A Striking Property of the Gravitational Hamiltonian
Abhay Ashtekar, Madhavan Varadarajan

TL;DR
This paper establishes a non-perturbative Hamiltonian framework for 2+1 dimensional gravity coupled with matter, demonstrating that total energy is non-negative and providing a formula for energy per unit length in 3+1 dimensions with symmetry, with implications for gravitational wave energy.
Contribution
It introduces a Hamiltonian formulation for 2+1 gravity with matter that shows the total energy is non-negative and bounded from above, and relates 3+1 dimensional gravitational energy to 2+1 dimensional models with symmetry.
Findings
Total energy is non-negative and zero only for Minkowski space.
Hamiltonian is bounded from above, contrary to usual field theories.
Provides a formula for energy per unit length of symmetric gravitational waves.
Abstract
{\sl A Hamiltonian framework for 2+1 dimensional gravity coupled with matter (satisfying positive energy conditions) is considered in the asymptotically flat context. It is shown that the total energy of the system is non-negative, vanishing if and only if space-time is (globally) Minkowskian. Furthermore, contrary to one's experience with usual field theories, the Hamiltonian is} {\rm bounded from above}. This is a genuinely non-perturbative result. {\sl In the presence of a space-like Killing field, 3+1 dimensional vacuum general relativity is equivalent to 2+1 dimensional general relativity coupled to certain matter fields. Therefore, our expression provides, in particular, a formula for energy per-unit length (along the symmetry direction) of gravitational waves with a space-like symmetry in 3+1 dimensions. A special case is that of cylindrical waves which have two hypersurface…
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