS(t,z)z^{\theta}z^{-\rho} are 3 fundamental solutions to the Dubrovin connection analytic inside the sector HηνHην+1H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}. Therefore, there exist matrices V+(η)V_{+}(\eta) and C(η)C(\eta), such that,

X(η,t,z)\displaystyle X(-\eta,t,z) =\displaystyle= S(t,z)zθzρC(η)1,\displaystyle S(t,z)z^{\theta}z^{-\rho}C(\eta)^{-1},
X(η,t,z)\displaystyle X(\eta,t,z) =\displaystyle= S(t,z)zθzρV+(η)C(η)1,\displaystyle S(t,z)z^{\theta}z^{-\rho}V_{+}(\eta)C(\eta)^{-1},

for all zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}. The matrix V+(η)V_{+}(\eta) is the Stokes matrix introduced earlier. Following Dubrovin (see [10]) we will refer to C(η)C(\eta) as the central connection matrix. The main goal in this section is to find a formula for C(η)C(\eta) in terms of the reflection vectors.

It is more convenient to work with the matrix X(η,t,z)X^{*}(-\eta,t,z) whose columns Xi(η,t,z)X^{*}_{i}(-\eta,t,z) are defined in Proposition 2.5.1, c). According to Proposition 2.5.1

X(η,t,z)=X(η,t,z)=S(t,z)zθzρC(η)1,\displaystyle X^{*}(-\eta,t,z)=X(-\eta,t,z)=S(t,z)z^{\theta}z^{-\rho}C(\eta)^{-1},

where zHηνHην+1z\in H_{\eta_{\nu}}\cap H_{-\eta_{\nu+1}}. The key formula will be proved in the following proposition (see [10], Theorem 4.19).

Proposition 2.6.1.

Let Ci(η)C^{i}(\eta) be the iith column of the matrix C(η)1C(\eta)^{-1}. Then

βi(m)=2π(q1eπ𝐢θeπ𝐢ρ+qeπ𝐢θeπ𝐢ρ)1Ci(η).\displaystyle\beta_{i}^{*}(m)=\sqrt{2\pi}\,(q^{-1}e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}+qe^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho})^{-1}C^{i}(\eta).
Proof.

By definition (see Proposition 2.5.1)

γi(η)eλ/zIβi(m)(t,λ)𝑑λ=2πq1(z)m+1/2Xi(η,t,z),\displaystyle\int_{\gamma_{i}(-\eta)}e^{\lambda/z}I^{(m)}_{\beta_{i}^{*}}(t,\lambda)d\lambda=-\sqrt{2\pi}q^{-1}(-z)^{-m+1/2}X_{i}^{*}(-\eta,t,z),

where zHηz\in H_{-\eta}. Let us analytically extend the above identity with respect to zz to the boundary of HηH_{-\eta}. On the RHS we use that Xi(η,t,z)=Xi(η,t,z)X_{i}^{*}(-\eta,t,z)=X_{i}(-\eta,t,z). Suppose that z𝐢η>0z\in-\mathbf{i}\eta\mathbb{R}_{>0} is on the right (compared to the η\eta-direction) part of the boundary of HηH_{-\eta}. The analytic continuation of the LHS is given by deforming the contour γi(η)\gamma_{i}(-\eta) to the line Li:=ui𝐢ηϵ+ηL_{i}:=u_{i}-\mathbf{i}\eta\epsilon+\eta\mathbb{R} where ϵ>0\epsilon>0 is a real number (see the blue contours on Figure 5). We get

(42) Lieλ/zIβi(m)(t,λ)𝑑λ=2πq1(z)m+1/2Xi(η,t,z),\int_{L_{i}}e^{\lambda/z}I^{(m)}_{\beta_{i}^{*}}(t,\lambda)d\lambda=-\sqrt{2\pi}q^{-1}(-z)^{-m+1/2}X_{i}(-\eta,t,z),

where z𝐢η>0.z\in-\mathbf{i}\eta\mathbb{R}_{>0}. Let us recall that Xi(η,t,z)=S(t,z)zθzρCi(η)X_{i}(-\eta,t,z)=S(t,z)z^{\theta}z^{-\rho}C^{i}(\eta), where logz\log z is determined from the branch of log\log in HηH_{-\eta} and the value logη\log\eta. Since we have restricted z𝐢η>0z\in-\mathbf{i}\eta\mathbb{R}_{>0} we get Arg(z)=Arg(η)π2\operatorname{Arg}(z)=\operatorname{Arg}(\eta)-\tfrac{\pi}{2}. On the other hand, in formula (42) the analytic branch of log(z)\log(-z) comes from the branch of log\log in HηH_{\eta} induced from log(η)=logηπ𝐢\log(-\eta)=\log\eta-\pi\mathbf{i}. In other words, Arg(z)=Arg(z)π\operatorname{Arg}(-z)=\operatorname{Arg}(z)-\pi. Therefore,

(z)m+1/2=eπ𝐢(m+1/2)zm+1/2=𝐢1qzm+1/2.\displaystyle(-z)^{-m+1/2}=e^{-\pi\mathbf{i}(-m+1/2)}\,z^{-m+1/2}=\mathbf{i}^{-1}qz^{-m+1/2}.

Let us rewrite (42) as follows

12π𝐢Lieλ/zIβi(m)(t,λ)𝑑λ=12πS(t,z)zθm+1/2zρCi(η).\displaystyle\frac{1}{2\pi\mathbf{i}}\int_{L_{i}}e^{\lambda/z}I^{(m)}_{\beta_{i}^{*}}(t,\lambda)d\lambda=\frac{1}{\sqrt{2\pi}}\,S(t,z)z^{\theta-m+1/2}z^{-\rho}C^{i}(\eta).

Let us substitute w=1/z𝐢η>0w=1/z\in\tfrac{\mathbf{i}}{\eta}\,\mathbb{R}_{>0}, Arg(w)=π2Arg(η)\operatorname{Arg}(w)=\tfrac{\pi}{2}-\operatorname{Arg}(\eta). Recalling the Laplace inversion formula we get that Iβi(m)(t,λ)I^{(m)}_{\beta_{i}^{*}}(t,\lambda) is the Laplace transform of the RHS, that is,

(43) Iβi(m)(t,λ)=12π0exλS(t,x1)xmθ1/2xρ𝑑xCi(η),I^{(m)}_{\beta_{i}^{*}}(t,\lambda)=\frac{1}{\sqrt{2\pi}}\,\int_{0}^{\infty}e^{-x\lambda}S(t,x^{-1})x^{m-\theta-1/2}x^{\rho}dx\,C^{i}(\eta),

where the integration is along the ww-ray, that is, Arg(x)=π2Arg(η)\operatorname{Arg}(x)=\tfrac{\pi}{2}-\operatorname{Arg}(\eta). Let us comment on the convergence of the above integral. Firstly, since the calibration S(t,x1)S(t,x^{-1}) is analytic at x=0x=0, we need to choose mm, such that, Re(m)0\operatorname{Re}(m)\gg 0. When xx is close to \infty, since the integrand is proportional to Xi(η,t,z)X_{i}(-\eta,t,z), the integrand has at most exponential growth of order euixe^{u_{i}x}. Therefore, the integral defines an analytic function for all λ\lambda in the half-plane Re((uiλ)x)<0\operatorname{Re}((u_{i}-\lambda)x)<0. The integral (43) is straightforward to compute because the calibration S(t,x1)S(t,x^{-1}) is an entire function. In other words, we may use the Taylor series expansion at x=0x=0. Let us also make the substitution x=y/λx=y/\lambda and restrict λ\lambda to be such that y>0y\in\mathbb{R}_{>0}. The RHS of (43) takes the following form

12πk=0Sk(t)(0ey(y/λ)k+mθ1/2(y/λ)ρdyλ)Ci(η).\displaystyle\frac{1}{\sqrt{2\pi}}\,\sum_{k=0}^{\infty}S_{k}(t)\left(\int_{0}^{\infty}e^{-y}(y/\lambda)^{k+m-\theta-1/2}(y/\lambda)^{\rho}\frac{dy}{\lambda}\,\right)C^{i}(\eta).

Note that (y/λ)ρ=eρlog(y/λ)(y/\lambda)^{\rho}=e^{\rho\log(y/\lambda)} and that log(y/λ)\log(y/\lambda) can be produced by acting with the differential operator m:=m\partial_{m}:=\tfrac{\partial}{\partial m}. The formula transforms into

12πk=0Sk(t)(0ey(y/λ)k+mθ1/2dyλ)eρmCi(η),\displaystyle\frac{1}{\sqrt{2\pi}}\,\sum_{k=0}^{\infty}S_{k}(t)\left(\int_{0}^{\infty}e^{-y}(y/\lambda)^{k+m-\theta-1/2}\frac{dy}{\lambda}\,\right)\cdot e^{\rho\overleftarrow{\partial}_{m}}C^{i}(\eta),

where the arrow over m\partial_{m} is to denote right action of the matrix differential operator ρm\rho\partial_{m}. We have to distinguish left and right action here because θ\theta and ρ\rho do not commute. The above integral is just the definition of the Γ\Gamma-function. We get

12πk=0Sk(t)(λθmk1/2Γ(m+kθ+1/2))eρmCi(η).\displaystyle\frac{1}{\sqrt{2\pi}}\,\sum_{k=0}^{\infty}S_{k}(t)\left(\lambda^{\theta-m-k-1/2}\Gamma(m+k-\theta+1/2)\right)\cdot e^{\rho\overleftarrow{\partial}_{m}}C^{i}(\eta).

Using the product formula

Γ(x)Γ(1x)=πsinπx=2π𝐢eπ𝐢xeπ𝐢x\displaystyle\Gamma(x)\Gamma(1-x)=\frac{\pi}{\sin\pi x}=\frac{2\pi\mathbf{i}}{e^{\pi\mathbf{i}x}-e^{-\pi\mathbf{i}x}}

with x=θmk+1/2x=\theta-m-k+1/2 we get

(44) 12πk=0Sk(t)(1)k(λθmk1/2Γ(θmk+1/2)2πeπ𝐢(θm)+eπ𝐢(θm))eρmCi(η).\frac{1}{\sqrt{2\pi}}\,\sum_{k=0}^{\infty}S_{k}(t)(-1)^{k}\left(\frac{\lambda^{\theta-m-k-1/2}}{\Gamma(\theta-m-k+1/2)}\,\frac{2\pi}{e^{\pi\mathbf{i}(\theta-m)}+e^{-\pi\mathbf{i}(\theta-m)}}\right)\cdot e^{\rho\overleftarrow{\partial}_{m}}\,C^{i}(\eta).

