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Frame bundle

In , the frame bundle of a smooth \pi: E \to M of n over a smooth manifold M is the principal \mathrm{GL}(n, \mathbb{R})-bundle F(E) \to M whose fiber over each point x \in M is the set of all ordered bases (frames) of the fiber E_x. The total space F(E) is constructed as the disjoint union \bigcup_{x \in M} F(E_x), where F(E_x) \cong \mathrm{GL}(n, \mathbb{R}), and the group \mathrm{GL}(n, \mathbb{R}) acts freely and transitively on the right on each fiber by . Local trivializations of E induce those of F(E) via the standard trivialization of \mathrm{GL}(n, \mathbb{R}), ensuring F(E) inherits a . For the tangent bundle TM of an n-dimensional manifold M, the associated frame bundle FM \to M (also called the linear frame bundle or tangent frame bundle) has fibers consisting of ordered bases of tangent vectors at each point, providing a canonical example central to the study of Riemannian and pseudo-Riemannian geometry. The frame bundle encodes the linear structure of E globally, allowing the reconstruction of E as an associated vector bundle F(E) \times_{\mathrm{GL}(n, \mathbb{R})} \mathbb{R}^n. Reductions of the structure group to subgroups like \mathrm{O}(n) yield orthonormal frame bundles, which are principal bundles supporting metric-compatible connections and G-structures on M. Frame bundles are fundamental for defining : a principal connection on F(E) (specified by a \mathfrak{gl}(n, \mathbb{R})-valued 1-form) induces a on sections of E, enabling along curves in M and the study of as an obstruction to flatness. In particular, the linear frame bundle FM carries a soldering form, a tautological \mathbb{R}^n-valued 1-form (taking values in the pullback of TM) that, together with the of the , identifies the tangent spaces of FM with the pullback of TM \oplus TM, facilitating the of local coordinate frames into global geometric objects. In higher-dimensional settings, frame bundles support tensorial structures like almost product tensors, decomposing the into horizontal and vertical components for adapted frames.

Definition and Construction

Principal bundle formulation

The frame bundle P(M) of an n-dimensional smooth manifold M is defined as the principal \mathrm{GL}(n, \mathbb{R})-bundle over M, where the fiber over each point x \in M consists of all ordered bases (frames) of the T_x M. Each such frame is an ordered n-tuple of linearly independent vectors in T_x M, forming the set \mathrm{GL}(T_x M, \mathbb{R}^n), which is acted upon freely and transitively by the general linear group \mathrm{GL}(n, \mathbb{R}). The structure group \mathrm{GL}(n, \mathbb{R}) acts on the right on P(M) by of linear maps: for u = (v_1, \dots, v_n) at x and A \in \mathrm{GL}(n, \mathbb{R}), the action is u \cdot A = (v_1, \dots, v_n) A, preserving the base point x and ensuring the projection \pi: P(M) \to M satisfies \pi(u \cdot A) = \pi(u) = x. This right action is , , and proper, establishing P(M) as in the category of smooth manifolds. Local trivializations of P(M) arise from an atlas \{ (U_\alpha, \psi_\alpha) \} on M, where \psi_\alpha: U_\alpha \to \mathbb{R}^n provides a local coordinate basis for T_x M with x \in U_\alpha; the trivialization map \phi_\alpha: \pi^{-1}(U_\alpha) \to U_\alpha \times \mathrm{GL}(n, \mathbb{R}) sends a frame u to (\pi(u), [\psi_\alpha]_*(u)), with [\psi_\alpha]_* the expressing u in coordinates, and is \mathrm{GL}(n, \mathbb{R})-equivariant. On overlaps U_\alpha \cap U_\beta, the transition functions are g_{\alpha\beta}: U_\alpha \cap U_\beta \to \mathrm{GL}(n, \mathbb{R}), given by the change-of-basis matrices g_{\alpha\beta}(x) = (\psi_\alpha \circ \psi_\beta^{-1})'(\psi_\beta(x)), which are smooth and invertible, satisfying the cocycle condition g_{\alpha\beta} g_{\beta\gamma} = g_{\alpha\gamma}. This formulation addresses the challenge of defining frames globally on M, where local coordinate charts provide bases but fail to extend consistently across the entire manifold due to topological obstructions. As a consequence, the tangent bundle TM emerges as the vector bundle associated to P(M) via the standard representation of \mathrm{GL}(n, \mathbb{R}) on \mathbb{R}^n.

