Modified gravity: a unified approach to metric-affine models
arXiv:2301.11051 · doi:10.1063/5.0150038
Abstract
The starting point of this work is the original Einstein action, sometimes called the Gamma squared action. Continuing from our previous results, we study various modified theories of gravity following the Palatini approach. The metric and the connection will be treated as independent variables leading to generalised theories which may contain torsion or non-metricity or both. Due to our particular approach involving the Einstein action, our setup allows us to formulate a substantial number of new theories not previously studied. Our results can be linked back to well-known models like Einstein-Cartan theory and metric-affine theories and also links to many recently studied modified gravity models. In particular we propose an Einstein-Cartan type modified theory of gravity which contains propagating torsion provided our function depends non-linearly on a boundary term. We also can state precise conditions for the existence of propagating torsion. Our work concludes with a brief discussion of cosmology and the role of cosmological torsion in our model. We find solutions with early-time inflation and late-time matter dominated behaviour. No matter sources are required to drive inflation and it becomes a purely geometrical effect.
Final version published in JMP
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- The Non-Relativistic Geometric Trinity of Gravity
- Spherically symmetric teleparallel geometries
- Spatial curvature in coincident gauge cosmology
- Stability of Gravity via Dynamical System Approach: a Comprehensive Bayesian Statistical Analysis
- Teleparallel Robertson-Walker geometries and applications
- Cosmological solutions in teleparallel gravity
- Observational tests of asymptotically flat spacetimes
- Cosmological fluids with boundary term couplings
- A new 2D formulation of modified General Relativity
- Scalar field source Teleparallel Robertson-Walker F(T)-gravity solutions
- Generating exact polytropes in non-conservative unimodular geometries
- Cosmological dynamical systems of non-minimally coupled fluids and scalar fields
- Diffeomorphism Invariance Breaking in Gravity and Cosmological Evolution
- Geometric formulation of -essence and late-time acceleration
- Dynamical systems approach to stellar modelling in gravity