Note that

2πeπ𝐢(θm)+eπ𝐢(θm)eρm=eρm2πeπ𝐢θeπ𝐢(mρ)+eπ𝐢θeπ𝐢(mρ),\displaystyle\frac{2\pi}{e^{\pi\mathbf{i}(\theta-m)}+e^{-\pi\mathbf{i}(\theta-m)}}\,e^{\rho\overleftarrow{\partial}_{m}}=e^{-\rho\overleftarrow{\partial}_{m}}\frac{2\pi}{e^{\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}(m-\rho)}+e^{-\pi\mathbf{i}\theta}e^{\pi\mathbf{i}(m-\rho)}},

where we used that eπ𝐢θρ=ρeπ𝐢θe^{\pi\mathbf{i}\theta}\rho=-\rho e^{\pi\mathbf{i}\theta} thanks to the commutation relation [θ,ρ]=ρ[\theta,\rho]=-\rho. The left action can be transformed into right action thanks to the following formula:

(λθmk1/2Γ(θmk+1/2))eρm=eρλm(λθmk1/2Γ(θmk+1/2)).\displaystyle\left(\frac{\lambda^{\theta-m-k-1/2}}{\Gamma(\theta-m-k+1/2)}\right)\cdot e^{-\rho\overleftarrow{\partial}_{m}}=e^{-\rho\partial_{\lambda}\partial_{m}}\left(\frac{\lambda^{\theta-m-k-1/2}}{\Gamma(\theta-m-k+1/2)}\right).

The above formula is proved by expanding eρm=l=0(ρ)lml/l!e^{-\rho\partial_{m}}=\sum_{l=0}^{\infty}(-\rho)^{l}\partial_{m}^{l}/l!, using the commutation relation θρl=ρl(θl)\theta\rho^{l}=\rho^{l}(\theta-l), and finally noting that the shift kk+1k\mapsto k+1 is equivalent to differentiation by λ\lambda. After all these remarks, we can easily transform (44) into

2πk=0Sk(t)(1)keρλm(λθmk1/2Γ(θmk+1/2))(q1eπ𝐢θeπ𝐢ρ+qeπ𝐢θeπ𝐢ρ)1Ci(η).\displaystyle\sqrt{2\pi}\,\sum_{k=0}^{\infty}S_{k}(t)(-1)^{k}e^{-\rho\partial_{\lambda}\partial_{m}}\left(\frac{\lambda^{\theta-m-k-1/2}}{\Gamma(\theta-m-k+1/2)}\,\right)\cdot\,(q^{-1}e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}+qe^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho})^{-1}C^{i}(\eta).

The infinite sum over kk is precisely our definition of the fundamental solution I(m)(t,λ)I^{(m)}(t,\lambda) of the second structure connection (m)\nabla^{(m)}. The formula for βi(m)\beta_{i}^{*}(m) follows. ∎

Now we are in position to derive the precise formulas relating the monodromy data of the 1st and the 2nd structure connections. Let us first state the following simple but very useful formula:

(45) gAT=Atg,AEnd(H)MatN×N(),g\,A^{T}=A^{t}\,g,\quad A\in\operatorname{End}(H)\cong\operatorname{Mat}_{N\times N}(\mathbb{C}),

where gg is the matrix of the Frobenius pairing, that is, gij=(/ti,/tj)g_{ij}=(\partial/\partial t_{i},\partial/\partial t_{j}), T is transposition with respect to the Frobenius pairing, and t is the usual transposition of matrices. In the above identity, we use a fixed basis of flat vector fields ϕi:=/ti\phi_{i}:=\partial/\partial t_{i} (1iN)(1\leq i\leq N) to identify the space End(H)\operatorname{End}(H) of linear operators in HH with the space MatN×N()\operatorname{Mat}_{N\times N}(\mathbb{C}) of matrices of size N×NN\times N. Let us also introduce the following convenient notation:

AT=(A1)T,At=(A1)t,AMatN×N().\displaystyle A^{-T}=(A^{-1})^{T},\quad A^{-t}=(A^{-1})^{t},\quad A\in\operatorname{Mat}_{N\times N}(\mathbb{C}).

Let us recall the well known relations between the Stokes matrices and the central connection matrix (see [10]).

Proposition 2.6.2.

The following formulas hold:

V+\displaystyle V_{+} =\displaystyle= Ctgeπ𝐢ρeπ𝐢θC1,\displaystyle C^{-t}ge^{-\pi\mathbf{i}\rho}e^{-\pi\mathbf{i}\theta}C^{-1},
V\displaystyle V_{-} =\displaystyle= Ctgeπ𝐢ρeπ𝐢θC1.\displaystyle C^{-t}ge^{\pi\mathbf{i}\rho}e^{\pi\mathbf{i}\theta}C^{-1}.
Proof.

The 2nd formula follows from the first one and the relation V=V+TV_{-}=V_{+}^{T}. Let us prove the first formula. Suppose that zVηνVην+1z\in V_{\eta_{\nu}}\cap V_{-\eta_{\nu+1}}. We have

(46) X(η,t,z)tgX(η,t,z)=(X(η,t,z)V)tgX(η,t,z)=Vt=V+,X(-\eta,t,-z)^{t}gX(-\eta,t,z)=(X(\eta,t,-z)V_{-})^{t}gX(-\eta,t,z)=V_{-}^{t}=V_{+},

where we used the quadratic relation X(η,t,z)tgX(η,t,z)=1X(-\eta,t,-z)^{t}gX(-\eta,t,z)=1 and the relation Vt=V+V_{-}^{t}=V_{+} – see Proposition 2.4.1 and its proof. On the other hand, by definition, we have X(η,t,z)=S(t,z)zθzρC1X(-\eta,t,z)=S(t,z)z^{\theta}z^{-\rho}C^{-1}. Let us analytically extend this identity in zz from zz to z-z along the anti-clockwise arc. We get a second identity of the form X(η,t,z)=S(t,z)zθeπ𝐢θzρeπ𝐢ρC1X(-\eta,t,-z)=S(t,-z)z^{\theta}e^{\pi\mathbf{i}\theta}z^{-\rho}e^{-\pi\mathbf{i}\rho}C^{-1}. Substituting these two formulas in (46) we get

V+=(S(t,z)zθeπ𝐢θzρeπ𝐢ρC1)tgS(t,z)zθzρC1=Ctgeπ𝐢ρeπ𝐢θC1,\displaystyle V_{+}=(S(t,-z)z^{\theta}e^{\pi\mathbf{i}\theta}z^{-\rho}e^{-\pi\mathbf{i}\rho}C^{-1})^{t}gS(t,z)z^{\theta}z^{-\rho}C^{-1}=C^{-t}ge^{-\pi\mathbf{i}\rho}e^{-\pi\mathbf{i}\theta}C^{-1},

where we used repeatedly formula (45), the symplectic condition S(t,z)TS(t,z)=1S(t,-z)^{T}S(t,z)=1, and the relation eπ𝐢θρ=ρeπ𝐢θe^{\pi\mathbf{i}\theta}\rho=-\rho e^{\pi\mathbf{i}\theta}. ∎

Let us introduce the matrix h(m)h(m) of the pairing hmh_{m}, that is, hij(m):=hm(ϕi,ϕj)h_{ij}(m):=h_{m}(\phi_{i},\phi_{j}). Let β(m)=[β1(m),,βN(m)]\beta(m)=[\beta_{1}(m),\dots,\beta_{N}(m)] be the matrix with columns the reflection vectors βi(m)\beta_{i}(m), that is, the entries of β(m)\beta(m) are defined by βi(m)=:k=1Nβki(m)ϕk\beta_{i}(m)=:\sum_{k=1}^{N}\beta_{ki}(m)\phi_{k}. Similarly, let β=[β1(m),,βN(m)]\beta^{*}=[\beta_{1}^{*}(m),\dots,\beta_{N}^{*}(m)] be the matrix whose columns are given by the dual vectors βi(m)\beta_{i}^{*}(m). Using formula (37) for the entries of W+=V+1W_{+}=V_{+}^{-1} and Propositions 2.5.4, we get that hm(βi(m),βj(m))h_{m}(\beta_{i}(m),\beta_{j}(-m)) coincides with the (i,j)(i,j)-entry of qV+1+q1V+tqV_{+}^{-1}+q^{-1}V_{+}^{-t}. Therefore,

(47) qV+1+q1V+t=β(m)th(m)β(m)qV_{+}^{-1}+q^{-1}V_{+}^{-t}=\beta(m)^{t}h(m)\beta(-m)

On the other hand, since by definition β(m)th(m)β(m)=1\beta^{*}(m)^{t}h(m)\beta(-m)=1, we get β(m)t=(qV+1+q1V+t)β(m)t\beta(m)^{t}=(qV_{+}^{-1}+q^{-1}V_{+}^{-t})\beta^{*}(m)^{t}, that is,

β(m)=β(m)(qV+t+q1V+1).\displaystyle\beta(m)=\beta^{*}(m)(qV_{+}^{-t}+q^{-1}V_{+}^{-1}).

Recalling Proposition 2.6.2 we get

qV+t+q1V+1=C(qeπ𝐢θeπ𝐢ρ+q1eπ𝐢θeπ𝐢ρ)g1Ct.\displaystyle qV_{+}^{-t}+q^{-1}V_{+}^{-1}=C(q\,e^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho}+q^{-1}\,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho})g^{-1}C^{t}.

