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Hitchin map on even very stable upward flows

Miguel González
ICMAT Madrid
mgonzalez.contacto@gmail.com
   Tamás Hausel
IST Austria
tamas.hausel@ist.ac.at
Abstract

We define even very stable Higgs bundles and study the Hitchin map restricted to their upward flows. In the GLn\mathrm{GL}_{n} case we classify the type (1,,1)(1,\dots,1) examples, and find that they are governed by a root system formed by the roots of even height. We discuss how the spectrum of equivariant cohomology of real and quaternionic Grassmannians, 4n4n-spheres and the real Cayley plane appear to describe the Hitchin map on even cominuscule upward flows. The even upward flows in question are the same as upward flows in Higgs bundle moduli spaces for quasi-split inner real forms. The latter spaces have been pioneered by Oscar García-Prada and his collaborators.

1 Introduction

This paper is a write-up of the second author’s talk [12] at the conference ”Moduli spaces and geometric structures” in honour of Oscar García-Prada on the occasion of his 60th birthday at ICMAT Madrid in September 2022.

In [14], motivated by mirror symmetry, the notion of very stable Higgs bundle was introduced. Let CC be a smooth projective curve. Let {\mathcal{M}} denote the moduli space of rank nn degree dd semistable Higgs bundles (E,Φ)(E,\Phi), where EE is a rank nn degree vector bundle and ΦH0(C;End(E)K)\Phi\in H^{0}(C;\textnormal{End}(E)\otimes K) is a Higgs field. There is a 𝕋{\mathbb{T}}-action on {\mathcal{M}} by scaling the Higgs field, i.e. λ𝕋\lambda\in{\mathbb{T}} acts by sending (E,Φ)(E,\Phi) to (E,λΦ)(E,\lambda\Phi). A fixed point s𝕋{\mathcal{E}}\in{\mathcal{M}}^{s{\mathbb{T}}} is called very stable, if the upward flow

W+:={:limλ0λ=}W^{+}_{\mathcal{E}}:=\{{\mathcal{F}}\in{\mathcal{M}}:\lim_{\lambda\to 0}\lambda\cdot{\mathcal{F}}={\mathcal{E}}\}\subset{\mathcal{M}}

is closed. In Section 2 we recall the basic properties of very stable upward flows in general as well as for the the moduli space of Higgs bundles {\mathcal{M}}.

One of the main results of [14] is the classification of very stable Higgs bundles (E,Φ)𝕋(E,\Phi)\in{\mathcal{M}}^{{\mathbb{T}}} of type (1,,1)(1,\dots,1). A fixed point is of type (1,,1)(1,\dots,1) when the vector bundle E=L0Ln1E=L_{0}\oplus\dots\oplus L_{n-1} is a direct sum of line bundles, and the Higgs field Φ|Li:LiLi+1KEK\Phi|_{L_{i}}:L_{i}\to L_{i+1}K\subset EK, which we denote by

bi:=Φ|LiHom(Li,Li+1K)H0(C;Li1Li+1K).\displaystyle b_{i}:=\Phi|_{L_{i}}\in\operatorname{Hom}(L_{i},L_{i+1}K)\cong H^{0}(C;L_{i}^{-1}L_{i+1}K).

Then we have

Theorem 1.1 ([14, Theorem 4.16]).

The type (1,,1)(1,...,1) Higgs bundle (E,Φ)𝕋(E,\Phi)\in{\mathcal{M}}^{\mathbb{T}} is very stable if and only if the divisor div(b1)++div(bn1){\rm div}(b_{1})+\dots+{\rm div}(b_{n-1}) is reduced.

We recall this classification in Theorem 2.11 below, and a reformulation of it in Remark 2.12 in terms of minuscule dominant weights of GL(n,)\mathrm{GL}(n,\mathbb{C}).

Garcia-Prada and Ramanan in [9] study involutions on the moduli space of Higgs bundles. One important involution θ:\theta:{\mathcal{M}}\to{\mathcal{M}} is given by θ(E,Φ):=(E,Φ)\theta(E,\Phi):=(E,-\Phi). In [9] it is shown that the fixed points θ{\mathcal{M}}^{\theta} correspond to U(p,np)U(p,n-p)-Higgs bundles (including the case p=0p=0, where U(0,n):=U(n)U(0,n):=U(n)). We recall these notions in Section 3.

In this paper we will be interested in the so-called even upward flows W2+W^{2+}_{\mathcal{E}} for any s𝕋θ{\mathcal{E}}\in{\mathcal{M}}^{s{\mathbb{T}}}\subset{\mathcal{M}}^{\theta} which are defined to be the upward flows {\mathcal{E}} in the semi-projective θ{\mathcal{M}}^{\theta}, or equivalently, the intersection W2+:=W+θW^{2+}_{\mathcal{E}}:=W^{+}_{\mathcal{E}}\cap{\mathcal{M}}^{\theta}. Then we can define even very stable Higgs bundles 𝕋{\mathcal{E}}\in{\mathcal{M}}^{{\mathbb{T}}} for which the even upward flow W2+θW^{2+}_{\mathcal{E}}\subset{\mathcal{M}}^{\theta} is closed. One of the main results of this paper is the following

Theorem 1.2.

The type (1,,1)(1,...,1) Higgs bundle (E,Φ)𝕋(E,\Phi)\in{\mathcal{M}}^{\mathbb{T}} is even very stable, if and only if the divisors div(b2)++div(bn2){\rm div}(b_{2})+\dots+{\rm div}(b_{n-2}) and div(bi)+div(bi+2k+1){\rm div}(b_{i})+{\rm div}(b_{i+2k+1}) for 1ii+2k+1n11\leq i\leq i+2k+1\leq n-1 are all reduced.

To clarify the meaning of this complicated looking set of divisors, we reformulate this theorem in Theorem 3.13 in terms of so-called even minuscule dominant weights using positive weights of even height.

As the Hitchin map restricted to very stable upward flows is finite flat and 𝕋{\mathbb{T}}-equivariant between affine spaces, with positive 𝕋{\mathbb{T}}-action of the same dimension it is suspectible of explicit description. In the type (1,,1)(1,\dots,1) very stable case, the second author found such an explicit description in [13] in terms of the spectrum of equivariant cohomology of the Grassmannian Grk(n)\textnormal{Gr}_{k}(\mathbb{C}^{n}). We will recall this in Section 4.2 below.

Finally in Section 4.3 we study the problem of modelling the Hitchin map on certain even very stable upward flows, in terms of the equivariant cohomology of homogeneous spaces. We will find in Theorem 4.3 that for GL2n\mathrm{GL}_{2n} the equivariant cohomology of quaternionic Grassmannians, for SO4n+2{\mathrm{SO}}_{4n+2} the equivariant cohomology of the 4n4n-sphere and finally for E6{\rm E}_{6} the equivariant cohomology of the real Cayley plane should model the Hitchin map on some specific even very stable flows. The appearance of these symmetric spaces is interesting, partly because they are not of Hermitian type, and also because they are quotients of the Nadler group [22] of the quasi-split real form of Hodge type (see [9, Section 2.3] for the definition).

In this paper we are concentrating on type (1,,1)(1,...,1) very stable and even very stable upward flows. By now there are many interesting results about other types of very stable or wobbly Higgs bundles see e.g. [20] for multiplicity algebras of type (2)(2) very stable Higgs bundles, [6] for many wobbly Higgs bundles - both papers in this conference proceedings - and [25] for a classification of all type (n1,n2)(n_{1},n_{2}) very stable components.

Acknowledgements. Most of the research for this paper was done when the first author visited the second author’s group at IST Austria as a summer intern in 2022. The first author is grateful for the hospitality and support received during this stay. We thank Oscar García-Prada for engineering the internship, and for constant support. We also thank Andreas Čap, Mischa Elkner, Tim Henke, Nigel Hitchin, Friedrich Knop, Jakub Löwit, David Nadler, Ana Peón-Nieto, Kamil Rychlewicz and Anna Sisák for useful discussions. The second author was supported by an FWF grant “Geometry of the top of the nilpotent cone” number P 35847.

2 Bialynicki-Birula decomposition

In this section we first recall the definition of a semi-projective variety and then collect the basics of the Bialynicki-Birula decomposition associated to such a variety.

Definition 2.1.

Let XX be a normal complex quasi-projective variety equipped with a 𝕋:=×\mathbb{T}:=\mathbb{C}^{\times} action. XX is semi-projective if the fixed point locus X𝕋X^{\mathbb{T}} is projective, and for every xXx\in X there is a pX𝕋p\in X^{\mathbb{T}} such that limλ0λx=p\lim\limits_{\lambda\to 0}\lambda x=p.

The latter is to be understood as the existence of a 𝕋\mathbb{T}-equivariant morphism f:𝔸1Xf:\mathbb{A}^{1}\to X such that f(1)=xf(1)=x and f(0)=pf(0)=p. Semi-projective varieties are endowed with a stratification in affine subvarieties known as the Bialynicki-Birula decomposition [3], which we now recall. We refer to [14, Section 2] for further details.

Definition 2.2.

Let XX be a semi-projective variety and αX𝕋\alpha\in X^{\mathbb{T}}. The upward flow from α\alpha is defined to be

Wα+:={xX:limλ0λx=α}.W_{\alpha}^{+}:=\{x\in X:\lim\limits_{\lambda\to 0}\lambda x=\alpha\}.

Similarly, the downward flow from α\alpha is

Wα:={xX:limλλx=α}.W_{\alpha}^{-}:=\{x\in X:\lim\limits_{\lambda\to\infty}\lambda x=\alpha\}.

The Bialynicki-Birula partition is X=αX𝕋Wα+X=\bigsqcup_{\alpha\in X^{\mathbb{T}}}W_{\alpha}^{+}. The core of XX is defined to be 𝒞:=αX𝕋Wα\mathcal{C}:=\bigsqcup_{\alpha\in X^{\mathbb{T}}}W_{\alpha}^{-}.

Definition 2.3.

For a connected component of the fixed locus, Fπ0(X𝕋)F\in\pi_{0}(X^{\mathbb{T}}), we define its attractor as WF+:=αFWα+W^{+}_{F}:=\bigcup_{\alpha\in F}W_{\alpha}^{+}, and its repeller as WF:=αFWαW^{-}_{F}:=\bigcup_{\alpha\in F}W_{\alpha}^{-}. The Bialynicki-Birula decomposition is X=Fπ0(X𝕋)WF+X=\bigsqcup_{F\in\pi_{0}(X^{\mathbb{T}})}W_{F}^{+}.

Given a smooth fixed point αXs𝕋\alpha\in X^{s\mathbb{T}}, the 𝕋\mathbb{T}-action on XX induces a representation of 𝕋\mathbb{T} on the tangent space TαXT_{\alpha}X. We denote, for kk\in\mathbb{Z}, the weight space (TαX)kTαX(T_{\alpha}X)_{k}\subset T_{\alpha}X where λ𝕋\lambda\in\mathbb{T} acts via multiplication by λk\lambda^{k}. This leads to a decomposition TαX=k(TαX)kT_{\alpha}X=\bigoplus_{k\in\mathbb{Z}}(T_{\alpha}X)_{k} in weight spaces. We denote Tα+X:=k>0(TαX)kT_{\alpha}^{+}X:=\bigoplus_{k>0}(T_{\alpha}X)_{k} the positive part and TαX:=k<0(TαX)kT_{\alpha}^{-}X:=\bigoplus_{k<0}(T_{\alpha}X)_{k} the negative part. We have:

Proposition 2.4.

Given a smooth fixed point αXs𝕋\alpha\in X^{s\mathbb{T}}, the upward flow Wα+W_{\alpha}^{+} (resp. the downward flow WαW_{\alpha}^{-}) is a locally closed 𝕋\mathbb{T}-invariant subvariety of XX which is isomorphic to Tα+XT^{+}_{\alpha}X (resp. TαXT^{-}_{\alpha}X) as varieties with 𝕋\mathbb{T}-action.

The proof was originally given in [3] for smooth complete XX. A proof for the general case is given in [14, Proposition 2.1].

Finally, suppose further that XsX^{s} is equipped with a symplectic form ωΩ2(Xs)\omega\in\Omega^{2}(X^{s}) such that, for λ𝕋\lambda\in\mathbb{T}, we have λ(ω)=λω\lambda^{*}(\omega)=\lambda\omega. This supposition is motivated by the fact that the semi-projective variety we will be studying, the moduli space of semistable Higgs bundles, is endowed with such a form. Then, we have:

Proposition 2.5.

For a smooth point αXs𝕋\alpha\in X^{s\mathbb{T}}, the subspaces Tα+XT^{+}_{\alpha}X and Tα0X:=(TαX)0TαXT^{\leq 0}_{\alpha}X:=(T_{\alpha}X)_{0}\oplus T^{-}_{\alpha}X of TαXT_{\alpha}X are Lagrangian. Moreover, the subvarieties Wα+W_{\alpha}^{+} and WFαW_{F_{\alpha}}^{-} are also Lagrangian.

The proof is given in [14, Proposition 2.10]. The main idea is that, for v(TαX)kv\in(T_{\alpha}X)_{k} and w(TαX)lw\in(T_{\alpha}X)_{l}, we have

λω(v,w)=λ(ω)(v,w)=ω(λv,λw)=ω(λkv,λlw)=λk+lω(v,w),\lambda\omega(v,w)=\lambda^{*}(\omega)(v,w)=\omega(\lambda\cdot v,\lambda\cdot w)=\omega(\lambda^{k}v,\lambda^{l}w)=\lambda^{k+l}\omega(v,w),

so that ω(v,w)\omega(v,w) can only be nonzero in the situation k+l=1k+l=1, which does not happen if k,l>0k,l>0 or if k,l0k,l\leq 0.

Definition 2.6.

We say that αXs𝕋\alpha\in X^{s\mathbb{T}} is very stable if Wα+𝒞={α}W^{+}_{\alpha}\cap\mathcal{C}=\{\alpha\}.

This definition was introduced in [14, Definition 4.1], where it was proven [14, Lemma 4.4] that αXs𝕋\alpha\in X^{s\mathbb{T}} is very stable if and only if Wα+XW^{+}_{\alpha}\subset X is closed.

