A Theory of Gravitation Covariant under }
arXiv:1706.07470
Abstract
We present a Lagrangian theory of gravitation that develops some ideas proposed several years ago. It is formulated on the 10-dimensional space of the local Lorentz frames (tetrads) and it is covariant under the symplectic group , locally isomorphyic to the anti-de Sitter group . The corresponding transformation formulas contain a constant , besides the light velocity . We also assume the covariance under the "total dilatations" of all the coordinates of the tangent spaces of . These symmetries, that we may call "augmented Lorentz covariance", are spontaneously broken and the corresponding (generalized) Goldstone fields, that we call "augmentons", behave as the components of a 5-vector of . Its square can be interpreted as the Brans-Dicke scalar field, that describes a variable gravitational coupling. The source of the augmentonic fields is provided by the Dirac fields. Finally, we discuss the physical relevance of the theory and its possible further developments.
arXiv comment45 pages
References in corpus (16)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Confrontation between General Relativity and Experiment
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- Generalized Lorentz invariance with an invariant energy scale
- Dictionary on Lie Superalgebras
- Interpretation of Quantum Field Theories with a Minimal Length Scale
- Inflation and reheating in theories with spontaneous scale invariance symmetry breaking
- The roots of scalar-tensor theory: an approximate history
- Negative energy and stability in scalar-tensor gravity
- Curved space-times by crystallization of liquid fiber bundles
- Cosmological Evidence for Modified Gravity (MOG)
- Invariant length scale in relativistic kinematics - Lessons from Dirichlet branes
- Geometries of Maximal Acceleration
- Lorentz Symmetry and Ultra-High-Energy Cosmic Rays
- On the Nature of the Relativity Principle