Faculty of Mathematics, University of Vienna, Oskar–Morgenstern–Platz 1, 1090 Wien, Austria
Faculty of Mathematics, UniDistance Suisse, Schinerstrasse 18, 3900 Brig, Switzerland
February 2, 2022
Given a parabolic geometry on a smooth manifold \(M\), we study a natural affine bundle \(A \to M\), whose smooth sections can be identified with Weyl structures for the geometry. We show that the initial parabolic geometry defines a reductive Cartan geometry on \(A\), which induces an almost bi-Lagrangian structure on \(A\) and a compatible linear connection on \(TA\). We prove that the split-signature metric given by the almost bi-Lagrangian structure is Einstein with non-zero scalar curvature, provided the parabolic geometry is torsion-free and \(|1|\)-graded. We proceed to study Weyl structures via the submanifold geometry of the image of the corresponding section in \(A\). For Weyl structures satisfying appropriate non-degeneracy conditions, we derive a universal formula for the second fundamental form of this image. We also show that for locally flat projective structures, this has close relations to solutions of a projectively invariant Monge-Ampere equation and thus to properly convex projective structures.
Parabolic geometries form a class of geometric structures that look very diverse in their standard description. This class contains important and well-studied examples like conformal and projective structures, non-degenerate CR structures of hypersurface type, path geometries, quaternionic contact structures, and various types of generic distributions. They admit a uniform conceptual description as Cartan geometries of type \((G,P)\) for a semisimple Lie group \(G\) and a parabolic subgroup \(P\subset G\) in the sense of representation theory. Such a geometry on a smooth manifold \(M\) is given by a principal \(P\)-bundle \(p : \mathcal{G} \to M\) together with a Cartan connection \(\omega \in \Omega^1(\mathcal{G},\mathfrak{g})\), which defines an equivariant trivialization of the tangent bundle \(T\mathcal G\). A standard reference for parabolic geometries is [16].
The group \(P\) can be naturally written as a semi-direct product \(G_0\ltimes P_+\) of a reductive subgroup \(G_0\) and a nilpotent normal subgroup \(P_+\). For a Cartan geometry \((p:\mathcal G\to M,\omega)\) the quotient \(\mathcal G_0:=\mathcal G/P_+\to M\) is a principal \(G_0\)-bundle, and some parts of \(\omega\) can be descended to that bundle. In the simplest cases, this defines a usual first order \(G_0\)-structure on \(M\), in more general situations a filtered analog of such a structure. Thus the Cartan geometry can be viewed as an extension of a first order structure. This reflects the fact that morphisms of parabolic geometries are in general not determined locally around a point by their 1-jet in that point, and the Cartan connection captures the necessary higher order information.
To work explicitly with parabolic geometries, one often chooses a more restrictive structure, say a metric in a conformal class, a connection in a projective class or a pseudo-Hermitian structure on a CR manifold, expresses things in terms of this choice and studies the effect of different choices. It turns out that there is a uniform way to do this that can be applied to all parabolic geometries, namely the concept of Weyl structures introduced in [15], see Chapter 5 of [16] for an improved exposition. Choosing a Weyl structure, one in particular obtains a linear connection on any natural vector bundle associated to a parabolic geometry, as well as an identification of higher order geometric objects like tractor bundles with more traditional natural bundles. The set of Weyl structures always forms an affine space modeled on the space on one-forms on the underlying manifold, and there are explicit formulae for how a change of Weyl structure affects the various derived quantities.
The initial motivation for this article were the results in [19] on projective structures. Such a structure on a smooth manifold \(M\) is given by an equivalence class \([\nabla]\) of torsion-free connections on its tangent bundle, where two connections are called equivalent if they have the same geodesics up to parametrization. While these admit an equivalent description as a parabolic geometry, the underlying structure \(\mathcal G_0\to M\) is the full frame bundle of \(M\) and thus contains no information. Hence there is the natural question, whether a projective structure can be encoded into a first order structure on some larger space constructed from \(M\). Indeed, in [19], the authors associate to a projective structure on an \(n\)-dimensional manifold \(M\) a certain rank \(n\) affine bundle \(A \to M\), whose total space can be canonically endowed with a neutral signature metric \(h\), as well as a non-degenerate \(2\)-form \(\Omega\). It turns out that the metric \(h\) is Einstein and \(\Omega\) is closed. Moreover, the pair \((h,\Omega)\) is related by an endomorphism of \(TA\) which squares to the identity map and its eigenbundles \(L^{\pm}\) are Lagrangian with respect to \(\Omega\). Equivalently, we may think of the pair \((h,\Omega)\) as an almost para-Kähler structure or as an almost bi-Lagrangian structure \((\Omega,L^+,L^-)\) on \(A\), see Section 3.1 for the formal definition and more details.
In addition, it is observed that the sections of \(A \to M\) are in bijective correspondence with the connections in the projective class. Consequently, all the submanifold notions of symplectic – and pseudo-Riemannian geometry can be applied to the representative connections of \([\nabla]\). This leads in particular to the notion of a minimal Lagrangian connection [28]. As detailed below, this concept has close relations to the concept of properly convex projective structures. These in turn provide a connection to the study of representation varieties and higher Teichmüller spaces, see [32] for a survey.
In an attempt to generalize these constructions to a larger class of parabolic geometries, we were led to a definition of \(A\to M\) that directly leads to an interpretation as a bundle of Weyl structures. This means that the space of sections of \(A\to M\) can be naturally identified with the space of Weyl structures for the geometry \((p:\mathcal G\to M,\omega)\). At some stage it was brought to our attention that a bundle of Weyl structures had been defined in that way already in the article [21] by M. Herzlich in the setting of general parabolic geometries. In this article, Herzlich gave a rather intricate argument for the existence of a connection on \(TA\) and used this to study canonical curves in parabolic geometries.
The crucial starting point for our results here is that a parabolic geometry \((p:\mathcal G\to M,\omega)\) can also naturally be interpreted as a Cartan geometry on \(A\) with structure group \(G_0\). This immediately implies that for any type of parabolic geometry, there is a canonical linear connection on any natural vector bundle over \(A\) as well as natural almost bi-Lagrangian structure on \(A\) that is compatible with the canonical connection. So in particular, we always obtain a non-degenerate two-form \(\Omega\in\Omega^2(A)\), a neutral signature metric \(h\) on \(TA\) as well as a decomposition \(TA=L^-\oplus L^+\) as a sum of Lagrangian subbundles.
Using the interpretation via Cartan geometries, it turns out that all elements of the theory of Weyl structures admit a natural geometric interpretation in terms of pulling back operations on \(A\) via the sections defined by a Weyl structure. This works for general parabolic geometries as shown in Section 2. In particular, we show that Weyl connections are obtained by pulling back the canonical connection on \(A\), while the Rho tensor (or generalized Schouten tensor) associated to a Weyl connection is given by the pullback of a canonical \(L^+\)-valued one-form on \(A\).
We believe that this interpretation of Weyl structures should be a very useful addition to the tool set available for the study of parabolic geometries. Indeed, working with the canonical geometric structures on \(A\) compares to the standard way of using Weyl structures, like working on a frame bundle compares to working in local frames.
For the second part of the article, we adopt a different point of view. From Section 3 on, we use the relation to Weyl structures as a tool for the study of the intrinsic geometric structure on \(A\) and its relation to non-linear invariant PDE. Our first main result shows that one has to substantially restrict the class of geometries in order to avoid getting into exotic territory. Recall that for a parabolic subgroup \(P\subset G\) the corresponding Lie subalgebra \(\mathfrak p\subset\mathfrak g\) can be realized as the non-negative part in a grading \(\mathfrak g=\oplus_{i=-k}^k\mathfrak g_i\) of \(\mathfrak g\), which is usually called a \(|k|\)-grading. There is a subclass of parabolic geometries that is often referred to as AHS structures, see e.g. [3, 4, 14], which is the case \(k=1\), see Section 2.2 and 14 for more details. This is exactly the case in which the underlying structure \(\mathcal G_0\to M\) is an ordinary first order \(G_0\)-structure. In particular, there is the notion of intrinsic torsion for this underlying structure. Vanishing of the intrinsic torsion is equivalent to the existence of a torsion free connection compatible with the structure and turns out to be equivalent to torsion-freeness of the Cartan geometry \((p:\mathcal G\to M,\omega)\). Using this background, we can formulate the first main result of Section 3, that we prove as Theorem 3.1:
Theorem 1. Let \((p:\mathcal G\to M,\omega)\) be a parabolic geometry of type \((G,P)\) and \(\pi:A\to M\) its associated bundle of Weyl structures. Then the natural 2-form \(\Omega\in\Omega^2(A)\) is closed if and only if \((G,P)\) corresponds to a \(|1|\)-grading and the Cartan geometry \((p:\mathcal G\to M,\omega)\) is torsion-free.
Hence we restrict our considerations to torsion-free AHS structures from this point on. Apart from projective and conformal structures, this contains also Grassmannian structures of type \((2,n)\) and quaternionic structures, for which there are many non-flat examples. For several other AHS structures, torsion-freeness implies local flatness, but the locally flat case is of particular interest for us anyway. Our next main result, which we prove in Theorem 3.4, vastly generalizes [19]:
Theorem 2. For any torsion-free AHS structure, the pseudo-Riemannian metric \(h\) induced by the canonical almost bi-Lagrangian structure on the bundle \(A\) of Weyl structures is an Einstein metric with non-zero scalar curvature.
While one could prove the aforementioned Theorems on a case by case basis by using the techniques from [19], our arguments instead rely on a careful analysis of the properties of the curvature tensor of the induced connection on \(TA\). Following [28], we next initiate the study of Weyl structures via the geometry of submanifolds in \(A\). We call a Weyl structure \(s : M \to A\) of a torsion-free AHS structure Lagrangian if \(s : M \to (A,\Omega)\) is a Lagrangian submanifold. Likewise, \(s\) is called non-degenerate if \(s : M \to (A,h)\) is a non-degenerate submanifold. We show that a Weyl structure is Lagrangian if and only if its Rho tensor is symmetric and that it is non-degenerate if and only if the symmetric part of its Rho tensor is non-degenerate.
In Theorem 3.7 we characterize Lagrangian Weyl structures that lead to totally geodesic submanifolds \(s(M)\subset A\), which provides a connection to Einstein metrics and reductions of projective holonomy. If \(s\) in addition is non-degenerate, then there is a well defined second fundamental form of \(s(M)\) with respect to any linear connection on \(TA\) that is metric for \(h\) and we show that this admits a natural interpretation as a \(\binom12\)-tensor field on \(M\). In our next main result, Theorem 3.8, we give explicit formulae for the second fundamental forms of the canonical connection and the Levi-Civita connection of \(h\). These are universal formulae in terms of the Weyl connection, the Rho-tensor, and its inverse, which are valid for all torsion-free AHS structures. As an application, we are able to characterize non-degenerate Lagrangian Weyl structures that are minimal submanifolds in \((A,h)\) in terms of a universal PDE. Again, this is a vast generalization of [28], where merely the case of projective structures on surfaces was considered.
In Section 4 we connect our results to the study of fully non-linear invariant PDE on AHS structures. A motivating example arises from the work of E. Calabi. In [7], Calabi related complete affine hyperspheres to solutions of a certain Monge-Ampère equation. This Monge-Ampère equation, when interpreted correctly, is an invariant PDE that one can associate to a projective structure and it is closely linked to properly convex projective manifolds, see [26]. In Theorem 4.3, we relate Calabi’s equation to our equation for a minimal Lagrangian Weyl structure and as Corollary 4.4, we obtain:
Corollary 1. Let \((M,[\nabla])\) be a closed oriented locally flat projective manifold. Then \([\nabla]\) is properly convex if and only if \([\nabla]\) arises from a minimal Lagrangian Weyl structure whose Rho tensor is positive definite.
The convention for the Rho tensor used here is chosen to be consistent with [16]. This convention is natural from a Lie theoretic viewpoint, but differs from the standard definition in projective – and conformal differential geometry by a sign. It should also be noted that a relation between properly convex projective manifolds and minimal Lagrangian submanifolds has been observed previously in [23, 22] (but not in the context of Weyl structures).
The notion of convexity for projective structures is only defined for locally flat structures. The above Corollary thus provides a way to generalize the notion of a properly convex projective structure to a class of projective structures that are possibly curved, namely those arising from a minimal Lagrangian Weyl structure. Going beyond projective geometry, this class of differential geometric structures is well-defined for all torsion-free AHS structures.
We conclude the article by showing that there are analogs of the projective Monge-Ampère equation for other AHS structures, and that these always can be described in terms of the Rho tensor, which provides a relation to submanifold geometry of Weyl structures. These topics will be studied in detail elsewhere.
AČ gratefully acknowledges support by the Austrian Science Fund (FWF): P 33559-N. A part of the research for this article was carried out while TM was visiting Forschungsinstitut für Mathematik (FIM) at ETH Zürich. TM thanks FIM for its hospitality and DFG for partial funding through the priority programme SPP 2026 “Geometry at Infinity”. We also thank M. Dunajski, J. Šilhan and V. Žadn`k for helpful discussions and the anonymous referee for interesting comments that helped improving the article significantly.
This section works in the setting of general parabolic geometries. We assume that the reader is familiar with the the basic concepts and only briefly collect what we need about parabolic geometries and Weyl structures. Then we define the bundle of Weyl structures and identify some of the geometric structures that are naturally induced on its total space. We then prove existence of a canonical connection and explain how these structures can be used as an equivalent encoding of the theory of Weyl structures.
The basic ingredient needed to specify a type of parabolic geometry is a semisimple Lie algebra \(\mathfrak g\) that is endowed with a so-called \(|k|\)-grading. This is a decomposition \[\mathfrak g=\mathfrak g_{-k}\oplus\dots\oplus\mathfrak g_{-1}\oplus\mathfrak g_0\oplus\mathfrak g_1\oplus\dots\oplus\mathfrak g_k\] of \(\mathfrak g\) into a direct sum of linear subspaces such that
\([\mathfrak g_i,\mathfrak g_j]\subset\mathfrak g_{i+j}\), where we agree that \(\mathfrak g_\ell=\{0\}\) for \(|\ell|>k\).
No simple ideal of \(\mathfrak g\) is contained in the subalgebra \(\mathfrak g_0\).
The subalgebra \(\mathfrak p_+=\mathfrak g_1\oplus\dots\oplus\mathfrak g_k\) is generated by \(\mathfrak g_1\).
In particular, this implies that the Lie subalgebra \(\mathfrak g_0\) naturally acts on each of the spaces \(\mathfrak g_i\) via the restriction of the adjoint action. Moreover, \(\mathfrak p:=\mathfrak g_0\oplus\mathfrak p_+\) is a Lie subalgebra of \(\mathfrak g\), which turns out to be a parabolic subalgebra in the sense of representation theory.
Such \(|k|\)-gradings can be easily described in terms of the structure theory of semisimple Lie algebras, see Section 3.2 of [16]. In particular, it turns out that any parabolic subalgebra is obtained in this way and, essentially, the classification of gradings is equivalent to the classification of parabolic subalgebras. Further, the decomposition \(\mathfrak p=\mathfrak g_0\oplus\mathfrak p_+\) is the reductive Levi decomposition, so it is a semi-direct product, \(\mathfrak p_+\) is the nilradical of \(\mathfrak p\), and the subalgebra \(\mathfrak g_0\) is reductive. Of course, also \(\mathfrak g_-:=\mathfrak g_{-k}\oplus\dots\oplus\mathfrak g_{-1}\) is a Lie subalgebra of \(\mathfrak g\), which is nilpotent by the grading property. It turns out that \(\mathfrak g_-\) and \(\mathfrak p_+\) are isomorphic.
Next, one chooses a Lie group \(G\) with Lie algebra \(\mathfrak g\). Then the normalizer of \(\mathfrak p\) in \(G\) has Lie algebra \(\mathfrak p\), and one chooses a closed subgroup \(P\subset G\) lying between this normalizer and its connected component of the identity. The subgroup \(P\) naturally acts on \(\mathfrak g\) and \(\mathfrak p\) via the adjoint action. More generally, one puts \(\mathfrak g^i:=\oplus_{j\geq i}\mathfrak g_j\) to define a filtration of \(\mathfrak g\) by linear subspaces that is invariant under the adjoint action of \(P\). This makes \(\mathfrak g\) into a filtered Lie algebra in the sense that \([\mathfrak g^i,\mathfrak g^j]\subset\mathfrak g^{i+j}\).
Having made these choices, there is the concept of a parabolic geometry of type \((G,P)\) on a manifold \(M\) of dimension \(\dim(G/P)\). This is defined as a Cartan geometry \((p:\mathcal G\to M,\omega)\) of type \((G,P)\), which means that \(p:\mathcal G\to M\) is a principal \(P\)-bundle and that \(\omega\in\Omega^1(\mathcal G,\mathfrak g)\) is a Cartan connection. This in turn means that \(\omega\) is equivariant for the principal right action, so \((r^g)^*\omega=\operatorname{Ad}(g^{-1})\circ\omega\), reproduces the generators of fundamental vector fields, and that \(\omega(u):T_u\mathcal G\to\mathfrak g\) is a linear isomorphism for each \(u\in\mathcal G\). In addition, one requires two conditions on the curvature of \(\omega\), which are called regularity and normality, which we don’t describe in detail.
While Cartan geometries provide a nice uniform description of parabolic geometries, this should be viewed as the result of a theorem rather than a definition. To proceed towards more common descriptions of the geometries, one first observes that the Lie group \(P\) can be decomposed as a semi-direct product. On the one hand, the exponential map restricts to a diffeomorphism from \(\mathfrak p_+\) onto a closed normal subgroup \(P_+\subset P\). On the other hand, one defines a closed subgroup \(G_0\subset P\) as consisting of those elements, whose adjoint action preserves the grading of \(\mathfrak g\) and observes that this has Lie algebra \(\mathfrak g_0\). Then the inclusion of \(G_0\) into \(P\) induces an isomorphism \(G_0\to P/P_+\).
Using this, one can pass from the Cartan geometry \((p:\mathcal G\to M,\omega)\) to an underlying structure by first forming the quotient \(\mathcal G_0:=\mathcal G/P_+\), which is a principal \(G_0\)-bundle. Moreover, for each \(i=-k,\dots,k\), there is a smooth subbundle \(T^i\mathcal G\subset T\mathcal G\) consisting of those tangent vectors that are mapped to \(\mathfrak g^i\subset\mathfrak g\) by \(\omega\). Since \(T^1\mathcal G\) is the vertical bundle of \(\mathcal G\to\mathcal G_0\), these subbundles descend to a filtration \(\{T^i\mathcal G_0:i=-k,\dots,0\}\) of \(T\mathcal G_0\). Moreover, for each \(i<0\), the component of \(\omega\) in \(\mathfrak g_i\) descends define a smooth section of the bundle \(L(T^i\mathcal G_0,\mathfrak g_i)\) of linear maps, so this can be viewed as a partially defined \(\mathfrak g_i\)-valued differential form.
