On constructing purely affine theories with matter
arXiv:1607.04250 · doi:10.1007/s10714-016-2103-9
Abstract
We explore ways to obtain the very existence of a space-time metric from an action principle that does not refer to it a priori. Although there are reasons to believe that only a non-local theory can viably achieve this goal, we investigate here local theories that start with Schroedinger's purely affine theory [21], where he gave reasons to set the metric proportional to the Ricci curvature aposteriori. When we leave the context of unified field theory, and we couple the non-gravitational matter using some weak equivalence principle, we can show that the propagation of shock waves does not define a lightcone when the purely affine theory is local and avoids the explicit use of the Ricci tensor in realizing the weak equivalence principle. When the Ricci tensor is substituted for the metric, the equations seem to have only a very limited set of solutions. This backs the conviction that viable purely affine theories have to be non-local.
arXiv comment13 pages
References in corpus (6)
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- Metric-affine approach to teleparallel gravity
- Spacetime metric from linear electrodynamics
- Volume elements of spacetime and a quartet of scalar fields
- On the energy-momentum current of the electromagnetic field in a pre-metric axiomatic approach. I
- Rotation in string cosmology
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