Some interesting quotes:
==page 1==
... Here, we are, however, seeking for an answer to a subtler question: Is there a Hamiltonian formalism for discretized gravity in terms of first-order tetrad-connection variables available? This is a difficult question, because there is a conceptual tension: A Hamiltonian always generates a differential equation, it generates a Hamiltonian flow, while, on the other hand, discretized theories are typically governed by difference equations instead [16].
This article develops a proposal resolving the tension. Following the Plebański principle, we start with the topological BF action [17]. We introduce a simplicial decomposition of the four-dimensional spacetime manifold, and discretize the action. This leads us to a sum over the two-dimensional simplicial faces. Every face contributes a one-dimensional integral over its bounding edges, thus turning the topological action into an integral over the entire system of edges—into an action over a one-dimensional branched manifold.
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==page 14==
Equation (50) is our final proposal, a proposal for an action for discretized gravity in first-order variables. At this point, neither do we know of any global solutions of the resulting equations of motion on an arbitrary two-complex, nor do we have a proof that they would correspond to any physical spacetime geometry. Yet, we do have positive evidence in favor of our proposal. First of all, we will see, that the constraint algebra closes, and that there are no secondary constraints. Then, the model has curvature. This curvature lies in the faces dual to the elementary triangles, and is given, just as in Regge calculus, by the sum over the boost-angles between the adjacent tetrahedra. Finally, and most importantly, the solutions of the equations of motion have a geometric interpretation and define a twisted geometry [24–26].
Twisted geometries are discrete geometries found in the semi-classical limit of loop quantum gravity [3, 28–30]. They are similar to Regge geometries insofar as they represent a collection of flat tetrahedra glued along their bounding triangles, but unlike Regge geometries there are no unique length variables: Every triangle has a unique area, and every tetrahedron has a unique volume, but the length of a triangle’s bounding side exists only locally.
III. DYNAMICS OF THE THEORY
In the last section, we gave a proposal for a gravitational action on a simplicial lattice. Now it is time to study the dynamics. The action (50) is local in t, and so are the resulting equations of motion, that tell us how the elementary configuration variables change as we move forward in t and go from one vertex to the next. This t-variable does however not have an immediate physical interpretation. It is no physical time, and does not measure duration as given by a clock.
A. Hamiltonian formulation
Symplectic structure: Let us first fix an arbitrary edge e in the discretization. Restricting our analysis to just a single edge is a matter of convenience. It allows us to use a condensed notation …
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==pages 23 and 24==
IV. CONCLUSION
Summary We have split our presentation into two halves. The first half gave the derivation of the action. ... A simplicial decomposition of the four-dimensional manifold brought us to the discretized action, and we saw that this discretized action can be written as a one-dimensional integral over the simplicial edges—as an action over a one-dimensional branched manifold. ...We then studied the discretized simplicity constraints in the spinorial representation and added them to our one-dimensional action. This introduced an additional element to the theory: The volume-weighted time-normals of the elementary tetrahedra. We argued that a consistent theory is possible only if we also treat these time normals as dynamical variables in the action. At each simplicial vertex these volume-weighted normals sum up to zero—this representing the geometricity of the four-simplex itself. We argued that this closure constraint represents a momentum conservation law for a system of particles scattering in a locally flat auxiliary spacetime, and we made an explicit proposal for an action realizing this idea. Each of these particles corresponds to an elementary tetrahedron in the simplicial complex, with their mass representing the three-volume of the elementary tetrahedra, and each interaction vertex representing a four-simplex in the discretization...
The second half of the paper studied the dynamics of the theory as derived from the action. Let us say it clearly: We have not shown that the equations of motion for the discretized theory would correspond to some version of the Einstein equations on a simplicial lattice. Nevertheless, we do have some definite results: First of all, there is a Hamiltonian formulation for the discretized theory, there is a phase space, constraints and a Hamiltonian. The Hamiltonian generates the t-evolution along the elementary edges of the discretization, and preserves both the first- and second class constraints. There are no secondary constraints. Next, we showed that the solutions of the equations of motion have a geometric interpretation in terms of twisted geometries.
Twisted geometries are piecewise flat geometries generalizing Regge geometries: In Regge calculus the edge lengths are the fundamental configuration variables, in twisted geometries there is no unique notion of length: Every tetrahedron has a unique volume, and every triangle has a unique area, but the length of a segment depends on whether we compute it from the flat metric in one simplex or the other.
Finally we gave an argument why the model has curvature. Going around a triangle we pick up a deficit angle, which is a measure for the curvature in the dual plane. We showed that this deficit angle will generically not vanish, in fact it is given by the integral of the Lagrange multiplier λ …
The relevance of the model The action (50) describes a system of finitely many degrees of freedom propagating and interacting along the simplicial edges. The system has a phase space, local gauge symmetries and a Hamiltonian. What happens if we quantize this model? Do we get yet another proposal for a theory of quantum gravity? Recent results [23, 27, 36, 58] point into a more promising direction and suggest a convergence of ideas: The finite-dimensional phase space can be trivially quantized. The constraints of the theory glue the quantum states over the individual edges so as to form a Hilbert space over the entire boundary of the underlying simplical manifold. The boundary states represent projected spin-network functions [59, 60] in the kinematical Hilbert space of loop quantum gravity. It is clear what should be done next: For any fixed boundary data we should define a path integral over the field configurations along the edges in the bulk. At this point, many details remain open, and we have only finished this construction for the corresponding model in three-dimensions [58], yet we do know, that whatever the mathematical details of the resulting amplitudes will be, they will define a version of spinfoam gravity [61].
Finally, there is the motion of the volume-weighted time normals, which endow the entire simplicial complex with a flow of conserved energy-momentum. As shown by Cortês and Smolin in a related paper [27], these momentum-variables introduce a causal structure, and allow us to view the simplicial complex as an energetic causal set [51, 52]—a generalization of causal sets carrying a local flow of energy-momentum between causally related events.
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I'll quote the abstract and give a link to the Cortês and Smolin paper in the next post.