The simplest case here is \(k=1\), for which the geometries in question are often referred to as AHS structures. In this case, one obtains a \(\mathfrak g_{-1}\)-valued one-form \(\theta\) on \(\mathcal G_0\), which is \(G_0\)-equivariant and whose kernel in each point is the vertical subbundle. This means that \((p_0:\mathcal G_0\to M,\theta)\) in this case simply is a classical first order structure corresponding to the adjoint action of \(G_0\) on \(\mathfrak g_{-1}\) (which turns out to be infinitesimally effective). According to a result of Kobayashi and Nagano (see [24]), the resulting class of structures for simple \(\mathfrak g\) is very peculiar, since these are the only irreducible first order structures of finite type, for which the first prolongation is non-trivial. This class contains important examples, like conformal structures, almost quaternionic structures, and almost Grassmannian structures.
For general \(k\), there is an interpretation of \(\mathcal G_0\) and the partially defined forms as a filtered analogue of a first order structure. This involves a filtration of the tangent bundle \(TM\) by smooth subbundles \(T^iM\) for \(i=-k,\dots,-1\) with prescribed (non–)integrability properties together with a reduction of structure group of the associated graded vector bundle to the tangent bundle. This leads to examples like hypersurface-type CR structures, in which the filtration is equivalent to a contact structure, while the reduction of structure group is defined by an almost complex structure on the contact subbundle. Further important example of such structures are path geometries, quaternionic contact structures and various types of generic distributions.
Except for two cases, the Cartan geometry can be uniquely (up to isomorphism) recovered from the underlying structure (see Section 3.1 of [16]), and indeed this defines an equivalence of categories. So in this case, one has two equivalent descriptions of the structure. The two exceptional cases are projective structures and a contact analogue of those. In these cases, the underlying structure contains no information respectively describes only the contact structure, and one in addition has to choose an equivalence class of connections in order to describe the structure. Still, these fit into the general picture with respect to Weyl structures, which we discuss next.
These provide the basic tool to explicitly translate between the description of a parabolic geometry as a Cartan geometry and the picture of the underlying structure. So let us suppose that \((p:\mathcal G\to M,\omega)\) is a Cartan geometry of type \((G,P)\) and that \(p_0:\mathcal G_0\to M\) is the underlying structure described in Section 2.1. The original definition of a Weyl structure used in [15] is as a \(G_0\)-equivariant section \(\sigma\) of the natural projection \(q:\mathcal G\to \mathcal G_0=\mathcal G/P_+\). One shows that such sections always exist globally and by definition, they provide reductions of the principal \(P\)-bundle \(p:\mathcal G\to M\) to the structure group \(G_0\subset P\). As a representation of \(G_0\), the Lie algebra \(\mathfrak g\) splits as \(\mathfrak g_-\oplus\mathfrak g_0\oplus\mathfrak p_+\) (and indeed further according to the \(|k|\)-grading). Thus, the pullback \(\sigma^*\omega\) splits accordingly into a sum of three \(G_0\)-equivariant one-forms with values in \(\mathfrak g_-\), \(\mathfrak g_0\) and \(\mathfrak p_+\), respectively, which then admit nice interpretations in terms of the underlying structure. The \(\mathfrak g_0\)-component defines a principal connection on \(\mathcal G_0\), which induces the Weyl connections on associated bundles. The component in \(\mathfrak p_+\) descends to a one-form on \(M\) with values in the associated graded to the cotangent bundle \(T^*M\), which is the Rho-tensor associated to the Weyl structure. The \(\mathfrak g_-\)-component also descends to \(M\) and provides an isomorphism between the tangent bundle \(TM\) and its associated graded bundle. For the structures we consider in this article, this component coincides with the soldering form that identifies \(\mathcal G_0\) as a reduction of structure group of \(TM\).
As observed in [21], any reduction of \(p:\mathcal G\to M\) to the structure group \(G_0\subset P\) comes from a Weyl structure. This is because the composition of \(q\) with the principal bundle morphism defining such a reduction clearly is an isomorphism of \(G_0\)-principal bundles. Thus one could equivalently define a Weyl structure as such a reduction of structure group and then observe that this defines a \(G_0\)-equivariant section of \(q:\mathcal G\to\mathcal G_0\). It is a classical result that reductions of \(\mathcal G\) to the structure group \(G_0\) can be equivalently described as smooth sections of the associated bundle with fiber \(P/G_0\). This motivates the following definition from [21].
Definition 2.1. The bundle of Weyl structures associated to the parabolic geometry \((p:\mathcal G\to M,\omega)\) is \(\pi:A:=\mathcal G\times_P(P/G_0)\to M\).
The correspondence between Weyl structures and smooth sections of \(\pi:A\to M\) can be easily made explicit. Given a \(G_0\)-equivariant section \(\sigma:\mathcal G_0\to\mathcal G\) one considers the map sending \(u_0\in \mathcal G_0\) to the class of \((\sigma(u_0),eG_0)\) in \(\mathcal G\times_P(P/G_0)\), where \(e\in P\) is the neutral element. By construction, the resulting smooth map \(\mathcal G_0\to A\) is constant on the fibers of \(p_0:\mathcal G_0\to M\) and thus descends to a smooth map \(s:M\to A\), which is a section of \(\pi\) by construction. Conversely, a section \(s\) of \(\pi\) corresponds to a smooth, \(G_0\)-equivariant map \(f:\mathcal G\to P/G_0\) characterized by the fact that \(s(x)\) is the class of \((u,f(u))\) for each \(u\) in the fiber of \(\mathcal G\) over \(x\). But then \(f^{-1}(eG_0)\) is a smooth submanifold of \(\mathcal G\) on which the projection \(q:\mathcal G\to\mathcal G_0\) restricts to a \(G_0\)-equivariant diffeomorphism. The inverse of this diffeomorphism gives the Weyl structure determined by \(s\).
From the definition, we can verify that the bundle of Weyl structures is similar to an affine bundle. This will also provide the well known affine structure on Weyl structures in our picture. To formulate this, recall first that the parabolic subgroup \(P\subset G\) is a semi-direct product of the subgroup \(G_0\subset P\) and the normal subgroup \(P_+\subset P\). In particular, any element \(g\in P\) can be uniquely written as \(g_0g_1\) with \(g_0\in G_0\) and \(g_1\in P_+\), compare with Theorem 3.1.3 of [16], and of course \(g_0g_1=(g_0g_1g_0^{-1})g_0\) provides the corresponding decomposition in the opposite order.
Proposition 2.2. Let \(\pi:A\to M\) be the bundle of Weyl structures associated to a parabolic geometry \((p:\mathcal G\to M,\omega)\). Then sections of \(\pi:A\to M\) can be naturally identified with smooth functions \(f:\mathcal G\to P_+\) such that \(f(u\cdot (g_0g_1))=g_1^{-1}g_0^{-1}f(u)g_0\) for each \(u\in\mathcal G\), \(g_0\in G_0\) and \(g_1\in P_+\).
Fixing one function \(f\) that satisfies this equivariancy condition, any other function which is equivariant in the same way can be written as \(\hat f(u)=f(u)h(u)\), where \(h:\mathcal G\to P_+\) is a smooth function such that \(h(u\cdot(g_0g_1))=g_0^{-1}h(u)g_0\).
Proof. The inclusion \(P_+\hookrightarrow P\) induces a smooth map \(P_+\to P/G_0\), and from the decomposition of elements of \(P\) described above, we readily see that this is surjective. On the other hand, writing the quotient projection \(P\to G_0\) as \(\alpha\), the map \(g\mapsto g\alpha(g)^{-1}\) induces a smooth inverse, so \(P/G_0\) is diffeomorphic to \(P_+\). Since \(A=\mathcal G\times_P(P/G_0)\), smooth sections of \(\pi:A\to M\) are in bijective correspondence with \(P\)-equivariant smooth functions \(\mathcal G\to P/G_0\), so these can be viewed as functions with values in \(P_+\). The equivariancy condition reads as \(f(u\cdot (g_0g_1))=g_1^{-1}g_0^{-1}\cdot f(u)\). But starting from \(\tilde g_1G_0\), we get \(g_1^{-1}g_0^{-1}\tilde g_1G_0=g_1^{-1}g_0^{-1}\tilde g_1g_0G_0\), and \(g_1^{-1}g_0^{-1}\tilde g_1g_0\in P_+\). This completes the proof of the first claim.
Given one function \(f:\mathcal G\to P_+\), of course any other such function can be uniquely written as \(\hat f=fh\) for a smooth function \(h:\mathcal G\to P_+\), so it remains to understand \(P\)-equivariance. What we assume is that \(f(u\cdot(g_0g_1))= g_1^{-1}g_0^{-1}f(u)g_0\) and we want \(\hat f\) to satisfy the analogous equivariancy condition. But this exactly requires that \(g_1^{-1}g_0^{-1}f(u)g_0h(u\cdot(g_0g_1))= g_1^{-1}g_0^{-1}f(u)h(u)g_0\), which is equivalent to the claimed equivariancy of \(h\). ◻
To connect to the well-known affine structure on the set of Weyl structures, we observe two alternative ways to express things using the exponential map. On the one hand, we have observed above that \(\exp:\mathfrak p_+\to P_+\) is a diffeomorphism. Thus we can write \(h(u)=\exp(\Upsilon(u))\) and equivariancy of \(h\) is equivalent to \(\Upsilon(u\cdot(g_0g_1))=\operatorname{Ad}(g_0)^{-1}(\Upsilon(u))\). On the other hand, in the proof of Theorem 3.1.3 of [16] it shown that also \((Z_1,\dots,Z_k)\mapsto\exp(Z_1)\cdots\exp(Z_k)\) defines a diffeomorphism \(\mathfrak g_1\oplus\dots\oplus \mathfrak g_k\to P_+\). Correspondingly, we can write \(h(u)=\exp(\Upsilon_1(u))\cdots\exp(\Upsilon_k(u))\) where \(\Upsilon_i:\mathcal G\to\mathfrak g_i\) is a smooth map for each \(i=1,\dots,k\). Again, equivariancy of \(h\) translates to \(\Upsilon_i(u\cdot(g_0g_1))=\operatorname{Ad}(g_0)^{-1}(\Upsilon_i(u))\) for each \(i\).
There is also a nice global way to express the affine structure. The filtration of \(TM\) induced by a parabolic geometry dualizes to a filtration of the cotangent bundle \(T^*M\) and we can form the associated graded bundle \(\operatorname{gr}(T^*M)\). The general theory implies that this can be realized as \(\mathcal G\times_{P}\operatorname{gr}(\mathfrak p_+)\cong\mathcal G_0\times_{G_0}\mathfrak p_+\).
Proposition 2.3. Let \(\pi:A\to M\) be the bundle of Weyl structures associated to a parabolic geometry \((p:\mathcal G\to M,\omega)\). Then for any smooth section \(s\) of \(\pi\), there is an induced diffeomorphism \(\varphi_s:T^*M\to A\).
Proof. Let \(\sigma:\mathcal G_0\to\mathcal G\) be the \(G_0\)-equivariant section determined by \(s\). Since \(\exp:\mathfrak p_+\to P_+\) is a diffeomorphism, we conclude that \(\Phi_s(u_0,Z):=\sigma(u_0)\exp(Z)\) defines a diffeomorphism \(\Phi_s:\mathcal G_0\times\mathfrak p_+\to \mathcal G\). Given \(g_0\in G_0\), the definition readily implies that \(\Phi_s(u\cdot g_0,\operatorname{Ad}(g_0^{-1})(Z))=\Phi_s(u_0,Z)\cdot g_0\). Hence there is an induced diffeomorphisms between the orbit spaces \(\operatorname{gr}(T^*M)=\mathcal G_0\times_{G_0}\mathfrak p_+\) and \(A=\mathcal G_0/G_0\). ◻
It was shown in [21] that the parabolic geometry \((p:\mathcal G\to M,\omega)\) gives rise to a connection on the tangent bundle \(TA\) of \(A\). The argument used to obtain this connection is rather intricate: There is the opposite parabolic subgroup \(P^{op}\) to \(P\) which corresponds to the Lie subalgebra \(\mathfrak g_-\oplus\mathfrak g_0\subset\mathfrak g\) and one considers the homogeneous space \(G/P^{op}\). Restricting the \(G\)-action to \(P\) and forming the associated bundle \(\mathcal G\times_P(G/P^{op})\) the Cartan connection \(\omega\) induces a natural affine connection on the total space of this bundle. It is then easy to see that \(P\cap P^{op}=G_0\), so acting with \(P\) on \(eP^{op}\) defines a \(P\)-equivariant open embedding \(A\to\mathcal G\times_P(G/P^{op})\), thus providing a connection on \(TA\) as claimed. Our first main result provides a more conceptual description of this connection, which directly implies compatibility with several additional geometric structures on \(A\).
Proposition 2.4. The canonical projection \(\mathcal G\to A\) is a \(G_0\)-principal bundle and \(\omega\) defines a Cartan connection on that bundle, so \((\mathcal G\to A,\omega)\) is a Cartan geometry of type \((G,G_0)\). In particular, the \(\mathfrak g_0\)-component of \(\omega\) defines a canonical principal connection on \(\mathcal G\to A\) and \(TA\cong\mathcal G\times_{G_0}(\mathfrak g/\mathfrak g_0)\), so this inherits a canonical linear connection. Finally, there is a natural splitting \(TA=L^-\oplus L^+\) into a direct sum of two subbundles of rank \(\dim(M)\), which is parallel for the connection and such that \(L^+\) is the vertical bundle of \(\pi\).
Proof. Mapping \(u\in\mathcal G\) to the class of \((u,eG_0)\) in \(\mathcal G\times_P(P/G_0)\) is immediately seen to be surjective and its fibers coincide with the orbits of \(G_0\) on \(\mathcal G\). Hence one obtains an identification of \(\mathcal G/G_0\) with \(A\), and it is well known that this makes the projection \(\mathcal G\to A\) into a \(G_0\)-principal bundle. The defining properties of \(\omega\) for the group \(P\) and the Lie algebra \(\mathfrak p\) then imply the corresponding properties for the group \(G_0\) and the Lie algebra \(\mathfrak g_0\), so \(\omega\) defines a Cartan connection on \(\mathcal G\to A\).
As a representation of \(G_0\), we get \(\mathfrak g=\mathfrak g_0\oplus(\mathfrak g_-\oplus\mathfrak p_+)\). This means that we have given a \(G_0\)-invariant complement to \(\mathfrak g_0\) in \(\mathfrak g\). Decomposing \(\omega\) accordingly, the component \(\omega_0\) in \(\mathfrak g_0\) is \(G_0\)-equivariant, thus defining a principal connection on \(\mathcal G\to A\), which induces linear connections on all associated vector bundles. Moreover, since \(\omega\) is a Cartan connection on \(\mathcal G\to A\), we can identify \(TA\) with the associated vector bundle \[\mathcal G\times_{G_0}(\mathfrak g/\mathfrak g_0)\cong\mathcal G\times_{G_0}(\mathfrak g_-\oplus\mathfrak p_+).\] This readily implies both the existence of a natural connection and of a compatible decomposition of \(TA\) with \(L^-=\mathcal G\times_{G_0}\mathfrak g_-\) and \(L^+=\mathcal G\times_{G_0}\mathfrak p_+\). The tangent map \(T\pi:TA\to TM\) is induced by the projection \(\mathfrak g/\mathfrak g_0\to\mathfrak g/\mathfrak p\). Identifying \(\mathfrak g/\mathfrak g_0\) with \(\mathfrak g_-\oplus\mathfrak p_+\) the kernel of this projection is \(\mathfrak p_+\), which shows that \(L^+\subset TA\) coincides with \(\ker(T\pi)\). ◻
This result also gives us a basic supply of natural vector bundles on \(A\), namely the vector bundles associated to the principal bundle \(\mathcal G\to A\) via representations of \(G_0\). Moreover, the principal connection on that bundle coming from \(\omega_0\) gives rise to an induced linear connection on each of these associated bundles. We will denote all these induced connections by \(D\). Given an associated bundle \(E\to A\), we can view \(D\) as an operator \(D:\Gamma(E)\to\Gamma(T^*A\otimes E)\). Of course the splitting \(TA=L^-\oplus L^+\) from Proposition 2.4 induces an analogous splitting of \(T^*A\), which allows us to split \(D\) into two partial connections \(D=D^-\oplus D^+\). Here \(D^\pm:\Gamma(E)\to\Gamma((L^\pm)^*\otimes E)\). Viewing \(D\) as a covariant derivative, \(D^\pm\) is defined by differentiating only in directions of the corresponding subbundle of \(TA\).
Recall that the natural vector bundles for the parabolic geometry \((p:\mathcal G\to M,\omega)\) are the associated vector bundles of the form \(\mathcal VM=\mathcal G\times_P\mathbb V\) for representations \(\mathbb V\) of \(P\). Throughout this article, we will only consider the case that the center \(Z(G_0)\) of the subgroup \(G_0\subset P\) acts diagonalizably on \(\mathbb V\). Together with the fact that \(G_0\) is reductive, this implies that \(\mathbb V\) is completely reducible as a representation of \(G_0\). One important subclass of natural bundles is formed by completely reducible bundles that correspond to representations of \(P\) on which the subgroup \(P_+\subset P\) acts trivially, which is equivalent to complete reducibility as a representation of \(P\). On the other hand, there are tractor bundles which correspond to restrictions to \(P\) of representations of \(G\).
Any representation \(\mathbb V\) of \(P\) can naturally be endowed with a \(P\)-invariant filtration of the form \(\mathbb V=\mathbb V^0\supset\mathbb V^1\supset\dots\supset\mathbb V^N\) as follows (see Section 3.2.12 of [16]). The smallest component \(\mathbb V^N\) consists of those elements, on which \(\mathfrak p_+\) acts trivially under the infinitesimal action. The larger components are characterized iteratively by the fact that \(v\in\mathbb V^j\) if and only if it is sent to \(\mathbb V^{j+1}\) by the action of any element of \(\mathfrak p_+\). Then one defines the associated graded representation \(\operatorname{gr}(\mathbb V):=\oplus_{i=0}^N\operatorname{gr}_i(\mathbb V)\) with \(\operatorname{gr}_i(\mathbb V):=(\mathbb V^i/\mathbb V^{i+1})\) and \(\mathbb V^{N+1}=\{0\}\). By construction, this is a completely reducible representation of \(P\).
