A spherically symmetric and stationary universe from a weak modification of general relativity
arXiv:0903.3645 · doi:10.1209/0295-5075/86/20004
Abstract
It is shown that a weak modification of general relativity, in the linearized approach, renders a spherically symmetric and stationary model of the universe. This is due to the presence of a third mode of polarization in the linearized gravity in which a "curvature" energy term is present. Such an energy can, in principle, be identified as the Dark Energy. The model can also help to a better understanding of the framework of the Einstein-Vlasov system.
Accepted for publication by Europhysics Letters
References in corpus (12)
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- Modified f(R) gravity unifying R^m inflation with \LambdaCDM epoch
- Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
- F(R) gravity equation of state
- Massive gravitational waves from the R^2 theory of gravity: production and response of interferometers
- Primordial production of massive relic gravitational waves from a weak modification of General Relativity
- A longitudinal component in massive gravitational waves arising from a bimetric theory of gravity
- Curvaton field and intermediate inflationary universe model
- Stochastic background of relic scalar gravitational waves from scalar-tensor gravity
- A solution of linearized Einstein field equations in vacuum used for the detection of the stochastic background of gravitational waves
- An oscillating Universe from the linearized R^{2} theory of gravity
- The importance of the ''magnetic'' components of gravitational waves in the response functions of interferometers