Local coordinate construction

The frame bundle of an n-dimensional smooth manifold M can be explicitly constructed using a coordinate atlas \{(U_\alpha, \phi_\alpha)\} that covers M, where each \phi_\alpha: U_\alpha \to \mathbb{R}^n is a onto an open subset \Omega_\alpha \subset \mathbb{R}^n. For a (U_\alpha, \phi_\alpha), the local trivialization \Phi_\alpha: \pi^{-1}(U_\alpha) \to U_\alpha \times \mathrm{GL}(n, \mathbb{R}) identifies the fiber over x \in U_\alpha with \mathrm{GL}(n, \mathbb{R}) by expressing frames relative to the coordinate frame \{\partial / \partial x^i \mid i=1,\dots,n\} at x, where x^i = \phi_\alpha^i(x). Specifically, an element of the fiber consists of an ordered n-tuple of linearly independent tangent vectors at x, represented in local coordinates by an invertible n \times n matrix A = (a^i_j), whose columns are the coordinate components of these vectors with respect to the basis \partial / \partial x^i; the trivialization maps this frame to (x, A). On overlaps U_\alpha \cap U_\beta \neq \emptyset, the trivializations \Phi_\alpha and \Phi_\beta are compatible via the transition map g_{\beta\alpha}: U_\alpha \cap U_\beta \to \mathrm{GL}(n, \mathbb{R}), defined by \Phi_\beta \circ \Phi_\alpha^{-1}(x, v) = (x, g_{\beta\alpha}(x) v) for x \in U_\alpha \cap U_\beta and v \in \mathbb{R}^n. Here, g_{\beta\alpha}(x) is the matrix of the coordinate change, given explicitly by g_{\beta\alpha}(x) = \frac{\partial \phi_\beta}{\partial \phi_\alpha}(x) = d(\phi_\beta \circ \phi_\alpha^{-1})_{\phi_\alpha(x)}, which belongs to \mathrm{GL}(n, \mathbb{R}) and ensures the bundle structure glues smoothly across charts. This construction yields a principal \mathrm{GL}(n, \mathbb{R})-bundle, as the transition functions satisfy the required cocycle condition g_{\gamma\beta} g_{\beta\alpha} = g_{\gamma\alpha} on triple overlaps. For the \mathbb{R}^n with the standard coordinate \phi: \mathbb{R}^n \to \mathbb{R}^n given by the , the frame bundle is trivialized globally as \mathbb{R}^n \times \mathrm{[GL](/page/GL)}(n, \mathbb{R}), where each over x \in \mathbb{R}^n consists of n-tuples of linearly independent vectors in \mathbb{R}^n, represented by invertible matrices relative to the \{\partial / \partial x^i\}. Similarly, for the circle S^1 parametrized by \theta \in (0, 2\pi) with U = S^1 \setminus \{\pi\} and \phi(\theta) = \theta, the frame bundle over U is trivialized to U \times \mathbb{R}^* (since \mathrm{[GL](/page/GL)}(1, \mathbb{R}) = \mathbb{R}^*), with elements as scalar multiples f(\theta) \cdot \frac{\partial}{\partial \theta} for f(\theta) \neq 0; a second covers the remaining point, and the on the overlap is the on \mathbb{R}^*, confirming the global triviality. These examples illustrate as collections of basis vectors adapted to local coordinates. This coordinate-based construction generalizes the atlas of the TM, where local trivializations map vectors to \mathbb{R}^n via d\phi_\alpha, to the frame bundle by instead mapping bases of spaces to \mathrm{[GL](/page/GL)}(n, \mathbb{R}) via change-of-basis matrices, thereby encoding the full linear structure at each point while preserving the smooth gluing via the same transitions.

