ncatlab.org

piecewise flat spacetime (changes) in nLab

  • ️Invalid Date

Showing changes from revision #18 to #19: Added | Removed | Changed

Context

Riemannian geometry

Gravity

gravity, supergravity

Formalism

Definition

Spacetime configurations

Properties

Spacetimes

black hole spacetimesvanishing angular momentumpositive angular momentum
vanishing chargeSchwarzschild spacetimeKerr spacetime
positive chargeReissner-Nordstrom spacetimeKerr-Newman spacetime

Quantum theory

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 1992): A combinatorial functional on piecewise flat spacetimes, depending on the edge lengths of a metric simplicial complex, was introduced by Regge 1961 (see also Barrett 1987) 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 1984, see Cheeger 2016 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 2008 and worked out in some detail by van de Meent 2011.

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 2000). 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 20000).

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 discussed 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 2008, van de Meent 2011, but in contrast to the assumption in general Regge calculus and generally of higher (co)dimension.

References

Regge calculus

See also

Application to FRW models of cosmology:

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

‘t Hooft-van de Meent

Causal dynamical triangulation

  • J. Ambjorn, R. Loll, Jan Ambjørn, Renate Loll: Non-perturbative Lorentzian Quantum Gravity, Causality and Topology Change , Nucl.Phys. Nucl. B536 Phys. (1998) B 407-434 (arXiv:hep-th/9805108536 ) (1998) 407-434 [[arXiv:hep-th/9805108](https://arxiv.org/abs/hep-th/9805108),doi:10.1016/S0550-3213(98)00692-0]

  • J. Ambjorn, J. Jurkiewicz, R. Loll, Jan AmbjørnDynamically Triangulating Lorentzian Quantum Gravity, J. Jurkiewicz, , Nucl.Phys. B610 (2001) 347-382 (Renate LollarXiv:hep-th/0105267: )Dynamically Triangulating Lorentzian Quantum Gravity_, Nucl. Phys. B 610 (2001) 347-382 [[arXiv:hep-th/0105267](https://arxiv.org/abs/hep-th/0105267), doi:10.1016/S0550-3213(01)00297-8]

  • J. Ambjorn, J. Jurkiewicz, R. Loll, Jan AmbjørnA non-perturbative Lorentzian path integral for gravity, J. Jurkiewicz, , Phys.Rev.Lett. 85 (2000) 924-927 (Renate LollarXiv:hep-th/0002050: )A non-perturbative Lorentzian path integral for gravity&, Phys. Rev. Lett. 85 (2000) 924-927 [[arXiv:hep-th/0002050](https://arxiv.org/abs/hep-th/0002050), doi:10.1103/PhysRevLett.85.924]

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

  • Jan Ambjorn, Lattice Quantum Gravity: EDT and CDT [[arXiv:2209.06555](https://arxiv.org/abs/2209.06555)]

Review:

  • Renate Loll: Quantum Gravity from Causal Dynamical Triangulations: A Review, Class. Quantum Grav. 37 013002 [[arXiv:1905.08669](https://arxiv.org/abs/1905.08669), doi:10.1088/1361-6382/ab57c7 ]

  • Jan Ambjørn, Lattice Quantum Gravity: EDT and CDT, in Handbook of Quantum Gravity, Springer (2023) [[arXiv:2209.06555](https://arxiv.org/abs/2209.06555)]

  • Dario Benedetti, Landau Theory of Causal Dynamical Triangulations, in: Handbook of Quantum Gravity, Springer (2023) [[arXiv:2212.11043](https://arxiv.org/abs/2212.11043)]

  • J. Ambjørn, R. Loll, Jan Ambjørn, Renate Loll: Causal Dynamical Triangulations: Gateway to Nonperturbative Quantum Gravity, in Encyclopedia of Mathematical Physics 2nd ed, Elsevier (2024) [[arXiv:2401.09399](https://arxiv.org/abs/2401.09399)]

  • Renate Loll: Renate Loll: Nonperturbative quantum gravity unlocked through computation, in: Quantum Gravity and Computation, Routledge (2025) [[arXiv:2501.17972](https://arxiv.org/abs/2501.17972)]

Relation Possible relation todark energy:

  • Mingwei Dai, Walter Freeman, Jack Laiho, Marc Schiffer, Judah Unmuth-Yockey: Dynamical Dark Energy from Lattice Quantum Gravity [[arXiv:2408.08963](https://arxiv.org/abs/2408.08963)]

Last revised on January 31, 2025 at 07:40:59. See the history of this page for a list of all contributions to it.