Some remarks about non-minimally coupled scalar field models
arXiv:1405.2465 · doi:10.1088/0264-9381/31/19/195011
Abstract
Several results related to flat Friedmann-Lema\^ıtre-Robertson-Walker models in the conformal (Einstein) frame of scalar-tensor gravity theories are extended. Scalar fields with arbitrary (positive) potentials and arbitrary coupling functions are considered. Mild assumptions under such functions (differentiable class, number of singular points, asymptotes, etc) are introduced in a straightforward manner in order to characterize the asymptotic structure on a phase space. We pay special attention to the possible scaling solutions. Numerical evidence confirming our results is presented.
arXiv comment32 pages, 6 figures. Matches the published version in CQG
References in corpus (135)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Dynamics of dark energy
- The Seventh Data Release of the Sloan Digital Sky Survey
- The Cosmological Constant and Dark Energy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- f(R) Theories Of Gravity
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Cosmological parameters from SDSS and WMAP
- f(R) theories
- Extended Theories of Gravity
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- Cosmological Constant - the Weight of the Vacuum
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- Cosmology and the Fate of Dilatation Symmetry
- Coupled Quintessence
- The 3D power spectrum of galaxies from the SDSS
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Exponential potentials and cosmological scaling solutions
- Dark Energy Constraints from the Cosmic Age and Supernova
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results
- Quantum deSitter cosmology and phantom matter
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
- Reconstruction of a scalar-tensor theory of gravity in an accelerating universe
- Quintom Cosmology: Theoretical implications and observations
- Reconstructing the Inflaton Potential --- an Overview
- Cosmological Evolution of a Quintom Model of Dark Energy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
- Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
- Scaling solutions in general non-minimal coupling theories
- A classification of scalar field potentials with cosmological scaling solutions
- The HST Key Project on the Extragalactic Distance Scale. XXVIII. Combining the Constraints on the Hubble Constant
- Quantum effects can render w<-1 on cosmological scales
- On Physical Equivalence between Nonlinear Gravity Theories
- The Cosmological Constant Problem and Quintessence
- Phenomenology of a realistic accelerating universe using only Planck-scale physics
- "Teleparallel" Dark Energy
- Dynamics of Linear Perturbations in f(R) Gravity
- A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy
- Cosmological parameters from supernova observations: A critical comparison of three data sets
- Inflationary Models with Logarithmic Potentials
- Crossing of the w=-1 Barrier by D3-brane Dark Energy Model
- Statefinder diagnostic for coupled quintessence
- Interactions in Scalar Field Cosmology
- Quintom models with an equation of state crossing -1
- Nonminimal torsion-matter coupling extension of f(T) gravity
- Cosmology of the Galileon from Massive Gravity
- Generalized Assisted Inflation
- Two-field Models of Dark Energy with Equation of State Across -1
- Dynamics of -essence
- Cosmology with positive and negative exponential potentials
- Dynamical behavior in cosmology
- Quintessential Difficulties
- Stationary dark energy with a baryon-dominated era: solving the coincidence problem with a linear coupling
- Coupled oscillators as models of quintom dark energy
- Intermediate inflation and the slow-roll approximation
- Quintom cosmologies admitting either tracking or phantom attractors
- Accelerated cosmological expansion due to a scalar field whose potential has a positive lower bound
- Dynamics of Assisted Inflation
- Enlarged quintessence cosmology
- Quintom cosmologies with arbitrary potentials
- Interacting Phantom Energy
- Universality class of holographic superconductors
- The Dynamics of Multi-Scalar Field Cosmological Models and Assisted Inflation
- Some aspects of the cosmological conformal equivalence between ``Jordan Frame'' and ``Einstein Frame''
- Interacting Quintessence, Cosmic Acceleration and the Coincidence Problem
- Dark energy from a quintessence (phantom) field rolling near potential minimum (maximum)
- Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter
- Correspondence between kinematical backreaction and scalar field cosmologies - the `morphon field'
- Exactly Solvable SFT Inspired Phantom Model
- Can we be tricked into thinking that w is less than -1?
- Scalar-field-dominated cosmology with a transient accelerating phase
- General Relativity and Weyl Geometry
- Dark energy exponential potential models as curvature quintessence
- Observing the Inflaton Potential
- Cosmological behavior in extended nonlinear massive gravity
- General analytic formulae for attractor solutions of scalar-field dark energy models and their multi-field generalizations
- Towards a Novel no-hair Theorem for Black Holes
- Scaling Solutions in Robertson-Walker Spacetimes
- Dilaton-derived quintessence scenario leading naturally to the late-time acceleration of the Universe
- Quintessence Model With Double Exponential Potential
- Integrable Scalar Cosmologies I. Foundations and links with String Theory
- Scalar Field Cosmologies and the Initial Space-Time Singularity
- Theoretical Limits on the Equation-of-State Parameter of Phantom Cosmology
- Cosmology of the proxy theory to massive gravity
- Interacting Phantom Energy and Avoidance of the Big Rip Singularity
- Cosmological Scaling Solutions and Multiple Exponential Potentials
- Phase structure of the massive chiral Gross-Neveu model from Hartree-Fock
- The conformal transformation's controversy: what are we missing?
