Effective Field Theory of Dark Energy: a Dynamical Analysis
arXiv:1310.6026 · doi:10.1088/1475-7516/2014/02/026
Abstract
The effective field theory (EFT) of dark energy relies on three functions of time to describe the background dynamics. The viability of these functions is investigated here by means of a thorough dynamical analysis. While the system is underdetermined, and one can always find a set of functions reproducing any expansion history, we are able to determine general compatibility conditions for these functions by requiring a viable background cosmology. In particular, we identify a set of variables that allows us to transform the non-autonomous system of equations into an infinite-dimensional one characterized by a significant recursive structure. We then analyze several autonomous sub-systems, obtained truncating the original one at increasingly higher dimension, that correspond to increasingly general models of dark energy and modified gravity. Furthermore, we exploit the recursive nature of the system to draw some general conclusions on the different cosmologies that can be recovered within the EFT formalism and the corresponding compatibility requirements for the EFT functions. The machinery that we set up serves different purposes. It offers a general scheme for performing dynamical analysis of dark energy and modified gravity models within the model independent framework of EFT; the general results, obtained with this technique, can be projected into specific models, as we show in one example. It also can be used to determine appropriate ansatze for the three EFT background functions when studying the dynamics of cosmological perturbations in the context of large scale structure tests of gravity.
matching version accepted by JCAP; references added
References in corpus (21)
- Dynamics of dark energy
- The Effective Field Theory of Inflation
- Conditions for the cosmological viability of f(R) dark energy models
- The Effective Field Theory of Cosmological Large Scale Structures
- Effective Field Theory for Inflation
- A Parameterized Post-Friedmann Framework for Modified Gravity
- Essential Building Blocks of Dark Energy
- A discriminating probe of gravity at cosmological scales
- Approaches to Understanding Cosmic Acceleration
- Large Scale Structure as a Probe of Gravitational Slip
- Distinguishing Modified Gravity from Dark Energy
- The Effective Theory of Quintessence: the w<-1 Side Unveiled
- Current constraints on the cosmic growth history
- The Parameterized Post-Friedmann Framework for Theories of Modified Gravity: Concepts, Formalism and Examples
- How to optimally parametrize deviations from General Relativity in the evolution of cosmological perturbations
- Observables and unobservables in dark energy cosmologies
- Effective Field Theory of Cosmological Perturbations
- A practical approach to cosmological perturbations in modified gravity
- Dynamical analysis of generalized Galileon cosmology
- Consistent perturbations in an imperfect fluid
- Cosmological Implications of the Effective Field Theory of Cosmic Acceleration
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- Do current cosmological observations rule out all Covariant Galileons?
- A comparison of Einstein-Boltzmann solvers for testing General Relativity
- Phenomenology of dark energy: general features of large-scale perturbations
- Effective field theory approach to modified gravity including Horndeski theory and Hořava-Lifshitz gravity
- The effective field theory of inflation/dark energy and the Horndeski theory
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- Cosmology in generalized Horndeski theories with second-order equations of motion
- An Extended action for the effective field theory of dark energy: a stability analysis and a complete guide to the mapping at the basis of EFTCAMB
- Testing Hu-Sawicki f(R) gravity with the Effective Field Theory approach
- EFTCAMB/EFTCosmoMC: massive neutrinos in dark cosmologies
- Constraints on modified gravity from Planck 2015: when the health of your theory makes the difference
- A note on the dynamical features for the extended cubic gravity
- Possibility of realizing weak gravity in redshift space distortion measurements
- Observational signatures of the theories beyond Horndeski
- On the stability conditions for theories of modified gravity in presence of matter fields
- Spatially covariant theories of gravity: disformal transformation, cosmological perturbations and the Einstein frame
- Effective field theory of modified gravity on the spherically symmetric background: leading order dynamics and the odd-type perturbations
- Diagnostic of Horndeski Theories
- Computing model independent perturbations in dark energy and modified gravity
- Cosmological disformal transformations to the Einstein frame and gravitational couplings with matter perturbations
- New scaling solutions in cubic Horndeski theories
- Inflationary gravitational waves in the effective field theory of modified gravity
- The effective field theory of K-mouflage
- Cosmological study of a symmetric teleparallel gravity model
- Constraining dark sector perturbations II: ISW and CMB lensing tomography
- Tackling non-linearities with the effective field theory of dark energy and modified gravity
- Separatrices in the Hamilton-Jacobi Formalism of Inflaton Models
- Flows into inflation: An effective field theory approach
- Constructing Viable Interacting Dark Matter and Dark Energy Models: A Dynamical Systems Approach
- A de Sitter limit analysis for dark energy and modified gravity models
- Flows into de Sitter space from anisotropic initial conditions: An effective field theory approach
- Dynamical analysis of Brans-Dicke Universe with inverse power-law effective potential
- Non-parametric exploration of minimally coupled gravity with phantom crossing