Let M be a simple Riemannian manifold with boundary ∂M. For (x,v)∈SM, let τ(x,v) denote the exit time of the geodesic starting at x with tangent vector v, i.e. τ(x,v) is the (necessarily unique, and finite) time at which expx(tv)∈∂M.
We let ∂+(SM) denote the set
∂+(SM)={(x,v)∈SM | x∈∂M,⟨v,ν⟩>0}
where ν denotes the inward unit normal to ∂M in M. The exponential map identifies SM with the set
Ω={(x,v,t)∈∂+(SM)×R | 0≤t≤τ(x,v)},
via (x,v,t)↦expx(tv). Let Φ:Ω→M denote this diffeomorphism. Then we have, for all f∈C∞(SM)
∫SMfdvol(SM)=∫Ω(Φ∗f)(Φ∗dvol(SM))=∫∂+(SM)∫τ(x,v)0f(ϕt(x,v))Φ∗dvol(SM).
Therefore, we can compute integrals of functions over SM by integrating along geodesics, provided that we can cmopute Φ∗dvol(SM). This is the content of the Santalo formula.
Theorem (Santalo formula). For all f∈C∞(SM), we have
∫SMfdvol(SM)=∫∂+(SM)∫τ(x,v)0f(ϕt(x,v))⟨v,ν⟩dtdvol(∂(SM))
Proof. Necessarily, we must have
Φ∗(dvol(SM))=a(x,v)dt∧dvol(∂(SM))),
for some function a(x,v). The reason we can assume that a is independent of t is that Φ is defined via geodesic flow, and geodesic flow preserves the volume form on SM. To compute the factor a(x,v), we just need to compute
i∂/∂tΦ∗(dvol(SM))=Φ∗(iΦ∗(∂/∂t)dvol(SM))
From the definition of Φ, we have that Φ∗(∂/∂t) is the Reeb vector field on SM, i.e. the vector field generating geodesic flow. Therefore, Φ∗(∂/∂t) is equal, at a point (x,v) to the horizontal lift of the vector v. Therefore, using the definition of the induced volume form on a hypersurface of a Riemannian manifold, we find
i∂/∂tΦ∗(dvol(SM))=⟨v,ν⟩dvol(∂(SM))
where ν is the inward pointing unit normal to ∂(SM) in SM. This shows that a(x,v)=⟨v,ν⟩ and completes the proof.
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