Non-singular Universes a la Palatini
arXiv:1101.4913 · doi:10.1088/1742-6596/314/1/012054
Abstract
It has recently been shown that f(R) theories formulated in the Palatini variational formalism are able to avoid the big bang singularity yielding instead a bouncing solution. The mechanism responsible for this behavior is similar to that observed in the effective dynamics of loop quantum cosmology and an f(R) theory exactly reproducing that dynamics has been found. I will show here that considering more general actions, with quadratic contributions of the Ricci tensor, results in a much richer phenomenology that yields bouncing solutions even in anisotropic (Bianchi I) scenarios. Some implications of these results are discussed.
4 pages, no figures. Contribution to the Spanish Relativity Meeting (ERE2010), 6-10 Sept. Granada, Spain
References in corpus (20)
- f(R) theories
- Quantum Nature of the Big Bang: Improved dynamics
- Quantum Nature of the Big Bang
- Quantum Nature of the Big Bang: An Analytical and Numerical Investigation
- Loop quantum cosmology of k=1 FRW models
- Are loop quantum cosmos never singular?
- Loop quantum cosmology and the k = - 1 RW model
- Closed FRW model in Loop Quantum Cosmology
- Bouncing Cosmologies in Palatini Gravity
- A no-go theorem for polytropic spheres in Palatini f(R) gravity
- Violation of the Equivalence Principle in Modified Theories of Gravity
- Hydrogen atom in Palatini theories of gravity
- Isotropic and Anisotropic Bouncing Cosmologies in Palatini Gravity
- Dynamical Aspects of Generalized Palatini Theories of Gravity
- Curvature singularities, tidal forces and the viability of Palatini f(R) gravity
- Microscopic and Macroscopic Behaviors of Palatini Modified Gravity Theories
- The dynamics of generalized Palatini Theories of Gravity
- Bouncing Palatini cosmologies and their perturbations
- Indistinguishable Macroscopic Behaviour of Palatini Gravities and General Relativity
- Bouncing Cosmologies