Dynamics

Geodesic Currents and Intersection Numbers

In this post I discuss geodesic currents and intersection numbers

Geodesic Currents

Throughout, let M be a closed orientable hyperbolic surface and let ˜M be its universal cover with the appropriately lifted metric. Two geodesic γ0,γ1:[0,)˜M are said to be asymptotic if there exists a TR so that

lim

We write \gamma_0 \sim \gamma_1 if this holds. We observe this forms an equivalence relation on the space of directed geodesics, and hence we can form the boundary at infinity \partial^\infty \tilde{M} to be the set of all equivalence classes of directed geodesics under this equivalence relation. We can also do this in backward time, and this forms the same boundary at infinity.

Notes that two distinct points (x,y) \in \partial^\infty \tilde{M} \times \partial^\infty \tilde{M} determine a unique geodesic (up to reparameterization). Since we’re focused on unit speed geodesics, it makes sense to define the space of oriented geodesics by

G(M) := \partial^\infty \tilde{M} \times \partial^\infty \tilde{M} \setminus \Delta.

Notice that this is a manifold with charts. Given a unit-speed geodesic \gamma on \tilde{M} with endpoints x,y \in \partial^\infty \tilde{M} we can let I(G) be the set of all unit-speed geodesics which intersect \gamma transversely. Then these geodesics are uniquely determined by two points of data – where they intersect \gamma and at what angle they intersect \gamma. This gives us charts \mathbb{R} \times (0,\pi) on G(M) (in the sense of a smooth manifold). On each chart we can define a measure

d\lambda := \frac{1}{2} \sin(\theta) d\theta dt,

and we can pull back this measure through each chart. We can check that these measures agree on overlaps of charts, and thus we can define a global measure \lambda_g on G(M).

We also observe that we can define the unoriented geodesics by

OG(M) := G(M)/\{ \pm\}.

It is not too hard to see that \lambda_g defined is independent of the orientation of the geodesic, so descends to a measure \lambda_g on OG(M) (which is invariant under the action of \pi_1(M)). We call said measure the Liouville current.

We can define a geodesic current of M to be a locally finite Borel measure on OG(M) invariant under the action of \pi_1(M). The space of geodesic currents is given by C(M), and this is endowed with the weak* topology. That is, \mu_n \rightarrow \mu if for every function \phi we have

\int \phi d\mu_n \rightarrow \int \phi d\mu.

Thus our first example of a geodesic current is the Liouville current. We now want to give a bunch of examples of geodesic currents arising from geodesics.

Let [\gamma] be a free homotopy class on M. Suppose it is a prime class, meaning there is not another class [\delta] so that [\delta]^k = [\gamma] for some integer k. Since everything is hyperbolic, there is a unique closed geodesic \gamma in this free homotopy class. We can lift this geodesic to a family of geodesics in \tilde{M} and define a measure j([\gamma]) which is simply the Dirac measure of this lift.

Claim: j([\gamma]) is a geodesic current.

Proof: Let’s first check that it is invariant under the action of \pi_1(M). Given a deck transformation p : \tilde{M} \rightarrow \tilde{M} and a Borel set U \subseteq \tilde{M} we have that p_*(j([\gamma]))(U) = j([\gamma])(p^{-1}(U)). Since deck transformations preserve the set of all lifts, we get that the number of lifts of the closed geodesic must be the same, so p_*(j([\gamma])) = j([\gamma]) and hence this measure is invariant under the \pi_1(M) action. It is a Borel measure by nature, and it is locally finite since the set is discrete. \blacksquare

Now we extend j by homogeneity to all classes – that is, j([\gamma]^p) = p j([\gamma]). If we label the collection of all free homotopy classes \mathcal{C}(M) this gives us a map j : \mathcal{C}(M) \rightarrow C(M). Since closed geodesics are dense, we get that the span of the image of j is dense inside of C(M). Thus (up to approximation) we have identified essentially all geodesic currents.

Since the Liouville current \lambda_g is so dependent on the metric, one might ask to what extend does it determine the metric? That is, does the Liouville current somehow uniquely determine what the metric is (up to isometry)? Recall that the marked length spectrum is a map \ell_g : \mathcal{C}(M) \rightarrow \mathbb{R}_{> 0} which takes free homotopy classes to the lengths of the unique geodesic inside of the free homotopy class. We have that Otal-Croke’s theorem says that the marked length spectrum determines the metric up to isometry – in other words, if g_1, g_2 are two metrics on M so that \ell_{g_1} = \ell_{g_2} then g_1 \simeq g_2. It turns out we can extend this to the Liouville current as well with the following observation.

