nLab piecewise flat spacetime

Contents

Context

Riemannian geometry

Riemannian geometry

Contents

Idea

If one allows pseudo-Riemannian manifolds with conical singularities then it makes sense to ask for spacetimes which are flat (isometric to pieces of Minkowski spacetime) away from strata of positive codimension, with all curvature concentrated in conical singularities on these lower-dimensional strata.

Such piecewise flat spacetimes have been considered as discretized models for smooth (non-singular and non-piecewise flat) spacetimes useful for computation (see Williams-Tuckey 92): A combinatorial functional on piecewise flat spacetimes, depending on the edge lengths of a metric simplicial complex, was introduced in Regge 61 (see also Barrett 87) with the idea that in an appropriate limit it approaches the Einstein-Hilbert action functional on non-singular spacetimes. This has become famous as Regge calculus. That this limit indeed works out has been proven (only) in Cheeger-Mueller-Schrader 84, see Cheeger 16 for review.

A variant of this perspective, but with the conical singularities constrained to be timelike as expected for “physical” singularities, has been initiated in ‘t Hooft 08 and worked out in some detail by van de Meent 11.

In both cases a more speculative motivation for considering piecewise flat spacetimes is the hope that it might help with defining quantum gravity, non-perturbatively (Regge-Williams 00). A direct attempt to define and compute a path integral quantization over piecewise flat spacetimes is known as “causal dynamical triangulation” (see Ambjorn-Jurkiewicz-Loll 00).

Piecewise flat spacetimes appear naturally in 3-dimensional gravity, which provides much of the inspiration and motivation of various approaches.

But piecewise flat spacetimes also appear naturally as the “far-horizon geometry” (“small $N$-limit”, see there) of BPS black brane spacetimes in supergravity theories, where considerations such as at M-theory on G2-manifolds suggest that the conical singularities have to be taken seriously as part of the physical model. These cone brane-singularities are necessarily time-like, as in ‘t Hooft 08, van de Meent 11, but in contrast to the assumption in general Regge calculus. Of course they are of higher dimension (and higher co-dimension) than considered in ‘t Hooft 08, van de Meent 11.

References

Regge calculus

• Tullio Regge, General relativity without coordinates, Nuovo Cim (1961) 19: 558 (doi:10.1007/BF02733251)

• Jeff Cheeger, Werner Müller, Robert Schrader, On the curvature of piecewise flat spaces, Comm. Math. Phys. Volume 92, Number 3 (1984), 405-454 (euclid:1103940867)

• John Barrett, The geometry of classical Regge calculus, Classical and Quantum Gravity, Volume 4, Number 6, 1987 (web)

• R. M. Williams, P. A. Tuckey, Regge calculus: a brief review and bibliography, Classical and Quantum Gravity, Volume 9, Number 5, 1992 (web)

• Tullio Regge, Ruth M. Williams, Discrete structures in gravity, J. Math. Phys.41:3964-3984, 2000 (arXiv:gr-qc/0012035)

• Jeff Cheeger, Curvature of piecewise flat spaces, talk at Courant institute 2016 (pdf, pdf)

• Aleksandar Mikovic, Piecewise Flat Metrics and Quantum Gravity (arXiv:2001.11439)

Application to FRW models of cosmology:

• Ren Tsuda, Takanori Fujiwara, Oscillating 4-Polytopal Universe in Regge Calculus (arXiv:2011.04120)

Causal dynamical triangulation

• J. Ambjorn, R. Loll, Non-perturbative Lorentzian Quantum Gravity, Causality and Topology Change, Nucl.Phys. B536 (1998) 407-434 (arXiv:hep-th/9805108)

• J. Ambjorn, J. Jurkiewicz, R. Loll, Dynamically Triangulating Lorentzian Quantum Gravity, Nucl.Phys. B610 (2001) 347-382 (arXiv:hep-th/0105267)

• J. Ambjorn, J. Jurkiewicz, R. Loll, A non-perturbative Lorentzian path integral for gravity, Phys.Rev.Lett. 85 (2000) 924-927 (arXiv:hep-th/0002050)

• R. Loll, Quantum Gravity from Causal Dynamical Triangulations: A Review (arXiv:1905.08669)

Last revised on November 10, 2020 at 01:10:01. See the history of this page for a list of all contributions to it.