Associated Vector Bundles

General construction from frame bundles

The general construction of associated vector bundles from a frame bundle proceeds via a linear representation of the structure group. Let P(M) denote the frame bundle of an n-dimensional smooth manifold M, which is a principal \mathrm{GL}(n,\mathbb{R})-bundle over M. Given a representation \rho: \mathrm{GL}(n,\mathbb{R}) \to \mathrm{GL}(V) of \mathrm{GL}(n,\mathbb{R}) on a finite-dimensional real vector space V, the associated vector bundle E = P(M) \times_\rho V is defined as the quotient space of the product P(M) \times V by the equivalence relation (p, v) \sim (p g, \rho(g^{-1}) v) for all p \in P(M), v \in V, and g \in \mathrm{GL}(n,\mathbb{R}). The projection map \pi: E \to M sends the equivalence class [p, v] to the base point x = \pi_{P(M)}(p) \in M, yielding a vector bundle over M with typical fiber V. This construction is standard in differential geometry and applies to any principal bundle with a compatible representation. The fibers of E over each x \in M consist of equivalence classes [p, v] where p \in P_x(M) is at x, forming a isomorphic to V. In particular, elements of the fiber E_x can be identified fiberwise with linear combinations of the frame vectors in p = (e_1, \dots, e_n) with coefficients determined by the action of \rho, effectively transforming vectors in V relative to the local . For the (defining) \rho: \mathrm{GL}(n,\mathbb{R}) \to \mathrm{GL}(\mathbb{R}^n) where \rho(g) w = g w for w \in \mathbb{R}^n, the associated bundle recovers the : TM \cong P(M) \times_{\mathrm{GL}(n,\mathbb{R})} \mathbb{R}^n. More generally, natural representations of \mathrm{GL}(n,\mathbb{R}) on tensor spaces, such as the on (\mathbb{R}^n)^* yielding the T^*M or the on \mathrm{End}(\mathbb{R}^n) yielding the bundle of endomorphisms \mathrm{End}(TM), produce tensor bundles associated to P(M). This construction is unique in the sense that any smooth vector bundle over M with typical fiber V and structure group a closed subgroup of \mathrm{GL}(\dim V, \mathbb{R}) arises as an associated bundle to its own frame bundle via the standard representation on V; moreover, when the representation factors through \mathrm{GL}(n,\mathbb{R}), such bundles can be realized from the frame bundle P(M) of the tangent space. This framework unifies the study of various geometric bundles on M under the principal bundle structure of P(M).

Identification with the tangent bundle

The tangent bundle TM of an n-dimensional smooth manifold M is canonically isomorphic to the associated vector bundle obtained from the frame bundle P(M), which is the principal \mathrm{GL}(n, \mathbb{R})-bundle of linear frames over M, via the defining (standard) representation of \mathrm{GL}(n, \mathbb{R}) on \mathbb{R}^n. Specifically, TM \cong P(M) \times_{\mathrm{GL}(n, \mathbb{R})} \mathbb{R}^n, where the equivalence class [p, \xi] for a frame p = (e_1, \dots, e_n) at a point x \in M and \xi = (\xi^1, \dots, \xi^n) \in \mathbb{R}^n corresponds to the v = \sum_{i=1}^n \xi^i e_i \in T_x M. This association is well-defined because the right action of g \in \mathrm{GL}(n, \mathbb{R}) transforms [p g, g^{-1} \xi] to the same vector \sum_i (g^{-1} \xi)^i (p g)_i = \sum_i \xi^i e_i. This construction applies the general method of forming associated bundles from principal bundles, specialized here to recover the globally over M. The zero section of TM, which maps each x \in M to the zero vector (x, 0) \in T_x M, corresponds under this to the [p, 0] for any p at x, independent of the choice of frame and thus lifting uniquely to the frame bundle in a manner. In contrast, a general v \in T_x M requires a choice of frame p to express its coordinates \xi such that v = \sum \xi^i e_i, highlighting the frame bundle's role in coordinatizing tangent spaces locally. Tangent vectors can be intrinsically defined as derivations on the space of smooth functions C^\infty(M), acting as v(f) = \frac{d}{dt}\big|_{t=0} f(\gamma(t)) for curves \gamma with \gamma(0) = x and \gamma'(0) = v, providing a frame-independent characterization. This contrasts with the frame expansion v = \sum \xi^i e_i, which relies on a local basis from the frame bundle to decompose v into components, bridging abstract derivations to concrete linear combinations. This identification ensures a global isomorphism between TM and the associated bundle, resolving potential inconsistencies arising from local coordinate choices in frame selections by gluing trivializations consistently via the principal bundle structure.

