2002
DOI: 10.1103/physrevd.66.084016
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Hexagon model for 3D Lorentzian quantum cosmology

Abstract: We formulate a dynamically triangulated model of three-dimensional Lorentzian quantum gravity whose spatial sections are flat two tori. It is shown that the combinatorics involved in evaluating the one-step propagator ͑the transfer matrix͒ is that of a set of vicious walkers on a two-dimensional lattice with periodic boundary conditions and that the entropy of the model scales exponentially with the volume. We also give explicit expressions for the Teichmüller parameters of the spatial slices in terms of the d… Show more

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Cited by 19 publications
(20 citation statements)
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“…The more “local” behavior — the Hausdorff dimension of a constant time slice, for example — is not yet well-understood. Neither is the role of moduli for spatial topologies more complicated than S 2 , although initial steps have been taken for the torus universe [115]. …”
Section: Quantum Gravity In 2 + 1 Dimensionsmentioning
confidence: 99%
“…The more “local” behavior — the Hausdorff dimension of a constant time slice, for example — is not yet well-understood. Neither is the role of moduli for spatial topologies more complicated than S 2 , although initial steps have been taken for the torus universe [115]. …”
Section: Quantum Gravity In 2 + 1 Dimensionsmentioning
confidence: 99%
“…In some cases, the resulting models might then be reformulated as "tiling" models on a fixed lattice [30][31][32].…”
Section: Endnotesmentioning
confidence: 99%
“…Once one decides to sum over lattice structure, one must provide a prescription to do so. The class of triangulations to be summed over can be restricted, for instance, in order to implement causality [16,17,29] or to symmetry-reduce models [30][31][32]. 1 Another possibility is to ask for models which are per se lattice or discretization independent.…”
Section: Introductionmentioning
confidence: 99%
“…According to equation (16), the extrinsic curvature is given by the projection onto t of the covariant derivative of the normal vector field, which in our Minkowski coordinates reduces to the usual coordinate derivative. In order to deal with the discontinuity of the normal vector field of t at the kink, we regularize it with the help of a family of smooth functions δ ε which e 0 e 1 s (1) s (2) ρ 1 ρ 2 converge to the delta function as ε → 0.…”
Section: The Case Of Piecewise Linear Manifoldsmentioning
confidence: 99%