The dynamics is coded into the hamiltonian constraint. A well
defined version of this constraint exists (see equation (35)), and thus a consistent theory exists, but a proof that the
classical limit of this theory is classical general relativity is
still lacking. Alternative versions of the hamiltonian constraint
have been proposed and are under investigation. In all these
cases, the hamiltonian has the crucial properties of acting on
nodes only. This implies that its action is naturally discrete
and combinatorial. This fact is possibly at the roots of the
finiteness of the theory. A large class of physical states which
are exact solutions of the dynamics are given by s-knots without
nodes; other exact states are related to knot theory invariants
(Section
7.1).
The theory can be extended to include matter, and there are strong indications that ultraviolet divergences do not appear. A spacetime covariant version of the theory, in the form of a topological sum over surfaces, is under development (Section 6.10).
The main physical results derived so far from the theory are
given by the explicit computation of the eigenvalues of area and
volume, some of which are given in equations (41
-
45
), and a derivation of the black hole entropy formula (Section
41
). The two main (related) open problems are to understand the
description of the low energy regime within the theory and to
choose the correct version of the hamiltonian constraint.
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Loop Quantum Gravity
Carlo Rovelli http://www.livingreviews.org/lrr-1998-1 © Max-Planck-Gesellschaft. ISSN 1433-8351 Problems/Comments to livrev@aei-potsdam.mpg.de |