Linear Frame Bundle

Role of smooth frame fields

A smooth frame field on an n-dimensional smooth manifold M is defined as a smooth section s: M \to P(M) of the linear frame bundle P(M), the principal \mathrm{GL}(n, \mathbb{R})-bundle over M whose fiber at each point x \in M comprises all ordered bases of the T_x M. This section assigns to every x \in M an ordered basis (e_1(x), \dots, e_n(x)) of T_x M such that each component map x \mapsto e_i(x) is smooth as a on M. Equivalently, a smooth frame field consists of n smooth fields on M that are linearly independent at every point, thereby providing a smooth pointwise basis for the TM. Such frame fields always exist locally on any smooth manifold M, as the standard coordinate vector fields \left( \frac{\partial}{\partial x^1}, \dots, \frac{\partial}{\partial x^n} \right) in a local (U, \phi) form a smooth local frame field over U. Globally, however, the existence of a smooth frame field requires the TM to be trivializable, meaning M must be parallelizable. Parallelizable manifolds admit a global smooth frame field spanning TM everywhere; prominent examples include \mathbb{R}^n, where the constant basis (\partial_1, \dots, \partial_n) serves as a global frame, and Lie groups, which possess global frames given by left-invariant vector fields derived from a basis of the . In contrast, most compact manifolds lack global frame fields due to topological constraints. Smooth frame fields establish local trivializations of the frame bundle P(M) via \mathrm{GL}(n, \mathbb{R})-equivariant diffeomorphisms to the trivial bundle M \times \mathrm{GL}(n, \mathbb{R}), enabling the representation of automorphisms of the as linear transformations in \mathrm{GL}(n, \mathbb{R}) over coordinate patches. These equivariant maps facilitate the analysis of bundle structure through transition functions in \mathrm{GL}(n, \mathbb{R}), and the basis fields of the generate local one-parameter subgroups of diffeomorphisms—i.e., flows—whose linear approximations describe automorphisms near each point. Topological obstructions to global frame fields arise from non-triviality of TM, often detected by characteristic classes like the Stiefel-Whitney classes. A classic example is provided by the hairy ball theorem, which asserts that no smooth nowhere-vanishing vector field exists on the even-dimensional sphere S^{2k} for k \geq 1; consequently, since a global frame field would yield n linearly independent smooth vector fields (including at least one nowhere zero), even spheres S^{2k} are not parallelizable. More broadly, only the spheres S^1, S^3, and S^7 among the low-dimensional spheres admit global frame fields, highlighting the rarity of parallelizability in higher dimensions.