Recalling Proposition 2.6.1 we get

(48) β(m)=2π(qeπ𝐢θeπ𝐢ρ+q1eπ𝐢θeπ𝐢ρ)1C1(qV+t+q1V+1)=2πg1Ct.\beta(m)=\sqrt{2\pi}(q\,e^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho}+q^{-1}\,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho})^{-1}C^{-1}(qV_{+}^{-t}+q^{-1}V_{+}^{-1})=\sqrt{2\pi}g^{-1}C^{t}.
Theorem 2.6.1.

a) The (i,j)(i,j)-entry of the central connection matrix is related to the components of the reflection vectors by the following formula:

Cij=12π(βi(m),ϕj).\displaystyle C_{ij}=\frac{1}{\sqrt{2\pi}}\,(\beta_{i}(m),\phi_{j}).

b) The pairing hmh_{m} can be computed by the following formula:

hm(a,b)=qa,b+q1b,a,a,bH,\displaystyle h_{m}(a,b)=q\langle a,b\rangle+q^{-1}\langle b,a\rangle,\quad\forall a,b\in H,

where ,\langle\ ,\ \rangle is the Euler pairing (21).

c) The reflection vectors βi(m)\beta_{i}(m) (1iN1\leq i\leq N) are independent of mm and the Gram matrix of the Euler pairing is upper-triangular:

βi,βj=0i>j,\displaystyle\langle\beta_{i},\beta_{j}\rangle=0\quad\forall i>j,

with 11’s on the diagonal: βi,βi=1\langle\beta_{i},\beta_{i}\rangle=1.

d) The Gram matrix of the Euler pairing in the basis βi\beta_{i} (1iN1\leq i\leq N) coincides with the inverse Stokes matrix V+1V_{+}^{-1}.

Proof.

a) According to (48) we have C=12πβ(m)tgC=\tfrac{1}{\sqrt{2\pi}}\beta(m)^{t}g. Comparing the (i,j)(i,j) entries in this matrix identity we get the formula stated in part a).

b) According to (47) we have

h(m)=β(m)t(qV+1+q1V+t)β(m)1.\displaystyle h(m)=\beta(m)^{-t}(qV_{+}^{-1}+q^{-1}V_{+}^{-t})\beta(-m)^{-1}.

Recalling Proposition 2.6.2 we get

qV+1+q1V+t=C(qeπ𝐢θeπ𝐢ρ+q1eπ𝐢θeπ𝐢ρ)g1Ct.\displaystyle qV_{+}^{-1}+q^{-1}V_{+}^{-t}=C(q\,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}+q^{-1}\,e^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho})g^{-1}C^{t}.

Finally, since β(m)=2πg1Ct\beta(m)=\sqrt{2\pi}g^{-1}C^{t} we get

h(m)=12πgC1C(qeπ𝐢θeπ𝐢ρ+q1eπ𝐢θeπ𝐢ρ)g1CtCtg=12πg(qeπ𝐢θeπ𝐢ρ+q1eπ𝐢θeπ𝐢ρ).\displaystyle h(m)=\frac{1}{2\pi}gC^{-1}\,C(q\,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}+q^{-1}\,e^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho})g^{-1}C^{t}\,C^{-t}g=\frac{1}{2\pi}g(q\,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}+q^{-1}\,e^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho}).

The above formula implies that

hm(ϕi,ϕj)=12π(ϕi,(qeπ𝐢θeπ𝐢ρ+q1eπ𝐢θeπ𝐢ρ)ϕj)=qϕi,ϕj+q1ϕj,ϕi.\displaystyle h_{m}(\phi_{i},\phi_{j})=\frac{1}{2\pi}(\phi_{i},(q\,e^{\pi\mathbf{i}\theta}e^{\pi\mathbf{i}\rho}+q^{-1}\,e^{-\pi\mathbf{i}\theta}e^{-\pi\mathbf{i}\rho})\phi_{j})=q\langle\phi_{i},\phi_{j}\rangle+q^{-1}\langle\phi_{j},\phi_{i}\rangle.

c) The fact that βi(m)\beta_{i}(m) is independent of mm follows immediately from part a) because the central connection matrix is independent of mm. The rest of the statement is an immediate consequence of Proposition 2.5.4 and part b). Indeed, if i<ji<j, then we have

q(βi|βj)=qβi,βj+q1βj,βi.\displaystyle q(\beta_{i}|\beta_{j})=q\langle\beta_{i},\beta_{j}\rangle+q^{-1}\langle\beta_{j},\beta_{i}\rangle.

On the other hand, recalling part b) with q=1q=1 we get (βi|βj)=βi,βj+βj,βi(\beta_{i}|\beta_{j})=\langle\beta_{i},\beta_{j}\rangle+\langle\beta_{j},\beta_{i}\rangle. The above identity is possible if an only if βj,βi=0\langle\beta_{j},\beta_{i}\rangle=0. Similarly, if i=ji=j, then we have

q+q1=qβi,βi+q1βi,βi=(q+q1)βi,βi\displaystyle q+q^{-1}=q\langle\beta_{i},\beta_{i}\rangle+q^{-1}\langle\beta_{i},\beta_{i}\rangle=(q+q^{-1})\langle\beta_{i},\beta_{i}\rangle

which implies that βi,βi=1\langle\beta_{i},\beta_{i}\rangle=1.

d) This part is an immediate consequence of formula (37) and parts b) and c). ∎

Remark 2.6.1.

Let us compare our notation to Dubrovin’s one in [10]. If η\eta is an admissible direction, then +=𝐢η1>0\ell_{+}=\mathbf{i}\eta^{-1}\mathbb{R}_{>0} is the positive part of an admissible line in the sense of Dubrovin. Then X(η,t,z)=Yleft(t,z1)X(\eta,t,z)=Y_{\rm left}(t,z^{-1}), X(η,t,z)=Yright(t,z1)X(-\eta,t,z)=Y_{\rm right}(t,z^{-1}), and S(t,z)zθzρ=Y0(t,z1)S(t,z)z^{\theta}z^{-\rho}=Y_{0}(t,z^{-1}). Note that the degree operator in Dubrovin is μ=θ\mu=-\theta while the nilpotent operators coincide R=ρR=\rho. It follows that the inverse Stokes matrix V+1V^{-1}_{+} coincides with Dubrovin’s Stokes matrix SS. Finally, the central connection matrix in our notation coincides with the Dubrovin’s one. ∎

3. Dubrovin conjecture

Following [9] (see also [6]) we present the so-called Dubrovin conjecture. Roughly speaking, Dubrovin conjecture relates the big quantum cohomology of a variety XX, as a Frobenius manifold, with its bounded derived category of coherent sheaves. The main goal is to give a reformulation of the conjecture in terms of the language introduced in the previous section.

3.1. Quantum cohomology

We recall some basic aspects about quantum cohomology, for a more detail account, for instance see [7]. Let XX be a smooth projective algebraic variety, with vanishing odd cohomology, and ¯g,n(X,d)\overline{\mathcal{M}}_{g,n}(X,d) be the Deligne-Mumford stack of nn-pointed stable maps of genus gg representing a class dH2(X,)d\in H_{2}(X,\mathbb{Z}). Let us consider the evaluation maps evi:¯g,n(X,d)X\operatorname{ev}_{i}:\overline{\mathcal{M}}_{g,n}(X,d)\rightarrow X, i=1,,ni=1,\dots,n, and the map ev:=ev1××evn:¯g,n(X,d)Xn\operatorname{ev}:=\operatorname{ev}_{1}\times\cdots\times\operatorname{ev}_{n}:\overline{\mathcal{M}}_{g,n}(X,d)\rightarrow X^{n}. Then, the descendant Gromov-Witten invariant is defined by the following formula:

α1ψl1,,αnψlng,n,d=[¯g,n(X,d)]virψ1l1ψnlnev(α1××αn),\displaystyle\langle\alpha_{1}\psi^{l_{1}},\dots,\alpha_{n}\psi^{l_{n}}\rangle_{g,n,d}=\int_{[\overline{\mathcal{M}}_{g,n}(X,d)]^{\mathrm{vir}}}\psi_{1}^{l_{1}}\cdots\psi_{n}^{l_{n}}\,\operatorname{ev}^{*}(\alpha_{1}\times\cdots\times\alpha_{n}),

where [¯g,n(X,d)]vir[\overline{\mathcal{M}}_{g,n}(X,d)]^{\mathrm{vir}} is the virtual fundamental class in the Chow ring CH(¯g,n(X,d))CH_{*}(\overline{\mathcal{M}}_{g,n}(X,d)) constructed in [4] and ψi\psi_{i} is the first Chern class of the tautological line bundle formed by the cotangent line at the ii-th marked point. In particular, genus-0 Gromov-Witten invariants (with no descendants) can be used to define a deformation of the cup product in cohomology.

Definition 3.1.1.

Let ω\omega be a complexified Kähler class on a smooth projective variety XX. Let ϕ1=1,,ϕN\phi_{1}=1,\dots,\phi_{N} be a basis of H(X,)H^{*}(X,\mathbb{C}) and τ=i=1Ntiϕi\tau=\sum_{i=1}^{N}t_{i}\phi_{i}. Then, the Gromov-Witten potential Φ\Phi is defined by the following formula:

Φ(τ)=n=0dH2(X,)1n!τn0,n,dqd\displaystyle\Phi(\tau)=\sum_{n=0}^{\infty}\sum_{d\in H_{2}(X,\mathbb{Z})}\frac{1}{n!}\langle\tau^{n}\rangle_{0,n,d}q^{d}

where τn0,n,d=τ,,τ0,n,d\langle\tau^{n}\rangle_{0,n,d}=\langle\tau,\dots,\tau\rangle_{0,n,d} (with τ\tau taken nn times) and qd=e2π𝐢dωq^{d}=e^{2\pi\mathbf{i}\int_{d}\omega}. ∎

If XX is a Fano variety, then there are only a finite number of dd’s such that τn0,n,d0\langle\tau^{n}\rangle_{0,n,d}\neq 0, so Φ[[t1,,tN]]\Phi\in\mathbb{C}[\![t_{1},\dots,t_{N}]\!], where the tit_{i}’s are the formal variables associated to the basis ϕi\phi_{i} (1iN)(1\leq i\leq N). Therefore Φ\Phi can be considered as a function on a formal neighbourhood of 0H(X,)0\in H^{*}(X,\mathbb{C}). In general, we fix an ample basis p1,,prp_{1},\dots,p_{r} of H2(X,)H1,1(X,)H^{2}(X,\mathbb{Z})\cap H^{1,1}(X,\mathbb{C}) and introduce the so called Novikov variables q1,,qrq_{1},\dots,q_{r}. The expression qd:=q1p1,dqrpr,dq^{d}:=q_{1}^{\langle p_{1},d\rangle}\cdots q_{r}^{\langle p_{r},d\rangle} is interpreted as an element in the ring of formal power series [[q]]:=[[q1,,qr]]\mathbb{C}[\![q]\!]:=\mathbb{C}[\![q_{1},\dots,q_{r}]\!] and the potential Φ\Phi is considered as a formal power series in the ring

[[q,t]]:=[[t1,q1et2,,qretr+1,tr+2,,tN]],\displaystyle\mathbb{C}[\![q,t]\!]:=\mathbb{C}[\![t_{1},q_{1}e^{t_{2}},\dots,q_{r}e^{t_{r+1}},t_{r+2},\dots,t_{N}]\!],

where we identified pi=ϕi+1p_{i}=\phi_{i+1} (1ir1\leq i\leq r) and we used the divisor equation to express Φ\Phi as a function of qieti+1q_{i}e^{t_{i+1}}. It is believed that the Gromov–Witten potential is convergent (see below for a more precise statement). In case of convergence, the complexified Kähler class is related to the Novikov variables via ω=12π𝐢(p1logq1++prlogqr)\omega=\tfrac{1}{2\pi\mathbf{i}}\left(p_{1}\log q_{1}+\cdots+p_{r}\log q_{r}\right).

