Einsteinian gravity from a topological action
Eckehard W. Mielke

TL;DR
This paper derives a curvature-squared gravity model from a topological action in 4D, showing how Einstein's equations with a cosmological constant naturally emerge, with implications for dark energy and dark matter.
Contribution
It introduces a novel derivation of Einstein gravity from a topological invariant using BRST formalism and explores modifications leading to Einstein's equations with a cosmological constant.
Findings
Exact vacuum solutions exhibit vacuum degeneracy.
Modifying duality yields Einstein's equations with a cosmological constant.
Potential implications for dark energy and dark matter models.
Abstract
The curvature-squared model of gravity, in the affine form proposed by Weyl and Yang, is deduced from a topological action in 4D. More specifically, we start from the Pontrjagin (or Euler) invariant. Using the BRST antifield formalism with a double duality gauge fixing, we obtain a consistent quantization in spaces of double dual curvature as classical instanton type background. However, exact vacuum solutions with double duality properties exhibit a `vacuum degeneracy'. By modifying the duality via a scale breaking term, we demonstrate that only Einstein's equations with an induced cosmological constant emerge for the topology of the macroscopic background. This may have repercussions on the problem of `dark energy' as well as `dark matter' modeled by a torsion induced quintaxion.
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