Solder form and canonical identification

The solder form on the linear frame bundle P(M) of an n-dimensional smooth manifold M is a canonical \mathbb{R}^n-valued 1-form \theta: TP(M) \to \mathbb{R}^n. For u \in P(M) corresponding to a frame p: \mathbb{R}^n \to T_{\pi(u)}M at the base point \pi(u) \in M, and for \xi \in T_u P(M), it is defined by \theta_u(\xi) = p^{-1} \left( \mathrm{d}\pi_u(\xi) \right), where \pi: P(M) \to M denotes the bundle projection and \mathrm{d}\pi_u: T_u P(M) \to T_{\pi(u)}M its differential. This form exhibits \mathrm{GL}(n,\mathbb{R})-equivariance under the right action R_g of the structure group, satisfying \theta_{u g} \left( \mathrm{d}R_g (\xi) \right) = g^{-1} \theta_u(\xi) for all g \in \mathrm{GL}(n,\mathbb{R}) and \xi \in T_u P(M). It vanishes on vertical tangent vectors—those in the of \mathrm{d}\pi—rendering it with respect to the trivial vertical , though it requires a choice of horizontal subbundle (via a ) for full horizontality in the principal bundle sense. The solder form induces a surjective \mathrm{d}\pi: TP(M) \to \pi^* TM with the vertical subbundle VP(M), yielding an TP(M)/VP(M) \cong \pi^* TM between the by the vertical directions and the of the . Under this identification, a \xi \in T_u P(M) projects to the base vector \mathrm{d}\pi_u(\xi) \in T_{\pi(u)}M, with coordinates in the p given by \theta_u(\xi), effectively "soldering" the fibers of P(M) to the tangent spaces of M via the inverse weighting. This highlights the frame bundle's role in linearizing the structure of M. In , the solder form provides the foundational "soldering" mechanism for Cartan connections on frame bundles, where it pairs with a \mathrm{GL}(n,\mathbb{R})-valued principal connection form to yield a full Cartan geometry modeling the manifold locally on a . It also forms the core of Élie Cartan's method of moving frames, enabling the of frames along submanifolds to compute invariants and symmetries systematically.

Orthonormal Frame Bundle

Reduction of structure group to O(n)

A Riemannian metric g on an n-dimensional smooth manifold M induces a reduction of the structure group of the linear frame bundle P(M), which is a principal \mathrm{GL}(n,\mathbb{R})-bundle, to the orthogonal group \mathrm{O}(n). This reduction yields the orthonormal frame bundle P^O(M), defined as the subbundle of P(M) whose fibers consist precisely of the orthonormal frames with respect to g. Specifically, for each point x \in M, the fiber P^O_x(M) comprises all ordered bases \{e_1, \dots, e_n\} of T_x M such that g(e_i, e_j) = \delta_{ij}, and \mathrm{O}(n) acts on these fibers by right multiplication, preserving orthonormality. The construction proceeds locally: over an open cover \{U_\alpha\} of M, the metric g admits local orthonormal coframes \{\theta^i_\alpha\} on each U_\alpha, which are \mathbb{R}^n-valued 1-forms satisfying g = \sum_{i=1}^n \theta^i \otimes \theta^i (in the standard Euclidean metric on \mathbb{R}^n). The dual frames to these coframes provide local sections of P^O(M), and the transition functions between overlapping trivializations take values in \mathrm{O}(n), ensuring compatibility with the metric. Globally, P^O(M) is a principal \mathrm{O}(n)-bundle over M, obtained as the subbundle of P(M) consisting of orthonormal frames, whose transition functions take values in \mathrm{O}(n). There exists a bijective correspondence between \mathrm{O}(n)-reductions of P(M) and Riemannian metrics on M: given such a reduction P^O(M) \hookrightarrow P(M), the metric g is uniquely determined by, given an orthonormal frame u over x \in M with associated isomorphism u: \mathbb{R}^n \to T_x M, g_x(\xi, \eta) = \langle u^{-1} \xi, u^{-1} \eta \rangle_{\mathbb{R}^n} for tangent vectors \xi, \eta \in T_x M, where \langle \cdot, \cdot \rangle_{\mathbb{R}^n} is the standard inner product on \mathbb{R}^n. Conversely, any Riemannian metric yields a unique \mathrm{O}(n)-reduction. This equivalence holds globally on M, as the metric provides compatible local orthonormal trivializations that glue smoothly. If M is orientable, the reduction can be further specialized to the special orthogonal group \mathrm{SO}(n) by selecting oriented orthonormal frames, corresponding to oriented Riemannian metrics. The fibers of P^O(M) are diffeomorphic to \mathrm{O}(n), a compact , in contrast to the non-compact fibers of P(M) diffeomorphic to \mathrm{GL}(n,\mathbb{R}); this thus selects a "smaller" of frames, though both have infinite cardinality as manifolds. Such reductions are facilitated by an Ehresmann connection on P(M), which allows horizontal lifts to define the subbundle structure.