2.1 Lagrangian upward flows in {\mathcal{M}}

In this section we introduce Higgs bundles and show how the previous theory of Bialynicki-Birula applies to the moduli space of semistable Higgs bundles. For this, we fix a smooth projective curve CC over the complex numbers with genus g2g\geq 2 and canonical line bundle KK.

Definition 2.7.

A Higgs bundle is a pair (E,Φ)(E,\Phi) where EE is a holomorphic vector bundle over CC and ΦH0(C,End(E)K)\Phi\in H^{0}(C,\textnormal{End}(E)\otimes K).

Such an object can be defined in more generality for a real reductive Lie group GG [7, Definition 3.1], giving GG-Higgs bundles. The above definition is recovered by setting G=GLn()G=GL_{n}(\mathbb{C}) for n=rankEn=\operatorname{rank}E. Recall that a Higgs bundle (E,Φ)(E,\Phi) is stable if, for every nonzero proper vector subbundle FEF\subset E such that Φ(F)FK\Phi(F)\subseteq F\otimes K, we have

μ(F):=degFrankF<μ(E):=degErankE,\mu(F):=\frac{\deg F}{\operatorname{rank}F}<\mu(E):=\frac{\deg E}{\operatorname{rank}E},

and it is semistable if for the same subbundles we have μ(F)μ(E)\mu(F)\leq\mu(E). We denote by :=nd\mathcal{M}:=\mathcal{M}^{d}_{n} the moduli space of semistable Higgs bundles of fixed rank nn and degree dd. It was constructed via gauge theory in [18] and by algebraic geometric methods in [23, 27]. It is a normal [28] quasi-projective variety with a hyperkähler metric at its smooth points, which are the stable Higgs bundles. In particular, it has a symplectic structure ωΩ2(s)\omega\in\Omega^{2}(\mathcal{M}^{s}).

This space also carries a natural 𝕋\mathbb{T}-action defined by (E,Φ)(E,λΦ)(E,\Phi)\mapsto(E,\lambda\Phi) which turns it into a semi-projective variety and such that λ(ω)=λω\lambda^{*}(\omega)=\lambda\omega. Thus, the Bialynicki-Birula theory from the previous section applies. The fixed locus 𝕋\mathcal{M}^{\mathbb{T}} can be identified as follows. We have, for any λ𝕋\lambda\in\mathbb{T}, an isomorphism of vector bundles fλAut(E)f_{\lambda}\in\operatorname{Aut}(E) such that

Φfλ=fλ(λΦ).\Phi\circ f_{\lambda}=f_{\lambda}\circ(\lambda\Phi). (2.1)

In other words, we have an action of 𝕋\mathbb{T} on EE which is linear on each fiber. Hence we can decompose E=L0LkE=L_{0}\oplus\dots\oplus L_{k} into weight spaces, where fλ|Li=λwiIdLif_{\lambda}|_{L_{i}}=\lambda^{w_{i}}\cdot\text{Id}_{L_{i}}. The compatibility condition (2.1) shows that, if viLiv_{i}\in L_{i}, then fλ(λΦ(vi))=Φ(fλ(vi))=λwiΦ(vi)f_{\lambda}(\lambda\cdot\Phi(v_{i}))=\Phi(f_{\lambda}(v_{i}))=\lambda^{w_{i}}\Phi(v_{i}), thus fλ(Φ(vi))=λwi1Φ(vi)f_{\lambda}(\Phi(v_{i}))=\lambda^{w_{i}-1}\Phi(v_{i}). Hence, Φ\Phi maps the space for weight wiw_{i} into the space for weight wi1w_{i}-1. In particular, the weights can be chosen to be of the form wi=w0iw_{i}=w_{0}-i and the Higgs field has the property Φ(Li)Li+1K\Phi(L_{i})\subseteq L_{i+1}\otimes K. From this, we can associate an invariant (rankL0,,rankLk)(\operatorname{rank}L_{0},\dots,\operatorname{rank}L_{k}) to the fixed point, known as the type.

The previous decomposition shows that, in fact, a Higgs bundle fixed by the 𝕋\mathbb{T}-action is nilpotent, since Φk+10\Phi^{k+1}\equiv 0. Another way of seeing this is via the Hitchin map:

h:𝒜:=i=1nH0(C,Ki)h:\mathcal{M}\to\mathcal{A}:=\bigoplus_{i=1}^{n}H^{0}(C,K^{i})

defined by the coefficients aiH0(C,Ki)a_{i}\in H^{0}(C,K^{i}) of the characteristic polynomial det(ΦxIn)=xn+j=1najxnj\det(\Phi-xI_{n})=x^{n}+\sum_{j=1}^{n}a_{j}x^{n-j}. This map is a proper, completely integrable Hamiltonian system [17, 23] whose fibers are Lagrangian at their smooth points, and the generic fibers are abelian varieties [26]. Moreover, by letting 𝕋\mathbb{T} act on H0(C,Ki)H^{0}(C,K^{i}) with weight ii, the Hitchin map is 𝕋\mathbb{T}-equivariant. Thus, 𝕋h1(0)\mathcal{M}^{\mathbb{T}}\subseteq h^{-1}(0) so that fixed points (E,Φ)(E,\Phi) have characteristic polynomial xnx^{n} and are nilpotent.

The upward and downward flows from the Bialynicki-Birula partition have been characterized in [14, Proposition 3.4 and 3.11]:

Proposition 2.8.

Let =(E,Φ)s𝕋\mathcal{E}=(E^{\prime},\Phi^{\prime})\in\mathcal{M}^{s\mathbb{T}} and (E,Φ)(E,\Phi)\in\mathcal{M}. We have (E,Φ)W+(E^{\prime},\Phi^{\prime})\in W_{\mathcal{E}}^{+} if and only if there exists a filtration

0=E0E1Ek=E0=E_{0}\subset E_{1}\subset\dots\subset E_{k}=E

such that Φ(Ei)Ei+1K\Phi(E_{i})\subseteq E_{i+1}\otimes K and the associated graded object verifies (GrE,Gr(Φ))(E,Φ)(\textnormal{Gr}{E},\textnormal{Gr}(\Phi))\simeq(E^{\prime},\Phi^{\prime}). The same is true replacing W+W^{+}_{\mathcal{E}} with WW^{-}_{\mathcal{E}} and the ascending filtration with a descending filtration.

The downward flows have a concrete characterization via the Hitchin map. Since the action of 𝕋\mathbb{T} on 𝒜\mathcal{A} is by positive weights, the core is just 𝒞𝒜={0}\mathcal{C}_{\mathcal{A}}=\{0\}. Because hh is 𝕋\mathbb{T}-equivariant, this shows that 𝒞:=𝒞h1(0)\mathcal{C}:=\mathcal{C}_{\mathcal{M}}\subset h^{-1}(0). On the other hand, the properness of hh shows that h1(0)h^{-1}(0) is projective and thus 𝒞=h1(0)\mathcal{C}=h^{-1}(0). This is typically called the nilpotent cone in this context. Notice that 𝕋{\mathbb{T}}-equivariance of hh implies 𝕋𝒞\mathcal{M}^{{\mathbb{T}}}\subseteq\mathcal{C}. From this, the notion of being very stable becomes:

Definition 2.9.

A Higgs bundle =(E,Φ)s𝕋\mathcal{E}=(E,\Phi)\in\mathcal{M}^{s\mathbb{T}} is very stable if the only nilpotent Higgs bundle in W+W_{\mathcal{E}}^{+} is \mathcal{E} itself. Otherwise, it is wobbly.

One interesting aspect of such objects is that the Hitchin map restricts nicely to the upward flow [14, Lemma 4.6]:

Proposition 2.10.

If s𝕋\mathcal{E}\in\mathcal{M}^{s\mathbb{T}} is very stable then h:W+𝒜h:W^{+}_{\mathcal{E}}\to\mathcal{A} is finite, flat, surjective and generically étale.

2.2 Examples of very stable Higgs bundles

In this section we recall from [14] some examples of very stable Higgs bundles. First we consider the fixed point component of type (n)(n). The fixed points of this type are elements of the form (E,0)(E,0) with EE a semistable Higgs bundle. Thus, this component is just the moduli space of semistable rank nn degree dd vector bundles, 𝒩\mathcal{N}. The upward flow for =(E,0)\mathcal{E}=(E,0) is given by W+={(E,Φ):ΦH0(C,End(E)K)}W_{\mathcal{E}}^{+}=\{(E,\Phi):\Phi\in H^{0}(C,\textnormal{End}(E)\otimes K)\}, so that \mathcal{E} is very stable if and only if the only nilpotent Higgs field ΦH0(C,End(E)K)\Phi\in H^{0}(C,\textnormal{End}(E)\otimes K) it admits is Φ0\Phi\equiv 0. This is the notion of very stable vector bundle introduced by Drinfeld and Laumon [21], for which they prove that very stable bundles form an open dense subset of the component.

Next, we shall focus on the type (1,1,,1)(1,1,\dots,1) case. The starting example of very stable Higgs bundle in this component is the canonical uniformising Higgs bundle, 0=(E0,Φ0)\mathcal{E}_{0}=(E_{0},\Phi_{0}), where

E0=𝒪K1K1n,E_{0}=\mathcal{O}\oplus K^{-1}\oplus\dots\oplus K^{1-n},

and, given a=(a1,,an)𝒜=H0(C,K)H0(C,Kn)a=(a_{1},\dots,a_{n})\in\mathcal{A}=H^{0}(C,K)\oplus\dots\oplus H^{0}(C,K^{n}), the Higgs field

Φa=(000an100an1010an2001a1)\Phi_{a}=\begin{pmatrix}0&0&\dots&0&a_{n}\\ 1&0&\dots&0&a_{n-1}\\ 0&1&\dots&0&a_{n-2}\\ \vdots&\vdots&\ddots&\vdots&\vdots\\ 0&0&\dots&1&a_{1}\end{pmatrix}

is given by the companion matrix. The map a(E0,Φa)a\mapsto(E_{0},\Phi_{a}) provides a section of the Hitchin map, known as the Hitchin section [19]. By means of Proposition 2.8, it follows that {(E0,Φa):a𝒜}W0+\{(E_{0},\Phi_{a}):a\in\mathcal{A}\}\subseteq W^{+}_{{\mathcal{E}}_{0}}. Moreover, since both are affine spaces of equal dimension dim/2\dim\mathcal{M}/2, the upward flow is precisely the Hitchin section, hence 0{\mathcal{E}}_{0} is very stable.

It is possible to completely classify very stable Higgs bundles of this type by starting with this example and performing Hecke transformations. First we note that the data of a type (1,1,,1)(1,1,\dots,1) fixed point is equivalent to the choice of a line bundle L0L_{0} over CC (that is, a divisor δ0\delta_{0} up to principal divisor), as well as effective divisors δ1,,δn1\delta_{1},\dots,\delta_{n-1} on CC. Indeed, such a fixed point (E,Φ)(E,\Phi) is of the form E=L0Ln1E=L_{0}\oplus\dots\oplus L_{n-1}, where for all jj we have rankLj=1\operatorname{rank}L_{j}=1, and Φ|Lj1=bj1\Phi|_{L_{j-1}}=b_{j-1} for nonconstant maps bj:Lj1LjKb_{j}:L_{j-1}\to L_{j}\otimes K, 1jn11\leq j\leq n-1. Thus, L0L_{0} is given, and δi\delta_{i} is obtained as the zero locus of bib_{i} with multiplicities. On the other hand, given (δ0,δ1,,δn1)(\delta_{0},\delta_{1},\dots,\delta_{n-1}) we construct EE by setting Li:=L0𝒪(δ1++δi1)KiL_{i}:=L_{0}\otimes\mathcal{O}(\delta_{1}+\dots+\delta_{i-1})\otimes K^{-i} and bi:=sδi𝒪(δi)=𝒪(Lj1LjK)b_{i}:=s_{\delta_{i}}\in\mathcal{O}(\delta_{i})=\mathcal{O}(L_{j-1}^{*}\otimes L_{j}\otimes K) the canonical section. We shall denote the bundle corresponding to δ:=(δ0,,δn1)\delta:=(\delta_{0},\dots,\delta_{n-1}) by δ=(Eδ,Φδ)\mathcal{E}_{\delta}=(E_{\delta},\Phi_{\delta}).

Another convenient way of labelling these points is via choosing a dominant weight of GL(n,)\mathrm{GL}(n,\mathbb{C}) at each point of CC, that is, a map

μ:CΛ+(GL(n,))={i=1naiωi:a0n1×},\mu:C\to\Lambda^{+}(\mathrm{GL}(n,\mathbb{C}))=\left\{\sum_{i=1}^{n}a_{i}\omega_{i}:a\in\mathbb{Z}_{\geq 0}^{n-1}\times\mathbb{Z}\right\},

where the ωi\omega_{i} are the fundamental weights. We require that the set C{μ=0}C\setminus\{\mu=0\} is finite. We then define

δμ:=(cCμ(c),ωnc,(cCμ(c),ωic)i=1,,n1),\delta_{\mu}:=\left(\sum_{c\in C}\langle{\mu}(c),\omega_{n}^{\vee}\rangle c,\left(\sum_{c\in C}\langle{\mu}(c),\omega_{i}^{\vee}\rangle c\right)_{i=1,\dots,n-1}\right),

and μ:=δμ\mathcal{E}_{\mu}:=\mathcal{E}_{\delta_{\mu}}. Conversely, we can retrieve the map μ\mu from δ\delta as

μδ(c)=δ0(c)ωn+i=1n1δi(c)ωiΛ+,{\mu}_{\delta}(c)=\delta_{0}(c)\omega_{n}+\sum_{i=1}^{n-1}\delta_{i}(c)\omega_{i}\in\Lambda^{+},

where D(c)D(c) for a divisor DD means the coefficient of cc in DD.