As an important special case, consider the restriction of the adjoint representation of \(G\) to \(P\). Then it turns out that, up to a shift in degree, the canonical \(P\)-invariant filtration is exactly the filtration \(\{\mathfrak g^i\}\) derived from the \(|k|\)-grading of \(\mathfrak g\) as in Section 2.1. In particular, this implies that \(\mathfrak g^2=[\mathfrak p_+,\mathfrak p_+]\) and similarly, the higher filtrations components form the lower central series of \(\mathfrak p_+\). Using this it is easy to see that the natural filtration on any representation \(\mathbb V\) of \(P\) has the property that \(\mathfrak g^i\cdot\mathbb V^j\subset\mathbb V^{i+j}\) for all \(i,j\geq 0\) under the infinitesimal representation of \(\mathfrak p=\mathfrak g^0\). This readily implies that there is a natural action of the associated graded \(\operatorname{gr}(\mathfrak p)\) on \(\operatorname{gr}(\mathbb{V} )\), which is compatible with the grading. Since the filtration of \(\mathfrak p\) is induced by the (non-negative part of the) grading on \(\mathfrak g\), we can identify \(\operatorname{gr}(\mathfrak p)\) with \(\mathfrak p\) via the inclusion of \(\mathfrak g_i\) into \(\mathfrak g^i\). Altogether, we get, for each \(i,j\geq 0\), bilinear maps \(\mathfrak g_i\times\operatorname{gr}_j(\mathbb V)\to\operatorname{gr}_{i+j}(\mathbb V)\), which are \(P\)-equivariant (with trivial action of \(P_+\)) by construction.
As a representation of the subgroup \(G_0\subset P\), the associated graded \(\operatorname{gr}(\mathbb V)\) is isomorphic to \(\mathbb V\). Indeed, we have observed above that \(\mathbb V\) is completely reducible as a representation of \(G_0\), so the same holds for each of the subrepresentations \(\mathbb V^j\subset\mathbb V\). In particular, there always is a \(G_0\)-invariant complement \(\mathbb V_j\) to the invariant subspace \(\mathbb V^{j+1}\subset\mathbb V^j\) and we put \(\mathbb V_N=\mathbb V^N\). By construction, we on the one hand get \(\mathbb V\cong\oplus\mathbb V_j\) and on the other hand \(\mathbb V_j\cong\mathbb V^j/\mathbb V^{j+1}\) which implies that claimed statement. Otherwise put, one can interpret the passage from \(\mathbb V\) to \(\operatorname{gr}(\mathbb V)\) as keeping the restriction to \(G_0\) of the \(P\)-action on \(\mathbb V\) and extending this by the trivial action of \(P_+\) to a new action of \(P\).
The construction of the associated graded has a direct counterpart on the level of associated bundles. Putting \(\mathcal VM:=\mathcal G\times_P\mathbb V\to M\), any of the filtration components \(\mathbb V^i\) defines a smooth subbundle \(\mathcal V^iM:=\mathcal G\times_P\mathbb V^i\to M\). Thus \(\mathcal VM\) is filtered by the smooth subbundles \(\mathcal V^iM\) and we can form the associated graded vector bundle \(\operatorname{gr}(\mathcal VM)=\oplus (\mathcal V^iM/\mathcal V^{i+1}M)\). It is easy to see that this can be identified with the associated bundle \(\mathcal G\times_P\operatorname{gr}(\mathbb V)\). However, the fact that \(\mathbb V\) and \(\operatorname{gr}(\mathbb V)\) are isomorphic as representations of \(G_0\) does not have a geometric interpretation without making additional choices. Hence on the level of associated bundles, it is very important to carefully distinguish between a filtered vector bundle and its associated graded.
Any representation \(\mathbb V\) of \(P\) defines a representation of \(G_0\) by restriction. Hence denoting by \(\pi:A\to M\) the bundle of Weyl structures, \(\mathbb V\) also gives rise to a natural vector bundle over \(A\) that we denote by \(\mathcal VA:=\mathcal G\times_{G_0}\mathbb V\to A\). Some information is lost in that process, however, for example \(\mathcal G\times_{G_0}\mathbb V\cong\mathcal G\times_{G_0}\operatorname{gr}(\mathbb V)\) for any representation \(\mathbb V\) of \(P\). Next, sections of \(\mathcal VA\to A\) can be naturally identified with smooth functions \(\mathcal G\to\mathbb V\) that are \(G_0\)-equivariant. Similarly, sections of \(\mathcal VM\to M\) are in bijective correspondence with smooth functions \(\mathcal G\to\mathbb V\), which are \(P\)-equivariant. Thus we see that there is a natural inclusion of \(\Gamma(\mathcal VM\to M)\) as a linear subspace of \(\Gamma(\mathcal VA\to A)\). We will denote this by putting a tilde over the name of a section of \(\mathcal VM\to M\) in order to indicate the corresponding section of \(\mathcal VA\to A\). So both the sections of \(\mathcal VM\to M\) and of its associated graded vector bundle can be interpreted as (different) subspaces of the space of sections of \(\mathcal VA\to A\).
Now we can describe the relations of bundles and sections explicitly.
Theorem 2.5. Let \((p:\mathcal G\to M,\omega)\) be a parabolic geometry of type \((G,P)\) and let \(\pi:A\to M\) be the corresponding bundle of Weyl structures. Fix a representation \(\mathbb V\) of \(P\) and consider the corresponding natural bundles \(\mathcal VM=\mathcal G\times_P\mathbb V\to M\) and \(\mathcal VA=\mathcal G\times_{G_0}\mathbb V\to A\). Then we have:
(1) \(\mathcal VA\) can be naturally identified with the pullback bundle \(\pi^*\mathcal VM\). In particular, \(L^-\cong\pi^*TM\) and \(L^+\cong\pi^*T^*M\).
(2) The operation \(\sigma\mapsto\tilde\sigma\) identifies \(\Gamma(\mathcal VM\to M)\) with the subspace of \(\Gamma(\mathcal VA\to A)\) consisting of those sections \(\tau\) for which \(D^+_{\varphi}\tau=-\varphi\bullet\tau\) for all \(\varphi\in\Gamma(L^+)\). Here \(\bullet:L^+\times\mathcal VA\to\mathcal VA\) is induced by the infinitesimal representation \(\mathfrak p_+\times\mathbb V\to\mathbb V\).
In particular, for a completely reducible bundle \(\mathcal VM\), \(\tilde\sigma=\pi^*\sigma\) and the image consists of all sections that are parallel for \(D^+\).
(3) Any section \(s:M\to A\) of \(\pi\) determines a natural pullback operator \(s^*:\Gamma(\mathcal VA\to A)\to\Gamma(\operatorname{gr}(\mathcal VM)\to M)\). In particular, choosing \(s\), \(\sigma\mapsto s^*\tilde\sigma\) defines a map \(\Gamma(\mathcal VM)\to\Gamma(\operatorname{gr}(\mathcal VM))\). This map is induced by a vector bundle isomorphism \(\mathcal VM\to\operatorname{gr}(\mathcal VM)\) that coincides with the isomorphism determined by the Weyl structure corresponding to \(s\) as in Section 5.1.3 of [16].
Proof. (1) follows directly from the construction: Mapping a \(G_0\)-orbit in \(\mathcal G\times\mathbb V\) to the \(P\)-orbit it generates, defines a bundle map \(\mathcal VA\to\mathcal VM\) with base map \(\pi:A\to M\). This evidently restricts to a linear isomorphism in each fiber and hence defines an isomorphism \(\mathcal VA\to\pi^*\mathcal VM\). The second statement follows from the well known facts that \(TM\cong\mathcal G\times_P(\mathfrak g/\mathfrak p)\) and \(T^*M\cong\mathcal G\times_P\mathfrak p_+\) and the fact that \(\mathfrak g/\mathfrak p\cong\mathfrak g_-\) as a representation of \(G_0\).
(2) Since \(P\) is a semi-direct product, \(P\)-equivariancy of a function is equivalent to equivariancy under \(G_0\) and \(P_+\) and equivariancy under \(P_+\) is equivalent to equivariancy for the infinitesimal action of \(\mathfrak p_+\). Hence for a \(G_0\)-equivariant function \(f:\mathcal G\to\mathbb V\), \(P\)-equivariancy is equivalent to the fact that for each \(u\in\mathcal G\) and \(Z\in\mathfrak p_+\) with fundamental vector field \(\zeta_Z\), we get \(\zeta_Z(u)\cdot f=Z\cdot f(u)\). Here in the left hand side the vector field differentiates the function, while in the right hand side we use the infinitesimal representation of \(\mathfrak p_+\) on \(\mathbb V\). Suppose that \(u\) projects to \(y\in A\). Then by definition, \(\zeta_Z(u)\) is the horizontal lift with respect to \(D\) of a tangent vector \(\varphi\in L^+_y\subset T_yA\). Hence \(\zeta_Z(u)\cdot f\) represents \(D_\varphi\tau(y)=D^+_\varphi\tau(y)\) in the, while \(Z\cdot f(u)\) of course represents \(\varphi\bullet\tau(y)\).
In the case of a completely reducible bundle, \(\bullet\) is the zero map, so we see that our subspace coincides with the \(D^+\)-parallel sections. On the other hand, for any section \(\sigma\in\Gamma(\mathcal VM)\), the pullback \(\pi^*\sigma\) is constant along the fibers of \(\pi\). Since we know from Proposition 2.4 that \(L^+\) is the vertical subbundle of \(\pi\), this implies that \(\pi^*\sigma=\tilde\sigma\).
(3) As we have noted already, for any representation \(\mathbb V\) of \(P\), the associated graded \(\operatorname{gr}(\mathbb V)\) is isomorphic to \(\mathbb V\) as a representation of \(G_0\). Thus we conclude from (1) that we can not only identify \(\mathcal VA\) with the pullback of \(\mathcal VM\) but also with the pullback of the associated graded vector bundle \(\operatorname{gr}(\mathcal VM)\). Hence for a smooth section \(s:M\to A\) and a point \(x\in M\), we can naturally identify the fiber \(\mathcal V_{s(x)}A\) with the fiber over \(x\) of \(\operatorname{gr}(\mathcal VM)\). This provides a pullback operator \(s^*:\Gamma(\mathcal VA)\to\Gamma(\operatorname{gr}(\mathcal VM))\), so \(\sigma\mapsto s^*\tilde\sigma\) defines an operator \(\Gamma(\mathcal VM)\to\Gamma(\operatorname{gr}(\mathcal VM))\). This operator is evidently linear over \(C^\infty(M,\mathbb R)\) and thus induced by a vector bundle homomorphism \(\mathcal VM\to\operatorname{gr}(\mathcal VM)\) with base map \(\operatorname{id}_M\). Suppose that for \(\sigma\in\Gamma(\mathcal VM)\) and \(x\in M\) we have \((s^*\tilde\sigma)(x)=0\). Then the function \(f:\mathcal G\to\mathbb V\) which corresponds to both \(\sigma\) and \(\tilde\sigma\) has to vanish along the fiber of \(\mathcal G\to A\) over \(s(x)\). But \(P\)-equivariancy then implies that \(f\) vanishes along the fiber of \(\mathcal G\to M\) over \(x\), so \(\sigma(x)=0\). This implies that our bundle map is injective in each fiber and since both bundles have the same rank it is an isomorphism of vector bundles.
The standard description of the isomorphism \(\mathcal VM\to\operatorname{gr}(\mathcal VM)\) induced by a Weyl structure is actually also phrased in the language of sections; Given the \(P\)-equivariant function \(f:\mathcal G\to\mathbb V\) corresponding to \(\sigma\) and the \(G_0\)-equivariant section \(\overline{s}:\mathcal G_0\to\mathcal G\) determined by \(s\), one considers the \(G_0\)-equivariant function \(f\circ\overline{s}\). This describes a section of \(\mathcal G_0\times_{G_0}\mathbb V\cong\mathcal G_0\times_{G_0}\operatorname{gr}(\mathbb V)\). Going through the identifications, it is clear that this coincides with the isomorphism described above. ◻
Remark 6. (1) In principle, the pullback operation defined in part (3) of Theorem 2.5 could also be interpreted as having values in \(\Gamma(\mathcal VM\to M)\). Since \(\mathcal VA\) does not contain any information about the \(\mathfrak p_+\)-action on \(\mathbb V\), the interpretation with values in \(\Gamma(\operatorname{gr}(\mathcal VM)\to M)\) seems much more natural to us.
(2) The comparison to the standard description of Weyl structures in part (3) of the theorem also implies how the isomorphisms \(\mathcal VM\to\operatorname{gr}(\mathcal VM)\) induced by sections \(s\) of \(A\to M\) are compatible with the affine structure on the space of these sections from Proposition 2.2, compare with Proposition 5.1.5 of [16]. It is also easy to give a direct proof of this result in our picture. One just has to interpret the affine structure in terms of sections of \(L^+\to A\) and then use the obvious solution of the differential equation \(D^+_\varphi\tau=\varphi\bullet\tau\) for appropriate sections \(\varphi\).
We next describe the interpretation of Weyl connections in our picture. At the same time, we obtain a nice description of the Rho-corrected derivative associated to a Weyl structure, that was first introduced in [10], see Section 5.1.9 of [16] for a discussion. The Rho-corrected derivative comes from a principal connection on \(\mathcal G\) determined by an equivariant section \(\sigma:\mathcal G_0\to\mathcal G\). One takes the component of \(\omega\) in \(\mathfrak p\) along the image of \(\sigma\) and extends it equivariantly to a principal connection. The name "Rho-corrected derivative" comes from the explicit formula of this derivative in terms of Weyl connection an the Rho-tensor. To obtain our description, we first observe that the pullback operation from part (3) of Theorem 2.5 clearly extends to differential forms with values in a natural vector bundle. Let \(\mathbb V\) be a representation of \(P\) with corresponding natural bundles \(\mathcal VM\to M\) and \(\mathcal VA\to A\). Then one can pull back a \(\mathcal VA\)-valued \(k\) form \(\varphi\) on \(A\) along a section \(s:M\to A\) to a \(\operatorname{gr}(\mathcal VM)\)-valued \(k\)-form \(s^*\varphi\) on \(M\) in an obvious way.
Theorem 2.6. Let \(\mathbb V\) be a representation of \(P\) and let \(\mathcal VM\to M\) and \(\mathcal VA\to A\) be the corresponding natural bundles. For \(\sigma\in\Gamma(\mathcal VM)\) consider the natural lift \(\tilde\sigma\in\Gamma(\mathcal VA)\). For a smooth section \(s:M\to A\) let \(\nabla^s\) be the Weyl connection of the Weyl structure determined by \(s\). Let \(\xi\in\mathfrak X(M)\) be a vector field with natural lift \(\tilde\xi\in\Gamma(L^-)\).
(1) The pullback \(s^*D\tilde\sigma\in\Omega^1(M,\operatorname{gr}(\mathcal VM))\) of \(D\tilde\sigma\in\Omega^1(A,\mathcal VA)\) coincides with the image of \(\nabla^s\sigma\in\Omega^1(M,\mathcal VM)\) under the isomorphism \(\mathcal VM\to\operatorname{gr}(\mathcal VM)\) induced by \(s\) as in Theorem 2.5.
(2) The pullback \(s^*(D^-_{\tilde\xi}\tilde\sigma)\in\Gamma(\operatorname{gr}(\mathcal VM))\) coincides with the image of the Rho-corrected derivative \(\nabla^{\mbox{\textsf{P}}}_\xi\sigma\in\Gamma(\mathcal VM)\) under the isomorphism induced by \(s\) as in Theorem 2.5.
Proof. Let \(\bar s:\mathcal G_0\to\mathcal G\) be the \(G_0\)-equivariant section corresponding to \(s\). For a point \(x\in M\), an element \(u\in\mathcal G\) with \(p(u)=x\) lies in the image of \(\bar s\) if and only if \(u\) projects to \(s(x)\in A\). Assuming this, put \(u_0=q(u)\) where \(q:\mathcal G\to\mathcal G_0\) is the projection, so \(u=\bar s(u_0)\). To compute \(\nabla^s\), we need the horizontal lift \(\hat\xi\in\mathfrak X(\mathcal G_0)\) of \(\xi\) for the principal connection \(\bar s^*\omega_0\). This is characterized by the fact that \(\hat\xi(u_0)\) projects onto \(\xi(x)\) and that \(\omega(u)(T_{u_0}\bar s\cdot\hat\xi(u_0))\) has vanishing \(\mathfrak g_0\)-component. But by construction \(T_{u_0}\bar s\cdot\hat\xi(u_0)\) projects onto \(T_xs\cdot\xi(x)\) and so vanishing of the \(\mathfrak g_0\)-component implies that this is the horizontal lift of \(T_xs\cdot\xi(x)\) in \(u\) corresponding to the principal connection \(\omega_0\) that induces \(D\). From this, (1) follows immediately.
The argument for (2) is closely similar. By definition, \(\tilde\xi(s(x))\) is the unique tangent vector that lies in \(L^-\) and projects onto \(\xi(x)\). The \(D\)-horizontal lift of this tangent vector in \(u\), by construction, is mapped to \(\mathfrak g_-\) by \(\omega\) and projects onto \(\xi(x)\in T_xM\). But this is exactly the characterizing property of the horizontal lift with respect to the principal connection \(\gamma^{\bar s}\) used in Section 5.1.9 of [16] to define the Rho-corrected derivative. Thus the restriction of the \(G_0\)-equivariant function \(\mathcal G\to\mathbb V\) representing \(D^-_{\tilde\xi}\tilde\sigma\) to \(\bar s(\mathcal G_0)\) coincides with the restriction of the \(P\)-equivariant function representing \(\nabla^{\mbox{\textsf{P}}}_\xi\sigma\) and the claim follows from Theorem 2.5. ◻
Using the pullback of bundle valued forms, we can also describe the Rho tensor in our picture. Recall that we use the convention of [15] and [16] for Rho tensors in the setting of general parabolic geometries, which differ by sign from the standard conventions for projective and conformal structures.
Proposition 2.7. Let us view the projection \(TA\to L^+\) as \(\mbox{\textsf{P}}\in\Omega^1(A,L^+)\). Then for each smooth section \(s:M\to A\), the pullback \(s^*\mbox{\textsf{P}}\in\Omega^1(M,\operatorname{gr}(T^*M))\) coincides with the Rho-tensor of the Weyl structure determined by \(s\) as defined in Section 5.1.2 of [16].