Relation to Riemannian metrics

The orthonormal frame bundle P^{O}(M) of a (M, g) is intrinsically tied to the metric structure, as the choice of g determines the reduction of the full frame bundle to the O(n), and conversely, the bundle defines the metric up to the choice of local trivializations. Specifically, given a local section s: U \to P^{O}(M) over an U \subset M, the Riemannian metric at a point p \in U is recovered by expressing tangent vectors in terms of the orthonormal frame provided by s(p). For X, Y \in T_p M, the metric is g_p(X, Y) = \langle s(p)^{-1}(X), s(p)^{-1}(Y) \rangle, where \langle \cdot, \cdot \rangle is the standard inner product on \mathbb{R}^n and s(p): \mathbb{R}^n \to T_p M is the linear given by the frame. This construction ensures that the frames in the bundle are orthonormal with respect to g, establishing a between Riemannian metrics on M and O(n)-reductions of the frame bundle. The orthonormal frame bundle itself inherits a natural Riemannian from g on M and the bi-invariant on O(n), often realized as the Sasaki-type on principal bundles. This bundle is defined such that for tangent vectors at a frame u \in P^{O}(M), it decomposes into and vertical components: the part pulls back the g via the \pi: P^{O}(M) \to M, while the vertical part uses the Killing form or standard on the fibers isomorphic to O(n). The O(n)-invariance of this ensures compatibility with the right action, making P^{O}(M) a Riemannian submersion over M. Consequently, the Levi-Civita of g on M induces a principal on P^{O}(M), whose distribution coincides with the subbundle defined by the orthogonality, thus embedding the geometry of M into that of the frame bundle. In Élie Cartan's moving frame approach, the geometry of the is captured through differential forms on the orthonormal frame bundle. The corresponds to an \mathfrak{so}(n)-valued 1-form \omega on P^{O}(M), which is equivariant under the O(n)-action and reproduces the in local coordinates. The of this is encoded in the curvature 2-form \Omega = d\omega + \omega \wedge \omega, also \mathfrak{so}(n)-valued, satisfying Cartan's second structure equation \Omega = d\theta + \omega \wedge \theta alongside the torsion-free solder form \theta. This formalism reveals the sectional curvatures of g as the components of \Omega evaluated on adapted frames, providing a coordinate-free description of Riemannian directly on the bundle. A key application of the orthonormal frame bundle lies in parallel transport, which is geometrized as horizontal lifts in the principal bundle setting. For a curve \gamma: [0,1] \to M, parallel transport of a tangent vector from \gamma(0) to \gamma(1) with respect to the Levi-Civita connection is equivalent to lifting \gamma horizontally to a curve in P^{O}(M) starting from a frame containing the initial vector, followed by the O(n)-action to adjust the frame. These O(n)-lifts preserve orthonormality and encode the holonomy of the connection, with closed curves generating the structure group elements that measure infinitesimal rotations induced by curvature.

