Gauss-Bonnet dark energy
arXiv:hep-th/0504052 · doi:10.1103/PhysRevD.71.123509
Abstract
We propose the Gauss-Bonnet dark energy model inspired by string/M-theory where standard gravity with scalar contains additional scalar-dependent coupling with Gauss-Bonnet invariant. It is demonstrated that effective phantom (or quintessence) phase of late universe may occur in the presence of such term when the scalar is phantom or for non-zero potential (for canonical scalar). However, with the increase of the curvature the GB term may become dominant so that phantom phase is transient and barrier may be passed. Hence, the current acceleration of the universe may be caused by mixture of scalar phantom and (or) potential/stringy effects. It is remarkable that scalar-Gauss-Bonnet coupling acts against the Big Rip occurence in phantom cosmology.
LaTeX file, 9 pages, some revision/errors corrected
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- Singularities in and Stability of Ooguri-Vafa-Verlinde Cosmologies
- Constraints on a scalar-tensor model with Gauss-Bonnet coupling from SN Ia and BAO observations
- Generic autonomous system approach to interacting dark energy models
- Entropic uncertainty and coherence in Einstein-Gauss-Bonnet gravity
- Acceleration of the universe in matter dominant era by conformal symmetry breaking
- Curvaton reheating and intermediate inflation in brane cosmology
- Perusing Buchbinder--Lyakhovich canonical formalism for Higher-Order Theories of Gravity
- Examples of exact exponential cosmological solutions with three isotropic subspaces in the Einstein-Gauss-Bonnet gravity
- Beyond : Gauss--Bonnet inflation with
- Correspondence between particle creation and dark components interaction in the context of gravity
- On the number of terms in the Lovelock products
- -cosmological dynamics in the FLRW background
- Some Classes of Gravitational Shock Waves from Higher Order Theories of Gravity
- Intermediate evolution using SNIa, and BAO
- Applications of Cosmological Perturbation Theory in the Late Universe
- Bayesian and Machine-Learning Analyses of Nonminimal Gravity and Tension