Proof. Take a point \(x\in M\), a tangent vector \(\xi\in T_xM\) and consider \(T_xs\cdot\xi\in T_{s(x)}A\). Choose a point \(u\in\mathcal G\) over \(s(x)\) and consider its image \(u_0=q(u)\in\mathcal G_0\). Since \(u\) projects to \(s(x)\), it lies in the image of the \(G_0\)-equivariant section \(\bar s:\mathcal G_0\to\mathcal G\) determined by \(s\), so \(u=\bar s(u_0)\). Taking a tangent vector \(\hat\xi\in T_{u_0}\mathcal G_0\), the tangent vector \(T_{u_0}\bar s\cdot\hat\xi\in T_u\mathcal G\), by construction, projects onto \(T_xs\cdot\xi\in T_{s(x)}A\). But then, by definition, the \(L^+\) component of \(T_xs\cdot\xi\) is obtained by projecting \(\omega(u)^{-1}(\omega_+(T_{u_0}\bar s\cdot\hat\xi))\) to \(T_{s(x)}A\), where \(\omega_+\) denotes the \(\mathfrak p_+\)-component of the Cartan connection \(\omega\). But the Rho-tensor of \(\bar s\) is defined as the \(\operatorname{gr}(T^*M)\)-valued form induced by the \(G_0\)-equivariant form \(\bar s^*\omega_+\), which completes the argument. ◻
Definition 2.8. The form \(\mbox{\textsf{P}}\in\Omega^1(A,L^+)\) defined by the projection \(TA\to L^+\) is called the universal Rho-tensor of the parabolic geometry \((p:\mathcal G\to M,\omega)\).
The curvature \(K\in\Omega^2(\mathcal G,\mathfrak g)\) of the Cartan connection \(\omega\) is defined by \(K(\xi,\eta)=d\omega(\xi,\eta)+[\omega(\xi),\omega(\eta)]\) for \(\xi,\eta\in\mathfrak X(\mathcal G)\). Since \(K\) is horizontal and \(P\)-equivariant, it can be interpreted as \(\kappa\in\Omega^2(M,\mathcal AM)\), where \(\mathcal AM=\mathcal G\times_P\mathfrak g\) is the adjoint tractor bundle. In the same way, we can interpret it as a two-form on \(A\) with values in the associated bundle \(\mathcal G\times_{G_0}\mathfrak g\). Since \(K\) is horizontal over \(M\), it follows that this two form vanishes upon insertion of one tangent vector from \(L^+\subset TA\). In view of the \(G_0\)-invariant decomposition \(\mathfrak g=\mathfrak g_-\oplus\mathfrak g_0\oplus\mathfrak p_+\) we can decompose that two-form further. To do this, we denote by \(\operatorname{End}_0(TA)\) the associated bundle \(\mathcal G\times_{G_0}\mathfrak g_0\). Via the adjoint action, this can naturally be viewed as a subbundle of \(L(TA,TA)\).
Definition 2.9. The components \(T\in \Omega^2(A,L^-)\), \(W\in\Omega^2(A,\operatorname{End}_0(TA))\) and \(Y\in \Omega^2(A,L^+)\) of the two form on \(A\) induced by \(K\) are called the universal torsion, the universal Weyl curvature and the universal Cotton-York tensor of the parabolic geometry \((p:\mathcal G\to M,\omega)\).
The following result follows directly from the definitions.
Proposition 2.10. For any smooth section \(s:M\to A\), the pullbacks \(s^*T\in\Omega^2(M,\operatorname{gr}(TM))\), \(s^*W\in\Omega^2(M,\operatorname{End}_0(TM))\) and \(s^*Y\in\Omega^2(M,\operatorname{gr}(T^*M))\) correspond to the components of the Cartan curvature \(\kappa\in\Omega^2(M,\mathcal AM)\) under the isomorphism \(\mathcal AM\cong\operatorname{gr}(\mathcal AM)\cong \operatorname{gr}(TM)\oplus\operatorname{End}_0(TM)\oplus\operatorname{gr}(T^*M)\) induced by the Weyl structure determined by \(s\).
These quantities are related to data associated to the Weyl structure determined by \(s\) in Section 5.2.9 of [16] and these results can be easily recovered in the current context.
On the level of \(A\), the best way to interpret the components of the Cartan curvature is via the torsion and curvature of the canonical connection \(D\). This interpretation will also be crucial for the analysis of the intrinsic geometric structure on \(A\) in Section 3 below. To formulate the result, we need a bit more notation. The Lie bracket is a \(G\)-equivariant, skew symmetric bilinear map \(\mathfrak g\times\mathfrak g\to\mathfrak g\). Now we can restrict this to entries from \(\mathfrak g_-\oplus\mathfrak p_+\) and then decompose the values according to \(\mathfrak g=(\mathfrak g_-\oplus\mathfrak p_+)\oplus\mathfrak g_0\), and the result will still be \(G_0\)-equivariant. The first component induces a two-form on \(A\) with values in \(TA\) which we denote by \(\{\ ,\ \}\). Similarly, the \(\mathfrak g_0\)-component of the bracket defines a two-form \(\{\ ,\ \}_0\) on \(A\) with values in \(\operatorname{End}_0(TA)\). Using this, we formulate
Theorem 2.11. Let \(A\to M\) be the bundle of Weyl structures associated to a parabolic geometry, and let \(D\) be the canonical connection on \(TA\). Let \(\tau\in\Omega^2(A,TA)\) be the torsion and \(\rho\in\Omega^2(A,L(TA,TA))\) be the curvature of \(D\). Then we have:
(1) The \(TA\)-valued two form \(\tau+\{\ ,\ \}\) vanishes upon insertion of one section of \(L^+\). On \(\Lambda^2L^-\), its components in \(L^-\) and \(L^+\) are the tensors \(T\) and \(Y\) from Definition 2.9, respectively.
(2) The curvature \(\rho\) has values in \(\operatorname{End}_0(TA)\subset L(TA,TA)\). Moreover, \(\rho+\{\ ,\ \}_0\) vanishes upon insertion of one section of \(L^+\) and coincides with the tensor \(W\) from Definition 2.9 on \(\Lambda^2L^-\).
Proof. This follows from well known results on the curvature and torsion of the affine connection induced by a reductive Cartan geometry. For \(\xi\in\mathfrak X(A)\), let \(\xi^h\in\mathfrak X(\mathcal G)\) be the horizontal lift. Then \(\omega(\xi^h):\mathcal G\to (\mathfrak g_-\oplus\mathfrak p_+)\) is the equivariant function corresponding to \(\xi\). Taking a second field \(\eta\), the bracket \([\xi^h,\eta^h]\) lifts \([\xi,\eta]\) so \(\omega_{\pm}([\xi^h,\eta^h])\) is the equivariant function representing \([\xi,\eta]\).
(1) From these considerations and the definition of the exterior derivative, it follows readily that \(d\omega_{\pm}(\xi^h,\eta^h)\) is the equivariant function representing \(\tau(\xi,\eta)\). On the other hand, the component of \([\omega(\xi^h),\omega(\eta^h)]\) in \(\mathfrak g_-\oplus\mathfrak p_+\) of course represents \(\{\xi,\eta\}\), so the claim follows from the definition of the curvature of a Cartan connection.
(2) It is also well known that \(-\omega_0([\xi^h,\eta^h])\) is the function representing \(\rho(\xi,\eta)\). Since the \(\mathfrak g_0\)-component of \([\omega(\xi^h),\omega(\eta^h)]\) clearly represents \(\{\xi,\eta\}_0\), the result again follows from the definition of the Cartan curvature. ◻
From here on, we take a different point of view. We study the geometry on the total space of the bundle of Weyl structures associated to a parabolic geometry from an intrinsic point of view, using the relation to parabolic geometries and Weyl structures as technical input. We shall see below that these structures become rather exotic in the case of general gradings, so we will restrict to parabolic geometries associated to \(|1|\)-gradings soon.
Consider a parabolic geometry \((p:\mathcal G\to M,\omega)\) of some type \((G,P)\) and let \(\pi:A\to M\) the associated bundle of Weyl structures. As we have noted in Section 2.2, the tangent bundle \(TA\) decomposes as \(L^-\oplus L^+\), where \(L^-=\mathcal G\times_{G_0}\mathfrak g_-\) and \(L^+=\mathcal G\times_{G_0}\mathfrak p_+\). It is also well known that \(\mathfrak g_-\) and \(\mathfrak p_+\) are dual as representations of \(G_0\) via the restriction of the Killing form of \(\mathfrak g\). Thus we obtain a non-degenerate pairing \(B\) mapping \(L^-\times L^+\) to the trivial real line bundle \(M\times\mathbb R\). This pairing can be extended as either a skew symmetric or a symmetric bilinear bundle map on \(TA\), thus defining \(\Omega\in\Omega^2(A)\) and \(h\in\Gamma(S^2T^*A)\). By construction, for each \(y\in A\) both values \(\Omega(y)\) and \(h(y)\) are non-degenerate bilinear forms on \(T_yA\) for which \(L^+_y\) and \(L^-_y\) are isotropic. The resulting structure \((\Omega,L^+,L^-)\) is called an almost bi-Lagrangian structure.
In particular, \(\Omega\in\Omega^2(A)\) is an almost symplectic structure and an obvious first question is when this structure is symplectic, i.e. when \(d\Omega=0\).
Theorem 3.1. Let \((p:\mathcal G\to M,\omega)\) be a parabolic geometry of type \((G,P)\) and \(\pi:A\to M\) its associated bundle of Weyl structures. Then the natural 2-form \(\Omega\in\Omega^2(A)\) is closed if and only if \((G,P)\) corresponds to a \(|1|\)-grading and the Cartan geometry \((p:\mathcal G\to M,\omega)\) is torsion-free.
Proof. Let \(D\) be the canonical connection on \(TA\) from Section 2.3. Since \(\Omega\) is induced by a \(G_0\)-invariant pairing on \(\mathfrak g_-\oplus\mathfrak g_+\) it satisfies \(D\Omega=0\). If \(D\) were torsion-free, then \(d\Omega\) would coincide with the complete alternation of \(D\Omega\) and thus would vanish, too. In the presence of torsion, there still is a relation as follows. Expanding \(D\Omega=0\) by inserting vector fields \(\xi,\eta,\zeta\in\mathfrak X(A)\), we obtain \[0=\xi\cdot\Omega(\eta,\zeta)-\Omega(D_\xi\eta,\zeta)-\Omega(\eta,D_\xi\zeta).\] Now one takes the sum of the right hand side over all cyclic permutations of the arguments and uses skew symmetry of \(\Omega\) to bring all derivatives of vector fields into the first component. Then one may use the definition of the torsion \(\tau\) of \(D\) to rewrite \(D_\xi\eta-D_\eta\xi\) as \([\xi,\eta]+\tau(\xi,\eta)\) and similarly for other combinations of the fields. Then the terms in which one field differentiates the value of \(\Omega\) together with the terms involving a Lie bracket add up to the exterior derivative. One concludes that \(D\Omega=0\) implies \[d\Omega(\xi,\eta,\zeta)=\textstyle\sum_{\text{cycl}}\Omega(\tau(\xi,\eta),\zeta),\] where in the right hand side we have the sum over all cyclic permutations of the arguments. Now let us assume that \((G,P)\) corresponds to a \(|k|\)-grading with \(k>1\). Then \(L^-\) and \(L^+\) decompose into direct sums of subbundles according to the grading of \(\mathfrak g_-\) and \(\mathfrak p_+\), respectively. Now we take \(\xi\in L^-\) of degree \(-1\), \(\eta\in L^+\) of degree \(i>1\) and \(\zeta\in L^+\) of degree \(i-1\). Then by Theorem 2.11, \(\tau\) coincides with \(\{\ ,\ \}\) on any two of these three fields. The restriction of \(d\Omega\) to the subbundles corresponding to these three degrees is induced by the trilinear map \(\mathfrak g_{-1}\times\mathfrak g_i\times\mathfrak g_{i-1}\to\mathbb R\) given by \((X,Y,Z)\mapsto \sum_{\text{cycl}}B([X,Y],Z)\), where \(B\) denotes the Killing form of \(\mathfrak g\). But \(B([X,Y],Z)\) is already totally skew, so \(d\Omega=0\) would imply that \(B([X,Y],Z)=0\) for all elements of the given homogeneities. But non-degeneracy of \(B\) shows that \(B([X,Y],Z)=0\) for all \(Z\) implies \([X,Y]=0\) while for \(Y\in\mathfrak g_i\), the equation \([X,Y]=0\) for all \(X\in\mathfrak g_{-1}\) implies \(Y=0\), see Proposition 3.1.2 in [16].
Thus we may assume from now on that \((G,P)\) corresponds to a \(|1|\)-grading. In this case, the bracket \(\{\ ,\ \}\) is identically zero, so by Theorem 2.11, \(\tau\) vanishes upon insertion of one element from \(L^+\). Hence we see that \(d\Omega\) vanishes upon insertion of two elements of \(L^+\). Decomposing \(\Lambda^3T^*A\) according to \(TA=L^-\oplus L^+\), the only potentially non-zero components of \(d\Omega\) thus are the ones in \(\Lambda^3(L^-)^*\) and in \(\Lambda^2(L^-)^*\otimes (L^+)^*\).
Now if \(\xi,\eta\in\Gamma(L^-)\) and \(\zeta\in\Gamma(L^+)\), then we simply obtain \(d\Omega(\xi,\eta,\zeta)=\Omega(T(\xi,\eta),\zeta)\), where \(T\) is defined in Definition 2.9. Non-degeneracy of \(\Omega\) shows that this vanishes for all \(\xi,\eta,\zeta\) if and only if \(T=0\). This shows that vanishing of \(T\) is a necessary condition for \(\Omega\) being closed. In the case of a \(|1|\)-grading, the pullback of \(T\) along a Weyl structure as in Proposition 2.10 is independent of the Weyl structure and gives the torsion of the Cartan geometry \((p:\mathcal G\to M,\omega)\).
To complete the proof, we thus have to show that (still in the case of a \(|1|\)-grading) vanishing of \(T\) implies that the component of \(d\Omega\) in \(\Lambda^3(L^-)^*\) vanishes identically. As above, Theorem 2.11 shows that this component is given by the sum of \(\Omega(Y(\xi,\eta),\zeta)\) over all cyclic permutations of its arguments. But by construction, this is simply the complete alternation of \(Y\), viewed as a section of \(\Lambda^2L^+\otimes L^+\) via the identification \((L^-)^*\cong L^+\). In terms of the Cartan geometry \((p:\mathcal G\to M)\), it thus suffices to show that the component \(\kappa_+\) of the Cartan curvature in \(\mathfrak p_+\) always has trivial complete alternation.
To do this, we first observe that for a \(|1|\)-graded Lie algebra \(\mathfrak g\), the subalgebra \(\mathfrak g_0\) always splits into its center \(\mathfrak z(\mathfrak g_0)\), which has dimension one, and a semisimple part \(\mathfrak g_0^{ss}\). For a torsion-free geometry, the component \(\kappa_0\) of \(\kappa\) with values in \(\mathfrak g_0\) is the lowest non-vanishing homogeneous component of \(\kappa\), which implies that its values have to lie in \(\mathfrak g_0^{ss}\), compare with Theorem 4.1.1 in [16]. Thus we conclude that, viewed as a function \(\mathcal G\to \mathfrak g\), \(\kappa\) has values in the subspace \(\mathfrak g_0^{ss}\oplus\mathfrak g_1\).
Now we can apply the Bianchi identity in the form of equation (1.25) in Proposition 1.5.9 of [16]. This contains four terms, three of which are evaluations of the function \(\kappa\) or its derivative along some vector field, so these have values in \(\mathfrak g_0^{ss}\oplus\mathfrak g_1\), too. Formulated in terms of functions, the Bianchi identity thus implies that for \(X_1,X_2,X_3\) the cyclic sum over the arguments of \([X_1,\kappa(\omega^{-1}(X_2),\omega^{-1}(X_3))]\) has trivial component in \(\mathfrak z(\mathfrak g_0)\). Now we can replace the \(X_i\) by their components in \(\mathfrak g_-\) without changing the \(\mathfrak g_0\)-component of \([X_1,\kappa(\omega^{-1}(X_2),\omega^{-1}(X_3))]\), which in addition depends only on the \(\mathfrak g_1\)-component of \(\kappa\). Now it is well known that for \(X\in\mathfrak g_{-1}\) and \(Z\in\mathfrak g_1\), the component of \([X,Z]\) in \(\mathfrak z(\mathfrak g_0)\) is a non-zero multiple of \(B(X,Z)\), where \(B\) denotes the Killing form. But this exactly shows that, up to a non-zero factor, the \(\mathfrak z(\mathfrak g_0)\)-component of \(\sum_{\text{cycl}}[X_1,\kappa(\omega^{-1}(X_2),\omega^{-1}(X_3))]\) represents the action of the complete alternation of \(\kappa_+\) on the three vector fields corresponding to the \(X_i\). Thus this complete alternation vanishes identically. ◻
Remark 14. (1) The failure of closedness of \(\Omega\) for \(|k|\)-gradings with \(k>1\) can be described more precisely. The map \((X,Y,Z)\mapsto B([X,Y],Z)\) that shows up in the proof defines a \(G\)-invariant element in \(\Lambda^3\mathfrak g^*\) and hence a bi-invariant \(3\)-form on \(G\). Restricting this to \(\Lambda^3(\mathfrak g_-\oplus\mathfrak p_+)^*\), one obtains a \(G_0\)-invariant trilinear form, which is non-zero provided that \(k>1\). This in turn induces a natural \(3\)-form on each manifold endowed with a Cartan Geometry of type \((G,G_0)\). On a bundle of Weyl structures, the proof of Theorem 3.1 shows that this form always is a component of \(d\Omega\).
(2) The parabolic geometries corresponding to \(|1|\)-gradings form a very interesting class of structures. For a \(|1|\)-grading, the subalgebras \(\mathfrak g_-\) and \(\mathfrak p_+\) become Abelian, whence the name “Abelian parabolic geometries” is sometimes used for these structures. The classification of \(|1|\)-gradings of simple Lie algebras is well known from the theory of Hermitian symmetric spaces, which motivates the more common name “AHS structures” where AHS is shorthand for “almost Hermitian symmetric”.
Suppose that \((G,P)\) corresponds to a \(|1|\)-grading on \(\mathfrak g\). As noted in Section 2.1, the underlying structure \(p_0:\mathcal G_0\to M\) of a Cartan geometry \((p:\mathcal G\to M)\) simply becomes a reduction of the linear frame bundle of \(M\) to the structure group \(G_0\subset GL(\mathfrak g_{-1})\). Thus AHS structures are a special class of G-structures, whose relevance is explained by the classification results by S. Kobayashi and T. Nagano in [24]. They prove that these are the only structures for which the group acts irreducibly, and which have the property that any automorphism is determined by a finite jet in a point but not by the one-jet in a point. In fact, automorphisms are always determined by the two-jet in a point and the equivalent canonical Cartan geometry of type \((G,P)\) is the most effective description for these structures.