Definition 3.1.2.

The big quantum cohomology of XX is the ring H(X,[[q,t]])H^{*}(X,\mathbb{C}[\![q,t]\!]), with the product given on generators by ϕiϕj=3Φtitjtkϕk\phi_{i}\bullet\phi_{j}=\sum\frac{\partial^{3}\Phi}{\partial{t_{i}}\partial{t_{j}}\partial{t_{k}}}\phi^{k}, where ϕ1,,ϕN\phi^{1},\dots,\phi^{N} form a Poincaré dual basis to ϕ1,,ϕN\phi_{1},\dots,\phi_{N}. We will denote this ring by QH(X)QH^{*}(X).∎

Remark 3.1.1.

If we set δ=i=1rti+1pi\delta=\sum_{i=1}^{r}t_{i+1}p_{i} and ϵ=t1ϕ1+i=r+1Ntiϕi\epsilon=t_{1}\phi_{1}+\sum_{i=r+1}^{N}t_{i}\phi_{i}, then

ϕiϕj=kn=0d1n!ϕi,ϕj,ϕk,ϵn0,n+3,dedδqdϕk.\displaystyle\phi_{i}\bullet\phi_{j}=\sum_{k}\sum_{n=0}^{\infty}\sum_{d}\frac{1}{n!}\langle\phi_{i},\phi_{j},\phi_{k},\epsilon^{n}\rangle_{0,n+3,d}e^{\int_{d}\delta}q^{d}\phi^{k}.

In addition, if we set ϵ=0\epsilon=0, then we get that

ϕiϕj|ϵ=0=kdϕi,ϕj,ϕk0,n+3,dedδqdϕk.\displaystyle\phi_{i}\bullet\phi_{j}|_{\epsilon=0}=\sum_{k}\sum_{d}\langle\phi_{i},\phi_{j},\phi_{k}\rangle_{0,n+3,d}e^{\int_{d}\delta}q^{d}\phi^{k}.

This restriction is known as the small quantum product and the corresponding ring is called small quantum cohomology ring. In fact, since the big quantum product is defined formally on H(X,[[q,t]])H^{*}(X,\mathbb{C}[\![q,t]\!]) in terms of t1,,tNt_{1},\dots,t_{N} and qdq^{d}, the small quantum cup product is obtained by restricting to H2(X,[[q]])H^{2}(X,\mathbb{C}[\![q]\!]), that is, setting t1=tr+2==tN=0t_{1}=t_{r+2}=\cdots=t_{N}=0 in the formula for ϕiϕj\phi_{i}\bullet\phi_{j}. This is equivalent to setting ϵ=0\epsilon=0.∎

Suppose now that the Novikov variables q1==qr=1q_{1}=\cdots=q_{r}=1 and that there exists a non-empty open subset MH(X,)M\subseteq H^{*}(X,\mathbb{C}) where the Gromow-Witten potential Φ\Phi converges. More precisely, we assume that MM contains τH(X,)\tau\in H^{*}(X,\mathbb{C}), such that, eti+1e^{t_{i+1}} (1ir1\leq i\leq r) and tjt_{j} (r+2jNr+2\leq j\leq N) are complex numbers with sufficiently small length (t1t_{1} could be arbitrary because Φ\Phi is polynomial in t1t_{1}). Let

g:H(X,)×H(X,),g(ξ,ζ)=Xξζ\displaystyle g:H^{*}(X,\mathbb{C})\times H^{*}(X,\mathbb{C})\rightarrow\mathbb{C},\quad g(\xi,\zeta)=\int_{X}\xi\cup\zeta

be the Poincaré pairing which will be taken as a Frobenius pairing. Put

E=c1(X)+i=1N(1deg(ϕi))titi,\displaystyle E=c_{1}(X)+\sum_{i=1}^{N}\Big{(}1-\mathrm{deg}_{\mathbb{C}}(\phi_{i})\Big{)}t_{i}\frac{\partial}{\partial t_{i}},

where deg\operatorname{deg}_{\mathbb{C}} is half of the standard cohomology degree. Then, MM equipped with the big quantum cup product defined above, the Poincaré pairing, and the Euler vector field EE is a Frobenius manifold of conformal dimension D:=dim(X)D:=\operatorname{dim}_{\mathbb{C}}(X). The semi-simplicity of the quantum cup product is an indication that the target smooth algebraic variety XX has many rational curves. Therefore, from the point of view of birational geometry, it is very important to understand when is the Frobenius manifold underlying the big quantum cohomology semisimple? Before trying to approach an answer to this question, we need to recall some background on the bounded derived category of coherent sheaves of XX.

3.2. Derived categories

For more details about derived categories we refer to [14]. Let 𝒯\mathcal{T} be a \mathbb{C}-linear triangulated category. Let us recall the following notation. Given an object E𝒯E\in\mathcal{T} put E[k]:=TkEE[k]:=T^{k}E where TT is the translation functor of the triangulated category. Furthermore, Hom(E,F)\operatorname{Hom}(E,F) denotes the complex vector space of morphisms in 𝒯\mathcal{T} from EE to FF. Let us introduce also the complex Hom(E,F)\operatorname{Hom}^{\bullet}(E,F) of vector spaces with a trivial differential whose component in degree kk is Homk(E,F):=Hom(E,F[k])\operatorname{Hom}^{k}(E,F):=\operatorname{Hom}(E,F[k]).

Definition 3.2.1.

An object EE in 𝒯\mathcal{T} is called exceptional if it satisfies the following conditions:

Homk(E,E)=0 for k0,Hom(E,E)=.\displaystyle\operatorname{Hom}^{k}(E,E)=0\mbox{ for }k\neq 0,\quad\operatorname{Hom}(E,E)=\mathbb{C}.\qed
Definition 3.2.2.

A sequence of objects (E1,,EN)(E_{1},\dots,E_{N}) is called an exceptional collection if every object EiE_{i} is exceptional and Hom(Ei,Ej)=0\mathrm{Hom}^{\bullet}(E_{i},E_{j})=0 for i>ji>j. An exceptional collection is said to be full if it generates 𝒯\mathcal{T} as a triangulated category. ∎

Following Bondal (see [5]) we would like to recall the mutation operations. An exceptional collection (E,F)(E,F) consisting of two objects is said to be an exceptional pair. Let (E,F)(E,F) be an exceptional pair. We define objects LEFL_{E}F and RFER_{F}E, such that, the following sequences are distinguished triangles

where for a complex of vector spaces VV^{\bullet} we denote by VkE[k]V^{k}\otimes E[-k] the direct sum of dim(Vk)\operatorname{dim}(V^{k}) copies of E[k]E[-k] and by VEV^{\bullet}\otimes E the direct sum of all VkE[k]V^{k}\otimes E[-k]. The map Hom(E,F)EF\operatorname{Hom}^{\bullet}(E,F)\otimes E\to F is induced from the tautological maps Hom(E,F[k])E[k]F\operatorname{Hom}(E,F[k])\otimes E[-k]\to F, that is, fix a basis fif_{i} of Hom(E,F[k])=Hom(E[k],F)\operatorname{Hom}(E,F[k])=\operatorname{Hom}(E[-k],F), then ifi\oplus_{i}f_{i} is a morphism iE[k]F\oplus_{i}E[-k]\to F. Similarly, the map EHom(E,F)FE\to\operatorname{Hom}^{\bullet}(E,F)^{*}\otimes F is induced from the tautological maps EHom(E,F[k])F[k]E\to\operatorname{Hom}(E,F[-k])^{*}\otimes F[-k], that is, fix a basis fif^{i} of Hom(E,F[k])\operatorname{Hom}(E,F[-k])^{*} and a dual basis fif_{i} of Hom(E,F[k])\operatorname{Hom}(E,F[-k]), then ifi\oplus_{i}f_{i} is a morphism from EiF[k]E\to\oplus_{i}F[-k]. Note that taking the dual changes the sign of the grading: Hom(E,F[k])\operatorname{Hom}(E,F[k])^{*} is in degree k-k while Hom(E,F[k])\operatorname{Hom}(E,F[k]) is in degree kk. It is easy to check that both (LEF,E)(L_{E}F,E) and (F,RF(E))(F,R_{F}(E)) are exceptional pairs. More generally, given an exceptional collection σ=(E1,,EN)\sigma=(E_{1},\dots,E_{N}) we define left mutation LiL_{i} and right mutation RiR_{i} by mutating the adjacent objects EiE_{i} and Ei+1E_{i+1}, that is,

Liσ\displaystyle L_{i}\sigma =\displaystyle= (E1,,Ei1,LEiEi+1,Ei,Ei+2,,EN),1iN1,\displaystyle(E_{1},\dots,E_{i-1},L_{E_{i}}E_{i+1},E_{i},E_{i+2},\dots,E_{N}),\quad 1\leq i\leq N-1,
Riσ\displaystyle R_{i}\sigma =\displaystyle= (E1,,Ei1,Ei+1,REi+1Ei,Ei+2,,EN),1iN1.\displaystyle(E_{1},\dots,E_{i-1},E_{i+1},R_{E_{i+1}}E_{i},E_{i+2},\dots,E_{N}),\quad 1\leq i\leq N-1.

