Conformally flat spacetimes and Weyl frames
arXiv:1101.5333 · doi:10.1007/s10701-011-9593-9
Abstract
We discuss the concepts of Weyl and Riemann frames in the context of metric theories of gravity and state the fact that they are completely equivalent as far as geodesic motion is concerned. We apply this result to conformally flat spacetimes and show that a new picture arises when a Riemannian spacetime is taken by means of geometrical gauge transformations into a Minkowskian flat spacetime. We find out that in the Weyl frame gravity is described by a scalar field. We give some examples of how conformally flat spacetime configurations look when viewed from the standpoint of a Weyl frame. We show that in the non-relativistic and weak field regime the Weyl scalar field may be identified with the Newtonian gravitational potential. We suggest an equation for the scalar field by varying the Einstein-Hilbert action restricted to the class of conformally-flat spacetimes. We revisit Einstein and Fokker's interpretation of Nordström scalar gravity theory and draw an analogy between this approach and the Weyl gauge formalism. We briefly take a look at two-dimensional gravity as viewed in the Weyl frame and address the question of quantizing a conformally flat spacetime by going to the Weyl frame.
LATEX - 18 pages
References in corpus (5)
Cited by in corpus (12)
- General Relativity and Weyl Geometry
- Gravity localization and mass hierarchy in scalar-tensor branes
- Space-time Philosophy Reconstructed via Massive Nordström Scalar Gravities? Laws vs. Geometry, Conventionality, and Underdetermination
- Present accelerated expansion of the universe from new Weyl-Integrable gravity approach
- Acceleration in Weyl integrable spacetime
- Solitons in curved spacetime
- Gauging the spacetime metric -- looking back and forth a century later
- A modified variational principle for gravity in modified Weyl geometry
- A brief review of a modified relativity that explains cosmological constant
- Stratified scalar field theories of gravitation with self-energy term and effective particle Lagrangian
- Lorentzian correction for the evolution of the CMB temperature
- Weyl geometry, anti-De Sitter space, and -theory