2.3 Hecke transformations

Now we explain Hecke transformations for Higgs bundles. These play a key role since they allow to relate the upward flows of the different fixed points in the type (1,1,,1)(1,1,\dots,1) component. In order to define Hecke transformations of (E,Φ)(E,\Phi), we start by choosing a point cCc\in C and a subspace VGr(k,E|c)V\in\textnormal{Gr}(k,E|_{c}) which is Φ|c\Phi|_{c}-invariant, that is, Φ|c(V)VK|c\Phi|_{c}(V)\subset V\otimes K|_{c}. The Hecke transformation V(E,Φ):=(E,Φ)\mathcal{H}_{V}(E,\Phi):=(E^{\prime},\Phi^{\prime}) is defined by diagram

0EEE|c/V0ΦΦΦ¯c0EKEKE|c/VK0,\begin{array}[]{ccccccc}0\to&E^{\prime}&{\to}&E&{\to}&E|_{c}/V&\to 0\\ &\Phi^{\prime}\downarrow&&\Phi\downarrow&&\overline{\Phi}_{c}\downarrow&\\ 0\to&E^{\prime}\otimes K&\to&E\otimes K&\to&E|_{c}/V\otimes K&\to 0\end{array},

where E|c/VE|_{c}/V is to be regarded as a skyscraper sheaf at cc. More details of the construction of this diagram can be found in [14, Definition 4.10].

It is possible to reach any μ\mathcal{E}_{\mu} from successive Hecke transformations that start at 0\mathcal{E}_{0}. This is due to the following fundamental operation: starting with 0\mathcal{E}_{0} and selecting the natural invariant subspace Vk=(LkLn1)|cV_{k}=(L_{k}\oplus\dots\oplus L_{n-1})|_{c}, the resulting Hecke transformation gives μc,k\mathcal{E}_{\mu_{c,k}}, where μc,k(c)=ωk\mu_{c,k}(c)=\omega_{k} and zero otherwise. This is explained in [14, Example 4.13]. For arbitrary μ\mu it suffices to iterate the previous operation for every cCc\in C, at the ωk\omega_{k} indicated by μ(c)\mu(c). One of the main results of [14] is that the upward flows are also related by Hecke transformations, from which the following classification can be deduced:

Theorem 2.11 ([14, Theorem 4.16]).

A stable fixed point of type (1,1,,1)(1,1,\dots,1), (Eδ,Φδ)s𝕋(E_{\delta},\Phi_{\delta})\in\mathcal{M}^{s\mathbb{T}}, is very stable if and only if the divisor δ1++δn1\delta_{1}+\dots+\delta_{n-1} is reduced.

Remark 2.12.

The previous statement can be rephrased as (Eμ,Φμ)(E_{\mu},\Phi_{\mu}) being very stable if and only if for every cCc\in C, either μ(c)=anωn\mu(c)=a_{n}\omega_{n} or μ(c)=anωn+ωk\mu(c)=a_{n}\omega_{n}+\omega_{k} where k{1,,n1}k\in\{1,\dots,n-1\} and ana_{n}\in\mathbb{Z}. In other words, the point is very stable if and only if for every cCc\in C, the weight μ(c)\mu(c) is minuscule, that is, minimal with respect to the partial ordering in Λ+(GL(n,))\Lambda^{+}(\mathrm{GL}(n,\mathbb{C})) given by μ1μ2μ1μ2Φ+={αΔ+aαα:aα0}\mu_{1}\geq\mu_{2}\iff\mu_{1}-\mu_{2}\in\Phi^{+}=\{\sum_{\alpha\in\Delta^{+}}a_{\alpha}\alpha:a_{\alpha}\in\mathbb{Z}_{\geq 0}\}, where Δ+\Delta^{+} denotes the set of positive roots.

3 Even very stable upward flows

In this section we extend the results summarized above to the subspace θ\mathcal{M}^{\theta}\subset\mathcal{M} of the moduli space defined by the fixed points of the subgroup C2={1,1}𝕋C_{2}=\{1,-1\}\subseteq\mathbb{T}, acting as the involution θ:(E,Φ)(E,Φ)\theta:(E,\Phi)\mapsto(E,-\Phi). Clearly, this subspace contains all the fixed points by the 𝕋\mathbb{T}-action, so the previous concepts can be extended naturally. Moreover, by [9, Theorem 6.3], the space θ\mathcal{M}^{\theta} contains the images of the maps U(p,q)\mathcal{M}_{U(p,q)}\rightarrow\mathcal{M}, given by extension of structure group, of the moduli spaces of U(p,q)U(p,q)-Higgs bundles (for the different U(p,q)U(p,q) with p+q=np+q=n, pqp\leq q) into the moduli space of GL(n,)\mathrm{GL}(n,\mathbb{C})-Higgs bundles. The stable locus θ,s\mathcal{M}^{\theta,s} is covered by these images, which are the Higgs bundles that we will consider.

We start by recalling the following definition from [4, Definition 3.3].

Definition 3.1.

A U(p,q)U(p,q)-Higgs bundle (E,Φ)(E,\Phi) is a holomorphic vector bundle EE of the form E=VWE=V\oplus W, where VV and WW are vector bundles of ranks pp and qq, respectively, and ΦH0(End(E)K)\Phi\in H^{0}(\textnormal{End}(E)\otimes K) is a section satisfying Φ(V)WK\Phi(V)\subset W\otimes K, Φ(W)VK\Phi(W)\subset V\otimes K.

We denote by U(p,q)s\mathcal{M}^{s}_{U(p,q)} the moduli space of stable U(p,q)U(p,q)-Higgs bundles, where stability is defined as for GL(n,)\mathrm{GL}(n,\mathbb{C})-Higgs bundles. As explained before, this space sits inside \mathcal{M} as the fixed point locus of the involution θ\theta, that is, a stable Higgs bundle (E,Φ)(E,\Phi) is a U(p,q)U(p,q)-Higgs bundle (for some pp and qq) if and only if (E,Φ)(E,Φ)(E,\Phi)\simeq(E,-\Phi) [9, Theorem 6.3]. We will often use interchangeably the moduli space U(p,q)\mathcal{M}_{U(p,q)} and its image inside \mathcal{M}.

Note that every fixed point =(E,Φ)\mathcal{E}=(E,\Phi) of the 𝕋\mathbb{T}-action is in particular fixed by 1-1 and hence a U(p,q)U(p,q)-Higgs bundle for some pp and qq. This can be seen more explicitly by observing that, in the decomposition E=E0Ek1E=E_{0}\oplus\dots\oplus E_{k-1} with Φ(Ei)Ei+1K\Phi(E_{i})\subset E_{i+1}\otimes K, the Higgs field Φ\Phi interchanges the summands with odd indices by those of even indices. In particular, type (1,1,,1)(1,1,\dots,1) fixed points are Higgs bundles for the quasi-split group U(p,p)U(p,p) or U(p,p+1)U(p,p+1).

Moreover, recall from Białynicki-Birula theory in Section 2 that the upward flow W+W^{+}_{\mathcal{E}} is an affine space isomorphic to the subspace of positive weights T+TT^{+}_{\mathcal{E}}\mathcal{M}\subset T_{\mathcal{E}}\mathcal{M}. It is easy to identify the subspace of U(p,q)U(p,q)-Higgs bundles.

Remark 3.2.

The U(p,q)U(p,q)-Higgs bundles in W+W^{+}_{\mathcal{E}}, that is, U(p,q)W+\mathcal{M}_{U(p,q)}\cap W^{+}_{\mathcal{E}}, correspond via the isomorphism W+T+W^{+}_{\mathcal{E}}\simeq T^{+}_{\mathcal{E}}\mathcal{M} to the vector subspace of positive, even weights T2+TT^{2+}_{\mathcal{E}}\mathcal{M}\subset T_{\mathcal{E}}\mathcal{M}.

This is because the even weights are precisely the vector subspace fixed by multiplication by 1-1, and the previous isomorphism is 𝕋\mathbb{T}-equivariant. In other words, we can view the locus of U(p,q)U(p,q)-Higgs bundles at the upward flow of a fixed point as a subspace:

Definition 3.3.

The even upward flow at \mathcal{E} is the subspace of W+W^{+}_{\mathcal{E}} corresponding to T2+T^{2+}_{\mathcal{E}}\mathcal{M} and is denoted by W2+W^{2+}_{\mathcal{E}}.

Note that this coincides with the standard upward flow when defined in θ\mathcal{M}^{\theta} instead of \mathcal{M}. Hence, we also have the following natural definition of very stable points:

Definition 3.4.

We say that \mathcal{E} is even very stable if W2+𝒞={}W^{2+}_{\mathcal{E}}\cap\mathcal{C}=\{\mathcal{E}\}, where 𝒞=h1(0)\mathcal{C}=h^{-1}(0)\subseteq\mathcal{M} denotes the locus of nilpotent Higgs bundles. Otherwise, it is said to be even wobbly.

We remark, as one of the main interests for this study, that the subspaces of even weights T2TT^{2}_{\mathcal{E}}\mathcal{M}\subset T_{\mathcal{E}}\mathcal{M} that we are considering are Lagrangian, since the symplectic form ω\omega pairs the subspace of weight kk with that of 1k1-k, as explained at the end of Section 2, so that the subspaces of even weights are paired with those of odd weights. In fact, the subvariety θ\mathcal{M}^{\theta}\subset\mathcal{M} itself is Lagrangian, as explained in [9, Theorem 8.10].

Obviously, a very stable fixed point is also even very stable. However, a wobbly fixed point \mathcal{E} can either remain even wobbly or instead be even very stable, depending on whether the nontrivial intersection (W+𝒞){}(W^{+}_{\mathcal{E}}\cap\mathcal{C})\setminus\{\mathcal{E}\} happens at even weights or not. We will classify the even very stable Higgs bundles of type (1,1,,1)(1,1,\dots,1), revealing that both situations already arise in this case. We follow the same notation of Subsection 2.2.

Proposition 3.5.

Let =(E,Φ)\mathcal{E}=(E,\Phi) be a smooth fixed point of type (1,1,,1)(1,1,\dots,1) . Suppose that there is some point cCc\in C such that bi(c)=bj(c)=0b_{i}(c)=b_{j}(c)=0 for some i,ji,j of different parity. Then \mathcal{E} is even wobbly.

Proof. The proof follows the approach of constructing a curve via Hecke transformations followed in the proof of [14, Theorem 4.16]. We will see that, in this situation, the curve can be constructed along even weights. We have that bk(c)=bk+l(c)=0b_{k}(c)=b_{k+l}(c)=0 where l>0l>0 and odd. We start by performing a Hecke transformation at the Φc\Phi_{c}-invariant subspace (L0Lk1)|cE|c(L_{0}\oplus\dots\oplus L_{k-1})|_{c}\subset E|_{c}, yielding

E=L0Lk1Lk(c)Ln1(c),E^{\prime}=L_{0}\oplus\dots\oplus L_{k-1}\oplus L_{k}(-c)\oplus\dots\oplus L_{n-1}(-c),
Φ=(00000b100000b200000bksc00000bn10),\Phi^{\prime}=\begin{pmatrix}0&0&\dots&0&\dots&0&0\\ b_{1}&0&\dots&0&\dots&0&0\\ 0&b_{2}&\dots&0&\dots&0&0\\ \vdots&\vdots&\ddots&\vdots&\ddots&\vdots&\vdots\\ 0&0&\dots&\frac{b_{k}}{s_{c}}&\dots&0&0\\ \vdots&\vdots&\ddots&\vdots&\ddots&\vdots&\vdots\\ 0&0&\dots&0&\dots&b_{n-1}&0\end{pmatrix},

where scH0(𝒪(c))s_{c}\in H^{0}(\mathcal{O}(c)) is the canonical section. This bundle is still stable [14, Lemma 4.17]. We have that V0=(Lk(c)Ln1(c))|cE|cV_{0}=(L_{k}(-c)\oplus\dots\oplus L_{n-1}(-c))|_{c}\subset E^{\prime}|_{c} is the (nk)(n-k)-dimensional Φc\Phi^{\prime}_{c}-invariant subspace that transforms (E,Φ)(E^{\prime},\Phi^{\prime}) back into (E(c),Φ)(E(-c),\Phi). Now let {v0,,vn1}\{v_{0},\dots,v_{n-1}\} be a basis of E|cE^{\prime}|_{c}, each vjv_{j} taken in the corresponding component. We define the following (nk)(n-k)-dimensional subspace:

V:=vk1+vk+l,vk,vk+1,,vk+l1,vk+l+1,vn1E|cV:=\left<v_{k-1}+v_{k+l},v_{k},v_{k+1},\dots,v_{k+l-1},v_{k+l+1},v_{n-1}\right>\subset E^{\prime}|_{c}

This is another Φc\Phi^{\prime}_{c}-invariant subspace, since Φc(vk1+vk+l)vk,vk+l+1\Phi^{\prime}_{c}(v_{k-1}+v_{k+l})\in\left<v_{k},v_{k+l+1}\right>, Φc(vm)vm+1\Phi^{\prime}_{c}(v_{m})\in\left<v_{m+1}\right> for m{k,,k+l2}{k+l+1,,n1}m\in\{k,\dots,k+l-2\}\cup\{k+l+1,\dots,n-1\}, and Φc(vk+l1)=0\Phi^{\prime}_{c}(v_{k+l-1})=0 (in this analysis we take vj=0v_{j}=0 for any j>n1j>n-1). Now, recall that there is an induced 𝕋\mathbb{T}-action on Grnk(E|c)Gr_{n-k}(E^{\prime}|_{c}) given by the 𝕋\mathbb{T}-action on EE^{\prime} with weight i-i on the ii-th summand of EE^{\prime}. With this, given λ𝕋\lambda\in\mathbb{T} we define Vλ:=λVV_{\lambda}:=\lambda V, that is:

Vλ=λl+1vk1+vk+l,vk,vk+1,,vk+l1,vk+l+1,vn1.V_{\lambda}=\left<\lambda^{l+1}v_{k-1}+v_{k+l},v_{k},v_{k+1},\dots,v_{k+l-1},v_{k+l+1},v_{n-1}\right>.