It turns out that these operations define an action of the braid group of NN strings on the set of exceptional collections, that is, the following commutation relations hold (see [5], Assertion 2.3):

RiLi=1(1iN1)\displaystyle R_{i}L_{i}=1\quad(1\leq i\leq N-1)

and

RiRi+1Ri=Ri+1RiRi+1,LiLi+1Li=Li+1LiLi+1,\displaystyle R_{i}R_{i+1}R_{i}=R_{i+1}R_{i}R_{i+1},\quad L_{i}L_{i+1}L_{i}=L_{i+1}L_{i}L_{i+1},

where 1iN21\leq i\leq N-2. Using mutations we can construct the so-called left Koszul dual of the exceptional sequence σ=(E1,,EN)\sigma=(E_{1},\dots,E_{N}), that is, the exceptional sequence defined by

σ~:=LN1(LN2LN1)(L1L2LN1)(σ)\displaystyle\widetilde{\sigma}:=L_{N-1}(L_{N-2}L_{N-1})\cdots(L_{1}L_{2}\cdots L_{N-1})(\sigma)

is called the left Koszul dual of σ\sigma. More explicitly,

σ~=(E~N,,E~1),E~1:=E1,E~i:=LE1LEi1(Ei)(2iN).\displaystyle\widetilde{\sigma}=(\widetilde{E}_{N},\dots,\widetilde{E}_{1}),\quad\widetilde{E}_{1}:=E_{1},\quad\widetilde{E}_{i}:=L_{E_{1}}\cdots L_{E_{i-1}}(E_{i})\quad(2\leq i\leq N).

In other words, using left translations (see [5], Section 2), we are moving first ENE_{N} to the left through E1,,EN1E_{1},\dots,E_{N-1}, then in the resulting collection we move EN1E_{N-1} to the left through E1,,EN2E_{1},\dots,E_{N-2} etc.. We are not going to use it but let us point out that one can define a right Koszul dual in a similar way, that is, R1(R2R1)(RN1RN2R1)(σ)R_{1}(R_{2}R_{1})\cdots(R_{N-1}R_{N-2}\cdots R_{1})(\sigma). As we will see now, the left (resp. right) Koszul dual corresponds to changing the admissible direction η\eta to η-\eta by an anti-clockwise (resp. clockwise) rotation.

Definition 3.2.3.

Let (E1,,EN)(E_{1},\dots,E_{N}) be a full exceptional collection. The helix generated by (E1,,EN)(E_{1},\dots,E_{N}) is the infinite collection (Ei)i(E_{i})_{i\in\mathbb{Z}} defined by the iterated mutations

Ei+N=REi+N1REi+1Ei,\displaystyle E_{i+N}=R_{E_{i+N-1}}\cdots R_{E_{i+1}}E_{i},
EiN=LEiN+1LEi1Ei\displaystyle E_{i-N}=L_{E_{i-N+1}}\cdots L_{E_{i-1}}E_{i}

A foundation of a helix is any family of NN consecutive objects (Ei+1,Ei+2,,Ei+N)(E_{i+1},E_{i+2},\dots,E_{i+N}). The collection (E1,,EN)(E_{1},\dots,E_{N}) is called the marked foundation. ∎

Definition 3.2.4.

Let [𝒯][\mathcal{T}] be the set of isomorphism classes of objects of 𝒯\mathcal{T}. The Grothendieck group K0(𝒯)K_{0}(\mathcal{T}) of 𝒯\mathcal{T} is defined as the quotient of the free abelian group generated by [𝒯][\mathcal{T}] and the Euler relations: [B]=[A]+[C][B]=[A]+[C] whenever there exist a triangle ABCA[1]A\rightarrow B\rightarrow C\rightarrow A[1] in 𝒯.\mathcal{T}.

We can define the so-called Grothendieck-Euler-Poincaré pairing as

χ(E,F)=i(1)idimHomi(E,F)\displaystyle\chi(E,F)=\sum_{i}(-1)^{i}\mathrm{dim}_{\mathbb{C}}\mathrm{Hom}^{i}(E,F)

for any pair of objects EE and FF in 𝒯\mathcal{T}. Note that on the level of KK-theoretic groups the left and right mutations take the form

[LEF]=[F]χ(E,F)[E],[RFE]=[E]χ(E,F)[F].\displaystyle[L_{E}F]=[F]-\chi(E,F)[E],\quad[R_{F}E]=[E]-\chi(E,F)[F].
Lemma 3.2.1.

Let σ=(E1,,EN)\sigma=(E_{1},\dots,E_{N}) be a full exceptional collection and σ~=(E~N,,E~1)\widetilde{\sigma}=(\widetilde{E}_{N},\dots,\widetilde{E}_{1}) be its left Koszul dual. Then χ(Ei,E~j)=δij\chi(E_{i},\widetilde{E}_{j})=\delta_{ij}.

Proof.

Let Bi=[Ei]K0(𝒯)B_{i}=[E_{i}]\in K_{0}(\mathcal{T}) and B~i=[E~i]K0(𝒯)\widetilde{B}_{i}=[\widetilde{E}_{i}]\in K_{0}(\mathcal{T}). Let us introduce the reflection σi(A):=Aq1h(A,Bi)Bi\sigma_{i}(A):=A-q^{-1}h(A,B_{i})B_{i} where h(A,B):=qχ(A,B)+q1χ(B,A)h(A,B):=q\chi(A,B)+q^{-1}\chi(B,A) and qq is generic, such that, h(,)h(\ ,\ ) is a non-degenerate pairing. Using that χ(Bi,Bj)=0\chi(B_{i},B_{j})=0 for i>ji>j, it is easy to check that

B~i=[LE1LE2LEi1(Ei)]=σ11σ21σi11(Bi).\displaystyle\widetilde{B}_{i}=[L_{E_{1}}L_{E_{2}}\cdots L_{E_{i-1}}(E_{i})]=\sigma_{1}^{-1}\sigma_{2}^{-1}\cdots\sigma_{i-1}^{-1}(B_{i}).

Note that the relations in the above formula are identical to the relations in (35). Therefore, if we define BiB_{i}^{*} and B~i\widetilde{B}_{i}^{*}, such that, h(Bi,Bj)=δijh(B_{i}^{*},B_{j})=\delta_{ij} and h(B~i,B~j)=δijh(\widetilde{B}_{i}^{*},\widetilde{B}_{j}^{*})=\delta_{ij}, then we have a relation corresponding to (36)

B~k=Bk+a=k+1Nq1h(Bk,Ba)Ba.\displaystyle\widetilde{B}_{k}^{*}=B_{k}^{*}+\sum_{a=k+1}^{N}q^{-1}h(B_{k},B_{a})B_{a}^{*}.

Note that q1h(Bk,Ba)=χ(Bk,Ba)q^{-1}h(B_{k},B_{a})=\chi(B_{k},B_{a}) because χ(Ba,Bk)=0\chi(B_{a},B_{k})=0 for a>ka>k. Let χB\chi_{B} be the Gram matrix of χ\chi in the basis B1,,BNB_{1},\dots,B_{N}, that is, χB,ij=χ(Bi,Bj)\chi_{B,ij}=\chi(B_{i},B_{j}). Similarly, let χB~,ij=χ(B~i,B~j)\chi_{\widetilde{B},ij}=\chi(\widetilde{B}_{i},\widetilde{B}_{j}) be the Gram matrix of χ\chi in the basis (B~1,,B~N)(\widetilde{B}_{1},\dots,\widetilde{B}_{N}). Suppose that T=(Tij)T=(T_{ij}) is the matrix describing the transition between the two bases: B~j=i=1NBiTij\widetilde{B}_{j}=\sum_{i=1}^{N}B_{i}T_{ij}. Then we have

δkj=h(B~k,B~j)=a,i=1NχB,kaTijh(Ba,Bi)=i=1Nχ(Bk,Bi)Tij\displaystyle\delta_{kj}=h(\widetilde{B}_{k}^{*},\widetilde{B}_{j})=\sum_{a,i=1}^{N}\chi_{B,ka}T_{ij}h(B_{a}^{*},B_{i})=\sum_{i=1}^{N}\chi(B_{k},B_{i})T_{ij}

which implies that

χ(Bi,B~j)=k=1Nχ(Bi,Bk)Tkj=δij.\displaystyle\chi(B_{i},\widetilde{B}_{j})=\sum_{k=1}^{N}\chi(B_{i},B_{k})T_{kj}=\delta_{ij}.\qed
Definition 3.2.5.

A unimodular Mukai lattice is a finitely generated free \mathbb{Z}-module VV with a unimodular bilinear form (not necessarily symmetric) .,.:V×V\langle.,.\rangle:V\times V\rightarrow\mathbb{Z}.
An element eVe\in V is called exceptional if e,e=1\langle e,e\rangle=1. A \mathbb{Z}-basis (e1,,en)(e_{1},\dots,e_{n}) of the Mukai lattice is called exceptional if ei,ei=1\langle e_{i},e_{i}\rangle=1, i\forall i and ej,ei=0\langle e_{j},e_{i}\rangle=0 for j>ij>i.∎

Remark 3.2.1.

The projection on K0(𝒯)K_{0}(\mathcal{T}) of a full exceptional collection in 𝒯\mathcal{T} is an exceptional basis. The pair (K0(𝒯)K_{0}(\mathcal{T}), χ\chi), where χ\chi is the Grothendieck-Euler-Poincaré pairing defined above, is a unimodular Mukai lattice. The matrix GG whose (i,j)(i,j)-entry is χ(Ei,Ej)\chi(E_{i},Ej) is called the Gram matrix associated to the exceptional collection (E1,,En).(E_{1},\dots,E_{n}).

