On the global evolution problem in 2+1 gravity
Lars Andersson, Vincent Moncrief, Anthony J. Tromba

TL;DR
This paper proves the existence of global constant mean curvature foliations in certain 2+1 dimensional Lorentzian manifolds, linking geometric analysis with solutions to Einstein's equations.
Contribution
It establishes the existence of global CMC foliations in 2+1 gravity models with high genus surfaces, using Hamiltonian reduction and Teichmüller space techniques.
Findings
Existence of global CMC foliations in 2+1 gravity models.
Reduction of Einstein equations to a Hamiltonian system on Teichmüller space.
Key estimates of Dirichlet energy are used in the proof.
Abstract
Existence of global CMC foliations of constant curvature 3-dimensional maximal globally hyperbolic Lorentzian manifolds, containing a constant mean curvature hypersurface with is proved. Constant curvature 3-dimensional Lorentzian manifolds can be viewed as solutions to the 2+1 vacuum Einstein equations with a cosmological constant. The proof is based on the reduction of the corresponding Hamiltonian system in constant mean curvature gauge to a time dependent Hamiltonian system on the cotangent bundle of Teichm\"uller space. Estimates of the Dirichlet energy of the induced metric play an essential role in the proof.
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