Note that this subspace is always nkn-k dimensional. This yields a curve within the connected subvariety Snk(Φ|c)Grnk(E|c)S_{n-k}(\Phi^{\prime}|_{c})\subset Gr_{n-k}(E^{\prime}|_{c}) of vector subspaces of the fiber E|cE^{\prime}|_{c} which are invariant by Φ|c\Phi^{\prime}|_{c}. As argued in the proof of [14, Theorem 4.16], this translates into a curve in the moduli space of Higgs bundles, defined by Vλ(E,Φ)λV(E,Φ)\mathcal{H}_{V_{\lambda}}(E^{\prime},\Phi^{\prime})\simeq\lambda\mathcal{H}_{V}(E^{\prime},\Phi^{\prime}). This curve connects V0(E,Φ)=(E(c),Φ)\mathcal{H}_{V_{0}}(E^{\prime},\Phi^{\prime})=(E(-c),\Phi) with a different fixed point, given by V(E,Φ)\mathcal{H}_{V_{\infty}}(E^{\prime},\Phi^{\prime}), where V=vk1,vk,vk+1,,vk+l1,vk+l+1,vn1V_{\infty}=\left<v_{k-1},v_{k},v_{k+1},\dots,v_{k+l-1},v_{k+l+1},v_{n-1}\right>. This fixed point is also stable [14, Lemma 4.18].

Moreover, since ll is odd, then l+1l+1 is even and we have that Vλ=VλV_{\lambda}=V_{-\lambda}, hence λV(E,Φ)λV(E,Φ)\lambda\mathcal{H}_{V}(E^{\prime},\Phi^{\prime})\simeq-\lambda\mathcal{H}_{V}(E^{\prime},\Phi^{\prime}) so that this curve is fixed by the action of 1-1 and hence it lies in W(E(c),Φ)2+W^{2+}_{(E(-c),\Phi)}. This shows that (E(c),Φ)(E(-c),\Phi) is even wobbly thus (E,Φ)(E,\Phi) as well. ∎

There are still more examples of even wobbly stable Higgs bundles of type (1,1,,1)(1,1,\dots,1), which are covered by the following proposition.

Proposition 3.6.

Let =(E,Φ)\mathcal{E}=(E,\Phi) be a smooth fixed point of rank n4n\geq 4. Suppose that b:=bn2b2b:=b_{n-2}\circ\dots\circ b_{2} has a multiple zero at cCc\in C. Then \mathcal{E} is even wobbly.

Proof. The proof is identical to that of Proposition 3.5, with the only difference being the construction of the invariant subspace VSnk(Φ|c)V\in S_{n-k}(\Phi^{\prime}|_{c}).

Let 1<i1<i2<<im<n11<i_{1}<i_{2}<\dots<i_{m}<n-1 be all the indices other than 11 and n1n-1 such that bik(c)=0b_{i_{k}}(c)=0. We can assume that all of them are of the same parity since otherwise we apply the previous proposition. We start again with a Hecke transform at (L0L1Lim1)|c(L_{0}\oplus L_{1}\dots\oplus L_{i_{m}-1})|_{c}. This yields (E,Φ)(E^{\prime},\Phi^{\prime}) with the same form as in the proof of Proposition 3.5.

Now we will construct a basis {v0,v1,,vn1}\{v_{0},v_{1},\dots,v_{n-1}\} of E|cE^{\prime}|_{c} as follows. We start with any nonzero v0L0|cv_{0}\in L_{0}^{\prime}|_{c}, then apply Φ|c\Phi^{\prime}|_{c} until a zero vector is obtained. This will produce a string: v1=Φ|c(v0)v_{1}=\Phi^{\prime}|_{c}(v_{0}), v2=Φ|c(v1)v_{2}=\Phi^{\prime}|_{c}(v_{1})\dots all the way up to vi11v_{i_{1}-1}, if b1(c)0b_{1}(c)\neq 0, or just v0v_{0} if b1(c)=0b_{1}(c)=0. The process then iterates: we pick vi1v_{i_{1}} (or v1v_{1} if b1(c)=0b_{1}(c)=0) nonzero in the corresponding summand and iterate, repeating until vn1v_{n-1}. By construction, the basis is partitioned in strings inside of which each element maps to the next one and the last one maps to zero. Also, each viv_{i} is in the corresponding summand Li|cL^{\prime}_{i}|_{c}. Let V0=vim,,vn1V_{0}=\left<v_{i_{m}},\dots,v_{n-1}\right>.

Now recall that im<n1i_{m}<n-1 and i12i_{1}\geq 2. Note that if m=1m=1, it is possible that i1=imi_{1}=i_{m}, meaning a multiple zero of bi1b_{i_{1}} at cc. In any case, we define the following (nim)(n-i_{m})-dimensional subspace:

V=vim+vi12,vim+1+vi11,vim+2,,vim+i11,vim+i1,,vn1.V=\left<v_{i_{m}}+v_{i_{1}-2},v_{i_{m}+1}+v_{i_{1}-1},v_{i_{m}+2},\dots,v_{i_{m}+i_{1}-1},v_{i_{m}+i_{1}},\dots,v_{n-1}\right>.

It is Φ|c\Phi^{\prime}|_{c}-invariant: each generator is taken to the next, and the last one to zero. Notice that it is important that im<n1i_{m}<n-1 since otherwise we get a 11-dimensional space that does not work, for vim+vi12vi11\left<v_{i_{m}}+v_{i_{1}-2}\right>\mapsto\left<v_{i_{1}-1}\right>. Also notice that if bn1(c)=0b_{n-1}(c)=0 then the second generator might map to zero instead of vim+2v_{i_{m}+2}, but this is not a problem for the invariance. We compute λV\lambda V:

V=vim+λimi1+2vi12,vim+1+λimi1+2vi11,vim+2,,vim+i11,vim+i1,,vn1.V=\left<v_{i_{m}}+\lambda^{i_{m}-i_{1}+2}v_{i_{1}-2},v_{i_{m}+1}+\lambda^{i_{m}-i_{1}+2}v_{i_{1}-1},v_{i_{m}+2},\dots,v_{i_{m}+i_{1}-1},v_{i_{m}+i_{1}},\dots,v_{n-1}\right>.

Once again this gives a curve in Snk(Φ|c)S_{n-k}(\Phi^{\prime}|_{c}) connecting V0V_{0} with a different VV_{\infty} such that the Hecke transform is a new fixed point and, since imi1+2i_{m}-i_{1}+2 is even, it follows that λV=λV\lambda V=-\lambda V, as desired. ∎

We now prove that these constitute all even wobbly cases.

Proposition 3.7.

Let δ=(E,Φ)\mathcal{E}_{\delta}=(E,\Phi) be a smooth fixed point of type (1,1,,1)(1,1,\dots,1). Suppose that for every cCc\in C we have that bi(c)=bj(c)=0b_{i}(c)=b_{j}(c)=0 implies ijmod2i\equiv j\mod 2, and bn2b2b_{n-2}\circ\dots\circ b_{2} has at most a single zero at cc. Then, \mathcal{E} is even very stable.

Proof. We argue by induction on deg(δn1++δ1)\deg(\delta_{n-1}+\dots+\delta_{1}), as we already know from Section 2.2 that the degree 0 case, which is the canonical uniformising Higgs bundle, is even very stable. Suppose that (E,Φ)W+𝒞(E^{\prime},\Phi^{\prime})\in W^{+}_{\mathcal{E}}\cap\mathcal{C} is a nilpotent element in the upward flow of \mathcal{E}, with the full filtration

0=W0W1Wn1Wn=E0=W_{0}\subset W_{1}\subset\dots\subset W_{n-1}\subset W_{n}=E^{\prime}

given by Proposition 2.8. Take one of the points cCc\in C with μδ(c)0\mu_{\delta}(c)\neq 0, and suppose first that bn1(c)=0b_{n-1}(c)=0. This means that V:=(Wn1)|cV^{\prime}:=(W_{n-1})|_{c} is Φ|c\Phi^{\prime}|_{c}-invariant, and, as explained in [14, Section 4], the Hecke transformation (E1,Φ1)=V(E,Φ)(E^{\prime}_{1},\Phi^{\prime}_{1})=\mathcal{H}_{V^{\prime}}(E^{\prime},\Phi^{\prime}) is stable, nilpotent and lies in the upward flow of (E1,Φ1):=V(E,Φ)(E_{1},\Phi_{1}):=\mathcal{H}_{V}(E,\Phi), where V=(L0Ln2)|cE|cV=(L_{0}\oplus\dots\oplus L_{n-2})|_{c}\subseteq E|_{c}. We have that (E1,Φ1)(E_{1},\Phi_{1}) is another type (1,1,,1)(1,1,\dots,1) point given by δ1=(δ01,,δn11)\delta^{1}=(\delta_{0}^{1},\dots,\delta_{n-1}^{1}) with the only difference being that δn11=δn1c\delta_{n-1}^{1}=\delta_{n-1}-c. Thus, by the induction hypothesis it follows that (E1,Φ1)(E_{1},\Phi_{1}) is even very stable, which results in the following two options:

  • If (E1,Φ1)≄(E1,Φ1)(E_{1}^{\prime},\Phi_{1}^{\prime})\not\simeq(E_{1},\Phi_{1}), since the latter is even very stable, we have that (E1,Φ1)(E_{1}^{\prime},\Phi_{1}^{\prime}) lies in an odd weight space of T(E1,Φ1)T_{(E_{1},\Phi_{1})}\mathcal{M} and, by using the invariant subspaces V1E1|cV_{1}^{\prime}\subseteq E_{1}^{\prime}|_{c} and V1E1|cV_{1}\subseteq E_{1}|_{c} such that V1(E1,Φ1)=(E,Φ)\mathcal{H}_{V_{1}^{\prime}}(E_{1}^{\prime},\Phi_{1}^{\prime})=(E^{\prime},\Phi^{\prime}) and V1(E1,Φ1)=(E,Φ)\mathcal{H}_{V_{1}}(E_{1},\Phi_{1})=(E,\Phi) (up to twisting by a fixed line bundle), it follows that (E,Φ)(E^{\prime},\Phi^{\prime}) also has odd weight in the upward flow for (E,Φ)(E,\Phi) and hence (E,Φ)Wδ2+(E^{\prime},\Phi^{\prime})\notin W_{\mathcal{E}_{\delta}}^{2+}.

  • If (E1,Φ1)(E1,Φ1)(E_{1}^{\prime},\Phi_{1}^{\prime})\simeq(E_{1},\Phi_{1}), then the one dimensional subspace V1E1|cV_{1}^{\prime}\subseteq E_{1}^{\prime}|_{c} such that V1(E1,Φ1)=(E,Φ)\mathcal{H}_{V_{1}^{\prime}}(E_{1}^{\prime},\Phi_{1}^{\prime})=(E^{\prime},\Phi^{\prime}) is one of the Φ1|c\Phi_{1}|_{c}-invariant subspaces in the pair (E1,Φ1)(E_{1},\Phi_{1}), which we know well since it comes from a Hecke transformation of the starting (E,Φ)(E,\Phi). Indeed, we have:

    E1=L0Ln2Ln1(c),E_{1}=L_{0}\oplus\dots\oplus L_{n-2}\oplus L_{n-1}(-c),
    Φ1=(00000b100000b200000bn200000bn1sc0).\Phi_{1}=\begin{pmatrix}0&0&\dots&0&0&0\\ b_{1}&0&\dots&0&0&0\\ 0&b_{2}&\dots&0&0&0\\ \vdots&\vdots&\ddots&\vdots&\vdots&\vdots\\ 0&0&\dots&b_{n-2}&0&0\\ 0&0&\dots&0&\frac{b_{n-1}}{s_{c}}&0\end{pmatrix}.

    Let V={v0,,vn1}V=\{v_{0},\dots,v_{n-1}\} be a basis of E1|cE_{1}|_{c}. From the starting hypotheses about (E,Φ)(E,\Phi), the only basis vectors that could vanish via Φ1|c\Phi_{1}|_{c} are {v0,vj1,vn2,vn1}\{v_{0},v_{j-1},v_{n-2},v_{n-1}\} where jj is the only index with 2jn22\leq j\leq n-2 such that bj(c)=0b_{j}(c)=0, if it exists. Necessarily, jn1mod2j\equiv n-1\mod 2. Also, if v0v_{0} vanishes then b1(c)=0b_{1}(c)=0 and hence n0mod2n\equiv 0\mod 2. Finally, vn2v_{n-2} vanishes if and only if bn1b_{n-1} had a multiple zero at cc.

    Since Φ1\Phi_{1} is nilpotent, the desired invariant 11-dimensional subspace must be of the form V1=vV_{1}^{\prime}=\left<v\right> where Φ1|c(v)=0\Phi_{1}|_{c}(v)=0, that is, v=αv0+βvj1+γvn2+δvn1v=\alpha v_{0}+\beta v_{j-1}+\gamma v_{n-2}+\delta v_{n-1}. Moreover,

    λV1=αλn1v0+βλnjvj1+γλvn2+δvn1\lambda\cdot V_{1}^{\prime}=\left<\alpha\lambda^{n-1}v_{0}+\beta\lambda^{n-j}v_{j-1}+\gamma\lambda v_{n-2}+\delta v_{n-1}\right>

    must verify that limλ0λV1=V1=vn1\lim\limits_{\lambda\to 0}\lambda V_{1}^{\prime}=V_{1}=\left<v_{n-1}\right>, which implies that δ0\delta\neq 0. Hence, because of the parity of the exponents of λ\lambda appearing in the expression for λV1\lambda\cdot V_{1}^{\prime}, if (E,Φ)=V1(E1,Φ1)(E^{\prime},\Phi^{\prime})=\mathcal{H}_{V_{1}^{\prime}}(E_{1}^{\prime},\Phi_{1}^{\prime}) were in an even weight space, that is, if λV1=λV1\lambda\cdot V_{1}^{\prime}=-\lambda\cdot V_{1}^{\prime}, it would be necessary that α=β=γ=0\alpha=\beta=\gamma=0, thus V1=V1V_{1}^{\prime}=V_{1}, meaning (E,Φ)(E,Φ)(E^{\prime},\Phi^{\prime})\simeq(E,\Phi).

This concludes the analysis for the bn1(c)=0b_{n-1}(c)=0 case. Now, if bn1(c)0b_{n-1}(c)\neq 0, we may also assume that b1(c)0b_{1}(c)\neq 0. This is because the involution (E,Φ)(E,Φt)(E,\Phi)\mapsto(E^{*},\Phi^{t}) of \mathcal{M} naturally bijects fixed points and upward flows, sending a point with b1(c)=0b_{1}(c)=0 to a point with bn1(c)=0b_{n-1}(c)=0. Hence, the remaining case is when the only bj(c)=0b_{j}(c)=0 happens at a single jj with 2jn22\leq j\leq n-2 and multiplicity one. This case is treated exactly as in the proof of [14, Theorem 4.16], which we now recall.