G-Structures

General theory of structure group reductions

A G-structure on an n-dimensional manifold M is defined as a principal G-subbundle P^G(M) of the linear frame bundle P(M), where G \subset \mathrm{GL}(n, \mathbb{R}) is a Lie subgroup, equivalently representing a reduction of the structure group of P(M) from \mathrm{GL}(n, \mathbb{R}) to G. This reduction endows the tangent bundle TM with additional geometric structure compatible with the action of G, generalizing the principal bundle formulation to closed subgroups. The construction of a G-structure proceeds either by selecting a smooth section of the quotient bundle P(M)/G \to M, which identifies fibers over each point with G-orbits in the space of frames, or equivalently via a G-valued atlas on M consisting of local G-frames whose transition functions take values in G. Local sections s: U \to P(M) over open sets U \subset M are required to be G-equivariant, ensuring that the resulting subbundle P^G(M) is smooth and principal with structure group G. This approach aligns with the general of principal bundles, where the reduction is locally trivialized by such atlases. For an involutive G-structure, Frobenius integrability characterizes the existence of an defined by the G-invariant subbundle: the associated horizontal distribution H \subset TP^G(M) is if and only if it is involutive, meaning [H, H] \subset H. This condition ensures the local existence of integral submanifolds foliating a neighborhood of each point, corresponding to a system generated by G-invariant forms that is completely . In the context of G-structures, involutivity often relates to the vanishing of the torsion of a compatible , allowing the structure to be locally modeled on the flat G-space. Global obstructions to the existence or further reduction of a G-structure are detected by elements in groups or characteristic classes associated to the bundle. Specifically, the H^*(\mathfrak{g}, V) of the \mathfrak{g} of G with coefficients in a V encodes deformations and integrability obstructions, while characteristic classes in the H^*(M; \mathbb{R}), such as those induced by polynomials on \mathfrak{g}, provide topological barriers to reducibility; for instance, the serves as an obstruction for certain orientation-preserving reductions. These , independent of choices of connection, arise from the and forms on P^G(M).

Examples and classifications

Prominent examples of G-structures arise in the study of almost complex, , and conformal geometries on manifolds. An almost complex structure on a manifold of even $2m corresponds to a reduction of the frame bundle's structure group to G = \mathrm{GL}(m, \mathbb{C}) \subset \mathrm{GL}(2m, \mathbb{R}). This reduction is equivalent to the existence of a J, an of the satisfying J^2 = -\mathrm{Id}, which endows the manifold with a complex structure locally. A symplectic structure on a $2m-dimensional manifold is given by a reduction to G = \mathrm{Sp}(2m, \mathbb{R}) \subset \mathrm{GL}(2m, \mathbb{R}), the group preserving a constant non-degenerate skew-symmetric . Geometrically, this manifests as a closed, non-degenerate 2-form \omega on the , enabling the formulation of and phase spaces. Unlike the almost case, symplectic structures are typically integrable by definition through the closedness of \omega. Conformal structures reduce the structure group to G = \mathrm{CO}(n) = \mathbb{R}^+ \times \mathrm{O}(n) \subset \mathrm{GL}(n, \mathbb{R}), preserving angles but not lengths. This corresponds to a conformal class of pseudo-Riemannian metrics, where metrics differ by positive scalar functions, and is central to Weyl geometry and scale-invariant theories. In general, each such G-structure is associated with a canonical tensor field on the manifold—for instance, the almost complex tensor J, the symplectic form \omega, or the conformal metric class—whose properties encode the geometric constraints imposed by the group reduction. Integrability conditions, such as the vanishing of the Nijenhuis tensor N_J = 0 for almost complex structures, ensure that the G-structure arises from a more rigid geometric object; for example, integrability of an almost complex structure yields a complex manifold, as established by the Newlander-Nirenberg theorem. Classifications of G-structures often rely on prolongation techniques, as developed in the equivalence methods of Cartan and Weyl. Weyl's classification identifies G-structures of finite type based on the order of their prolongations, where the prolongation process iteratively extends the structure to higher-order jet bundles until invariants determine local ; notably, conformal and projective structures are second-order, admitting unique prolongations to affine structures. groups provide another classification framework, acting as the maximal subgroups to which the structure group can be reduced while preserving a compatible , thereby capturing the intrinsic symmetries and properties of the manifold. The formalization of G-structures traces to Élie Cartan's development of the moving frames method in the and , which unified local solvability of overdetermined partial differential equations with group actions on manifolds, laying the groundwork for modern infinitesimal geometry.

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