We are interested in the case where the triangulated category 𝒯\mathcal{T} is the bounded derived category of coherent sheaves of a smooth algebraic variety XX, which we denote by Db(X)D^{b}(X). It is interesting to know in which cases Db(X)D^{b}(X) has a full exceptional collection.

3.3. Original formulation of Dubrovin conjecture

For a smooth Fano variety we have formulated two questions. The first one is about the semisimplicity of the big quantum cohomology and the second one is about the existence of a full exceptional collections in Db(X)D^{b}(X). At first sight, the questions seem unrelated but this is not the case. In fact, the main content of Dubrovin conjecture is precisely that the answer of these two questions should be linked. In his ICM talk in 1998, following a proposal of Alexey Bondal, Dubrovin proposed the following conjecture (see [9] and also [6]).

Conjecture 3.3.1 (Dubrovin 1998).

Let XX be a Fano variety.

  1. (1)

    The big quantum cohomology QH(X)QH^{*}(X) is semisimple if and only if Db(X)D^{b}(X) admits a full exceptional collection (E1,,EN)(E_{1},\dots,E_{N}), where N=dimH(X)N=\mathrm{dim}_{\mathbb{C}}H^{*}(X).

  2. (2)

    The Stokes matrix for the first structure connection S=(sij)S=(s_{ij}) is equal to the Gram matrix for (E1,,EN)(E_{1},\dots,E_{N}), i.e., sij=χ(Ei,Ej)s_{ij}=\chi(E_{i},E_{j}).

  3. (3)

    The central connection matrix CC hast the form C=CC′′C=C^{\prime}C^{\prime\prime}, where the columns of C′′C^{\prime\prime} are the components of ch(Ej)H+(X)\mathrm{ch}(E_{j})\in H^{+}(X) and C:H(X)H(X)C^{\prime}:H^{*}(X)\rightarrow H^{*}(X) is some operator satisfying C(c1(X)a)=c1(X)C(a)C^{\prime}(c_{1}(X)a)=c_{1}(X)C^{\prime}(a) for any aH(X)a\in H^{*}(X).

There are two important developments that lead to a modification of the conjecture. First of all, it was suggested by Arend Bayer (see [3]) that the Fano condition is not important, so it should be dropped. Second, a precise statement about the central connection matrix, was proposed independently in [13] by Galkin-Golyshev-Iritani and in [6] by Cotti-Dubrovin-Guzzetti. An important role in this refinement is played by the so-called Gamma class.

3.4. Refined version of the conjecture

Let XX be a smooth projective variety of complex dimension DD. The cohomology class (see [13]) Γ^X=Γ^X+:=i=1DΓ(1+δi)\widehat{\Gamma}_{X}=\widehat{\Gamma}^{+}_{X}:=\prod_{i=1}^{D}\Gamma(1+\delta_{i}), where δ1,,δD\delta_{1},\dots,\delta_{D} are the Chern roots of TXTX and Γ(X)\Gamma(X) is the Gamma function, is called the Gamma class. Following [6], we introduce also the class Γ^X=i=1DΓ(1δi)\widehat{\Gamma}_{X}^{-}=\prod_{i=1}^{D}\Gamma(1-\delta_{i}).

Remark 3.4.1.

Gamma classes appear in the study of integral structures of quantum cohomology in the work of Iritani [21] and the work of Katzarkov-Kontsevich-Pantev [23] on noncommutative Hodge structures. It also appears in physics under the hemisphere partition functions studied by Hori-Romo in [20].∎

Remark 3.4.2.

The Gamma class Γ^X\widehat{\Gamma}_{X} can be expended as

Γ^X=exp(Ceuc1(X)+k2(1)k(k1)!ζ(k)chk(TX)\displaystyle\widehat{\Gamma}_{X}=\mathrm{exp}(-C_{eu}c_{1}(X)+\sum_{k\geqslant 2}(-1)^{k}(k-1)!\zeta(k)\operatorname{ch}_{k}(TX)

where CeuC_{eu} is the Euler constant. This is obtained from the Taylor expansion for the Gamma function. ∎

The other ingredient introduced in [6] is given by two morphisms 𝔄X±:K0(X)H(X,)\mathfrak{A}^{\pm}_{X}:K_{0}(X)\rightarrow H^{*}(X,\mathbb{C}) which are defined as follows. Let EDb(X)E\in D^{b}(X). Since XX is smooth, the object EE is isomorphic to a bounded complex of locally free sheaves FF^{\bullet}, therefore a graded version of the Chern character can be defined as Ch(E):=j(1)jCh(Fj)\operatorname{Ch}(E):=\sum_{j}(-1)^{j}\operatorname{Ch}(F^{j}) where Ch(Fj)=αe2π𝐢α\operatorname{Ch}(F^{j})=\sum_{\alpha}e^{2\pi\mathbf{i}\alpha} where the sum is over the Chern roots α\alpha of FjF^{j}. Note that the standard Chern character is ch(E):=j(1)jch(Fj)\operatorname{ch}(E):=\sum_{j}(-1)^{j}\operatorname{ch}(F^{j}) where ch(Fj)=αeα\operatorname{ch}(F^{j})=\sum_{\alpha}e^{\alpha}. In other words, the difference between Ch\operatorname{Ch} and ch\operatorname{ch} is in re-scaling each Chern root by 2π𝐢2\pi\mathbf{i}. The morphisms 𝔄X±\mathfrak{A}_{X}^{\pm} are defined as follows:

(50) 𝔄X±(E)=𝐢D¯(2π)D2Γ^±(X)exp(±π𝐢c1(X))Ch(E),\mathfrak{A}_{X}^{\pm}(E)=\frac{\mathbf{i}^{\overline{D}}}{(2\pi)^{\frac{D}{2}}}\widehat{\Gamma}^{\pm}(X)\cup\mathrm{exp}(\pm\pi\mathbf{i}c_{1}(X))\cup\operatorname{Ch}(E),

where D¯{0,1}\overline{D}\in\{0,1\} is the remainder of the division of DD by 2.2. In order to define the monodromy data of a Frobenius manifold, Cotti–Dubrovin–Guzzetti have introduced chambers Ω\Omega_{\ell} for every oriented line \ell\subset\mathbb{C} with orientation specified by a unit vector e𝐢ϕe^{\mathbf{i}\phi}, ϕ[0,2π)\phi\in[0,2\pi). In our notation, Ω\Omega_{\ell} is an open subset of the Frobenius manifold MH(X,)M\subset H^{*}(X,\mathbb{C}) consisting of semi-simple points tt, such that,

  1. (i)

    The canonical coordinates u1(t),,uN(t)u_{1}(t),\dots,u_{N}(t) are pairwise distinct.

  2. (ii)

    The vector η:=𝐢e𝐢ϕ\eta:=\mathbf{i}e^{\mathbf{i}\phi} is an admissible direction, that is, 𝐢e𝐢ϕ\mathbf{i}e^{\mathbf{i}\phi} is not parallel to uiuju_{i}-u_{j} for all iji\neq j.

In every chamber Ω\Omega_{\ell}, the canonical coordinates are enumerated according to the so-called lexicographical order: if i<ji<j then Re(uiuj)e𝐢ϕ<0\operatorname{Re}(u_{i}-u_{j})e^{-\mathbf{i}\phi}<0, or equivalently if we stand at uiu_{i} and look in the admissible direction η:=𝐢e𝐢ϕ\eta:=\mathbf{i}e^{\mathbf{i}\phi}, then uju_{j} is on our right. The Frobenius manifold underlying quantum cohomology has a natural calibration given by the SS-matrix S(t,z)=1+S1(t)z1+S2(t)z2+S(t,z)=1+S_{1}(t)z^{-1}+S_{2}(t)z^{-2}+\cdots where Sk(t)End(H(X,))S_{k}(t)\in\operatorname{End}(H^{*}(X,\mathbb{C})) are defined by

(Sk(t)ϕa,ϕb):=ϕaψk1,ϕb0,2(t).\displaystyle(S_{k}(t)\phi_{a},\phi_{b}):=\langle\phi_{a}\psi^{k-1},\phi_{b}\rangle_{0,2}(t).

The nilpotent operator ρ:=c1(TX)\rho:=c_{1}(TX)\cup. The monodromy data is defined as explained in Sections 2.4 and 2.6. Namely, there are unique solutions X(±η,t,z)Ψ(t)R(t,z)eU/zX(\pm\eta,t,z)\sim\Psi(t)R(t,z)e^{U/z} as z0z\to 0 holomorphic for zH±ηz\in H_{\pm\eta} where HηH_{\eta} (resp. HηH_{-\eta}) is the right (resp. left) half-plane bounded by the oriented line \ell. The 3 solutions to the quantum connection X(η,t,z)X(-\eta,t,z), X(η,t,z)X(\eta,t,z), and S(t,z)zθzρS(t,z)z^{\theta}z^{-\rho} are analytic in zz in a sector containing the positive part of the line \ell and hence we can define the Stokes matrix V+V_{+} and the central connection matrix CC by

X(η,t,z)=X(η,t,z)V+,X(η,t,z)=S(t,z)zθzρC1.\displaystyle X(-\eta,t,z)=X(\eta,t,z)V_{+},\quad X(-\eta,t,z)=S(t,z)z^{\theta}z^{-\rho}C^{-1}.

We refer to Remark 2.6.1 where we explained the correspondence between our notation and the Dubrovin’s notation. Let us point out that the notation for the central connection matrix in [10] and [6] are different: one is the inverse of the other. We stick to the notation from [10].

Conjecture 3.4.1 (Refined Dubrovin conjecture 2018, see conjecture 5.2 in [6]).

Let XX be a smooth Fano variety of Hodge-Tate type, then

  1. (1)

    The big quantum cohomology QH(X)QH^{*}(X) is semisimple if and only if there exists a full exceptional collection in Db(X)D^{b}(X).

  2. (2)

    If QH(X)QH^{*}(X) is semisimple and convergent, then for any oriented line \ell (of slope ϕ[0,2π)\phi\in[0,2\pi)) in the complex plane, there is a correspondence between \ell-chambers and helices with a marked foundation (E1,,EN)(E_{1},\dots,E_{N}) in Db(X)D^{b}(X).

