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Einstein's gravity from a polynomial affine model

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arxiv 1505.04634 v2 pith:M5SXWGVY submitted 2015-05-18 gr-qc hep-thmath-phmath.MP

classification gr-qchep-thmath-phmath.MP
keywords fieldaffinemodeltheorycoupledeffectiveeinsteinequations
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We show that the effective field equations for a recently formulated polynomial affine model of gravity, in the sector of a torsion-free connection, accept general Einstein manifolds---with or without cosmological constant---as solutions. Moreover, the effective field equations are partially those obtained from a gravitational Yang--Mills theory known as Stephenson--Kilmister--Yang theory. Additionally, we find a generalization of a minimally coupled massless scalar field in General Relativity within a "minimally" coupled scalar field in this affine model. Finally, we present a brief analysis of the propagators of the gravitational theory, and count the degrees of freedom. For completeness we prove that a Birkhoff-like theorem is valid for the analyzed sector.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Emergent metric and geodesic analysis in cosmological solutions of (torsion-free) Polynomial Affine Gravity

    gr-qc 2019-08 conditional novelty 5.0 of 10

    In torsion-free polynomial affine gravity, the Ricci tensor can serve as an emergent metric, and self-parallel curves can reproduce the spatial geodesics of Friedmann-Robertson-Walker cosmology.

  2. A polynomial affine model of gravity: after ten years

    gr-qc 2024-12 conditional novelty 3.0 of 10

    A ten-year review of polynomial affine gravity, covering the most general diffeomorphism-invariant action, its field equations, cosmological solutions, and emergent metrics.

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