The torsion-freeness condition that shows up in Theorem 3.1 has a natural interpretation in the language of \(G_0\)-structures. As noted in the proof, the torsion \(T\) associated to a Weyl structure in this case is independent of the Weyl structure. It turns out that this coincides with the intrinsic torsion of the \(G_0\)-structure (i.e. the component of the torsion that is independent of the choice of connection). Thus torsion-freeness of the Cartan geometry corresponds to the usual notion of integrability in the language of \(G_0\)-structures.
(3) For some types of AHS-structures, torsion-freeness implies local flatness. Locally flat structures can be equivalently be characterized as being obtained from local charts with values in the homogeneous model \(G/P\), for which the transition functions are given by restrictions of left actions of elements of \(g\). This case anyway plays a very important role in the results we are going to prove, so our results are also relevant to these types of AHS structures.
From this point on, we restrict the discussion to torsion-free geometries of some type \((G,P)\) that corresponds to a \(|1|\)-grading of \(\mathfrak g\), so that by Theorem 3.1 \(\Omega\) defines a symplectic structure on \(A\). Recall from Section 2.4 that any vector field \(\xi\in\mathfrak X(M)\) determines a section \(\tilde\xi\in\Gamma(L^-)\), and since \(\mathfrak g_-\) is a completely reducible representation in the \(|1|\)-graded case, we get \(D^+\tilde\xi=0\). Similarly, a one-form \(\alpha\in\Omega^1(M)\) defines a section \(\tilde\alpha\in\Gamma(L^+)\) such that \(D^+\tilde\alpha=0\). We further know that \(L^-\cong\pi^*TM\) and \(L^+=\pi^*T^*M\). This implies that starting with local frames for \(TM\) and \(T^*M\) defined on some open set \(U\subset M\), the lifts form local frames for \(L^\pm\) defined on \(\pi^{-1}(U)\), so together, these form a local frame for \(TA\). One may in particular use dual local frames for \(TM\) and \(T^*M\) in which case the resulting local frame for \(TA\) is nicely adapted to the almost bi-Lagrangian structure and thus both to \(\Omega\) and to \(h\). As a preparation for the following computations, we next compute the Lie brackets of such sections.
Proposition 3.2. Consider a torsion-free AHS structure \((p:\mathcal G\to M,\omega)\) and let \(\pi:A\to M\) be the corresponding bundle of Weyl structures. Let \(\xi,\eta\in\mathfrak X(M)\) be vector fields and \(\alpha,\beta\in\Omega^1(M)\) be one-forms on \(M\) and consider the corresponding sections \(\tilde\xi,\tilde\eta\in\Gamma(L^-)\) and \(\tilde\alpha,\tilde\beta\in\Gamma(L^+)\).
Then for the Lie brackets on \(A\), we get \([\tilde\alpha,\tilde\beta]=0\) and \([\tilde\xi,\tilde\alpha]=D_{\tilde\xi}\tilde\alpha\in\Gamma(L^+)\). Finally, the \(L^-\)-component of \([\tilde\xi,\tilde\eta]\) coincides with \(\widetilde{[\xi,\eta]}\), while its \(L^+\)-component coincides with \(-Y(\tilde\xi,\tilde\eta)\), see Definition 2.9.
Proof. By definition of the torsion \[ \tau(X,Z)=D_XZ-D_ZX-[X,Z]\](3.1) for all \(X,Z\in\mathfrak X(A)\). If at least one of the two fields is a section of \(L^+\), then the left hand side of (3.1) vanishes by Theorem 2.11. Moreover, all the sections coming from \(M\) are parallel in \(L^+\)-directions. This immediately shows that \([\tilde\alpha,\tilde\beta]=0\) and \(0=D_{\tilde\xi}\tilde\alpha-[\tilde\xi,\tilde\alpha]\). In view of torsion-freeness, Theorem 2.11 further tells us that \(\tau(\tilde\xi,\tilde\eta)=Y(\tilde\xi,\tilde\eta)\in\Gamma(L^+)\). Inserting \(X=\tilde\xi\) and \(Z=\tilde\eta\) into the right hand side of (3.1), the first two terms are sections of \(L^-\), so the claim about the \(L^+\)-component of \([\tilde\xi,\tilde\eta]\) follows. Finally, since \(\tilde\xi\) and \(\tilde\eta\) are lifts to \(A\) of \(\xi\) and \(\eta\), the bracket \([\tilde\xi,\tilde\eta]\in\mathfrak X(A)\) is a lift of \([\xi,\eta]\). Since \(\widetilde{[\xi,\eta]}\) is the unique section of \(L^-\) that projects onto \([\xi,\eta]\), it has to coincide with the \(L^-\)-component of that lift. ◻
In particular, we see that, while \(L^+\) always defines an involutive distribution, \(L^-\) is only involutive if the curvature component \(Y\) from Definition 2.9 vanishes identically. From the interpretation via the Cartan curvature, one easily concludes that this is equivalent to local vanishing of the Cartan curvature. Thus our structure is bi-Lagrangian (in the sense that both subbundles \(L^\pm\) are integrable) if and only if the initial parabolic geometry is locally flat.
We next study the pseudo-Riemannian metric \(h\) induced on \(A\). By definition, the subbundles \(L^\pm\) are isotropic for \(h\), so this metric always has split signature \((n,n)\), where \(n=\dim(M)\). Our main next aim will be to prove that the metric \(h\) is always Einstein. As a first step in this direction, consider the canonical connection \(D\) and its curvature \(\rho\in\Omega^2(A,\operatorname{End}_0(TA))\) as described in Section 2.7.
Lemma 3.3. The Ricci-type contraction of \(\rho\) is a non-zero multiple of \(h\).
Proof. By Theorem 2.11, \(\rho+\{\ ,\ \}_0\) vanishes upon insertion of one section of \(L^+\) and coincides with \(W\) on \(\Lambda^2(L^-)^*\). Decomposing \(\Lambda^2TA^*\) according to \(TA=L^+\oplus L^-\), we conclude that the component of \(\rho\) in \(\Lambda^2(L^+)^*\) vanishes, its component in \((L^-)^*\otimes (L^+)^*\) is induced by \(-\{\ ,\ \}_0\), and the component in \(\Lambda^2(L^-)^*\) is induced by \(W\). On the other hand, \(\operatorname{End}_0(TA)=\mathcal G\times_{G_0}\mathfrak g_0\), so this is a subbundle of \(((L^-)^*\otimes L^-)\oplus ((L^+)^*\otimes L^+)\subset TA^*\otimes TA\). Thus we conclude that the Ricci-type contraction of \(\rho\) vanishes on \(L^+\times L^+\), while its components on \(L^-\times L^+\) and \(L^-\times L^-\) are induced by the Ricci-type contractions of \(-\{\ ,\ \}_0\) and \(W\), respectively. By Proposition 2.10, the pullback of \(W\) along any section \(s:M\to A\) represents the Weyl curvature of the Weyl structure determined by \(s\). In the torsion-free case, this is well known to have values in an irreducible representation of \(G_0\) that occurs with multiplicity one in \(\Lambda^*\mathfrak g_-^*\otimes\mathfrak g\), which implies that any contraction of \(W\) vanishes identically.
Hence we see that the Ricci type contraction of \(\rho\) has values in \((L^-)^*\otimes (L^+)^*\) and is induced by the Ricci type contraction of \(-\{\ ,\ \}_0\), so this is a natural bundle map, and we can compute it on the inducing representations. Take a basis \(\{e_i\}\) of \(\mathfrak g_{-1}\) and let \(\{e^i\}\) be the dual basis of \(\mathfrak g_{-1}^*\cong\mathfrak g_1\), which means that for the Killing form \(B\), we get \(B(e_i,e^j)=\delta_i^j\). Now we have to view the \(\mathfrak g_0\) component of the bracket \([\ ,\ ]\) in \(\mathfrak g\) as a map sending \((\mathfrak g_-\oplus\mathfrak p_+)^2\) to an endomorphism of \(\mathfrak g_-\oplus\mathfrak p_+\) via the adjoint action. Hence for \(X,Y\in\mathfrak g_{-1}\) and \(Z,W\in\mathfrak g_1\), the Ricci type contraction sends \(\binom{X}{Z}\) and \(\binom{Y}{W}\) to \[\textstyle\sum_iB\big(\big[\big[\binom{X}{Z},\binom{e_i}{0}\big],\binom{Y}{W}\big], \binom0{e^i})+\sum_i B\big(\big[\big[\binom{X}{Z},\binom{0}{e^i}\big], \binom{Y}{W}\big],\binom{e_i}{0}\big).\] Expanding the first sum using invariance of the Killing form and the fact that \(\mathfrak g_{-1}\) is abelian, we obtain \[\textstyle\sum_iB([[Z,e_i],Y],e^i)=\sum_iB(Z,[e_i,[Y,e^i]])=\sum_iB(Z,[Y,[e_i,e^i]]),\] and in the same way the second sum gives \(\sum_iB([X,[e_i,e^i]],W)\). But the element \(\sum_i[e_i,e^i]\in\mathfrak g_0\) is obtained from the identity map in \(\mathfrak g_{-1}\otimes\mathfrak g_{-1}^*\) via the isomorphism to \(\mathfrak g_{-1}\otimes\mathfrak g_1\) and the bracket in \(\mathfrak g\). Since these both are \(\mathfrak g_0\)-equivariant, \(\sum_i[e_i,e^i]\) is \(\mathfrak g_0\)-invariant and thus contained in the center of \(\mathfrak g_0\). In the \(|1|\)-graded case, this center is spanned by the grading element \(E\). In addition, \(B(E,\textstyle\sum_i[e_i,e^i])=\sum_iB([E,e_i],e^i)=-\dim(\mathfrak g_{-1})\), so \(\sum_i[e_i,e^i]\) is a non-zero multiple of \(E\). Hence the whole contraction gives a non-zero multiple of \(B(Z,Y)+B(X,W)=h(\binom{X}{Z},\binom{Y}{W})\). ◻
Now by construction, the canonical connection \(D\) satisfies \(Dh=0\), so \(D\) is metric for \(h\). This implies that the Levi-Civita connection \(\nabla\) of \(h\) can be computed from \(D\) and its torsion \(\tau\). Indeed, we claim that for \(\xi,\eta,\zeta\in\mathfrak X(A)\), \(h(\nabla_\xi\eta,\zeta)\) is given by \[ h(D_\xi\eta,\zeta)-\tfrac12h(\tau(\xi,\eta),\zeta)+\tfrac12h(\tau(\xi,\zeta),\eta)+ \tfrac12h(\tau(\eta,\zeta),\xi).\](3.2) This evidently defines a linear connection \(\nabla\) on \(TA\). Moreover, the last three terms in (3.2) are visibly skew symmetric in \(\eta\) and \(\zeta\), whence the fact that \(D\) is metric with respect to \(h\) implies that \(\nabla\) is metric with respect to \(h\), too. On the other hand, since the last two terms in (3.2) are symmetric in \(\xi\) and \(\eta\), and \(\tau\) is the torsion of \(D\), one immediately verifies that \(\nabla\) is torsion-free. Let us write \(C\in\Gamma(\otimes^2T^*A\otimes TA)\) for the contorsion tensor between \(\nabla\) and \(D\), so \(C(\xi,\eta)=\nabla_\xi\eta-D_\xi\eta\) and the last three terms in (3.2) explicitly express \(h(C(\xi,\eta),\zeta)\). Using this, we prove the following result
Theorem 3.4. For any torsion-free AHS structure, the pseudo-Riemannian metric \(h\) induced by the canonical almost bi-Lagrangian structure on the bundle \(A\) of Weyl structures is an Einstein metric with non-zero scalar curvature.
Proof. Theorem 2.11 in the torsion-free case shows that \(\tau\) vanishes upon insertion of one section of \(L^+\) and has values in \(L^+\). Thus equation (3.2) shows that \(h(C(\xi,\eta),\zeta)\) vanishes if one of the three fields is a section of \(L^+\). This shows that the only non-zero component of \(C\) is the one mapping \(L^-\times L^-\) to \(L^+\). Now it is standard how to compute the curvature of \(\nabla\) from \(C\) and the curvature \(\rho\) of \(D\) via differentiating the equation defining \(C\). The result contains terms in which \(C\) is differentiated as well as terms in which values of \(C\) are inserted into \(C\). From the form of \(C\) we have just deduced, it follows that the latter terms vanish identically.
Using this, one computes that for \(\xi,\eta,\zeta\in\mathfrak X(A)\) the difference \(R(\xi,\eta)(\zeta)-\rho(\xi,\eta)(\zeta)\) is given by \[ D_\xi(C(\eta,\zeta))-D_\eta(C(\xi,\zeta))+C(\xi,D_\eta\zeta)-C(\eta,D_\xi\zeta)-C([\xi,\eta],\zeta).\](3.3) (This is just the covariant exterior derivative of \(C\) with respect to \(D\) evaluated on \(\xi\) and \(\eta\) and then applied to \(\zeta\).) In view of Lemma 3.3, it suffices to prove that the Ricci-type contraction of this expression vanishes. To compute this contraction, we leave \(\xi\) and \(\zeta\) as entries, insert the elements of a local frame of \(TA\) for \(\eta\) and hook the result into \(h\) together with the elements of the dual frame. First of all, (3.3) visibly vanishes for \(\zeta\in\Gamma(L^+)\). If we insert for \(\eta\) an element of a frame for \(L^-\), then the element of the dual frame will sit in \(L^+\). Since \(C\) has values in \(L^+\), these summands do not contribute to the contraction. Thus we only have to take into account the case that we insert elements of a frame for \(L^+\) for \(\eta\), and then the first and fourth term of (3.3) visibly vanish. The remaining three terms vanish if \(\xi\) is a section of \(L^+\), so what we have to compute is \[\textstyle\sum_ih\left(-D^+_{e^i}(C(\xi,\zeta))+C(\xi,D^+_{e^i}\zeta)-C([\xi,e^i],\zeta),e_i\right)\] for a smooth local frame \(\{e^i\}\) for \(L^+\) with dual frame \(\{e_i\}\) for \(L^-\) and local sections \(\xi,\zeta\in\Gamma(L^-)\). Now we can take \(\xi\) and \(\zeta\) and the local frames to be obtained from vector fields respectively one-forms on \(M\). Then \(D^+_{e^i}\zeta=0\), while \([\xi,e^i]\in\Gamma(L^+)\) by Proposition 3.2 and thus \(C([\xi,e^i],\zeta)=0\).
Thus we are left with computing \(\sum_ih(D^+_{e^i}(C(\xi,\zeta)),e_i)\) with the frames, \(\xi\) and \(\zeta\) all coming from \(M\). In particular, \(e_i\) is parallel for \(D^+\) so since \(D\) is metric for \(h\), we may rewrite this as \(\sum_ie^i\cdot h(C(\xi,\zeta),e_i)\). We can then insert the formula for \(h(C(\xi,\zeta),e_i)\) resulting from (3.2), taking into account that on entries from \(L^-\) the torsion \(\tau\) is determined by the tensor \(Y\) from Definition 2.9. Viewing \(Y\) as a section of \(\Lambda^2(L^-)^*\otimes (L^-)^*\), this leads to \[\textstyle\sum_ie^i\cdot h(C(\xi,\zeta),e_i)=\tfrac12\sum_ie^i\cdot (-Y(\xi,\zeta,e_i)+Y(\xi,e_i,\zeta)+Y(\zeta,e_i,\xi)).\] From the proof of Theorem 3.1, we know that the complete alternation of \(Y\) vanishes, which allows us to rewrite this as \(\sum_ie^i\cdot Y(\zeta,e_i,\xi)\). Under the standing assumption that all sections come from \(M\), they are parallel for \(D^+\), so we can complete the proof by showing that \(\sum_i(D^+_{e^i}Y)(\zeta,e_i,\xi)=0\).
Now by definition, \(Y\) is a component of the Cartan curvature, which descends to a well defined section of the bundle \(\Lambda^2T^*M\otimes\mathcal AM\), where \(\mathcal AM=\mathcal G\times_P\mathfrak g\). By torsion freeness, the full Cartan curvature has the form \((0,W,Y)\) with respect to the decomposition \(\mathfrak g=\mathfrak g_{-1}\oplus\mathfrak g_0\oplus\mathfrak g_1\). Hence by Theorem 2.5, we get \[D^+_\varphi(0,W,Y)=(0,D^+_\varphi W,D^+_\varphi,Y)=-\varphi\bullet (0,W,Y),\] and the action \(\bullet\) is induced by the Lie bracket on \(\mathfrak g\). Since this bracket vanishes on \(\mathfrak g_1\times\mathfrak g_1\) and defines the action of \(\mathfrak g_0\) on \(\mathfrak g_{\pm 1}\), we conclude that \(D^+W=0\) and \(D^+_\varphi Y=W(\varphi)\), where we view \(W\) as an section of \(\Lambda^2(L^--)^*\otimes\operatorname{End}(L^+)\cong \Lambda^2(L^--)^*\otimes(L^-)^*\otimes (L^+)^*\) in the right hand side. But this implies that \(\sum_i(D^+_{e^i}Y)(\zeta,e_i,\xi)\) is given by evaluating a trace of \(W\) on \(\zeta\) and \(\xi\) and thus vanishes. ◻
Remark 18. In the special case of a projective structure on a surface \(\Sigma\), the resulting Einstein metric on the four-manifold \(A\) is also anti-self-dual, see [19] and also [8].
Remark 19. The automorphisms of a projective structure on a smooth manifold \(M\) lift to become isometric symplectomorphisms of \((A,\Omega,h)\), see [19]. For background about automorphisms of a parabolic geometry, see [1, 16, 20].
Remark 20. A pair \((h,\Omega)\), consisting of a split-signature metric \(h\) and a symplectic form \(\Omega\) that are related by an endomorphism which squares to become the identity map, is also known as an almost para-Kähler structure. Here, following [6], we refer to such a pair, or rather its associated triple \((\Omega,L_+,L_-)\), as an almost bi-Lagrangian structure.
Viewed as a section of \(\pi:A\to M\), any Weyl structure defines an embedding of \(M\) into \(A\), and we can now study this embedding via submanifold geometry related to the almost bi-Lagrangian structure. In particular, we can pull back the two-form \(\Omega\) and the pseudo-Riemannian metric to \(M\) along \(s\), and this naturally leads to the following definitions.
Definition 3.5. Let \((p:\mathcal G\to M,\omega)\) be a torsion-free AHS structure and let \(s:M\to A\) be a smooth section.
(1) The Weyl structure corresponding to \(s\) is called Lagrangian if and only if \(s^*\Omega=0\) and thus \(s(M)\subset A\) is a Lagrangian submanifold.
