The Weinstein conjecture predicts that the Reeb vector field of every contact form defining a contact structure on a closed manifold has a periodic orbit; on open (non-compact) contact manifolds this statement fails outright — the standard contact structure on R2n+1\mathbb{R}^{2n+1} carries the Reeb field ∂z\partial_z, which has no periodic orbits. The problem, developing the discussion in Dörner–Geiges–Zehmisch's survey of periodic Reeb orbits — which defines property (W)(W) for contact manifolds, records simple open manifolds where (W)(W) fails together with recent progress establishing it for a number of open contact manifolds, and asks whether local changes in the topology or the contact form on (R2n+1,αst)(\mathbb{R}^{2n+1},\alpha_{st}) force periodic Reeb orbits — is to characterize the open contact manifolds (M,ξ)(M,\xi) for which every defining contact form has a periodic Reeb orbit, and in the model case of contact forms on (R2n+1,ξst)(\mathbb{R}^{2n+1},\xi_{st}) that are standard at infinity, to find dynamical conditions forcing periodic orbits in dimensions 2n+1≥52n+1\ge 5, where Geiges–Röttgen–Zehmisch showed that even the existence of trapped orbits does not suffice. Despite sustained activity (virtually contact structures, cotangent bundles over non-compact bases, and the singular bmb^m-contact line), no general characterization and no higher-dimensional analogue of the Eliashberg–Hofer trapped-orbit theorem is known.

Background

A contact form on a (2n+1)(2n+1)-dimensional manifold MM is a 1-form α\alpha such that α∧(dα)n\alpha\wedge(d\alpha)^n is nowhere vanishing; its Reeb vector field RαR_\alpha is uniquely determined by ιRαdα=0\iota_{R_\alpha}d\alpha=0 and α(Rα)=1\alpha(R_\alpha)=1. The hyperplane field ξ=ker⁡α\xi=\ker\alpha is a (cooriented) contact structure, and α\alpha is unique up to multiplication by a positive function, so properties of the Reeb flow that hold for every defining form are properties of the contact structure (M,ξ)(M,\xi) itself. A periodic Reeb orbit is a trajectory that closes up; it is contractible if it is null-homotopic in MM (the period need not be minimal). Weinstein (1979) conjectured that on a closed manifold the Reeb flow of every defining form has a periodic orbit — property (W)(W); a stronger property (W∘)(W^\circ) demands a contractible periodic orbit. For closed manifolds, (W)(W) is known in many cases, notably for all closed orientable 3-manifolds by Taubes's Seiberg–Witten argument, but remains open in full generality.

On open (non-compact) manifolds the naive conjecture fails: for the standard contact form αst=dz+12∑j(xj dyj−yj dxj)\alpha_{st}=dz+\frac{1}{2}\sum_j(x_j\,dy_j-y_j\,dx_j) on R2n+1\mathbb{R}^{2n+1}, the Reeb field is ∂z\partial_z, which has no periodic orbits. The meaningful question is therefore which open contact manifolds satisfy (W)(W). A contact form is called standard at infinity if it agrees with αst\alpha_{st} outside a compact set, and a Reeb orbit is trapped if it enters a compact region without leaving it again (but never closes up). Eliashberg and Hofer (1994), via filling arguments with holomorphic discs (discs solving a Cauchy–Riemann type equation in the symplectization, the cylinder R×M\mathbb{R}\times M equipped with the symplectic form d(etα)d(e^t\alpha)), proved a global Darboux theorem: a contact form on R3\mathbb{R}^3 that is standard at infinity and has no periodic Reeb orbit is diffeomorphic to the standard pair; consequently, in dimension three a trapped orbit forces a periodic one. This picture collapses in higher dimensions: Geiges–Röttgen–Zehmisch (Invent. Math. 2014) constructed, for every n≥2n\ge 2, a contact form α=h αst\alpha=h\,\alpha_{st} with h>0h>0 and h−1h-1 compactly supported — the contact structure ξst\xi_{st} is unchanged — whose Reeb flow has a trapped orbit (built from an irrational linear flow on a Clifford torus, a product of circles in Cn\mathbb{C}^n) but no periodic orbit at all. Related work sharpens both sides: Reeb dynamics detects the diffeomorphism type of odd-dimensional balls (Geiges–Zehmisch), Reeb traps can be converted into Hamiltonian plugs (Geiges–Röttgen–Zehmisch), and minimal sets of Denjoy type — aperiodic minimal invariant sets borrowed from Denjoy's classical construction in circle dynamics — can trap Reeb orbits (Arai–Inaba–Kano). On the positive side, periodic orbits are forced on special classes of open contact manifolds: starshaped hypersurfaces (bounding a region star-shaped with respect to a point) and non-compact hypersurfaces in R2n\mathbb{R}^{2n}, cotangent bundles over non-compact bases (van den Berg–Pasquotto–Vandervorst and coauthors), via linking of orbits with compact sets (Suhr–Zehmisch), and on non-compact covers of closed manifolds carrying a virtually contact structure — a lift of a contact form to a cover that is bounded with all derivatives (Bae 2014; Bae–Wiegand–Zehmisch 2020). More recently, the singular bmb^m-contact setting (contact forms singular along a hypersurface, studied by Miranda–Oms and Peralta-Salas) was shown to run hand-in-hand with the Weinstein conjecture on non-compact manifolds with convex ends, where again only partial existence results are available and counterexamples to the naive singular conjecture exist.

