Abstract
A topological extension of general relativity is presented. The
superposition principle of quantum mechanics, as formulated by the
Feynman path integral, is taken as a starting point. It is argued that
the trajectories that enter this path integral are distinct and thus
that space-time topology is multiply connected. Specifically, space-time
at the Planck scale consists of a lattice of three-tori that facilitates
many distinct paths for particles to travel along. To add gravity, mini
black holes are attached to this lattice. These mini black holes
represent Wheeler's quantum foam and result from the fact that GR is not
conformally invariant. The number of such mini black holes in any
time-slice through four-space is found to be equal to the number of
macroscopic (so long-lived) black holes in the entire universe. This
connection, by which macroscopic black holes induce mini black holes, is
a topological expression of Mach's principle. The proposed topological
extension of GR can be tested because, if correct, the dark energy
density of the universe should be proportional the total number of
macroscopic black holes in the universe at any time. This prediction,
although strange, agrees with current astrophysical observations.
| Original language | English |
|---|---|
| Article number | 012149 |
| Number of pages | 4 |
| Journal | Journal of Physics Conference Series |
| Volume | 410 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - Feb-2013 |
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