(2) The Weyl structure corresponding to \(s\) is called non-degenerate if and only if \(s^*h\in\Gamma(S^2T^*M)\) is non-degenerate and thus defines a pseudo-Riemannian metric on \(M\).
These properties can easily be characterized in terms of the Rho tensor.
Proposition 3.6. A Weyl structure is Lagrangian if and only if its Rho tensor is symmetric and non-degenerate if and only if the symmetric part of its Rho tensor is non-degenerate.
Proof. For a point \(x\in M\) and a tangent vector \(\xi\in T_xM\) consider \(T_xs\cdot\xi\in T_{s(x)}(A)\). Since this is a lift of \(\xi\), its \(L^-\)-component has to coincide with \(\tilde\xi(s(x))\). On the other hand, by Proposition 2.7, the \(L^+\)-component of \(T_xs\cdot\xi\) corresponds to \(\mbox{\textsf{P}}(x)(\xi)\in T^*_xM\). Pulling back the pairing between \(L^-\) and \(L^+\), one thus obtains the map \((\xi,\eta)\mapsto \mbox{\textsf{P}}(x)(\eta)(\xi)\) and thus the result follows from the definitions of \(\Omega\) and \(h\). ◻
Remark 23. (1) For any type of parabolic geometry, there are natural line bundles called bundles of scales, an example in the AHS-case is provided by the bundle \(\mathcal EM\) in Theorem 4.2 below. If \(\mathcal EM\) is any bundle of scales on \(M\), then mapping a Weyl structure to the induced Weyl connection on \(\mathcal EM\) induces a bijective correspondence between Weyl structures and linear connections on \(\mathcal EM\). Fixing \(\mathcal EM\), one calls a Weyl structure closed if the corresponding linear connection on \(\mathcal EM\) is flat and exact if in addition there is a global parallel section of \(\mathcal EM\), see [15] and Section 5.1 of [16]. For general types of geometries there is a larger freedom of choice of bundles of scales, but for AHS-structures all bundles of scales lead to the same subclasses of closed and exact Weyl structures.
Together with the general theory of Weyl structures, Proposition 3.6 implies that, on a torsion-free AHS-structure, a Weyl structure is Lagrangian if and only if it is closed. This follows from the relation between curvature and torsion of a Weyl connection and the Cartan curvature as discussed in Example 5.2.3 of [16] in the setting of AHS structures. By Theorem 5.2.3 of that reference, the curvature \(R\in\Omega^2(M,\mathcal G\times_g\mathfrak g_0)\) of the Weyl connection corresponding to \(s\in\Gamma(A)\) can be computed as \(s^*W+\partial s^*\mbox{\textsf{P}}\) for the quantities from Proposition 2.10 and a certain natural bundle map \(\partial\). For the action on a bundle of scales, the component of \(R\) with values in the center \(\mathfrak z(\mathfrak g_0)\) is relevant. For a torsion free geometry, \(W\) is the lowest non-zero component of the Cartan curvature and hence by general results has values in an irreducible subrepresentation which cannot meet this center. Hence the curvature of the Weyl connection is only induced by \(\partial s^*\mbox{\textsf{P}}\), and the component of this in \(\mathfrak z(\mathfrak g_0)\) is immediately seen to be the skew part of the Rho tensor up to a non-zero factor.
This result nicely corresponds to the fact that for the canonical symplectic structure on any cotangent bundle \(T^*N\), the image of a one-form \(\alpha\in\Omega^1(N)\) in \(T^*N\) is a Lagrangian submanifold if and only if \(d\alpha=0\).
(2) In the case of an AHS-structure, the cotangent bundle \(T^*M\) coincides with the associated graded bundle, so Proposition 2.3 shows that a Weyl structure \(s\) determines a diffeomorphism \(\varphi_s:T^*M\to A\). Now we can use this to pull back the geometric structures on \(A\) to \(T^*M\) and in particular, in the torsion-free case, compare the pullback of the symplectic form \(\Omega\in\Omega^2(A)\) to the canonical symplectic structure on \(T^*M\). Recall that the diffeomorphism \(\varphi_s\) is induced by \(\Phi_s:\mathcal G_0\times\mathfrak p_+\to\mathcal G\), \(\Phi_s(u_0,Z)=\sigma(u_0)\cdot\exp(Z)\), where \(\sigma:\mathcal G_0\to\mathcal G\) is the equivariant section determined by \(s\).
Equivariancy of the Cartan connection \(\omega\in\Omega^1(\mathcal G,\mathfrak g)\) then implies that the pullback \(\Phi_s^*\omega\) can be easily expressed explicitly in terms of \(\sigma^*\omega\). Denoting by \(q:\mathcal G_0\times\mathfrak p_+\to T^*M\) the canonical projection, the definition of \(\Omega\) in Section 3.1 shows that \(q^*\varphi_s^*\Omega=\Phi_s^*\Omega\) sends tangent vectors \(\xi,\eta\) to the alternation of the pairing between \((\Phi_s^*\omega)_-(\xi)\in\mathfrak g_{-1}\) and \((\Phi_s^*\omega)_+(\eta)\in\mathfrak g_1\). On the other hand, it is easy to explicitly describe \(q^*\alpha\in\Omega^1(\mathcal G_0\times\mathfrak p_+)\), where \(\alpha\in\Omega^1(T^*M)\) is the canonical one-form. From this, one can explicitly compute the pullback \(-q^*d\alpha\) of the canonical symplectic form on \(T^*M\) and show that it equals the sum of \(\Phi_s^*\Omega\) and the pullback of the alternation of the Rho-tensor. In particular, generalizing a result from [28] in the projective case, we conclude that \(\varphi_s:T^*M\to A\) is a symplectomorphism if and only if the Weyl-structure \(s\) is Lagrangian. Indeed, it turns out that also the split-signature metric \(\varphi_s^*h\) on \(T^*M\) can be computed explicitly in terms of the underlying AHS-structure. All this will be taken up in more detail elsewhere.
To start the geometric study of Lagrangian Weyl structures, we can characterize when \(s\) has the property that the submanifold \(s(M)\subset A\) is totally geodesic.
Theorem 3.7. Let \((p:\mathcal G\to M,\omega)\) be a torsion-free AHS structure and \(\pi:A\to M\) its bundle of Weyl structures. Let \(s:M\to A\) be a smooth section corresponding to a Lagrangian Weyl structure, let \(\nabla^s\) denote the corresponding Weyl connections and \(\mbox{\textsf{P}}^s\) the corresponding Rho-tensor. Then the following conditions are equivalent:
(1) The submanifold \(s(M)\subset A\) is totally geodesic for the canonical connection \(D\).
(2) The submanifold \(s(M)\subset A\) is totally geodesic for the Levi-Civita connection of \(h\).
(3) \(\nabla^s\mbox{\textsf{P}}^s=0\)
Proof. We will use abstract index notation to carry out the computations and denote the Rho tensor of \(s\) just by \(\mbox{\textsf{P}}\), so this has the form \(\mbox{\textsf{P}}_{ij}\) and is symmetric by assumption. Since for each \(y\in A\) and \(x:=\pi(y)\in M\), we can identify \(L^-_y\) with \(T_xM\) and \(L^+_y\) with \(T^*_xM\), we can use the index notation also on \(A\), but here tangent vectors have the form \((\xi^i,\alpha_j)\). In this language the proof of Proposition 3.6 shows that for \(x\in M\) the tangent space \(T_{s(x)}s(M)\) consists of all pairs of the form \((\xi^i,\mbox{\textsf{P}}_{ja}\xi^a)\). The condition that \(s(M)\) is totally geodesic with respect to \(D\) means that for vector field \((\xi,\alpha)\) on \(A\) that is tangent to \(s(M)\) along \(s(M)\), also the covariant derivative in directions tangent to \(s(M)\) is tangent to \(s(M)\).
In particular, for a vector field \(\eta\in\mathfrak X(M)\), we know from above that \((\widetilde{\eta^j},\widetilde{\mbox{\textsf{P}}_{kb}\eta^b})\in\mathfrak X(A)\) is tangent to \(s(M)\) along \(s(M)\). Since these fields are parallel for \(D^+\), we see that \(s(M)\) is totally geodesic for \(D\) if and only if all derivatives with respect to \(D\) of that field are tangent to \(s(M)\) along \(s(M)\). But this can be checked by pulling back the components of \(D(\widetilde{\eta^j},\widetilde{\mbox{\textsf{P}}_{kb}\eta^b})\) along \(s\), which by Theorem 2.6 leads to \(\nabla^s_i\eta^j\) and \[ \nabla^s_i\mbox{\textsf{P}}_{ka}\eta^a=\eta^a\nabla^s_i\mbox{\textsf{P}}_{ka}+\mbox{\textsf{P}}_{ka}\nabla^s_i\eta^a,\](3.4) respectively. So evidently, the result is tangent to \(s(M)\) if and only if \(\eta^a\nabla^s_i\mbox{\textsf{P}}_{ka}=0\) and since this has to hold for each \(\eta\), we conclude that (1) is equivalent to (3).
To deal with (2), we use the information on the contorsion tensor \(C\) from Section 3.3. As observed in the proof of Theorem 3.4, the only non-zero component of \(C\) maps \(L^-\times L^-\) to \(L^+\). This means that \((\widetilde{\eta^j},\widetilde{\mbox{\textsf{P}}_{kb}\eta^b})\) is also parallel in \(L^+\)-directions for the Levi-Civita connection, so as above, we can use the pull back of the full derivative along \(s\) and the result has to be tangent to \(s(M)\). We write the pullback of \(C\) along \(s\) as \(C_{ijk}\) using the convention that \(C(\xi,\eta)_k=\xi^i\eta^jC_{ijk}\). Now formula (3.2) from Section 3.3 expresses \(C\) in terms of the torsion \(\tau\) of \(D\) (with \(h\) just playing the role of identifying \(L^+\) with the dual of \(L^-\)) and we know that the torsion corresponds to the Cartan curvature quantity \(Y\), see Theorem 2.11. Writing the pullback of this along \(s\) in abstract index notion as \(Y_{ijk}\), we conclude form formula (3.2) that \(C_{ijk}=\tfrac12(-Y_{ijk}+Y_{ikj}+Y_{jki})\). The pullback of the derivative along \(s\) again has first component \(\nabla^s_i\eta^j\) but for the second component, we have to add \(C_{iak}\eta^a\) to the right hand side of (3.4).
But it is a well known fact (see Theorem 5.2.3 of [16]) that the pullback of \(Y\) along \(s\) is given by the covariant exterior derivative of the Rho-tensor of \(s\) and since \(\nabla^s\) is torsion-free, this is expressed in abstract index notation as \(Y_{ijk}=\nabla^s_i\mbox{\textsf{P}}_{jk}-\nabla^s_j\mbox{\textsf{P}}_{ik}\). Inserting this into the formula for \(C_{ijk}\), we immediately conclude that we have to add \(\eta^a\nabla^s_a\mbox{\textsf{P}}_{ik}-\eta^a\nabla^s_k\mbox{\textsf{P}}_{ia}\) to (3.4). As above, this implies that (2) is equivalent to \[ \nabla^s_i\mbox{\textsf{P}}_{ka}+\nabla^s_a\mbox{\textsf{P}}_{ik}-\nabla^s_k\mbox{\textsf{P}}_{ia}=0.\](3.5) Of course, (3.5) is satisfied if \(\nabla^s\mbox{\textsf{P}}=0\). Conversely, if (3.5) holds, then summing over all cyclic permutations of the indices shows that the total symmetrization of \(\nabla^s\mbox{\textsf{P}}\) has to vanish. But subtracting three times this total symmetrization from the left hand side of (3.5), one obtains \(-2\nabla^s_k\mbox{\textsf{P}}_{ia}\), so this has to vanish, too. ◻
The result of Theorem 3.7 is particularly interesting if \(s\) is non-degenerate. By Proposition 3.6 this implies that \(\mbox{\textsf{P}}^s\) defines a pseudo-Riemannian metric on \(M\) and since \(\nabla^s\) is torsion-free, \(\nabla^s\mbox{\textsf{P}}^s=0\) implies that \(\nabla^s\) is the Levi-Civita connection of \(\mbox{\textsf{P}}^s\). On the other hand, \(\mbox{\textsf{P}}^s\) is always related to the Ricci-type contraction of the curvature of \(\nabla^s\), see Section 4.1.1 of [16]. In particular, for projective structures, symmetry of \(\mbox{\textsf{P}}^s\) implies that it is a non-zero multiple of the Ricci curvature of \(\nabla^s\), see [2], so in this case \(\mbox{\textsf{P}}^s\) defines an Einstein metric on \(M\). The condition that a projective structure contains the Levi-Civita connection of an Einstein metric can be expressed as a reduction of projective holonomy, see [12] and [11].
For a non-degenerate Lagrangian Weyl structure \(s\), there is a well defined second fundamental form of \(s(M)\) with respect to any linear connection on \(TA\) which is metric for \(h\). Extending the result of Theorem 3.7 in this case, we can next explicitly compute the second fundamental forms for \(D\) and for the Levi-Civita connection. To formulate the result, we use abstract index notation as in the proof of Theorem 3.7.
Fix the section \(s:M\to A\) corresponding to a non-degenerate, Lagrangian Weyl structure. By non-degeneracy, the Rho tensor \(\mbox{\textsf{P}}_{ij}\) of \(s\) admits an inverse \(\mbox{\textsf{P}}^{ij}\in\Gamma(S^2TM)\) which is characterized by \(\mbox{\textsf{P}}^{ij}\mbox{\textsf{P}}_{jk}=\delta^i_k\). In the proof of Theorem 3.7, we have seen that \(T_{s(x)}s(M)\) is spanned by all elements of the form \((\eta^i,\mbox{\textsf{P}}_{ka}\eta^a)\) with \(\eta^i\in T_xM\). The definition of \(h\) readily implies that the normal space \(T^\perp_{s(x)}s(M)\) consists of all pairs of the form \((\eta^i,-\mbox{\textsf{P}}_{jk}\eta^k)\), so we can identify both the tangent and the normal space in \(s(x)\) with \(T_xM\) via projection to the first component. Correspondingly, the second fundamental form of \(s(M)\) (with respect to any connection on \(TA\) which is metric for \(h\)) can be viewed as a \(\binom12\)-tensor field on \(M\). We denote the second fundamental form of \(s : M \to (A,h)\) with respect to \(D\) by \(\mathrm{II}^s_{D}\) and with respect to the Levi-Civita connection of \(h\) by \(\mathrm{II}^s_h\).
Theorem 3.8. Let \((p:\mathcal G\to M,\omega)\) be a torsion-free AHS-structure with bundle of Weyl structures \(\pi:A\to M\). Let \(s:M\to A\) be a non-degenerate, Lagrangian Weyl structure with Weyl connection \(\nabla^s\) and Rho-tensor \(\mbox{\textsf{P}}\in\Gamma(S^2T^*M)\), then \[\mathrm{II}^s_{D}=-\tfrac12 \mbox{\textsf{P}}^{ka}\nabla^s_i\mbox{\textsf{P}}_{ja} \qquad\text{and}\qquad \mathrm{II}^s_{h}=-\tfrac12 \mbox{\textsf{P}}^{ka}(\nabla^s_i\mbox{\textsf{P}}_{ja}+\nabla^s_j\mbox{\textsf{P}}_{ia}-\nabla^s_a\mbox{\textsf{P}}_{ij}).\]
Proof. We only have to project the derivatives computed in the proof of Theorem 3.7 to the normal space. From the description of tangent and normal spaces, it follows readily that projecting \((\xi^i,\alpha_j)\) to the normal space and taking the \(L^-\)-component of the result, one obtains \(\tfrac12(\xi^i-\mbox{\textsf{P}}^{ia}\alpha_a)\). Using this, the formulae follow directly from the the proof of Theorem 3.7. ◻
We conclude this article by discussing a relation between the geometry on the bundle \(A\) of Weyl structures and non-linear invariant PDE associated to AHS structures. We will mainly consider the prototypical example of a projectively invariant PDE of Monge-Ampère type. We briefly discuss analogs of this and other invariant non-linear PDE for specific types of AHS structures, but this will be taken up in detail elsewhere.
We start by deriving an alternative description of the bundle \(A\to M\) of Weyl structures associated to an AHS structure \((p:\mathcal G\to M,\omega)\) based on tractor bundles. As mentioned in Section 2.4, these are bundles associated to representations of \(P\) that are restrictions of representations of \(G\). An important feature of these bundles is that they inherit canonical linear connections from the Cartan connection \(\omega\). Together with some algebraic ingredients, these form the basis for the machinery of BGG sequences that was developed in [17] and [9], which will provide input to some of the further developments. We have also met the canonical invariant filtration on representations of \(P\) in Section 2.4 and the corresponding filtration of associated bundles by smooth subbundles. For representations of \(G\), these admit a simpler description, that we derive first. In most of the examples we need below, this description is rather obvious, so readers not interested in representation theory aspects can safely skip the proof of this result.
Recall that for any \(|k|\)-grading on \(\mathfrak g\), there is a unique grading element \(E\), such that for \(i=-k,\dots,k\) the subspace \(\mathfrak g_i\) is the eigenspace with eigenvalue \(i\) for the adjoint action of \(E\). In particular, \(E\) has to lie in the center of the subalgebra \(\mathfrak g_0\). In the case of a \(|1|\)-grading, this center has dimension \(1\) and thus is spanned by \(E\).
Lemma 4.1. Consider a Lie group \(G\) with simple Lie algebra \(\mathfrak g\) that is endowed with a \(|1|\)-grading with grading element \(E\), and let \(G_0\subset P\subset G\) be subgroups associated to this grading. Let \(\mathbb V\) be a representation of \(G\) which is irreducible as a representation of \(\mathfrak g\). Then there is a \(G_0\)-invariant decomposition \(\mathbb V=\mathbb V_0\oplus\dots\oplus\mathbb V_N\) such that
Each \(\mathbb V_j\) is an eigenspace of \(E\).
For \(i\in\{-1,0,1\}\) and each \(j\), we have \(\mathfrak g_i\cdot\mathbb V_j\subset\mathbb V_{i+j}\).
For each \(j>0\), restriction of the representation defines a surjection \(\mathfrak g_1\otimes\mathbb V_{j-1}\to\mathbb V_j\).
The canonical \(P\)-invariant filtration on \(\mathbb V\) is given by \(\mathbb V^j=\oplus_{\ell\geq j}\mathbb V_\ell\).
