Quantum general relativity and the classification of smooth manifolds

Details Quantum general relativity and the classification of smooth manifolds Quantum general relativity and the classification of smooth manifolds

2004-04-21

arxiv.org/abs/gr-qc/0404088v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

41 pages, LaTeX2e with combined eps/PicTeX figures; v2: inaccuracies fixed

Scientific paper

The gauge symmetry of classical general relativity under space-time diffeomorphisms implies that any path integral quantization which can be interpreted as a sum over space-time geometries, gives rise to a formal invariant of smooth manifolds. This is an opportunity to review results on the classification of smooth, piecewise-linear and topological manifolds. It turns out that differential topology distinguishes the space-time dimension d=3+1 from any other lower or higher dimension and relates the sought-after path integral quantization of general relativity in d=3+1 with an open problem in topology, namely to construct non-trivial invariants of smooth manifolds using their piecewise-linear structure. In any dimension d<=5+1, the classification results provide us with triangulations of space-time which are not merely approximations nor introduce any physical cut-off, but which rather capture the full information about smooth manifolds up to diffeomorphism. Conditions on refinements of these triangulations reveal what replaces block-spin renormalization group transformations in theories with dynamical geometry. The classification results finally suggest that it is space-time dimension rather than absence of gravitons that renders pure gravity in d=2+1 a `topological' theory.

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