We have the Φ|c\Phi^{\prime}|_{c}-invariant jj-dimensional subspace V:=(Wj1)|cV^{\prime}:=(W_{j-1})|_{c} giving a nilpotent (E1,Φ1)=V(E,Φ)(E_{1}^{\prime},\Phi_{1}^{\prime})=\mathcal{H}_{V^{\prime}}(E^{\prime},\Phi^{\prime}) in the upward flow of (E1,Φ1)=(E1,Φ1):=V(E,Φ)(E_{1},\Phi_{1})=(E_{1},\Phi_{1}):=\mathcal{H}_{V}(E,\Phi), where V=(L0Lj1)|cE|cV=(L_{0}\oplus\dots\oplus L_{j-1})|_{c}\subseteq E|_{c}. Exactly as before, if (E1,Φ1)≄(E1,Φ1)(E_{1}^{\prime},\Phi_{1}^{\prime})\not\simeq(E_{1},\Phi_{1}), the induction hypothesis gives (E,Φ)Wδ2+(E^{\prime},\Phi^{\prime})\notin W_{\mathcal{E}_{\delta}}^{2+}. Otherwise, notice that Φ1|c\Phi_{1}^{\prime}|_{c} is now a regular nilpotent, so the only Φ1|c\Phi_{1}^{\prime}|_{c}-invariant (nj)(n-j)-dimensional subspace is V1=V1=(LjLn1)|cV_{1}^{\prime}=V_{1}=(L_{j}\oplus\dots\oplus L_{n-1})|_{c}. Hence (up to tensoring everything by a fixed line bundle) we have (E,Φ)=V1(E1,Φ1)=(E,Φ)(E^{\prime},\Phi^{\prime})=\mathcal{H}_{V_{1}}(E_{1},\Phi_{1})=(E,\Phi). ∎

3.1 Even minuscule weights in GL(n,)\mathrm{GL}(n,\mathbb{C})

We will now see how the conditions found before arise naturally in the context of the root system of the structure group GL(n,)\mathrm{GL}(n,\mathbb{C}) of EE. We have ω1,,ωn1,ωnΛ+\omega_{1},\dots,\omega_{n-1},\omega_{n}\in\Lambda^{+} the fundamental weights. Recall that the height of a root is the number of simple roots in its decomposition. In terms of the fundamental weights the positive roots of height k{1,,n1}k\in\{1,\dots,n-1\} can be indexed by p{1,,nk}p\in\{1,\dots,n-k\} and given by:

αk,p:=ωp1+ωp+ωp+k1ωp+k,\alpha_{k,p}:=-\omega_{p-1}+\omega_{p}+\omega_{p+k-1}-\omega_{p+k},

where ω0\omega_{0} is understood as 0. In particular, the simple roots are the positive roots of height 11 of the form α1,p=ωp1+2ωpωp+1\alpha_{1,p}=-\omega_{p-1}+2\omega_{p}-\omega_{p+1} for p=1,,n1p=1,\dots,n-1. The highest root αn1,1=ω1+ωn1ωn\alpha_{n-1,1}=\omega_{1}+\omega_{n-1}-\omega_{n} has height n1n-1.

Definition 3.8.

For dominant weights λ,μ\lambda,\mu, we define the even partial ordering as

λ2μλμΦ2+,\lambda\geq_{2}\mu\iff\lambda-\mu\in\Phi^{2+},

where

Φ2+={k even,1pnkck,pαk,p:ck,p0}\Phi^{2+}=\left\{\sum_{\begin{subarray}{c}k\text{ even,}\\ 1\leq p\leq n-k\end{subarray}}c_{k,p}\alpha_{k,p}:c_{k,p}\in\mathbb{Z}_{\geq 0}\right\}

is the set of positive linear combinations of even positive roots. Minimal elements for this ordering are called even minuscule.

We will say for a weight λ\lambda that its ii-th coordinate/entry, λi\lambda_{i}, is the coefficient of ωi\omega_{i} when λ\lambda is written in the basis {ω1,,ωn}\{\omega_{1},\dots,\omega_{n}\}. The position of the ii-th coordinate will be just ii. Now we will characterize the even minuscule weights, seeing that the conditions exactly match those for even very stable Higgs bundles. The characterization will be carried out solely via combinatorial arguments.

Proposition 3.9.

Let λ\lambda be a dominant weight such that at least one of these holds:

  1. 1.

    The weight λ\lambda has nonzero coordinates at two positions 1i<jn11\leq i<j\leq n-1 with ijmod2i\not\equiv j\mod 2.

  2. 2.

    The weight λ\lambda verifies λ2++λn22\lambda_{2}+\dots+\lambda_{n-2}\geq 2.

Then λ\lambda is not even minuscule.

Proof. For the first situation, if λ\lambda has nonzero coordinates at ii and jj, where ji:=kj-i:=k is an odd positive number, then consider μ:=λαi,k+1\mu:=\lambda-\alpha_{i,k+1}. Because of the nonzero coordinates at ii and jj it follows that μ\mu is dominant. By construction, μ<λ\mu<\lambda.

If λ2++λn22\lambda_{2}+\dots+\lambda_{n-2}\geq 2, choose indices i,ji,j such that 2ijn22\leq i\leq j\leq n-2 with either iji\neq j and λi,λj1\lambda_{i},\lambda_{j}\geq 1, or i=ji=j and λi2\lambda_{i}\geq 2. We can assume the positions are of the same parity, since otherwise we apply the previous. Hence write k:=jik:=j-i a nonnegative even number. Defining μ:=λ(αk+2,i+αk+2,i1)\mu:=\lambda-(\alpha_{k+2,i}+\alpha_{k+2,i-1}) works as before, since αk+2,i+αk+2,i1=ωi1+ωi+ωj+1ωj+2ωi2+ωi1+ωjωj+1=ωi2+ωi+ωjωj+2\alpha_{k+2,i}+\alpha_{k+2,i-1}=-\omega_{i-1}+\omega_{i}+\omega_{j+1}-\omega_{j+2}-\omega_{i-2}+\omega_{i-1}+\omega_{j}-\omega_{j+1}=-\omega_{i-2}+\omega_{i}+\omega_{j}-\omega_{j+2}. ∎

Remark 3.10.

Notice in the last part of the previous proof that 2i,jn22\leq i,j\leq n-2 is indeed required: for example, if i=1i=1 we cannot take p=i1=0p=i-1=0. Similarly we need for αk+2,i\alpha_{k+2,i} to make sense that in(k2)=nk+2i\leq n-(k-2)=n-k+2 which is equivalent to jn2j\leq n-2.

As an example for the proof, take n=9n=9 and λ=(0,1,0,0,0,1,0,0,0)\lambda=(0,1,0,0,0,1,0,0,0). Following the proof, we can consider α6,2+α6,1=(1,1,0,0,0,0,1,1,0)+(1,0,0,0,0,1,1,0,0)=(0,1,0,0,0,1,0,1,0)\alpha_{6,2}+\alpha_{6,1}=(-1,1,0,0,0,0,1,-1,0)+(1,0,0,0,0,1,-1,0,0)=(0,1,0,0,0,1,0,-1,0), so that μ=(0,0,0,0,0,0,0,1,0)\mu=(0,0,0,0,0,0,0,1,0) is lower than λ\lambda.

For the reciprocal, the combinatorial arguments will be easier if we stop considering ω0\omega_{0} as zero and rather see it as an extra linearly independent vector. That is, we view the weight space W:=ω1,,ωn1,ωnW:=\left<\omega_{1},\dots,\omega_{n-1},\omega_{n}\right> as a subspace of a new vector space W~:=ω0,ω1,,ωn1,ωn\widetilde{W}:=\left<\omega_{0},\omega_{1},\dots,\omega_{n-1},\omega_{n}\right> which is a dimension higher. We have a projection π:W~W\pi:\widetilde{W}\to W. We define α~k,p:=ωp1+ωp+ωp+k1ωp+k\widetilde{\alpha}_{k,p}:=-\omega_{p-1}+\omega_{p}+\omega_{p+k-1}-\omega_{p+k} as before but in W~\widetilde{W} (i.e. we do not consider ω0=0\omega_{0}=0 in that expression anymore), so that π(α~k,p)=αk,p\pi(\widetilde{\alpha}_{k,p})={\alpha}_{k,p}. We also lift the even positive lattice as:

Φ~2+={k even,1pnkck,pα~k,p:ck,p0},\widetilde{\Phi}^{2+}=\left\{\sum_{\begin{subarray}{c}k\text{ even,}\\ 1\leq p\leq n-k\end{subarray}}c_{k,p}\widetilde{\alpha}_{k,p}:c_{k,p}\in\mathbb{Z}_{\geq 0}\right\},

so that π(Φ~2+)=Φ2+\pi(\widetilde{\Phi}^{2+})=\Phi^{2+}.

For example, in this new vector space the simple positive roots have the following lifts: α~1=(1,2,1,0,0,)\widetilde{\alpha}_{1}=(-1,2,-1,0,0,\dots), α~2=(0,1,2,1,0,0,)\widetilde{\alpha}_{2}=(0,-1,2,-1,0,0,\dots) etcetera. As can be seen, this avoids the situation of the negative coordinate being truncated at the beginning. In this setting we have the following facts about Φ~2+\widetilde{\Phi}^{2+}, which will be the only ones we will need for our proof:

Lemma 3.11.

Take a nonzero x~=(x0,x1,,xn1,xn)Φ~2+\widetilde{x}=(x_{0},x_{1},\dots,x_{n-1},x_{n})\in\widetilde{\Phi}^{2+}. We have:

  1. 1.

    The values x0x_{0} and xnx_{n} are not positive.

  2. 2.

    The values j=0nxj\sum\limits_{j=0}^{n}x_{j}, j evenxj\sum\limits_{j\text{ even}}x_{j} and j oddxj\sum\limits_{j\text{ odd}}x_{j} are all zero.

  3. 3.

    The value j=2n2xj\sum\limits_{j=2}^{n-2}x_{j} is not negative.

  4. 4.

    The first and last nonzero coordinates of x~\widetilde{x} are negative.

Proof. Immediate, by induction on the number of positive even roots into which x~\widetilde{x} decomposes. First, it is clear that any α~k,p\widetilde{\alpha}_{k,p} for even kk has all those properties. Second, it is easy to check that the sum of any two vectors with those properties keeps satisfying them. Hence the result follows. ∎

Proposition 3.12.

Let λ\lambda be a dominant weight that is not even minuscule. Then at least one of these hold:

  1. 1.

    The weight λ\lambda has nonzero coordinates at two positions 1i<jn11\leq i<j\leq n-1 with ijmod2i\not\equiv j\mod 2.

  2. 2.

    The weight λ\lambda verifies λ2++λn22\lambda_{2}+\dots+\lambda_{n-2}\geq 2.

Proof. Take μ<λ\mu<\lambda. Denote x:=λμΛ2+x:=\lambda-\mu\in\Lambda^{2+}. Since λ=x+μ\lambda=x+\mu and the coordinates of μ\mu at positions between 11 and n1n-1 are non negative, it suffices to check that either xx has positive coordinates at positions between 11 and n1n-1 of different parity, or that the sum of the positive coordinates in positions {2,,n2}\{2,\dots,n-2\} of xx, which we shall denote SS from now on, verifies S2S\geq 2.

In order to do this we can work with a lift x~Λ~2+\widetilde{x}\in\widetilde{\Lambda}^{2+} of xx by lifting each of the positive even roots in some decomposition. We will prove that x~\widetilde{x} has at least one of the two desired properties, and, since x0,xn0x_{0},x_{n}\leq 0 by Lemma 3.11, then x=π(x~)x=\pi(\widetilde{x}) will also have them and the proof will be complete.

Assume that x~\tilde{x} has every positive coordinate between 11 and n1n-1 at even positions. We will show that S0S\neq 0 and S1S\neq 1, hence S2S\geq 2.

If S=0S=0 this means there are no positive entries in positions {2,,n2}\{2,\dots,n-2\}. By Lemma 3.11, part 33 there are no negative entries either. So we have x~:=(x0,x1,0,,0,xn1,xn)\tilde{x}:=(x_{0},x_{1},0,\dots,0,x_{n-1},x_{n}). Now if nn is even then by Lemma 3.11, part 22 we have x0+xn=0x_{0}+x_{n}=0 hence x0=xn=0x_{0}=x_{n}=0, the latter by Lemma 3.11, part 11. But, since x1=xn1x_{1}=-x_{n-1} this contradicts Lemma 3.11, part 44 reaching a contradiction. If nn is odd then x0+xn1=0x_{0}+x_{n-1}=0 and x1+xn=0x_{1}+x_{n}=0. By assumption that positive entries are in even positions, we have x1=xn=0x_{1}=x_{n}=0 and we reach the same contradiction.

If S=1S=1 there will be exactly one positive entry in positions {2,,n2}\{2,\dots,n-2\} of value 11, say the ii-th one. By assumption ii is even. By Lemma 3.11, part 33, from positions 22 to n2n-2 there could either be no negative entries or one negative entry of value 1-1 at position jj. Now a case by case analysis follows.

  • If nn is odd, the case jj odd is excluded because we would get, summing odd entries, that x1+xn1=0x_{1}+x_{n}-1=0 and we have x1,xn0x_{1},x_{n}\leq 0, the first by assumption and the second by Lemma 3.11, part 11. So we have x1=xn=0x_{1}=x_{n}=0 and either jj is even or there is no jj at all. In either case we find, summing the even entries, that x0+xn1{0,1}x_{0}+x_{n-1}\in\{0,-1\}, from which it is impossible that both are negative, contradicting Lemma 3.11, part 44.

  • If nn is even, the case jj odd is again excluded since, summing odd entries, we get x1+xn11=0x_{1}+x_{n-1}-1=0, but by assumption both x1x_{1} and xn1x_{n-1} are not positive. Hence x1=xn1=0x_{1}=x_{n-1}=0 and jj is even or there is no jj at all. In this case we have to distinguish: if there is no jj then x0+xn=1x_{0}+x_{n}=-1 so both cannot be negative at the same time, and since the only other nonzero entry is the 11 at the ii-th position, Lemma 3.11, part 44 is contradicted. If there is a jj then x0+xn=0x_{0}+x_{n}=0, so that x0=xn=0x_{0}=x_{n}=0 and once again we have a contradiction with Lemma 3.11, part 44.