  3. (3)

    The monodromy data computed in an \ell-chamber Ω\Omega_{\ell}, in the lexicographical order, is related to the following geometric data of the corresponding exceptional collection (E1,,EN)(E_{1},\dots,E_{N}) (the marked foundation):

    1. (3a)

      The Stokes matrix V+V_{+} is equal to the Gram matrix of the Grothendieck-Poincaré-Euler product on K0(X)K_{0}(X)_{\mathbb{C}}, computed with respect to the exceptional basis ([E1],,[EN])([E_{1}],\dots,[E_{N}]), that is, V+,ij=χ(Ei,Ej)V_{+,ij}=\chi(E_{i},E_{j}).

    2. (3b)

      The inverse central connection matrix C1C^{-1} coincides with the matrix associated with the \mathbb{C}-linear morphism 𝔄X:K0(X)H(X,)\mathfrak{A}^{-}_{X}:K_{0}(X)_{\mathbb{C}}\rightarrow H^{*}(X,\mathbb{C}) defined above – see (50). The matrix is computed with respect to the exceptional basis ([E1],,[EN])([E_{1}],\dots,[E_{N}]) and any pre-fixed cohomological basis {ϕα}α=1N\{\phi_{\alpha}\}_{\alpha=1}^{N}.

Some parts of the Dubrovin conjecture, in its original or refined forms, have been verified for several Fano varieties, see [6] for a detailed account about the cases where the conjecture has been proved.

3.5. Exceptional collections, reflection vectors, and Dubrovin conjecture

Motivated by the definition of a distinguished basis in singularity theory (see [1, 12]), let us define a distinguished system of reference paths. Recall that we have fixed a reference point (t,λ)(t^{\circ},\lambda^{\circ}), such that, |ui|<|λ||u_{i}^{\circ}|<|\lambda^{\circ}| for all ii and Re(ui)Re(uj)\operatorname{Re}(u_{i}^{\circ})\neq\operatorname{Re}(u_{j}^{\circ}) for all iji\neq j where ui:=ui(t)u_{i}^{\circ}:=u_{i}(t^{\circ}) are the canonical coordinates of tt^{\circ}. Let Δ\Delta be the disk with center 0 and radius λ\lambda^{\circ} (recall that λ\lambda^{\circ} is a positive real number).

Definition 3.5.1.

A system of paths (C1,,CN)(C_{1},\dots,C_{N}) inside Δ\Delta is said to be a distinguished system of reference paths if

  1. (i)

    The path CiC_{i} has no self-intersections and it connects λ\lambda^{\circ} with one of the points u1,,uNu_{1}^{\circ},\dots,u_{N}^{\circ}.

  2. (ii)

    For each pair of paths CiC_{i} and CjC_{j} with iji\neq j, the only common point is λ\lambda^{\circ}.

  3. (iii)

    The paths C1,,CNC_{1},\dots,C_{N} exit the point λ\lambda^{\circ} in an anti-clockwise order counted from the boundary of the disk Δ\Delta.∎

Two distinguished systems of reference paths C=(C1,,CN)C^{\prime}=(C_{1}^{\prime},\dots,C_{N}^{\prime}) and C′′=(C1′′,,CN′′)C^{\prime\prime}=(C^{\prime\prime}_{1},\dots,C^{\prime\prime}_{N}) will be considered homotopy equivalent if there exists a continuous family C(s)=(C1(s),,CN(s))C(s)=(C_{1}(s),\dots,C_{N}(s)), s[0,1]s\in[0,1], such that, C(s)C(s) is a distinguished system of reference paths s[0,1]\forall s\in[0,1] and C(0)=CC(0)=C^{\prime} and C(1)=C′′C(1)=C^{\prime\prime} (for more details see [12], Section 5.7). The braid group on NN strings acts naturally on the set of homotopy equivalence classes of distinguished reference paths. Namely, we have the operations

Li(C1,,CN):=(C1,,Ci1,LCiCi+1,Ci,,CN),1iN1,\displaystyle L_{i}(C_{1},\dots,C_{N}):=(C_{1},\dots,C_{i-1},L_{C_{i}}C_{i+1},C_{i},\dots,C_{N}),\quad 1\leq i\leq N-1,

where LCiCi+1L_{C_{i}}C_{i+1} is a small perturbation of the composition of Ci+1C_{i+1} and the anti-clockwise simple loop corresponding to CiC_{i}. Similarly, we have the operation

Ri(C1,,CN):=(C1,,Ci1,Ci+1,RCi+1Ci,Ci+2,,CN),1iN1,\displaystyle R_{i}(C_{1},\dots,C_{N}):=(C_{1},\dots,C_{i-1},C_{i+1},R_{C_{i+1}}C_{i},C_{i+2},\dots,C_{N}),\quad 1\leq i\leq N-1,

where RCi+1CiR_{C_{i+1}}C_{i} is a small perturbation of the composition of CiC_{i} and the clockwise simple loop corresponding to Ci+1C_{i+1}. The operation RiR_{i} is inverse to LiL_{i} and the following braid group relations are satisfied:

LiLi+1Li=Li+1LiLi+1,RiRi+1Ri=Ri+1RiRi+1,1iN2.\displaystyle L_{i}L_{i+1}L_{i}=L_{i+1}L_{i}L_{i+1},\quad R_{i}R_{i+1}R_{i}=R_{i+1}R_{i}R_{i+1},\quad 1\leq i\leq N-2.

The braid group on NN strings acts transitively on the set of homotopy equivalence classes of distinguished reference paths. This is almost an immediate consequence of the definition of a braid (see [12], Proposition 5.15).

Remark 3.5.1.

In singularity theory, one usually requires the order of the distinguished system of reference paths to be clockwise. We change it to anti-clockwise in order to have an agreement between the lexicographical order defined by an admissible direction. ∎

Remark 3.5.2.

The operations LiL_{i} and RiR_{i} are usually denoted by αi\alpha_{i} and βi+1\beta_{i+1}. Our notation is motivated by the corresponding notation for left and right mutations in the case of exceptional collections. ∎

Partially motivated by the work of Milanov–Xia (see [26], Conjecture 1.6), we would like to propose the following conjecture.

Conjecture 3.5.1.

If β1,,βN\beta_{1},\dots,\beta_{N} is a set of reflection vectors corresponding to a system of distinguished reference paths, then there exists a full exceptional collection (F1,,FN)(F_{1},\dots,F_{N}) in Db(X)D^{b}(X), such that, βi=ΨQ(Fi)\beta_{i}=\Psi_{Q}(F_{i}) for all ii.

Conjecture 3.5.1 is weaker than Conjecture 1.6 in [26]. Namely, the proposal in [26] is that every full exceptional collection determines a set of reflection vectors. This is more difficult to prove. Nevertheless, it is expected that any two full exceptional collections are related by a sequence of mutations. If this expectation is correct then Conjecture 1.6 in [26] is equivalent to Conjecture 3.5.1.

Theorem 3.5.1.

Conjecture 3.5.1 is equivalent to the refined Dubrovin conjecture.

Proof.

Let us consider the case when all Novikov variable q1==qr=1q_{1}=\cdots=q_{r}=1. The general case can be obtained by applying the divisor equation. Suppose that the distinguished system of reference paths is given by Ci(η)C_{i}(\eta) (1iN1\leq i\leq N) where η\eta is an admissible direction. Assuming that the refined Dubrovin conjecture holds, let us derive the formulas for the reflection vectors in Conjecture 3.5.1. Note that the exceptional collection F1,,FNF_{1},\dots,F_{N} will be different from E1,,ENE_{1},\dots,E_{N}. The inverse central connection matrix defines a map C1:NH(X,)C^{-1}:\mathbb{C}^{N}\to H^{*}(X,\mathbb{C}) which according to the refined Dubrovin conjecture is given by

C1(ei)=𝐢D¯(2π)D/2Γ^Xeπ𝐢ρCh(Ei).\displaystyle C^{-1}(e_{i})=\frac{\mathbf{i}^{\overline{D}}}{(2\pi)^{D/2}}\widehat{\Gamma}^{-}_{X}\cup e^{-\pi\mathbf{i}\rho}\cup\operatorname{Ch}(E_{i}).

If ϕaH(X,)\phi_{a}\in H^{*}(X,\mathbb{C}) is one of the basis vectors, then we have

ϕa=C1(C(ϕa))=12πi=1NC1(ei)(βi,ϕa),\displaystyle\phi_{a}=C^{-1}(C(\phi_{a}))=\frac{1}{\sqrt{2\pi}}\sum_{i=1}^{N}C^{-1}(e_{i})(\beta_{i},\phi_{a}),

where we used the formula for the (i,a)(i,a)-entry of CC from Theorem 2.6.1, part a). We get

ϕa=𝐢D¯(2π)(1+D)/2i=1NΓ^Xeπ𝐢ρCh(Ei)(βi,ϕa).\displaystyle\phi_{a}=\frac{\mathbf{i}^{\overline{D}}}{(2\pi)^{(1+D)/2}}\sum_{i=1}^{N}\widehat{\Gamma}^{-}_{X}\cup e^{-\pi\mathbf{i}\rho}\cup\operatorname{Ch}(E_{i})(\beta_{i},\phi_{a}).

Let us multiply the above identity, using the classical cup product, by Γ^X+Ch(Fj)\widehat{\Gamma}^{+}_{X}\cup\operatorname{Ch}(F_{j}) where FjK0(X)F_{j}\in K^{0}(X) will be specified later on. Recall that

Γ^X+Γ^X=δΓ(1+δ)Γ(1δ)=δ2π𝐢δeπ𝐢δeπ𝐢δ=eπ𝐢ρ(2π𝐢)degTd(X),\displaystyle\widehat{\Gamma}^{+}_{X}\widehat{\Gamma}^{-}_{X}=\prod_{\delta}\Gamma(1+\delta)\Gamma(1-\delta)=\prod_{\delta}\frac{2\pi\mathbf{i}\delta}{e^{\pi\mathbf{i}\delta}-e^{-\pi\mathbf{i}\delta}}=e^{-\pi\mathbf{i}\rho}(2\pi\mathbf{i})^{\rm deg}\operatorname{Td}(X),

where the product is over all Chern roots of TXTX and Td(X)\operatorname{Td}(X) is the Todd class of TXTX. Note also that e2π𝐢c1(TX)=Ch(K)e^{-2\pi\mathbf{i}c_{1}(TX)}=\operatorname{Ch}(K) where KK is the canonical bundle of XX. We get

Γ^X+Ch(Fj)ϕa=𝐢D¯(2π)(1+D)/2Ch(FjK)(2π𝐢)deg(Td(X))i=1NCh(Ei)(βi,ϕa).\displaystyle\widehat{\Gamma}^{+}_{X}\cup\operatorname{Ch}(F_{j})\cup\phi_{a}=\frac{\mathbf{i}^{\overline{D}}}{(2\pi)^{(1+D)/2}}\operatorname{Ch}(F_{j}\otimes K)\,(2\pi\mathbf{i})^{\rm deg}(\operatorname{Td}(X))\sum_{i=1}^{N}\operatorname{Ch}(E_{i})(\beta_{i},\phi_{a}).