Proof. Note first that the \(|1|\)-grading of \(\mathfrak g\) induces a \(|1|\)-grading on the complexification \(\mathfrak g^{\mathbb C}\) of \(\mathfrak g\), which has the same grading element \(E\) as \(\mathfrak g\). It is also well known that there is a Cartan subalgebra of \(\mathfrak g^{\mathbb C}\) that contains \(E\). Complexifying \(\mathbb V\) and \(\mathfrak g\) if necessary and then passing back to the \(E\)-invariant subspace \(\mathbb V\), we conclude that \(E\) acts diagonalizably on \(\mathbb V\). Denoting the \(\lambda\)-eigenspace for \(E\) in \(\mathbb V\) by \(\mathbb V_\lambda\), it follows readily that \(\mathfrak g_i\cdot\mathbb V_\lambda\subset\mathbb V_{\lambda+i}\) for \(i\in\{-1,0,1\}\). Now take an eigenvalue \(\lambda_0\) with minimal real part, let \(N\) be the smallest positive integer such that \(\lambda_0+N+1\) is not an eigenvalue of \(E\) and put \(\mathbb V_j:=\mathbb V_{\lambda_0+j}\) for \(j=0,\dots,N\). Then, by construction, \(\mathfrak g_{-1}\) acts trivially on \(\mathbb V_0\), \(\mathfrak g_1\) acts trivially on \(\mathbb V_N\), and each \(\mathbb V_j\) is \(\mathfrak g_0\)-invariant. This shows that \(\mathbb V_0\oplus\dots\oplus\mathbb V_N\) is \(\mathfrak g\)-invariant and hence has to coincide with \(\mathbb V\) by irreducibility.
By definition, the adjoint action of each element \(g_0\in G_0\) preserves the grading of \(\mathfrak g\), which easily implies that \(\operatorname{Ad}(g_0)(E)\) acts on \(\mathfrak g_i\) by multiplication by \(i\) for \(i\in\{-1,0,1\}\). This means that \(\operatorname{Ad}(g_0)(E)-E\) lies in the center of \(\mathfrak g\), so \(\operatorname{Ad}(g_0)(E)=E\). But then for \(v\in\mathbb V\), we can compute \(E\cdot g_0\cdot v\) as \(\operatorname{Ad}(g_0)(E)\cdot g_0\cdot v=g_0\cdot E\cdot v\). This shows that each \(\mathbb V_j\) is \(G_0\)-invariant and it only remains to prove the last two claimed properties of the decomposition.
We put \(\tilde{\mathbb V}_0:=\mathbb V_0\) and for \(j>0\), we inductively define \(\tilde{\mathbb V}_j\) as the image of the map \(\mathfrak g_1\otimes\tilde{\mathbb V}_{j-1}\to\mathbb V_j\). Then, by construction, each \(\tilde{\mathbb V}_j\) is a \(\mathfrak g_0\)-invariant subspace of \(\mathbb V_j\), so \(\tilde{\mathbb V}:=\oplus_{j=0}^N\tilde{\mathbb V}_j\subset\mathbb V\) is invariant under the actions of \(\mathfrak g_0\) and \(\mathfrak g_1\). But for \(X\in\mathfrak g_{-1}\) and \(Z\in\mathfrak g_1\), we have \([X,Z]\in\mathfrak g_0\) and for \(v\in\mathbb V\) we get \[X\cdot Z\cdot v=Z\cdot X\cdot v+[Z,X]\cdot v.\] This inductively shows that \(\tilde{\mathbb V}\) is invariant under the action of \(\mathfrak g_{-1}\). Thus it is \(\mathfrak g\)-invariant and hence has to coincide with \(\mathbb V\) by irreducibility, so it remains to verify the claimed description of the canonical \(P\)-invariant filtration.
To do this, we first claim that an element \(v\in\mathbb V\) such that \(Z\cdot v=0\) for all \(Z\in\mathfrak g_1\) has to be contained in \(\mathbb V_N\). It suffices to prove this for the complexification, so we may assume that both \(\mathfrak g\) and \(\mathbb V\) are complex and so there is a highest weight vector \(v_0\in\mathbb V\) which is unique up to scale by irreducibility. It is then well known that \(\mathbb V\) is spanned by vectors obtained from \(v_0\) by the iterated action of elements in negative root spaces of \(\mathfrak g\). Since on such elements \(E\) has non-positive eigenvalues, we conclude that \(v_0\in\mathbb V_N\). Now assume that for some \(j<N\), the space \(W:=\{v\in\mathbb V_j:\mathfrak g_1\cdot v=\{0\}\}\) is non-trivial. Then, by construction, this is a \(\mathfrak g_0\)-invariant subspace of \(\mathbb V_j\) on which the center of \(\mathfrak g_0\) acts by a scalar, so it must contain a vector that is annihilated by all elements in positive root spaces of \(\mathfrak g_0\). But since any positive root space of \(\mathfrak g\) either is a positive root space of \(\mathfrak g_0\) or is contained in \(\mathfrak g_1\), this has to be a highest weight vector for \(\mathfrak g\), which contradicts uniqueness of \(v_0\) up to scale.
Having proved the claim, we can first interpret it as showing that \(\mathbb V^N=\mathbb V_N\). From this the description of the \(P\)-invariant filtration follows by backwards induction: Suppose that that we have shown that \(\mathbb V^{N-j}=\mathbb V_{N-j}\oplus\dots\oplus\mathbb V_N\) and let \(w\in\mathbb V\) be such that for all \(Z\in\mathfrak g_1\), we have \(Z\cdot w\in\mathbb V^{N-j}\). Decomposing \(w=w_0+\dots+w_N\), we conclude that for all \(i<N-j-1\) we must have \(Z\cdot w_i=0\) and hence \(w\in\mathbb V_{N-j-1}\oplus\dots\oplus\mathbb V_N\). Together with the obvious fact that \(\oplus_{\ell\geq N-j-1}\mathbb V_\ell\subset\mathbb V^{N-j-1}\), this implies the description of the \(P\)-invariant filtration. ◻
Using this, we can now prove an alternative description of the bundle of Weyl structures that, as we shall see in the examples below, generalizes the construction of [19].
Theorem 4.2. Suppose that \((G,P)\) corresponds to a \(|1|\)-grading of the Lie algebra \(\mathfrak g\) of \(G\). Let \(\mathbb V\) be a representation of \(G\), which is non-trivial and irreducible as a representation of \(\mathfrak g\), with natural \(P\)-invariant filtration \(\{\mathbb V^j:j=0,\dots,N\}\) such that \(\mathbb V/\mathbb V^1\) has real dimension \(1\). For a parabolic geometry \((p:\mathcal G\to M,\omega)\) of type \((G,P)\) let \(\mathcal VM\) be the tractor bundle induced by \(\mathbb V\), \(\mathcal V^jM\) the subbundle corresponding to \(\mathbb V^j\), and define \(\mathcal EM\) to be the real line bundle \(\mathcal VM/\mathcal V^1M\).
Then the bundle \(A\to M\) of Weyl structures can be naturally identified with the open subbundle in the projectivization \(\mathcal P(\mathcal VM/\mathcal V^2M)\) formed by all lines that are transversal to the subbundle \(\mathcal V^1M/\mathcal V^2M\) of hyperplanes. This in turn leads to an identification of \(A\to M\) with the bundle of all linear connections on the line bundle \(\mathcal EM\to M\).
Proof. By assumption \(\mathbb V^1\subset\mathbb V\) is a \(P\)-invariant hyperplane, so this descends to a \(P\)-invariant hyperplane \(\mathbb V^1/\mathbb V^2\) in \(\mathbb V/\mathbb V^2\). Passing to the projectivization, the complement of this hyperplane is a \(P\)-invariant open subset \(U\subset\mathcal P(\mathbb V/\mathbb V^2)\) and hence defines a natural open subbundle in the associated bundle \(\mathcal P(\mathcal VM/\mathcal V^2M)\).
Now take the decomposition \(\mathbb V=\oplus_{j=0}^N\mathbb V_j\) from Lemma 4.1. Then \(\mathbb V_0\) is a line in \(\mathbb V\) transversal to \(\mathbb V^1\) and hence defines a point \(\ell_0\in U\). We claim that the \(P\)-orbit of \(\ell_0\) is all of \(U\), while its stabilizer subgroup in \(P\) coincides with \(G_0\). This shows that \(U\cong P/G_0\) and thus implies the first claimed description of \(A\to M\). As observed in Section 2.4, an element \(g\in P\) can be written uniquely as \(\exp(Z)g_0\) for \(g_0\in G_0\) and \(Z\in\mathfrak g_1\). We know that \(\mathbb V_0\) is \(G_0\)-invariant, so for \(w\in\ell_0\) we get \(g_0\cdot w=aw\) for some nonzero element \(a\in\mathbb R\). On the other hand, \(\exp(Z)\cdot w=w+Z\cdot w+\tfrac12Z\cdot Z\cdot w+\dots\), and all but the first two summands lie in \(\mathbb V^2\). This shows that the action of \(\exp(Z)g_0\) sends \(\ell_0\) to the line in \(\mathbb V/\mathbb V^2\) spanned by \(w+Z\cdot w+\mathbb V^2\). But from Lemma 4.1, we know that the action defines a surjection \(\mathfrak g_1\otimes\mathbb V_0\to\mathbb V_1\), which shows that \(P\cdot\ell_0=U\). On the other hand, it is well known that \(\mathfrak g_1\) is an irreducible representation of \(\mathfrak g_0\). Thus also \(\mathfrak g_1\otimes\mathbb V_0\) is irreducible, so \(Z\cdot w=0\) if and only \(Z=0\), which shows that the stabilizer of \(\ell_0\) in \(P\) coincides with \(G_0\).
For the second description, we need some input from the machinery of BGG sequences. There is a natural invariant differential operator \(S:\Gamma(\mathcal EM)\to\Gamma(\mathcal VM)\) which splits the tensorial map \(\Gamma(\mathcal VM)\to\Gamma(\mathcal EM)\) induced by the quotient projection \(\mathcal VM\to\mathcal EM\). It turns out that the operator \(\Gamma(\mathcal EM)\to\Gamma(\mathcal VM/\mathcal V^{i+1}M)\) induced by \(S\) has order \(i\), so there is an induced vector bundle map from the jet prolongation \(J^i\mathcal EM\) to \(\mathcal VM/\mathcal V^{i+1}M\). As proved in [5], the representation \(\mathbb V\) determines an integer \(i_0\) such that this is an isomorphism for all \(i\leq i_0\). For a non-trivial representation \(i_0\geq 1\), so we conclude that \(J^1\mathcal EM\cong \mathcal VM/\mathcal V^2M\). Since \(S\) splits the tensorial projection, we see that, in a point \(x\in M\), the hyperplane \(\mathcal V^1_xM/\mathcal V^2_xM\) corresponds to the jets of sections vanishing in \(x\). Thus lines in \(\mathcal VM/\mathcal V^2M\) that are transversal to \(\mathcal V^1M/\mathcal V^2M\) exactly correspond to lines in \(J^1\mathcal EM\) that are transversal to the kernel of the natural projection to \(\mathcal EM\). Choosing such a line is equivalent to choosing a splitting of this projection and thus of the jet exact sequence for \(J^1\mathcal EM\). It is well known that the choice of such a splitting is equivalent to the choice of a linear connection on \(\mathcal EM\). ◻
Example 28. (1) Oriented projective structures. For \(n\geq 2\), put \(G:=SL(n+1,\mathbb R)\) and let \(P\) be the stabilizer of the ray in \(\mathbb R^{n+1}\) spanned by the first element \(e_0\) in the standard basis. Taking the complementary hyperplane spanned by the remaining basis vectors, one obtains a \(|1|\)-grading on the Lie algebra \(\mathfrak g\) of \(G\) by decomposing into blocks of sizes \(1\) and \(n\) as in \(\left(\begin{smallmatrix}\mathfrak g_0 & \mathfrak g_1\\ \mathfrak g_{-1} & \mathfrak g_0 \end{smallmatrix}\right)\). The subgroup \(G_0\subset P\) is then easily seen to consist of all block diagonal matrices in \(P\).
Now we define \(\mathbb V:=\mathbb R^{(n+1)*}\), the dual of the standard representation of \(G\). In terms of the dual of the standard basis, this decomposes as the sum of \(\mathbb V_0:=\mathbb R\cdot e_0^*\) and \(\mathbb V_1\) spanned by the remaining basis vectors. All properties claimed in Lemma 4.1 are obviously satisfied in this case. The tractor bundle \(\mathcal VM\) corresponding to \(\mathbb V\) is usually called the (standard) cotractor bundle \(\mathcal T^*M\) and the line bundle \(\mathcal EM\) is the bundle \(\mathcal E(1)\) of projective \(1\)-densities. Since \(\mathbb V^2=\{0\}\) in this case, Theorem 4.2 realizes \(A\) as an open subbundle in \(\mathcal P(\mathcal T^*M)\), and this is exactly the construction from [19]. In fact, it is well known that \(\mathcal T^*M\cong J^1\mathcal E(1)\) in this case, this is even used as a definition in [2].
More generally, for \(k\geq 2\), we can take \(\mathbb V\) to be the symmetric power \(S^k\mathbb R^{(n+1)*}\). This visibly decomposes as \(\mathbb V_0\oplus\dots\oplus\mathbb V_k\), where \(\mathbb V_i\) is spanned by the symmetric products of \((e_0^*)^{k-i}\) with \(i\) other basis elements. This corresponds to the tractor bundle \(S^k\mathcal T^*M\), while the quotient \(\mathbb V/\mathbb V^1\) induces the \(k\)th power of \(\mathcal E(1)\), which is usually denoted by \(\mathcal E(k)\) and called the bundle of projective \(k\)-densities. Again, all properties claimed in Lemma 4.1 are obviously satisfied.
(2) Conformal structures. For \(p+q=n\geq 3\), we put \(G:=SO(p+1,q+1)\) and we take a basis \(e_0,\dots,e_{n+1}\) for the standard representation \(\mathbb R^{n+2}\) of \(G\) such that the non-trivial inner products are \(\langle e_0,e_{n+1}\rangle=1\), and \(\langle e_i,e_i\rangle=1\) for \(1\leq i\leq p\) and \(\langle e_i,e_i\rangle=-1\) for \(p+1\leq i\leq n\). Splitting matrices into blocks of sizes \(1\), \(n\), and \(1\) defines a \(|1|\)-grading of \(\mathfrak g\) according to \(\left(\begin{smallmatrix} \mathfrak g_0 & \mathfrak g_1 & 0\\ \mathfrak g_{-1} & \mathfrak g_0 & * \\ 0 & * & * \end{smallmatrix}\right)\), where entries marked by \(*\) are determined by other entries of the matrix. Again \(G_0\) turns out to consist of block diagonal matrices and is isomorphic to the conformal group \(CO(p+1,q+1)\) via the adjoint action on \(\mathfrak g_{-1}\). In view of 14 we conclude that a parabolic geometry of type \((G,P)\) on a manifold \(M\) is equivalent to a conformal structure.
The standard representation \(\mathbb V\) of \(G\) now decomposes as \(\mathbb V=\mathbb V_0\oplus\mathbb V_1\oplus\mathbb V_2\), with the subspaces spanned by \(e_0\), \(\{e_1,\dots,e_n\}\), and \(e_{n+1}\), respectively. This induces the standard tractor bundle \(\mathcal TM\) on conformal manifolds, and the bundle induced by \(\mathbb V/\mathbb V^1\) is the bundle \(\mathcal E[1]\) of conformal \(1\)-densities. Hence Theorem 4.2 in this case realizes \(A\) as an open subbundle of the projectivization of the quotient of \(\mathcal TM\) by its smallest filtration component. Again, it is well known that this quotient is isomorphic to \(J^1\mathcal E[1]\).
Alternatively, for \(k\geq 2\), we can take \(\mathbb V\) to be the trace-free part \(S^k_0\mathbb R^{n+2}\) in the symmetric power of the standard representation. This leads to the bundle \(S^k_0\mathcal TM\) and the line bundle \(\mathcal E[k]\) of conformal densities of weight \(k\). Here the decomposition from Lemma 4.1 becomes a bit more complicated, since the individual pieces \(\mathbb V_j\) are not irreducible representations of \(G_0\) in general. Still the properties claimed in Lemma 4.1 are obvious via the construction from the decomposition of the standard representation.
(3) Almost Grassmannian structures. Here we choose integers \(2\leq p\leq q\), put \(n=p+q\), take \(G:=SL(n,\mathbb R)\) and \(P\subset G\) the stabilizer of the subspace spanned by the first \(p\) vectors of the standard basis of the standard representation \(\mathbb R^n\) of \(G\). Fixing the complementary subspace spanned by the remaining \(q\) vectors in that basis, one obtains a decomposition of the Lie algebra \(\mathfrak g\) of \(G\) into blocks of sizes \(p\) and \(q\), which defines a \(|1|\)-grading as in the projective case. Then \(G_0\) again turns out to consist of block diagonal matrices and hence is isomorphic to \(S(GL(p,\mathbb R)\times GL(q,\mathbb R))\), while \(\mathfrak g_{-1}\) can be identified with the space of \(q\times p\)-matrices endowed with the action of \(G_0\) defined by matrix multiplication from both sides.
Hence the corresponding geometries exist in dimension \(pq\) and they are essentially given by an identification of the tangent bundle with a tensor product of two auxiliary bundles of rank \(p\) and \(q\), respectively, see Section 4.1.3 of [16]. There it is also shown that for these types of structures the Cartan curvature has two fundamental components, but their nature depends on \(p\) and \(q\). For \(p=q=2\), such a structure is equivalent to a split-signature conformal structure, so we will not discuss this case here. If \(p=2\) and \(q>2\), then one of these quantities is the intrinsic torsion of the structure, but the second is a curvature, so this is a case in which there are non-flat, torsion-free examples. For \(p>3\), the intrinsic torsion splits into two components, and torsion-freeness of a geometry implies local flatness.
The basic choice of a representation \(\mathbb V\) that Theorem 4.2 can be applied to is given by \(\Lambda^p\mathbb R^{n*}\), the \(p\)th exterior power of the dual of the standard representation. This decomposes as \(\mathbb V=\mathbb V_0\oplus\dots\oplus\mathbb V_p\), where \(\mathbb V_j\) is spanned by wedge products of elements of the dual of the standard basis that contain \(p-j\) factors from \(\{e_1^*,\dots,e_p^*\}\). The properties claimed in Lemma 4.1 can be easily deduced from the construction from the dual of the standard representation.
This is the prototypical example of the non-linear PDE that we want to study. In the setting of projective geometry, we have met the density bundles \(\mathcal E(k)\) for \(k>0\) in 28. We define \(\mathcal E(-k)\) to be the line bundle dual to \(\mathcal E(k)\) and use the convention that adding “\((k)\)” to the name of a bundle indicates a tensor product with \(\mathcal E(k)\) for \(k\in\mathbb Z\). The first step towards the construction of the projective Monge-Ampère equation is that there is a projectively invariant, linear, second order differential operator \(H:\Gamma(\mathcal E(1))\to \Gamma(S^2T^*M(1))\) called the projective Hessian. Indeed, this is the first operator in the BGG sequence determined by the standard cotractor bundle, see [13].
