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2013-09-03

IMPA conference: Michael Hutchings

Questions:

(1) Can we improve lower bound on number of closed Reeb orbits?
(2) Can we get existence with a priori upper bound on length?
(3) Can we replace Reeb vector fields with something else?

Theorem for (1): Hutchings & Taubes. 2008. M^3 contact, compact, oriented. At least two distinct orbits for non-degenerate. If manifold is not S^3 or lens space, then have at least 3 (again, assume non-degenerate).

Theorem (Cristofaro-Gardiner & Gripp-Ramos 2012)
Every possibly degenerate contact form on a closed oriented M^3 has two embedded Reeb orbits.

Conjecture (Ekeland-Hofer): every star-shaped hypersurface in \mathbb{R}^{2n} has at least n closed Reeb orbits.

If contact form non-degenerate, conjecture follows by an argument from CH algebra. (Jean Gutt explained this to me earlier. [INSERT EXPLANATION HERE])

Colin-Honda 2008: for many contact structures \xi on closed oriented Y^3, every contact form \ker \alpha = \xi has infinitely many distinct orbits. (Uses linearized CH.)

Conjecture: Y^3 closed oriented connected different from S^3 or a lens space, then every contact form on Y has infinitely many embedded Reeb orbits.

Definition: volume of (Y, \alpha) is \int \alpha \wedge d\alpha.

Question: Does there exist c(Y, \xi) so A(\gamma)^2 \le c(Y, \xi) vol(Y, \alpha) for some closed \gamma?

Stronger version: c(Y, \xi) \le 1.

\newcommand{\vol}{\mathrm{vol}}


Examples: Take a prequantization bundle with Euler class e and \omega = 2\pi e. Take some positive function f \colon \Sigma \to \mathbb{R}. Then look at f \alpha_0.

Conjecture holds for this example, since vol( Y, f \alpha_0) = 2 \pi \int_{\Sigma} f^2 \omega \ge 4 \pi^2 e \min(f^2). Action of critical fibres are 2\pi f(x) (where x is a critical point of f.)

Another example: relationship to systolic inequalities.
Take g a Riemannian metric on S^2 with area 4 \pi. Then, action of a Reeb orbit agrees with the length of the corresponding geodesic.

Go to double cover S^3 and take pull-back contact form. This gives volume 16 \pi^2. Reeb orbits are even geoedeics (geods which determine plane curves with odd rotation number). The conjecture then says there is an even geodesic of length \le 4 \pi.

This is sharp for the round metric (double cover of a great circle on S^2).

Calabi-Croke example: two flat equilateral triangles glued together to give metric of area 4 \pi and no closed geodesics of length \le 2 \pi. However! exists an even geodesic of length \le 4 \pi.

Sketch of proof : suppose Y has only two Reeb orbits. Then, some trickery and work shows that you can construct a foliation from u map. (Foliation by cylinders) This gives a genus 1 Heegaard splitting.

Some consequences of isomorphism to SW Floer homology:
non-canonical \mathbb{Z} grading when c_1(\xi) + 2 PD(\Gamma) is torsion.

For sufficiently negative grading, ECH vanishes. For sufficiently large grading, U : ECH_* \to ECH_{*-2} is isomorphism. Infinitely many * so ECH_* non-zero.

Filtered ECH: look at subcomplex filtered by action. This depends heavily on the contact form.

Michael with Daniel & Vinicius (2012) : consider sequence of classes so that U \sigma_{k+1} = \sigma_k. Then they show \lim_k c_{\sigma_k}(Y, \alpha)^2/ k = 2 \vol(Y, \alpha).

Another theorem with the usual suspects: Suppose (Y, \alpha) closed connected 3-man. Then, either exists a short Reeb orbit OR at least 3 embedded Reeb orbits.

Idea uses some trickery with the U map. I guess the key idea is that having 2 orbits means that the picture looks an awful lot like the ellipsoid.





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