The only remaining task to complete the proof is to work out the case where all positive entries of x~\tilde{x} are at odd positions instead of even ones. There is a symmetry in Φ~2+\tilde{\Phi}^{2+} via ωkωnk\omega_{k}\mapsto\omega_{n-k} that will change odd positions and even positions if nn is odd. So the only remaining cases are for even nn, which can be approached exactly the same as before:

  • If S=0S=0 then the previous argument for even nn did not use the positions of positive entries being even so it still works when they are odd.

  • If S=1S=1 we now have that ii is odd. If jj were even, summing the even entries we get x0+xn1=0x_{0}+x_{n}-1=0 which is not possible (x0,xn0x_{0},x_{n}\leq 0) so that jj is either odd or does not exist. If it is odd, we sum the odd entries to get x1+xn1=0x_{1}+x_{n-1}=0, which yields a contradiction with Lemma 3.11, part 44. If it does not exist, we get x1+xn1=1x_{1}+x_{n-1}=-1, from which they cannot both be negative and we reach the same contradiction.

Thus, we can rephrase the condition for even wobbliness as follows:

Theorem 3.13.

Let μ:CΛ+{\mu}:C\to\Lambda^{+}. Then μs𝕋{\mathcal{E}}_{\mu}\in{\mathcal{M}}^{s{\mathbb{T}}} is even very stable if and only if for every cCc\in C, the dominant weight μ(c){\mu}(c) is even minuscule.

As an example, the fixed point in rank n=4n=4 associated to μ(c)=ω1+ω3\mu(c)=\omega_{1}+\omega_{3} and μ(d)0\mu(d)\neq 0 for dcd\neq c is even very stable, while being wobbly in the usual sense. In rank n=2n=2 every fixed point is even very stable, which can be deduced more easily by the lack of even weights in downward flows. This is because the only weights appearing in the upward flows in rank n=2n=2 are those appearing in the Hitchin base, which are 11 and 22. We then know that a negative weight kk is paired to a nonnegative one, 1k1-k, via the symplectic form ω\omega, hence the only possible negative weight is k=1k=-1.

As a final remark, it is possible to work with higher order automorphisms defined by (E,Φ)(E,ζrΦ)(E,\Phi)\mapsto(E,\zeta_{r}\Phi), where ζr\zeta_{r} is a primitive rr-th root of unity, giving subspaces r\mathcal{M}^{r}\subset\mathcal{M} and the corresponding notions of rr-very stable bundles. Most of the results presented here naturally generalize to that situation (by using rr-minuscule weights), however in this case there is no longer an associated real group and the subspaces considered are not Lagrangian.

4 Hitchin map on upward flows

One important motivation to consider very stable upward flows in [14] was the observation that the Hitchin map

h:=h|W+:W+𝒜h_{\mathcal{E}}:=h|_{W^{+}_{\mathcal{E}}}:W^{+}_{\mathcal{E}}\to{\mathcal{A}}

restricted to them is proper. Furthermore W+T+W^{+}_{\mathcal{E}}\cong T_{\mathcal{E}}^{+}{\mathcal{M}} as 𝕋{\mathbb{T}}-varieties. Thus in the very stable case hh_{\mathcal{E}} is a proper, even finite flat [14, Lemma 4.6], 𝕋{\mathbb{T}}-equivariant morphism between semi-projective affine spaces of the same dimension. As such it is suspectible for explicit description.

4.1 Equivariant cohomology of homogeneous spaces

We will describe the Hitchin map explicitely on some very stable upward flows in terms of equivariant cohomology. First we recall some of the basic properties of equivariant cohomology see e.g. [1] for more details.

Let G\mathrm{G} be a connected complex affine (or compact Lie) group. Consider the classifying G\mathrm{G}-bundle EGBGE\mathrm{G}\to B\mathrm{G}, where EGE\mathrm{G} is contractible. BGB\mathrm{G} is called the classifying space, and its cohomology ring can be computed as follows:

HG:=H(BG;)H(BT;)WG[𝔱]WG,H^{*}_{\mathrm{G}}:=H^{*}(B\mathrm{G};\mathbb{C})\cong H^{*}(B{\rm T};\mathbb{C})^{\mathrm{W}_{\mathrm{G}}}\cong\mathbb{C}[\mathfrak{t}]^{\mathrm{W}_{\mathrm{G}}},

where 𝔱=Lie(T)\mathfrak{t}=\mathop{\mathchoice{\mbox{\rm Lie}}{\mbox{\rm Lie}}{\mbox{\rm\scriptsize Lie}}{\mbox{\rm\tiny Lie}}}\nolimits({\rm T}) is the Lie algebra of a maximal torus TG{\rm T}\subset\mathrm{G} and WG\mathrm{W}_{\mathrm{G}} is the Weyl group of G\mathrm{G}.

Let now G\mathrm{G} act on a variety (or manifold) XX. We can form the Borel, or homotopy, quotient XG:=(EG×X)/GX_{\mathrm{G}}:=(E\mathrm{G}\times X)/\mathrm{G}, by the diagonal action of G\mathrm{G}, which is an XX-bundle over BGB\mathrm{G}. Its cohomology ring is what is taken to be its equivariant cohomology

HG(X;):=H(XG;).H^{*}_{\mathrm{G}}(X;\mathbb{C}):=H^{*}(X_{\mathrm{G}};\mathbb{C}).

As XGX_{\mathrm{G}} is an XX-bundle over BGB\mathrm{G} we get a ring map HGHG(X;)H^{*}_{\mathrm{G}}\to H^{*}_{\mathrm{G}}(X;\mathbb{C}), making HG(X;)H^{*}_{\mathrm{G}}(X;\mathbb{C}) an HGH^{*}_{\mathrm{G}}-algebra.

Let now T<H<G{\rm T}<{\rm H}<\mathrm{G} be a connected closed subgroup containing the maximal torus T{\rm T} of G\mathrm{G}. Because EGE\mathrm{G} is contractible, we have EG/HEH/HE\mathrm{G}/{\rm{H}}\sim E{\rm{H}}/{\rm{H}} so we can compute the G\mathrm{G}-equivariant cohomology of the homogeneous space G/H\mathrm{G}/{\rm{H}} as follows:

HG(G/H;)H((EG×G/H)/G;)H(EG/H;)HH,H^{*}_{\mathrm{G}}(\mathrm{G}/{\rm{H}};\mathbb{C})\cong H^{*}((E\mathrm{G}\times\mathrm{G}/{\rm{H}})/\mathrm{G};\mathbb{C})\cong H^{*}(E\mathrm{G}/{\rm{H}};\mathbb{C})\cong H^{*}_{{\rm{H}}},

with the ring map HGHHH^{*}_{\mathrm{G}}\to H^{*}_{{\rm{H}}} from the natural map BHBGB{\rm{H}}\to B\mathrm{G} induced from the embedding HG{\rm H}\subset\mathrm{G}. This way we have a simple way to compute equivariant cohomology of a homogeneous space explicitly as in the following diagram of graded algebras:

HG(G/H;)[𝔱]WHHG[𝔱]WG.\displaystyle\begin{array}[]{ccc}H^{*}_{\mathrm{G}}(\mathrm{G}/{\rm{H}};\mathbb{C})&\cong&\mathbb{C}[\mathfrak{t}]^{\mathrm{W}_{\rm{H}}}\\ \uparrow&&\uparrow\\ H^{*}_{\mathrm{G}}&\cong&\mathbb{C}[\mathfrak{t}]^{\mathrm{W}_{\mathrm{G}}}.\end{array} (4.4)

Note that the structure maps above are finite free, meaning that they define a finite free module. This is because the equivariant cohomology of equal rank homogeneous spaces are equivariantly formal [10, (1.2)], for example because they have no odd cohomology [11, Theorem VII, p. 467].

We will see below that on certain very stable upward flows the Hitchin map can be modelled by the spectrum of equivariant cohomology of appropriate homogenous spaces. For this reason we also take the spectrum of (4.4) and record the corresponding diagram:

Spec(HG(G/H;))𝔱//WHSpec(HG)𝔱//WG.\displaystyle\begin{array}[]{ccc}\operatorname{Spec}(H^{*}_{\mathrm{G}}(\mathrm{G}/{\rm{H}};\mathbb{C}))&\cong&\mathfrak{t}/\!\!/{\mathrm{W}_{\rm{H}}}\\ \downarrow&&\downarrow\\ \operatorname{Spec}(H^{*}_{\mathrm{G}})&\cong&\mathfrak{t}/\!\!/{\mathrm{W}_{\mathrm{G}}}.\end{array} (4.8)

We note that half the grading on cohomology will induce the 𝕋{\mathbb{T}}-action on 𝔱//WH\mathfrak{t}/\!\!/{\mathrm{W}_{\rm{H}}}, which agrees with the 𝕋{\mathbb{T}}-action induced from weight one action on 𝔱\mathfrak{t}. The down arrows in the diagram then become 𝕋{\mathbb{T}}-equivariant finite flat (ultimately because of equivariant formality), in particular proper, morphisms.

Because we will also consider how certain involutions act on the equivariant cohomology of homogeneous spaces, here we record the following lemma. To formulate it recall that for a unital commutative ring RR with 22 invertible and with involution θ:RR\theta:R\to R, the coinvariant ring is defined as

Rθ:=R/(rθ(r))rRR/(rR:θ(r)=r).R_{\theta}:=R/(r-\theta(r))_{r\in R}\cong R/(r\in R:\theta(r)=-r).

While if AA is a commutative RR-algebra and θ:AA\theta:A\to A also acts on AA, compatibly with the action on RR, then AθA_{\theta} is naturally an RθR_{\theta}-algebra, called the coinvariant algebra. Their relevance is in forming the fixed point scheme of the affine RR-scheme Spec(A)\operatorname{Spec}(A) under the involution Spec(θ):Spec(A)Spec(A)\operatorname{Spec}(\theta):\operatorname{Spec}(A)\to\operatorname{Spec}(A), which we also denote by θ\theta. We get that the fixed point scheme

Spec(A)θSpec(Aθ)\displaystyle\operatorname{Spec}(A)^{\theta}\cong\operatorname{Spec}(A_{\theta}) (4.9)

is an affine RθR_{\theta}-scheme. Using arguments from [24] we have the following

Lemma 4.1.

Let G\mathrm{G} be a connected complex reductive group (or a connected compact Lie group), and τ:GG\tau:\mathrm{G}\to\mathrm{G} a complex algebraic (smooth) involution, with TG{\rm T}\subset\mathrm{G} a τ\tau-stable torus. Let G0τ\mathrm{G}_{0}^{\tau} denote the identity component of the fixed point group Gτ\mathrm{G}^{\tau}. Assume that

HGHG0τ\displaystyle H^{*}_{\mathrm{G}}\twoheadrightarrow H^{*}_{\mathrm{G}^{\tau}_{0}} (4.10)

is surjecive. Let θ:=τ:HGHG\theta:=\tau^{*}:H^{*}_{\mathrm{G}}\to H^{*}_{\mathrm{G}} denote the induced action on the cohomology of BGB\mathrm{G}. Then we have that the coinvariant algebra

(HG)θHG0τ.(H^{*}_{\mathrm{G}})_{\theta}\cong H^{*}_{\mathrm{G}_{0}^{\tau}}.

Moreover if THG{\rm T}\subset{\rm H}\subset\mathrm{G} is a τ\tau-invariant closed connected subgroup, such that HHHH0τH^{*}_{\rm H}\twoheadrightarrow H^{*}_{{\rm H}^{\tau}_{0}} is surjective, then we have the commutative diagram:

HG(G/H;)θ(HH)θHH0τHG0τ(G0τ/H0τ;)(HG)θ(HG)θHG0τHG0τ\begin{array}[]{ccccccc}H^{*}_{\mathrm{G}}(\mathrm{G}/{\rm H};\mathbb{C})_{\theta}&\cong&(H^{*}_{\rm{H}})_{\theta}&\cong&H^{*}_{\rm{H}^{\tau}_{0}}&\cong&H^{*}_{\mathrm{G}_{0}^{\tau}}(\mathrm{G}_{0}^{\tau}/{\rm H}_{0}^{\tau};\mathbb{C})\\ \uparrow&&\uparrow&&\uparrow&&\uparrow\\ (H^{*}_{\mathrm{G}})_{\theta}&\cong&(H^{*}_{\mathrm{G}})_{\theta}&\cong&H^{*}_{\mathrm{G}_{0}^{\tau}}&\cong&H^{*}_{\mathrm{G}_{0}^{\tau}}\end{array}

Proof. We know that HG[𝔱]WH^{*}_{\mathrm{G}}\cong\mathbb{C}[\mathfrak{t}]^{\mathrm{W}}, the algebra of invariant polynomials on 𝔱\mathfrak{t} by the Weyl group W\mathrm{W} of G\mathrm{G}. By [29, Lemma 6.1] we can choose algebra generators p1,,prp_{1},\dots,p_{r} in [𝔱]W\mathbb{C}[\mathfrak{t}]^{\mathrm{W}} such τ(pi)=ϵipi\tau(p_{i})=\epsilon_{i}p_{i}, where ϵi=±1\epsilon_{i}=\pm 1. By [29, Lemma 6.5] the generators with ϵi=1\epsilon_{i}=1 give the generators of [𝔱τ]Wτ,\mathbb{C}[\mathfrak{t}^{\tau}]^{\mathrm{W}^{\tau}}, where WτW^{\tau} is the subgroup of WW fixed by τ\tau, itself a reflection group on 𝔱τ\mathfrak{t}^{\tau}. Thus the number of pip_{i}’s with ϵi=1\epsilon_{i}=1 is exactly the dimension of 𝔱τ\mathfrak{t}^{\tau}, which in turn agrees with the rank of G0τ{\rm\mathrm{G}_{0}^{\tau}}.

