Einstein-Proca theory from the Einstein-Cartan formulation
Will Barker, Sebastian Zell

TL;DR
This paper develops a gravity theory with a massive vector field derived from quadratic curvature, using Einstein-Cartan formulation to avoid ghosts and strong coupling issues, and explores implications for dark matter production.
Contribution
It introduces a novel Einstein-Cartan based gravity model with propagating torsion that naturally yields Einstein-Proca fields without instabilities.
Findings
Ghost and strong-coupling problems are avoided through nonlinear analysis.
The theory constrains Einstein-Proca model parameters.
Potential implications for fermionic dark matter production are discussed.
Abstract
We construct a theory of gravity in which a propagating massive vector field arises from a quadratic curvature invariant. The Einstein-Cartan formulation and a partial suppression of torsion ensure the absence of ghost and strong-coupling problems, as we prove with nonlinear Lagrangian and Hamiltonian analysis. Augmenting General Relativity with a propagating torsion vector, our theory provides a purely gravitational origin of Einstein-Proca models and constrains their parameter space. As an outlook to phenomenology, we discuss the gravitational production of fermionic dark matter.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Pulsars and Gravitational Waves Research