Observation: If \lambda_{g_1} = \lambda_{g_2} then \ell_{g_1} = \ell_{g_2}.

To prove this, we’ll need to discuss the intersection form.

Intersection Form

Define the following bundles:

  • With regards to a metric, we have the unit tangent bundle is given by
T_1 \tilde{M} := \{(x,v) \in T \tilde{M} \ | \ \|v\|_x^2 = 1\}.
  • We have the projective unit tangent bundle is given by
PT_1 \tilde{M} := T_1\tilde{M}/\alpha \text{ where } \alpha : T_1 \tilde{M} \rightarrow T_1 \tilde{M}, \ \alpha(x,v) = (x,-v).

This is equipped with the usual projection map \pi : PT_1 \tilde{M} \rightarrow \tilde{M} with \pi(x, \pm v) = x.

  • We have the geodesic intersection bundle is given by
I_1 \tilde{M} := \{(\pm v, \pm w) \in PT_1 \tilde{M} \times PT_1 \tilde{M} \ | \ \pi(\pm v) = \pi(\pm w), v \neq \pm w\}.

The intersection form is a continuous symmetric bilinear map i : C(M) \times C(M) \rightarrow \mathbb{R} defined by

i(\alpha, \beta) := (\alpha \times \beta)(I_1 \tilde{M}).

We make the following observation which justifies the name.

Observation: Suppose \alpha, \beta are closed geodesics on M, then i(j([\alpha]), j([\beta])) is the number of transverse intersections of \alpha and \beta.

Idea: To help with notation, just identify \alpha with j([\alpha]) and similarly with \beta. Observe that

i(\alpha, \beta) = \int_{I_1 \tilde{M}} d\alpha \times d\beta = \int_{x \in \tilde{M}}\int_{(\pm v, \pm w) \in (I_1)_x \tilde{M}} d\alpha(x, \pm v) d\beta(x, \pm w)..

Consequently d\alpha(x, \pm v) = 1 iff (x, v) or (x,-v) lies on the geodesic \alpha. Thus d\alpha(x, \pm v) d\beta (x, \pm w) = 1 iff \alpha and \beta intersect transversely at x. We sum over all such points and this gives us the desired result. \blacksquare

There’s also an interesting connection to the Liouville current.

Claim: Using similar identifications to above, we have that i(\alpha, \lambda_g) = \ell_g([\alpha]).

Proof: Notice that

i(\alpha, \lambda_g) = \int_{x \in \tilde{M}}\int_{(\pm v, \pm w) \in (I_1)_x \tilde{M}} d\alpha(x, \pm v) d\lambda_g(x, \pm w).

Notice that this is going to be the measure of all unoriented geodesics which intersect the geodesic \alpha transversely. Hence in this local chart around \alpha (choosing some orientation for it) we see that this integral is the same as

i(\alpha, \lambda_g) = \int_0^{\ell_g(\alpha)} \int_0^\pi \frac{1}{2} \sin(\theta) d\theta dx = \ell_g(\alpha).

The result follows. \blacksquare

Consequently, \lambda_g determines the marked length spectrum, in the sense that for every free homotopy class the functional \lambda_g^* := i(\cdot, \lambda_g) on the space of free homotopy classes gives us the marked length spectrum. So if two Liouville currents are the same, i.e. \lambda_{g_1} = \lambda_{g_2}, then the corresponding marked length spectrums must be the same (up to isometry). This gives us the following way of restating Otal-Croke’s theorem (matching the observation above).

Theorem: Given two negatively curved metrics g_1, g_2 on M, if \lambda_{g_1} = \lambda_{g_2} then g_1 \simeq g_2.

Another way to think of this is that there is a function taking (negatively curved) metrics and giving Liouville currents. Otal-Croke’s theorem says that for surfaces this function on the space quotiented out by the equivalence relation given by isometries is injective.

We also wish to study i(\lambda_g, \lambda_g). There’s an interesting property here as well.

Observation: We have that i(\lambda_g, \lambda_g) = \frac{\pi}{2} A(g), where A(g) is the area.

We omit the proof here and refer the reader to this article instead (the calculation isn’t hard, it’s just tedious to write out).

References

In no particular order.

(i) Lengths and volumes in Riemannian manifolds by Croke and Dairbekov.

(ii) Length Spectral Rigidity of Non-Positively Curved Surfaces by Frazier.

(iii) Teichmuller Theory Notes by Curtis McMullen.

(iv) What’s a Geodesic Current by Noelle Sawyer.

(v) Partial Marked Length Spectrum Rigidity of Negatively Curved Surfaces by Noelle Sawyer.

Written on January 30, 2022