A. Ashtekar et M. Varadarajan, STRIKING PROPERTY OF THE GRAVITATIONAL HAMILTONIAN, Physical review. D. Particles and fields, 50(8), 1994, pp. 4944-4956
The Hamiltonian framework for (2+1)-dimensional gravity coupled with m
atter (satisfying positive energy conditions) is considered in the asy
mptotically hat context. It is shown that the total energy of the syst
em is non-negative, vanishing if and only if space-time is (globally)
Minkowskian. Furthermore, contrary to one's experience with usual held
theories, the Hamiltonian is bounded from above. This is a genuinely
nonperturbative result. In the presence of a spacelike Killing field,
(3+1)-dimensional vacuum general relativity is equivalent to (2+1)-dim
ensional general relativity coupled to certain matter fields. Therefor
e, our expression provides, in particular, a formula for energy per-un
it length (along the symmetry direction) of gravitational waves with a
spacelike symmetry in 3+1 dimensions. A special case is that of cylin
drical waves which have two hypersurface orthogonal, spacelike Killing
fields. In this case, our expression is related to the ''c energy'' i
n a nonpolynomial fashion. While in the weak field limit the two agree
, in the strong field regime they differ significantly. By constructio
n, our expression yields the generator of the time translation in the
full theory, and therefore represents the physical energy in the gravi
tational field.