Qualitative evolution in f(R) cosmologies
arXiv:1602.00685 · doi:10.1007/s10714-016-2019-4
Abstract
We investigate the qualitative evolution of (D+1)-dimensional cosmological models in f(R) gravity for the general case of the function f(R). The analysis is specified for various examples, including the (D+1)-dimensional generalization of the Starobinsky model, models with polynomial and exponential functions. The cosmological dynamics are compared in the Einstein and Jordan representations of the corresponding scalar-tensor theory. The features of the cosmological evolution are discussed for Einstein frame potentials taking negative values in certain regions of the field space.
17 pages, 3 figures
References in corpus (14)
- Dynamics of dark energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Disappearing cosmological constant in f(R) gravity
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- Universality Class in Conformal Inflation
- Observational signatures of f(R) dark energy models that satisfy cosmological and local gravity constraints
- The Unity of Cosmological Attractors
- Non-singular exponential gravity: a simple theory for early- and late-time accelerated expansion
- Viability of f(R) Theories with Additional Powers of Curvature
- Integrable Scalar Cosmologies I. Foundations and links with String Theory
- Singular Inflation
- A quantitative analysis of singular inflation with scalar-tensor and modified gravity