Problem Statement

Let (M,ξ)(M,\xi) be an open (non-compact) cooriented contact manifold, and say that (M,ξ)(M,\xi) satisfies the Weinstein conjecture, property (W)(W), if the Reeb vector field of every contact form defining ξ\xi has a periodic orbit (the contractible-orbit strengthening (W∘)(W^\circ) may be treated in parallel).

(i) Characterize the open contact manifolds satisfying (W)(W): give necessary and sufficient conditions — in terms of the topology of MM, invariants of the contact structure ξ\xi, or dynamical properties of defining forms — under which periodic Reeb orbits are forced for every defining contact form. Since (W)(W) is by definition a property of the pair (M,ξ)(M,\xi), an admissible characterization is a criterion that decides, for each open contact manifold, whether it satisfies (W)(W), in terms of data other than the periodic-orbit property itself; a condition that merely restates (W)(W) does not qualify — for instance 'there exists a defining form α\alpha of ξ\xi such that every defining form of ξ\xi has a periodic Reeb orbit', which is equivalent to (W)(W) only because the class of defining forms is nonempty. Conditions may be phrased through the topology of MM, through invariants of ξ\xi, or through properties of defining forms, provided they are not reformulations of (W)(W) (or of (W∘)(W^\circ)).

(ii) Model case: on (R2n+1,ker⁡αst)(\mathbb{R}^{2n+1},\ker\alpha_{st}) with n≥2n\ge 2, consider contact forms α=h αst\alpha=h\,\alpha_{st} with h>0h>0 and h−1h-1 compactly supported, i.e. contact forms standard at infinity. Since Geiges–Röttgen–Zehmisch showed that the existence of a trapped orbit does not force a periodic orbit in these dimensions, identify dynamical conditions on the Reeb flow RαR_\alpha — in the spirit of the Eliashberg–Hofer theorem for n=1n=1 — that do force a periodic Reeb orbit. Such a condition must be checkable from the Reeb dynamics without presupposing the existence of a periodic orbit: the tautological condition 'RαR_\alpha has a periodic orbit' is excluded, since it is trivially sufficient and its failure is trivially aperiodic behavior.

Parts (i) and (ii) address one scientific objective: determining exactly when periodic Reeb orbits are forced on open contact manifolds. They are not interchangeable, however. (R2n+1,ξst)(\mathbb{R}^{2n+1},\xi_{st}) itself fails (W)(W), so (ii) is a question about individual contact forms standard at infinity, whereas (i) asks for a property of open contact manifolds that holds for all their defining forms; a result of type (ii) therefore does not by itself characterize the open contact manifolds satisfying (W)(W). Both parts are required: a resolution must supply a characterization for (i) and at least one non-tautological forcing condition for (ii), so a complete answer to (i) alone does not resolve the task.

References

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