Let us integrate the above identity over XX. For dimensional reasons, we can replace the expression Ch(FjK)(2π𝐢)deg(Td(X))Ch(Ei)\operatorname{Ch}(F_{j}\otimes K)\,(2\pi\mathbf{i})^{\rm deg}(\operatorname{Td}(X))\operatorname{Ch}(E_{i}) with (2π𝐢)Dch(FjK)Td(X)ch(Ei).(2\pi\mathbf{i})^{D}\operatorname{ch}(F_{j}\otimes K)\,\operatorname{Td}(X)\operatorname{ch}(E_{i}). Recalling the Hierzerbruch–Riemann–Roch formula we get

(Γ^X+Ch(Fj),ϕa)=𝐢D¯+D(2π)(d1)/2i=1Nχ(EiFjK)(βi,ϕa).\displaystyle(\widehat{\Gamma}^{+}_{X}\cup\operatorname{Ch}(F_{j}),\phi_{a})=\mathbf{i}^{\overline{D}+D}(2\pi)^{(d-1)/2}\sum_{i=1}^{N}\chi(E_{i}\otimes F_{j}\otimes K)(\beta_{i},\phi_{a}).

Since the Poincare pairing is non-degenerate, the above formula implies

(51) Γ^X+Ch(Fj)=𝐢D¯+D(2π)(D1)/2i=1Nχ(EiFjK)βi.\widehat{\Gamma}^{+}_{X}\cup\operatorname{Ch}(F_{j})=\mathbf{i}^{\overline{D}+D}(2\pi)^{(D-1)/2}\sum_{i=1}^{N}\chi(E_{i}\otimes F_{j}\otimes K)\,\beta_{i}.

Let us recall that by Serre duality, that is, Hi(X,E)HDi(X,EK)H^{i}(X,E^{\vee})\cong H^{D-i}(X,E\otimes K)^{\vee}, we have χ(EK)=(1)Dχ(E).\chi(E\otimes K)=(-1)^{D}\chi(E^{\vee}). Therefore,

𝐢D¯+Dχ(EiFjK)=𝐢D¯Dχ(EiFj)=(1)(D¯D)/2Fj,Ei.\displaystyle\mathbf{i}^{\overline{D}+D}\chi(E_{i}\otimes F_{j}\otimes K)=\mathbf{i}^{\overline{D}-D}\chi(E_{i}^{\vee}\otimes F^{\vee}_{j})=(-1)^{(\overline{D}-D)/2}\langle F_{j},E_{i}^{\vee}\rangle.

Clearly, we can choose KK-theoretic vector bundles F1,,FNF_{1},\dots,F_{N}, such that, Fj,Ei=(1)(D¯D)/2δi,j\langle F_{j},E_{i}^{\vee}\rangle=(-1)^{(\overline{D}-D)/2}\,\delta_{i,j}. Once this choice is made, we get from (51) that βj=Ψ(Fj)\beta_{j}=\Psi(F_{j}) where Ψ=Ψq|q1==qr=1\Psi=\left.\Psi_{q}\right|_{q_{1}=\cdots=q_{r}=1}. We claim that F1,,FNF_{1},\dots,F_{N} are the K-theoretic classes of a full exceptional collection. Indeed, recalling Lemma 3.2.1, it is sufficient to choose a full exceptional collection (G1,,GN)(G_{1},\dots,G_{N}), such that, its left Koszul dual is (EN,,E1)(E_{N}^{\vee},\dots,E_{1}^{\vee}). Once we do this, we can simply put Fi=Gi[D¯D2]F_{i}=G_{i}[\tfrac{\overline{D}-D}{2}]. In order to define GiG_{i}, we simply have to invert the sequence of mutation operations that define the left Koszul dual, that is,

(G1,,GN)=(RN1RN2R1)(RN1RN2R2)(RN1RN2)RN1(EN,,E1).\displaystyle(G_{1},\dots,G_{N})=(R_{N-1}R_{N-2}\cdots R_{1})(R_{N-1}R_{N-2}\cdots R_{2})\cdots(R_{N-1}R_{N-2})R_{N-1}(E_{N}^{\vee},\dots,E_{1}^{\vee}).

In order to complete the proof that the refined Dubrovin conjecture implies Conjecture 3.5.1 we need only to recall the braid group action. More precisely, note that after a small perturbation the system of reference paths (C1(η),,CN(η))(C_{1}(\eta),\dots,C_{N}(\eta)) corresponding to an admissible direction η\eta becomes a distinguished system of reference paths. Therefore, we need only to check the following statement. Suppose that Conjecture 3.5.1 holds for a distinguished system of reference paths γ=(C1,,CN)\gamma=(C_{1},\dots,C_{N}) satisfying the extra condition βi,βj=0\langle\beta_{i},\beta_{j}\rangle=0 for i>ji>j where β1,,βN\beta_{1},\dots,\beta_{N} are the reflection vectors corresponding to γ\gamma. Then we calim that the conjecture holds for LiγL_{i}\gamma and moreover LiγL_{i}\gamma satisfies the extra condition: β~i,β~j=0\langle\widetilde{\beta}_{i},\widetilde{\beta}_{j}\rangle=0 for i>ji>j where β~1,,β~N\widetilde{\beta}_{1},\dots,\widetilde{\beta}_{N} are the reflection vectors corresponding to LiγL_{i}\gamma. Note that

β~i=σi1(βi+1),β~i+1=βi,β~k=βk,ki,i+1.\displaystyle\widetilde{\beta}_{i}=\sigma_{i}^{-1}(\beta_{i+1}),\quad\widetilde{\beta}_{i+1}=\beta_{i},\quad\widetilde{\beta}_{k}=\beta_{k},\quad k\neq i,i+1.

We have

β~i=σi1(βi+1)=βi+1qhm(βi+1,βi)βi=βi+1βi,βi+1βi.\displaystyle\widetilde{\beta}_{i}=\sigma_{i}^{-1}(\beta_{i+1})=\beta_{i+1}-qh_{m}(\beta_{i+1},\beta_{i})\beta_{i}=\beta_{i+1}-\langle\beta_{i},\beta_{i+1}\rangle\beta_{i}.

It is straightforward to check that β~i,β~j=0\langle\widetilde{\beta}_{i},\widetilde{\beta}_{j}\rangle=0 for i>ji>j. Thanks to formula (11), it is easy to check that if βk=Ψ(Fk)\beta_{k}=\Psi(F_{k}) for some exceptional collection ϕ=(F1,,FN)\phi=(F_{1},\dots,F_{N}), then β~k=Ψ(F~k)\widetilde{\beta}_{k}=\Psi(\widetilde{F}_{k}) where (F~1,,F~N)=Liϕ(\widetilde{F}_{1},\dots,\widetilde{F}_{N})=L_{i}\phi, that is, Conjecture 3.5.1 holds for LiγL_{i}\gamma.

Finally, for the inverse statement, that is, Conjecture 3.5.1 implies the refined Dubrovin conjecture, one just has to go backwards. We leave the details as an exercise. ∎

Let us point out the following important property of a distinguished bases which was obtained as a byproduct of the proof of Theorem 3.5.1.

Proposition 3.5.1.

Let β1,,βN\beta_{1},\dots,\beta_{N} be a set of reflection vectors corresponding to a distinguished system of reference paths. Then the Gram matrix of the Euler pairing is upper triangular: βi,βj=0\langle\beta_{i},\beta_{j}\rangle=0 for all i>ji>j and βi,βi=1\langle\beta_{i},\beta_{i}\rangle=1.

Indeed, if the reference paths correspond to an admissible direction, then the statement was already proved in Theorem 2.6.1, part c). In the proof of Theorem 3.5.1 we proved that the statement is invariant under the action of the braid group. Therefore, since the braid group acts transitively on the set of distinguished system of reference paths, the statement of Proposition 3.5.1 is clear.

Remark 3.5.3.

Galkin–Golyshev–Iritani proposed in [13] the so-called Γ\Gamma-Conjecture II. Roughly this conjecture says that the columns of the central connection matrix are the components of (2π)D2Γ^X+Ch(Ei)(2\pi)^{-\tfrac{D}{2}}\widehat{\Gamma}^{+}_{X}\cup\operatorname{Ch}(E_{i}), where D=dimXD=\mathrm{dim}_{\mathbb{C}}X, for an exceptional collection (E1,,EN)(E_{1},\dots,E_{N}). It was proved in [6] that Γ\Gamma-conjecture II is equivalent to part (3b) of the refined Dubrovin conjecture. Moreover, it was proved in [13] that Γ\Gamma-conjecture II implies part (3a) of the refined Dubrovin conjecture. Therefore, Conjecture 3.5.1 is also equivalent to Γ\Gamma-conjecture II. ∎

Remark 3.5.4.

Halpern-Leistner proposed in [19] the so-called noncommutative minimal model program. This is a set of conjectures about canonical paths on the space of stability conditions Stab(X)/𝔾a\mathrm{Stab}(X)/\mathbb{G}_{a} that imply previous conjectures about Db(X)D^{b}(X). In particular, it implies one direction of Dubrovin conjecture regarding the existence of exceptional collections. It would be interesting to see the relations between the canonical paths in the noncommutative minimal model program and the reflection vectors corresponding to a system of distinguished reference paths in Conjecture 3.5.1. ∎

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