Finally, all pip_{i}’s with ϵi=1\epsilon_{i}=-1 restrict trivially to 𝔱τ\mathfrak{t}^{\tau}. Thus by the assumption (4.10) the restriction of those with ϵi=1\epsilon_{i}=1 generate [𝔱τ]WG0τHG0τ\mathbb{C}[\mathfrak{t}^{\tau}]^{\mathrm{W}_{\mathrm{G}_{0}^{\tau}}}\cong H^{*}_{\mathrm{G}_{0}^{\tau}}, and as there are rank(G0τ)\operatorname{rank}(\mathrm{G}_{0}^{\tau}) of them, they should restrict algebraically independent. Thus the kernel of the surjection is generated by the anti-invariant generators, showing the claim (HG)θHG0τ(H^{*}_{\mathrm{G}})_{\theta}\cong H^{*}_{\mathrm{G}_{0}^{\tau}}.

The second statement follows from the first and (4.4). ∎

Remark 4.2.

The assumption of surjection (4.10) is quite restrictive. For simple G\mathrm{G} it only happens [24, after (4.1)] for the symmetric pairs

(G,G0τ)(SL2n+1,SO2n+1),(SL2n,Spn),(SO2n,SO2n1), and (E6,F4).(\mathrm{G},\mathrm{G}^{\tau}_{0})\cong(\mathrm{SL}_{2n+1},{\mathrm{SO}}_{2n+1}),(\mathrm{SL}_{2n},\mathrm{Sp}_{n}),({\mathrm{SO}}_{2n},{\mathrm{SO}}_{2n-1}),\mbox{ and }(\rm{E}_{6},\rm{F}_{4}).

All these examples will appear in §4.3 below.

4.2 Explicit Hitchin map on very stable upward flows

First we recall from [13] how to describe hk:=hkh_{k}:=h_{{\mathcal{E}}_{k}} for the very stable upward flows Wk+:=Wk+W_{k}^{+}:=W^{+}_{{\mathcal{E}}_{k}} explicitly, where k:=μck{\mathcal{E}}_{k}:={\mathcal{E}}_{\mu_{c}^{k}}, cCc\in C fixed and μck:CΛ+\mu^{k}_{c}:C\to\Lambda^{+} is defined by μck(c)=ωk\mu^{k}_{c}(c)=\omega_{k} and 0 otherwise.

Let us define the evaluation map at cCc\in C

evc:𝒜n{\rm ev}_{c}:{\mathcal{A}}\to\mathbb{C}^{n}

sending the characteristic polynomial (a1,,an)𝒜(a_{1},\dots,a_{n})\in{\mathcal{A}} to

(a1(c),,an(c))Kc1××Kcnn(a_{1}(c),\dots,a_{n}(c))\in K^{1}_{c}\times\dots\times K^{n}_{c}\cong\mathbb{C}^{n}

after identifying the fiber KK\cong\mathbb{C}. We can further identify

n𝔤𝔩n//GLn𝔱n//SnSpec(H(BGLn,)),\mathbb{C}^{n}\cong{\mathfrak{g}\mathfrak{l}}_{n}/\!\!/\mathrm{GL}_{n}\cong\mathfrak{t}_{n}/\!\!/{S_{n}}\cong\operatorname{Spec}(H^{*}(B{\mathrm{GL}}_{n},\mathbb{C})),

where 𝔤𝔩n=Lie(GLn){\mathfrak{g}\mathfrak{l}}_{n}={\mathop{\mathchoice{\mbox{\rm Lie}}{\mbox{\rm Lie}}{\mbox{\rm\scriptsize Lie}}{\mbox{\rm\tiny Lie}}}\nolimits}(\mathrm{GL}_{n}) and 𝔱n=Lie(Tn)\mathfrak{t}_{n}={\mathop{\mathchoice{\mbox{\rm Lie}}{\mbox{\rm Lie}}{\mbox{\rm\scriptsize Lie}}{\mbox{\rm\tiny Lie}}}\nolimits}({\rm T}_{n}) the Lie algebra of the maximal torus TnGLn{\rm T}_{n}\subset\mathrm{GL}_{n}, and the symmetric group SnS_{n} is the Weyl group of GLn\mathrm{GL}_{n}. Then with the notation HGLn:=H(BGLn;)H^{*}_{\mathrm{GL}_{n}}:=H^{*}(B{\mathrm{GL}}_{n};\mathbb{C}) for the cohomology ring of the classifying space BGLnB{\mathrm{GL}}_{n} we have the following pull back diagram from [13]

Wk+Spec(HGLn2(Grk(n),))hk𝒜evcSpec(HGLn2),\begin{array}[]{ccc}W^{+}_{k}&\twoheadrightarrow&\operatorname{Spec}(H^{2*}_{\mathrm{GL}_{n}}(\rm{Gr}_{k}(\mathbb{C}^{n}),\mathbb{C}))\\ \!\!\!\!\!\!h_{k}\downarrow&\lrcorner&\downarrow\\ {\mathcal{A}}&\stackrel{{\scriptstyle{\rm ev}_{c}}}{{\twoheadrightarrow}}&\operatorname{Spec}(H^{2*}_{\mathrm{GL}_{n}})\end{array},

where Grk(n)\textnormal{Gr}_{k}(\mathbb{C}^{n}) is the Grassmannian of kk-dimensional subspaces in n\mathbb{C}^{n} with the usual action of GLn\mathrm{GL}_{n}. Additionally, all maps are 𝕋{\mathbb{T}}-equivariant with respect to the usual 𝕋{\mathbb{T}}-action on Wk+W_{k}^{+}\subset{\mathcal{M}} and 𝒜{\mathcal{A}}, and the one induced by the grading on HGLn2(Grk(n);)H^{2*}_{\mathrm{GL}_{n}}(\textnormal{Gr}_{k}(\mathbb{C}^{n});\mathbb{C}) and HGLn2H^{2*}_{\mathrm{GL}_{n}}. In other words the Hitchin map hkh_{k} can be modelled by the equivariant cohomology of the Grassmannian Grk(n){\rm Gr}_{k}(\mathbb{C}^{n}).

4.3 Explicit Hitchin map on even very stable upward flows

We can then ask what models the even Hitchin map hkθ:Wk2+𝒜θh^{\theta}_{k}:\mathrm{W}_{k}^{2+}\to{\mathcal{A}}^{\theta}. We can note that θ\theta acts on {\mathcal{M}} as 1𝕋-1\in{\mathbb{T}} in the natural 𝕋{\mathbb{T}}-action, thus we can induce an action of θ\theta on HGLn2(Grk(n);)H^{2*}_{\mathrm{GL}_{n}}(\textnormal{Gr}_{k}(\mathbb{C}^{n});\mathbb{C}) and HGLn2H^{2*}_{\mathrm{GL}_{n}} as 1𝕋-1\in{\mathbb{T}}. Therefore we have

Wk2+Spec(HGLn2(Grk(n),))θhkθ𝒜θevcSpec(HGLn2)θ,\displaystyle\begin{array}[]{ccc}W^{2+}_{k}&\twoheadrightarrow&\operatorname{Spec}(H^{2*}_{\mathrm{GL}_{n}}(\rm{Gr}_{k}(\mathbb{C}^{n}),\mathbb{C}))^{\theta}\\ \!\!\!\!\!\!h^{\theta}_{k}\downarrow&\lrcorner&\downarrow\\ {\mathcal{A}}^{\theta}&\stackrel{{\scriptstyle{\rm ev}_{c}}}{{\twoheadrightarrow}}&\operatorname{Spec}(H^{2*}_{\mathrm{GL}_{n}})^{\theta}\end{array}, (4.14)

and, as a result, the even Hitchin map hkθh^{\theta}_{k} can be modelled on the θ\theta-fixed point scheme

Spec(HGLn2(Grk(n),))θ.\operatorname{Spec}(H^{2*}_{\mathrm{GL}_{n}}(\rm{Gr}_{k}(\mathbb{C}^{n}),\mathbb{C}))^{\theta}.

For simplicity we will start with GL2n\mathrm{GL}_{2n} and an even number 0<2k<2n0<2k<2n. To understand the fixed point scheme Spec(HGLn2(Gr2k(2n),))θ\operatorname{Spec}(H^{2*}_{\mathrm{GL}_{n}}(\rm{Gr}_{2k}(\mathbb{C}^{2n}),\mathbb{C}))^{\theta} we recall a presentation of the equivariant cohomology of the Grassmannian. In practice it can be done by following through the restriction of invariant polynomials in (4.4).

Let e1,,e2k,f1,,f2n2k,c1,,c2ne_{1},\dots,e_{2k},f_{1},\dots,f_{2n-2k},c_{1},\dots,c_{2n} be variables of degree given by their index. Then we have the following presentation of the graded ring HGLn2(Gr2k(2n),)H^{2*}_{\mathrm{GL}_{n}}(\textnormal{Gr}_{2k}(\mathbb{C}^{2n}),\mathbb{C})\cong

[e1,,e2k,f1,,f2n2k,c1,,c2n]((t2k+e1t2k1++e2k)(t2n2k+f1t2n2k1++f2n2k)(t2n+c1t2n1++c2n)),\frac{\mathbb{C}[e_{1},\dots,e_{2k},f_{1},\dots,f_{2n-2k},c_{1},\dots,c_{2n}]}{\left((t^{2k}+e_{1}t^{2k-1}+\dots+e_{2k})(t^{2n-2k}+f_{1}t^{2n-2k-1}+\dots+f_{2n-2k})-(t^{2n}+c_{1}t^{2n-1}+\dots+c_{2n})\right)},

where the ideal is generated by the coefficients of the given polynomial in tt. It is naturally an algebra over HGL2n[c1,,c2n]H^{*}_{\mathrm{GL}_{2n}}\cong\mathbb{C}[c_{1},\dots,c_{2n}]. The action of θ\theta is easy to figure out in this presentation, namely, all elements of degree ii will get multiplied by (1)i(-1)^{i}. To compute the fixed point scheme (4.9) we will have to determine the coinvariant algebra of this θ\theta-action. To form the coinvariant algebra we add to the ideal the algebra elements which are acted upon by θ\theta as 1-1, that is we add the odd degree generators to the ideal. This way we get the following presentation of the coinvariant algebra: HGL2n2(Gr2k(2n),))θH^{2*}_{\mathrm{GL}_{2n}}({\rm Gr}_{2k}(\mathbb{C}^{2n}),\mathbb{C}))_{\theta}\cong

[e2,,e2k,f2,,f2n2k,c2,,c2n]((t2k+e2t2k2++e2k)(t2n2k+f2t2n2k2++f2n2k)(t2n+c2t2n2++c2n)),\frac{\mathbb{C}[e_{2},\dots,e_{2k},f_{2},\dots,f_{2n-2k},c_{2},\dots,c_{2n}]}{\left((t^{2k}+e_{2}t^{2k-2}+\dots+e_{2k})(t^{2n-2k}+f_{2}t^{2n-2k-2}+\dots+f_{2n-2k})-(t^{2n}+c_{2}t^{2n-2}+\dots+c_{2n})\right)},

where all generators have even degree, and the ideal is generated by the coefficients of the indicated polynomial in t2t^{2}. This is an algebra over [c2,,c2n]\mathbb{C}[c_{2},\dots,c_{2n}] which we can and will identify with HSp(n):=H(BSp(n),)H^{*}_{{\rm Sp}(n)}:=H^{*}(B{\rm Sp}(n),\mathbb{C}) the cohomology ring of the classifying space of the compact unitary symplectic group. In turn, we can identify HGL2n2(Gr2k(2n),))θH^{2*}_{\mathrm{GL}_{2n}}({\rm Gr}_{2k}(\mathbb{C}^{2n}),\mathbb{C}))_{\theta} with the equivariant cohomology HSp(n)(Grk(n),)H^{*}_{{\rm Sp}(n)}(\textnormal{Gr}_{k}({\mathbb{H}}^{n}),\mathbb{C}) of the quaternionic Grassmannian Grk(n)\textnormal{Gr}_{k}({\mathbb{H}}^{n}) of kk-dimensional {\mathbb{\mathbb{H}}}-subspaces of n{\mathbb{H}}^{n}, which is a non-Hermitian compact homogeneous space isomorphic to Sp(n)/Sp(k)×Sp(nk)\mathrm{Sp}(n)/\mathrm{Sp}(k)\times\mathrm{Sp}(n-k).

We can summarize our observation in the following diagram:

Spec(HGL2n2(Gr2k(2n),))θSpec(HSp(n)2(Grk(n),))Spec(HGL2n2)θSpec(HSp(n)2)\displaystyle\begin{array}[]{ccc}\operatorname{Spec}(H^{2*}_{\mathrm{GL}_{2n}}({\textnormal{Gr}}_{2k}(\mathbb{C}^{2n}),\mathbb{C}))^{\theta}&\cong&\operatorname{Spec}(H^{2*}_{\mathrm{Sp}(n)}(\textnormal{Gr}_{k}(\mathbb{H}^{n}),\mathbb{C}))\\ \downarrow&&\downarrow\\ \operatorname{Spec}(H^{2*}_{\mathrm{GL}_{2n}})^{\theta}&\cong&\operatorname{Spec}(H^{2*}_{\mathrm{Sp}(n)})\end{array} (4.18)

Thus, in light of (4.14), the Hitchin map h2kθh^{\theta}_{2k} on the even upward flow W2k2+W_{2k}^{2+} can be modelled by the spectrum of the equivariant cohomology of the quaternionic Grassmannian Grk(n)\textnormal{Gr}_{k}(\mathbb{H}^{n}).