Now for a section \(\sigma\in\Gamma(\mathcal E(1))\), \(H(\sigma)\) defines a symmetric bilinear form on each tangent space of \(M\), and such a form has a well defined determinant. In projective geometry, this determinant admits an interpretation as a density as follows. In the setting of part (1) of 28, the top exterior power \(\Lambda^{n+1}\mathbb R^{(n+1)*}\) is a trivial representation, which implies that the bundle \(\Lambda^{n+1}\mathcal T^*M\) is canonically trivial. Identifying \(\mathcal T^*M\) with \(J^1\mathcal E(1)\), the jet exact sequence \(0\to T^*M(1)\to J^1\mathcal E(1)\to\mathcal E(1)\to 0\) implies that \(\Lambda^{n+1}\mathcal T^*M\cong\Lambda^nT^*M(n+1)\), so \(\Lambda^nT^*M\cong\mathcal E(-n-1)\). This isomorphism can be encoded as a tautological section of \(\Lambda^nTM(-n-1)\). To form the determinant of \(H(\sigma)\), one now takes the tensor product of two copies of this canonical section and of \(n\) copies of \(H(\sigma)\) and forms the unique (potentially) non-trivial complete contraction of the result (so the two indices of each copy of \(H(\sigma)\) have to be contracted into different copies of the tautological form). This shows that \(\det(H(\sigma))\) can be naturally interpreted as a section of \(\mathcal E(-n-2)\).
Assuming that \(\sigma\in\Gamma(\mathcal E(1))\) is nowhere vanishing, we can form \(\sigma^k\in\Gamma(\mathcal E(k))\) for any \(k\in\mathbb Z\), and hence \[ \det(H(\sigma))=\pm\sigma^{-n-2}\](4.1) is a projectively invariant, fully non-linear PDE on nowhere vanishing sections of \(\mathcal E(1)\). Observe that multiplying \(\sigma\) by a constant, the two sides of the equation scale by different powers of the constant, so allowing a constant factor instead of just a sign in the right hand side of the equation would only be a trivial modification.
Let us first observe that a nowhere vanishing section \(\sigma\in\mathcal E(1)\) uniquely determines a Weyl structure. In the language of Theorem 4.2 this can be either described as the structure corresponding to the flat connection on \(\mathcal E(1)\) determined by \(\sigma\) or as the one corresponding to the line in \(\mathcal T^*M\) spanned by \(S(\sigma)\), where \(S\) denotes the BGG splitting operator. From either interpretation it is clear that this Weyl structure remains unchanged if \(\sigma\) is multiplied by a non-zero constant. Alternatively, one can easily verify that any projective class on \(M\) contains a unique connection such that \(\sigma\) is parallel for the induced connection on \(\mathcal E(1)\).
To deal with non-flat cases in the following theorem, we use a concept of mean curvature tailored to the case of connections compatible with an almost bi-Lagrangian structure that was introduced in [18]. That article uses the terminology of (almost) para-Kähler structures, which is slightly different from ours, but it is easy to translate between the two.
Theorem 4.3. Let \(M\) be an oriented smooth manifold of dimension \(n\) which is endowed with a projective structure. Let \(\sigma\in\Gamma(\mathcal E(1))\) be a nowhere-vanishing section and let us denote by \(\nabla^\sigma\) the Weyl connections of the Weyl structure determined by \(\sigma\) and by \(\mbox{\textsf{P}}^{\sigma}\) its Rho tensor. Then we have:
(1) An appropriate constant multiple of \(\sigma\) satisfies (4.1) if and only if \(\nabla^\sigma(\det(\mbox{\textsf{P}}^{\sigma}))=0\) and \(\det(\mbox{\textsf{P}}^\sigma)\) is nowhere vanishing.
(2) The Weyl structure determined by \(\sigma\) is always Lagrangian. If \(M\) is projectively flat, then an appropriate constant multiple of \(\sigma\) satisfies (4.1) if and only if this Weyl structure is non-degenerate and the image of the corresponding section \(s:M\to A\) is a minimal submanifold. This extends to curved projective structures provided that minimality of \(s(M)\) is defined as vanishing of the mean curvature form associated to the canonical connection \(D\) via the definition in [18].
Proof. It is well known how to decompose the curvature of a linear connection on \(TM\) into the projective Weyl curvature and the Rho-tensor, see Section 3.1 of [2] (taking into account the sign conventions mentioned in Section 2.6). It is also shown there that the Bianchi identity shows that the skew part of the Rho tensor is a non-zero multiple of the trace of the curvature tensor, which describes the action of the curvature on the top exterior power of the tangent bundle and thus on density bundles. This readily implies that \(\mbox{\textsf{P}}^\sigma\) is symmetric, so the Weyl structure defined by \(\sigma\) is Lagrangian by Proposition 3.6.
(1) It is well known that the projective Hessian in terms of a linear connection \(\nabla\) in the projective class and its Rho tensor \(\mbox{\textsf{P}}\) is given by the symmetrization of \(\nabla^2\sigma-\mbox{\textsf{P}}\sigma\), see Section 3.2 of [13]. (The different sign is caused by different sign conventions for the Rho-tensor.) But by definition \(\nabla^\sigma\sigma=0\) and \(\mbox{\textsf{P}}^{\sigma}\) is symmetric, so we conclude that \(H(\sigma)=-\mbox{\textsf{P}}^\sigma\sigma\) and hence \(\det(H(\sigma))=(-1)^n\sigma^n\det(\mbox{\textsf{P}}^{\sigma})\). Now for each \(k\neq 0\), the sections of \(\mathcal E(k)\) that are parallel for \(\nabla^\sigma\) are exactly the constant multiples of \(\sigma^k\), so (1) follows readily.
(2) Since \(\mbox{\textsf{P}}^\sigma\) is symmetric, \(\det(\mbox{\textsf{P}}^\sigma)\) is nowhere vanishing if and only if \(\mbox{\textsf{P}}^\sigma\) is non-degenerate. By Proposition 3.6, this is equivalent to non-degeneracy of the Weyl structure determined by \(\sigma\), and we assume this from now on. Let us write \(\det(\mbox{\textsf{P}}^{\sigma})\) in terms of the tautological section \(\epsilon\) of \(\Lambda^nTM(-n-1)\) as above as \(C(\epsilon\otimes\epsilon\otimes(\mbox{\textsf{P}}^{\sigma})^{\otimes^n})\), where \(C\) denotes the appropriate contraction. Applying \(\nabla^\sigma\) to this, we observe that \(C\) and \(\epsilon\) are projectively invariant bundle maps and thus parallel for any Weyl connection. Thus we conclude that \[\nabla^\sigma\det(\mbox{\textsf{P}}^{\sigma})=(n-1)C\left(\epsilon\otimes\epsilon\otimes(\mbox{\textsf{P}}^{\sigma})^{\otimes^{n-1}} \otimes\nabla^\sigma\mbox{\textsf{P}}^\sigma\right).\] Here we have used that the contraction is symmetric in the bilinear forms we enter and in the right hand side the form index of \(\nabla^{\sigma}\) remains uncontracted. Since we assume that \(\mbox{\textsf{P}}^\sigma\) is invertible, linear algebra tells us that contracting two copies of \(\epsilon\) with \((\mbox{\textsf{P}}^{\sigma})^{\otimes^{n-1}}\) gives \(\det(\mbox{\textsf{P}}^\sigma)\Phi\), where \(\Phi\in\Gamma(S^2TM)\) is the inverse of \(\mbox{\textsf{P}}^\sigma\). Returning to the abstract index notation used in Theorem 3.8 and writing \(\nabla\) and \(\mbox{\textsf{P}}\) instead of \(\nabla^\sigma\) and \(\mbox{\textsf{P}}^\sigma\), we conclude that \(\nabla\det(\mbox{\textsf{P}})=0\) is equivalent to \(0=\mbox{\textsf{P}}^{ab}\nabla_i\mbox{\textsf{P}}_{ab}\).
On the other hand, we know the second fundamental form of \(s(M)\subset A\) from Theorem 3.8. To determine the mean curvature, we have to contract an inverse metric into this expression, and we already know that this inverse metric is just \(\mbox{\textsf{P}}^{ij}\). Vanishing or non-vanishing of the result is independent of the final contraction with \(\mbox{\textsf{P}}^{kc}\). Thus we conclude that \(s(M)\subset A\) is minimal if and only if \[ 0=\mbox{\textsf{P}}^{ab}(2\nabla_a\mbox{\textsf{P}}_{bi}-\nabla_i\mbox{\textsf{P}}_{ab}).\](4.2) In the proof of Theorem 3.8, we have also noted that the Cotton-York tensor is given by the alternation of \(\nabla_i\mbox{\textsf{P}}_{jk}\) in the first two indices. It is well known that this vanishes for projectively flat structures (see [2]) and hence in the projectively flat case, \(\nabla_i\mbox{\textsf{P}}_{jk}\) is completely symmetric. Using this, the claim in the projectively flat case follows immediately.
In the non-flat case, we first have to determine the map \(\varphi\) from Lemma 4 of [18]. In our notation, the map \(P\) used there is given by \(P|_{L^\pm}=\pm\operatorname{id}\). Using this, the beginning of the proof of Theorem 3.7 readily shows that, in the notation used there, for \(\xi\in T_xM\cong L^-_{s(x)}\), we get \(\varphi(\xi^i)=(\xi^i,-\mbox{\textsf{P}}_{ja}\xi^a)\). Now we can combine this with the formula for \(II_D\) from Theorem 3.8, which describes the operator \(\widehat{A}\) used in [18]. This easily shows that, up to a non-zero factor, that the operator \(\widehat{h}\) from [18] is given by \[\widehat{h}(\xi^i,\eta^j,\zeta^k)=\xi^i\eta^j\zeta^k\mbox{\textsf{P}}_{ia}\mbox{\textsf{P}}^{ab}\nabla^s_j\mbox{\textsf{P}}_{kb}.\] By definition, the mean curvature form \(\widehat{H}\) from [18] is the trace over the first and third entry of this. Thus we have to contract \(\widehat{h}_{ijk}\) with \(\mbox{\textsf{P}}^{ik}\), which again leads to \(\mbox{\textsf{P}}^{ab}\nabla^s_j\mbox{\textsf{P}}_{ab}\). ◻
Remark 30. In the special case of a two-dimensional projective structure the minimality condition (4.2) was previously obtained in [28].
A deep relation between solutions of the projective Monge-Ampère equation and properly convex projective structures was established in the works [25] by Labourie and [26] by Loftin. Recall that a projective manifold \((M,[\nabla])\) is called properly convex if it arises as a quotient of a properly convex open set \(\tilde{M}\subset \mathbb{RP}^n\) by a group \(\Gamma\) of projective transformations which acts discretely and properly discontinuously. The projective line segments contained in \(\tilde{M}\) project to \(M\) to become the geodesics of \([\nabla]\). Therefore, locally, the geodesics of a properly convex projective structure \([\nabla]\) can be mapped diffeomorphically to segments of straight lines, that is, \([\nabla]\) is locally flat. Combining the work of Labourie and Loftin with Theorem 4.3, we obtain:
Corollary 4.4. Let \((M,[\nabla])\) be a closed oriented locally flat projective manifold. Then \([\nabla]\) is properly convex if and only if \([\nabla]\) arises from a minimal Lagrangian Weyl structure whose Rho tensor is positive definite.
Proof. Suppose that the flat projective structure \([\nabla]\) arises from a minimal Lagrangian Weyl structure \(s\) whose Rho tensor \(\mbox{\textsf{P}}^s\) is positive definite. Since \(s\) is Lagrangian, \(\mbox{\textsf{P}}^s\) is a constant negative multiple of the Ricci tensor of the Weyl connection \(\nabla^s\), see [2], and taking into account the sign issue mentioned in Section 2.6. By Theorem 3.8, the nowhere vanishing density \(\det(\mbox{\textsf{P}}^s)\) is preserved by \(\nabla^s\), whence an appropriate power defines a volume density that is parallel for \(\nabla^s\). Finally, projective flatness implies that the pair \((\nabla^s,\mbox{\textsf{P}}^s)\) satisfies the hypothesis of Theorem 3.2.1 of [25], which then implies that \([\nabla]\) is properly convex.
Conversely, suppose that \([\nabla]\) is properly convex. By [26] there is a solution \(\sigma\) to the projective Monge-Ampère equation with right hand side \((-1)^{n+2}\sigma^{n+2}\) and such that \(\sigma\) is negative for the natural orientation on \(\mathcal E(1)\). By Theorem 4.3, \([\nabla]\) arises from a minimal Lagrangian Weyl structure. Since the Hessian of \(\sigma\) is positive definite, so is the Rho tensor. ◻
Remark 32. Existence and uniqueness of minimal Lagrangian Weyl structures for a given torsion-free AHS structure is an interesting fully non-linear PDE problem. In the special case of projective surfaces, some partial results regarding uniqueness have been obtained in [27] and [30]. See also [31] for a connection to dynamical systems and [29] for a related variational problem on the space of conformal structures.
We conclude this article with some remarks on analogs of the projective Monge-Ampère equation for other AHS structures. The first observation is that a small representation theoretic condition is sufficient to obtain an analog of the projectively invariant Hessian, which again is closely related to the Rho tensor.
To formulate this, we need a bit of background. Suppose that \((G,P)\) corresponds to a \(|1|\)-grading of \(G\) and let \(G_0\subset P\) be the subgroup determined by the grading. Then this naturally acts on each \(\mathfrak g_i\), and there is an induced representation on \(S^2\mathfrak g_1\). We can decompose this representation into irreducibles and there is a unique component whose highest weight is twice the highest weight of \(\mathfrak g_1\). This is called the Cartan square of \(\mathfrak g_1\) and denoted by \(\circledcirc^2\mathfrak g_1\). It comes with a canonical \(G_0\)-equivariant projection \(\pi:\otimes^2\mathfrak g_1\to\circledcirc^2\mathfrak g_1\). For any parabolic geometry of type \((G,P)\), this induces a natural subbundle \(\circledcirc^2T^*M\subset S^2T^*M\) and a natural bundle map \(\pi:\otimes^2T^*M\to\circledcirc^2T^*M\).
Proposition 4.5. Suppose that \((G,P)\) corresponds to a \(|1|\)-grading on the simple Lie algebra \(\mathfrak g\) of \(G\). Suppose further, that there is a representation \(\mathbb V\) of \(G\) satisfying the assumptions of Theorem 4.2 whose complexification is a fundamental representation of the complexification of \(\mathfrak g\), and let \(\mathcal EM\) denote the natural line bundle induced by \(\mathbb V/\mathbb V^1\).
(1) There is an invariant differential operator \(H:\Gamma(\mathcal EM)\to\Gamma(\circledcirc^2T^*M\otimes\mathcal EM)\) of second order.
(2) For a nowhere vanishing section \(\sigma\in\Gamma(\mathcal EM)\), let \(\mbox{\textsf{P}}^\sigma\) be the Rho tensor of the Weyl structure determined by \(\sigma\). Then \(H(\sigma)\) is a non-zero multiple of \(\pi(\mbox{\textsf{P}}^\sigma)\sigma\), where \(\pi\) is the projection to the Cartan square.
Proof. (1) The representation \(\mathbb V\) induces a tractor bundle on parabolic geometries of type \((G,P)\) to which the construction of BGG sequences can be applied. The first operator \(H\) in the resulting sequence is defined on \(\Gamma(\mathcal EM)\). Now the condition that \(\dim(\mathbb V/\mathbb V^1)=1\) implies that the complexification of \(\mathbb V\) is the fundamental representation corresponding to the simple root that induces the \(|1|\)-grading that defines \(\mathfrak p\). Since the complexification of \(\mathbb V\) is a fundamental representation, the results of [5] show that the first operator in the BGG sequence has order two and the target space claimed in (1).
(2) It is also known in general (see [14] or [10]) how to write out \(H\) in terms of a Weyl structure with Weyl connection \(\nabla^s\) and Rho tensor \(\mbox{\textsf{P}}^s\): For \(\sigma\in\Gamma(\mathcal EM)\), one then has to form \(\nabla^2\sigma-\mbox{\textsf{P}}^s\sigma\), symmetrize and then project to the Cartan square. But if \(s\) is the Weyl structure determined by \(\sigma\), then by definition \(\nabla^s\sigma=0\) and \(\mbox{\textsf{P}}^s=\mbox{\textsf{P}}^\sigma\), which implies the claim. ◻
Observe that 28 provides representations \(\mathbb V\) that satisfy the assumptions of the proposition for conformal and for almost Grassmannian structures. Hence for these two geometries an invariant Hessian is available. It is worth mentioning that, for conformal structures, \(\pi(\mbox{\textsf{P}}^\sigma)\) is the trace-free part of \(\mbox{\textsf{P}}^\sigma\).
It is also a general fact that the top-exterior power of \(T^*M\) is isomorphic to a positive, integral power of the dual \(\mathcal E^*M\) of \(\mathcal EM\): By definition, the grading element \(E\) acts by multiplication by \(\dim(\mathfrak g_1)\) on the top exterior power of \(\mathfrak g_1\), which represents the top exterior power of \(T^*M\). On the other hand, the construction implies that a generator of \(\mathbb V_0\subset\mathbb V\) will be a lowest weight vector of the complexification of \(\mathbb V\), so \(E\) acts by a negative number on this. The fact that we deal with a fundamental representation implies that \(\dim(\mathfrak g_{-1})\) is an integral multiple of that number. As in the projective case, this can be phrased as the existence of a tautological section, which can then be used together with copies of \(H(\sigma)\) to obtain a section of a line bundle, which can be trivial, a tensor power of \(\mathcal E\) or a tensor power of \(\mathcal E^*\). In any case, a nowhere vanishing section of \(\mathcal E\) determines a canonical section of that bundle (which is the constant \(1\) in the trivial case), so there is an invariant version of the Monge-Ampère equation. In view of part (2) of Proposition 4.5, for these equations there is always an analog of part (1) of Theorem 4.3.
For some of the structures, there are additional natural sections that can be used together with powers of \(H(\sigma)\) to construct other non-linear invariant operators, for example, the conformal metric for conformal structures and partial (density valued) volume forms for Grassmannian structures. Again part (2) of Proposition 4.5 shows that all these equations can be phrased as equations on \(\mbox{\textsf{P}}^\sigma\), so there should be a relation to submanifold geometry of Weyl structures in the style of part (2) of Theorem 4.3. All this will be taken up in detail elsewhere.