In fact, we can find similar coincidences of coinvariant algebras of the equivariant cohomology of cominuscule flag varieties in some other types. Cominuscule flag varieties correspond to maximal parabolic subgroups associated to minuscule coweights, or equivalently to simple roots, which occur with coefficient 11 in the highest root (see also [14, §8] for more context). For example we can consider the action of θ\theta on

HSO(4n+2)2(SO(4n+2)/SO(2)×SO(4n),)\displaystyle H^{2*}_{{\mathrm{SO}}(4n+2)}({\mathrm{SO}}(4n+2)/{\mathrm{SO}}(2)\times{\mathrm{SO}}(4n),\mathbb{C}) (4.19)

given by (1)deg(-1)^{deg}, where deg=deg=* is the degree of the grading on (4.19). The Hermitian symmetric space SO(4n+2)/SO(2)×SO(4n){\mathrm{SO}}(4n+2)/{\mathrm{SO}}(2)\times{\mathrm{SO}}(4n) is an even quadric, a cominuscule flag variety for the special orthogonal group SO4n+2{\mathrm{SO}}_{4n+2}. The corresponding coinvariant algebra

HSO(4n+2)2(SO(4n+2)/SO(2)×SO(4n),)θHSO(4n+1)2(SO(4n+1)/SO(4n),),H^{2*}_{{\mathrm{SO}}(4n+2)}({\mathrm{SO}}(4n+2)/{\mathrm{SO}}(2)\times{\mathrm{SO}}(4n),\mathbb{C})_{\theta}\cong H^{2*}_{{\mathrm{SO}}(4n+1)}({\mathrm{SO}}(4n+1)/{\mathrm{SO}}(4n),\mathbb{C}),

can be identified with the SO(4n+1){\mathrm{SO}}(4n+1)-equivariant cohomology ring of the sphere

S4nSO(4n+1)/SO(4n).S^{4n}\cong{\mathrm{SO}}(4n+1)/{\mathrm{SO}}(4n).

In fact we have the following diagram

HSO(4n+2)2(SO(4n+2)/SO(2)×SO(4n),)θHSO(4n+1)2(SO(4n+1)/SO(4n),)(HSO(4n+2)2)θHSO(4n+1)2.\displaystyle\begin{array}[]{ccc}H^{2*}_{{\mathrm{SO}}(4n+2)}({\mathrm{SO}}(4n+2)/{\mathrm{SO}}(2)\times{\mathrm{SO}}(4n),\mathbb{C})_{\theta}&\cong&H^{2*}_{{\mathrm{SO}}(4n+1)}({\mathrm{SO}}(4n+1)/{\mathrm{SO}}(4n),\mathbb{C})\\ \uparrow&&\uparrow\\ \left(H^{2*}_{{\mathrm{SO}}(4n+2)}\right)_{\theta}&\cong&H^{2*}_{{\mathrm{SO}}(4n+1)}\end{array}. (4.23)

In other words we can expect that the Hitchin map on even cominuscule upward flows in the SO4n+2{\mathrm{SO}}_{4n+2} Higgs moduli space – equivalently the Hitchin map on cominuscule upward flows in the SO(2n+2,2n){\mathrm{SO}}(2n+2,2n)-Higgs moduli space – to be modelled by the spectrum of the equivariant cohomology of the sphere S4nS^{4n}.

For our final example we can consider the unique cominuscule flag variety for the exceptional E6{\rm E}_{6}. It is the complex Cayley plane E6/Spin(10)×U(1){\rm E}_{6}/{\rm Spin}({10})\times{\rm U}(1) which is a compact Hermitian symmetric space. We can identify the coinvariant algebra of the θ=(1)deg\theta=(-1)^{deg} action on its equivariant cohomology ring:

HE62(E6/Spin(10)×U(1),)θHF42(F4/Spin(9),)(HE62)θHF42.\displaystyle\begin{array}[]{ccc}H^{2*}_{{\rm E}_{6}}({\rm E}_{6}/{\rm Spin}({10})\times{\rm U}(1),\mathbb{C})_{\theta}&\cong&H^{2*}_{{\rm F}_{4}}({\rm F}_{4}/{\rm Spin}(9),\mathbb{C})\\ \uparrow&&\uparrow\\ \left(H^{2*}_{{\rm E}_{6}}\right)_{\theta}&\cong&H^{2*}_{{\rm F}_{4}}\end{array}. (4.27)

Thus we expect to model the Hitchin map on even cominuscule upward flows in the E6{\rm E}_{6} Higgs moduli space – equivalently on the cominuscule upward flows in the E6(2)E_{6(2)}-Higgs moduli space – by the spectrum of equivariant cohomology of the real Cayley plane F4/Spin(9){\rm F}_{4}/{\rm Spin}(9).

Mysteriously, in the above examples the symmetric spaces whose equivariant cohomology we found to give the θ\theta-coinvariant algebra of the equivariant cohomology of the cominuscule flag variety are homogeneous spaces for the Nadler group [22, Table 1] of the corresponding quasi-split real form of Hodge type. That is

U(n,n)Spn,SO(2n+2,2n)SO4n+1, and E6(2)F4.{\rm U}(n,n)^{\vee}\cong\mathrm{Sp}_{n},{\mathrm{SO}}(2n+2,2n)^{\vee}\cong{\mathrm{SO}}_{4n+1},\mbox{ and }{\rm E}_{6(2)}^{\vee}\cong{\rm F}_{4}.

Conjecturally, [2, §7] the Higgs bundle moduli space for the Nadler group should give the support of the mirror of the Lagrangian brane given by the Higgs moduli space attached to a real form. However these appearances of the Nadler group remain to be understood.

Even more surprising is that the Nadler groups in the above examples happen to be the fixed point subgroups of an involution of the ambient Langlands dual group. The corresponding anti-holomorphic involution can then be used to construct [5] an anti-holomorphic involution in the cominuscule flag varieties in the above examples, and show that the Lagrangian fixed point manifold is isomorphic to the corresponding non-Hermitian compact symmetric spaces we have found above. Thus by uniformly denoting this anti-holomorphic involution by τ\tau we get that

Gr2k(2n)τGrk(n)\textnormal{Gr}_{2k}(\mathbb{C}^{2n})^{\tau}\cong\textnormal{Gr}_{k}(\mathbb{H}^{n})
(SO(4n+2)/SO(2)×SO(4n))τSO(4n+1)/SO(4n)({\mathrm{SO}}(4n+2)/{\mathrm{SO}}(2)\times{\mathrm{SO}}(4n))^{\tau}\cong{\mathrm{SO}}(4n+1)/{\mathrm{SO}}(4n)

and

(E6/Spin(10)×U(1))τF4/Spin(9).({\rm E}_{6}/{\rm Spin}({10})\times{\rm U}(1))^{\tau}\cong{\rm F}_{4}/{\rm Spin}(9).

Using Lemma 4.1 it can be shown - by observing that precisely the even degree generators of invariant polynomials survive for the τ\tau-fixed groups - that in each of these cases τ\tau induces our

τ=θ=(1)deg\displaystyle\tau^{*}=\theta=(-1)^{deg} (4.28)

on equivariant cohomology, where again degdeg is half the degree of a homogeneous cohomology class. In turn, this observation and again Lemma 4.1 can be used to geometrically prove our final

Theorem 4.3.

The diagrams in (4.18), (4.23), (4.27) commute and are induced by the involution τ\tau.

Remark 4.4.

Because of (4.28) we can deduce, by the Lefschetz fixed point theorem, that the signatures of our Hermitian symmetric spaces X=G/HX=\mathrm{G}/\rm{H} agree

sign(X)=tr(θ:H(X)H(X))=χ(Xτ)\displaystyle{\rm sign}(X)=\textnormal{tr}(\theta:H^{*}(X)\to H^{*}(X))=\chi(X^{\tau}) (4.29)

with the Euler characteristic of the corresponding non-Hermitian symmetric spaces XτX^{\tau}. The quantity sign(X){\rm sign}(X) is relevant in our considerations as it agrees with the rank of the coinvariant algebra HG(X)θH^{*}_{\mathrm{G}}(X)_{\theta}, which in turn should compute the multiplicity of the even Hitchin map on the corresponding even cominuscule upward flow.

It is interesting to note that a very similar approach to (4.29) was studied in [16, Remark (1) p.337 ] to determine the signature of our Hermitian symmetric spaces as the Euler characteristic of XσX^{\sigma}, using the involution σ:XX\sigma:X\to X induced by the split real form - instead of our real form given by the Nadler group. The fixed point sets are different in the type AA-case - certain real Grassmannians - from our quaternionic Grassmannians but the induced actions on the cohomology σ=τ=θ\sigma^{*}=\tau^{*}=\theta agree, because the real forms σ\sigma and τ\tau are inner to each other.

Remark 4.5.

The involution σ\sigma however suggests a solution for modelling the even Hitchin system inside the equivariant cohomology of the last family of cominuscule flag varieties with non-zero signature. Namely, we can consider the anti-holomorphic action of σ\sigma on Gr2k(2n+1)\textnormal{Gr}_{2k}(\mathbb{C}^{2n+1}) with fixed point set Gr2k(2n+1)σGr2k(2n+1)\textnormal{Gr}_{2k}(\mathbb{C}^{2n+1})^{\sigma}\cong\textnormal{Gr}_{2k}(\mathbb{R}^{2n+1}). Then it appears that we have σ\sigma inducing

HSL2n+12(Gr2k(2n+1),)θHSO2n+12(Gr2k(2n+1),)(HSL2n+12)θHSO2n+12.\displaystyle\begin{array}[]{ccc}H^{2*}_{\mathrm{SL}_{2n+1}}(\textnormal{Gr}_{2k}(\mathbb{C}^{2n+1}),\mathbb{C})_{\theta}&\cong&H^{2*}_{{\mathrm{SO}}_{2n+1}}(\textnormal{Gr}_{2k}(\mathbb{R}^{2n+1}),\mathbb{C})\\ \uparrow&&\uparrow\\ \left(H^{2*}_{\mathrm{SL}_{2n+1}}\right)_{\theta}&\cong&H^{2*}_{{\mathrm{SO}}_{2n+1}}\end{array}. (4.33)

The subtlety of this case is that Gr2k(2n+1)\textnormal{Gr}_{2k}(\mathbb{R}^{2n+1}) is no longer simply connected, thus the usual computation of its equivariant cohomology (4.4) does not apply. One can proceed by first determining the equivariant cohomology ring of its universal double cover - the oriented Grassmannian - from (4.4), and then take invariants of the cover map. In fact, recently the equivariant cohomology of Gr2k(2n+1)\textnormal{Gr}_{2k}(\mathbb{R}^{2n+1}) was computed in [15, Theorem 5.23], and the result matches the coinvariant algebra HSL2n+12(Gr2k(2n+1),)θH^{2*}_{\mathrm{SL}_{2n+1}}(\textnormal{Gr}_{2k}(\mathbb{C}^{2n+1}),\mathbb{C})_{\theta}. We note that in this example the group SO2n+1{\mathrm{SO}}_{2n+1} is the Langlands dual of the Nadler group Spn\mathrm{Sp}_{n} of our quasi-split real form SU(n,n+1){\mathrm{SU}}(n,n+1) of Hodge type. In particular, their classifying spaces have isomorphic cohomology

HSO2n+1[𝔱SO2n+1]WSO2n+1[𝔱Spn]WSpnHSpn,\displaystyle H^{*}_{{\mathrm{SO}}_{2n+1}}\cong\mathbb{C}[\mathfrak{t}_{{\mathrm{SO}}_{2n+1}}]^{{\rm W}_{{\mathrm{SO}}_{2n+1}}}\cong\mathbb{C}[\mathfrak{t}_{\mathrm{Sp}_{n}}]^{{\rm W}_{\mathrm{Sp}_{n}}}\cong H^{*}_{\mathrm{Sp}_{n}}, (4.34)

because WSO2n+1WSpn{\rm W}_{{\mathrm{SO}}_{2n+1}}\cong{\rm W}_{\mathrm{Sp}_{n}}, 𝔱SO2n+1𝔱Spn\mathfrak{t}_{{\mathrm{SO}}_{2n+1}}\cong\mathfrak{t}_{\mathrm{Sp}_{n}}^{*} and the two representations in (4.34) can be identified by the Killing form.

Remark 4.6.

The final example of symmetric pairs from Remark 4.2 we have not discussed yet is (SO4n,SO4n1)({\mathrm{SO}}_{4n},{\mathrm{SO}}_{4n-1}). In this case τ\tau will induce on the cohomology of our cominuscule flag variety an involution

θτ:=τ:HSO4n(SO4n/SO2×SO4n2;)HSO4n(SO4n/SO2×SO4n2;),\theta_{\tau}:=\tau^{*}:H^{*}_{{\mathrm{SO}}_{4n}}({\mathrm{SO}}_{4n}/{\mathrm{SO}}_{2}\times{\mathrm{SO}}_{4n-2};\mathbb{C})\to H^{*}_{{\mathrm{SO}}_{4n}}({\mathrm{SO}}_{4n}/{\mathrm{SO}}_{2}\times{\mathrm{SO}}_{4n-2};\mathbb{C}),

which is different from the usual Hodge type (1)deg(-1)^{deg} unlike in the previous cases (4.28). In fact we expect that this θτ\theta_{\tau} will be the involution corresponding to the (only) quasi-split real form SO(2n+1,2n1){\mathrm{SO}}(2n+1,2n-1) which is not split or of Hodge type. Thus we expect that the spectrum of the diagram we get from Lemma 4.1

HSO4n2(SO4n/SO2×SO4n2;)θτHSO4n12(SO4n1/SO4n2;)(HSO4n2)θτHSO4n12\displaystyle\begin{array}[]{ccc}H^{2*}_{{\mathrm{SO}}_{4n}}({\mathrm{SO}}_{4n}/{\mathrm{SO}}_{2}\times{\mathrm{SO}}_{4n-2};\mathbb{C})_{\theta_{\tau}}&\cong&H^{2*}_{{\mathrm{SO}}_{4n-1}}({\mathrm{SO}}_{4n-1}/{\mathrm{SO}}_{4n-2};\mathbb{C})\\ \uparrow&&\uparrow\\ \left(H^{2*}_{{\mathrm{SO}}_{4n}}\right)_{\theta_{\tau}}&\cong&H^{2*}_{{\mathrm{SO}}_{4n-1}}\end{array} (4.38)

models the Hitchin map on a cominuscule upward flow in the SO(2n+1,2n1){\mathrm{SO}}(2n+1,2n-1)-Higgs moduli space.

Remark 4.7.

Oscar García-Prada has pointed out to us that the symmetric pairs in Remark 4.2 precisely correspond to the complexifications of the maximal split subgroups of the non-split quasi-split real forms in [8, Table 1. p. 2914]. They are used [8, Theorem 6.13.(1)] to construct the Hitchin-Kostant-Rallis section in the quasi-split real form cases. This demystifies their appearance in our descriptions of the Hitchin maps on cominuscule upward flows in the quasi-split Higgs moduli spaces in the diagrams (4.18), (4.23), (4.27),(4.33) and (4.38) above.

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