- Dark energy, dissipation and the coincidence problem
- Dynamics of Scalar Field Dark Matter With a Cosh-like Potential
- Tensor-multi-scalar theories from multidimensional cosmology
- Exact Analysis of Scaling and Dominant Attractors Beyond the Exponential Potential
- Integrable cosmological models with non-minimally coupled scalar fields
- Phase Space Analysis of Quintessence Cosmologies with a Double Exponential Potential
- Generalised Scalar Field Potentials and Inflation
- Auxiliary fields representation for modified gravity models
- On the Past Asymptotic Dynamics of Non-minimally Coupled Dark Energy
- Singularities In Scalar-Tensor Cosmologies
- Dynamics of a scalar field in Robertson-Walker spacetimes
- Quasi-dilaton non-linear massive gravity: Investigations of background cosmological dynamics
- Stable Exact Solutions in Cosmological Models with Two Scalar Fields
- Interacting viscous dark fluids
- Construction of Exact Solutions in Two-Fields Models and the Crossing of the Cosmological Constant Barrier
- Dynamics of a Self-interacting Scalar Field Trapped in the Braneworld for a Wide Variety of Self-interaction Potentials
- f(R) Gravity and its Cosmological Implications
- Late-time oscillatory behaviour for self-gravitating scalar fields
- Qualitative analysis of Kantowski-Sachs metric in a generic class of models
- Energy exchange for homogeneous and isotropic universes with a scalar field coupled to matter
- Fixed points in interacting dark energy models
- Varying-Alpha Cosmologies with Potentials
- Dynamics of Generalized Assisted Inflation
- Scalar-field cosmologies with an arbitrary potential
- Asymptotic behavior of a scalar field with an arbitrary potential trapped on a Randall-Sundrum's braneworld: the effect of a negative dark radiation term on a Bianchi I brane
- Stability analysis of an autonomous system in loop quantum cosmology
- Three fluid cosmological model using Lie and Noether symmetries
- The recollapse problem of closed FRW models in higher-order gravity theories
- Non-minimally Coupled Cosmological Models with the Higgs-like Potentials and Negative Cosmological Constant
- Thawing models in the presence of a generalized Chaplygin gas
- Heteroclinic orbit and tracking attractor in cosmological model with a double exponential potential
- Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
- Exact Scaling Solutions in Normal and Brans-Dicke Models of Dark Energy
- Comment to the paper `Conformal transformations single out a unique measure of distance'
- Perturbative stability of SFT-based cosmological models
- Evolution of density perturbations in double exponential quintessence models
- Covariant and gauge-invariant linear scalar perturbations in multiple scalar field cosmologies
- Qualitative Analysis of Early Universe Cosmologies
- Expanding universes in the conformal frame of gravity
- Constraints on scalar-tensor theories from observations
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- Dynamical systems applied to cosmology: dark energy and modified gravity
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- Interacting quintessence from a variational approach Part I: algebraic couplings
- Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
- On the possibility of blue tensor spectrum within single field inflation
- Dynamics and cosmological evolution in Λ-varying cosmology
- Dynamics in Varying vacuum Finsler-Randers Cosmology
- Cosmological Evolution and Exact Solutions in a Fourth-order Theory of Gravity
- Non-minimally coupled scalar field cosmology with torsion
- Interacting quintessence in light of Generalized Uncertainty Principle: Cosmological perturbations and dynamics
- Unified dark sectors in scalar-torsion theories of gravity
- Intermediate accelerated solutions as generic late-time attractors in a modified Jordan-Brans-Dicke theory
- Modified gravity and cosmology with nonminimal (derivative) coupling between matter and the Einstein tensor
- Brans--Dicke cosmology does not have the CDM phase as an universal attractor
- Time-averaging axion-like interacting scalar fields models
- Generalized Scalar Field Cosmologies: A Global Dynamical Systems Formulation
- Generalized scalar field cosmologies: theorems on asymptotic behavior
- Averaging Generalized Scalar Field Cosmologies I: Locally Rotationally Symmetric Bianchi III and open Friedmann-Lemaître-Robertson-Walker models
- Extended analysis for the Evolution of the Cosmological history in Einstein-aether Scalar Field theory
- Averaging Generalized Scalar Field Cosmologies II: Locally Rotationally Symmetric Bianchi I and flat Friedmann-Lemaître-Robertson-Walker models
- The Chameleon Effect in the Jordan Frame of the Brans--Dicke Theory
- Revisiting slow-roll inflation in nonminimal derivative coupling with potentials
- Higher Order Lagrangians inspired by the Pais-Uhlenbeck Oscillator and their cosmological applications
- Scalar field evolution at background and perturbation levels for a broad class of potentials
- Complex Scalar fields in Scalar-Tensor and Scalar-Torsion theories
- Quantization of Einstein-aether Scalar field Cosmology
- Compact Q-balls and Q-shells in a multi-component model
- Energy momentum tensor of a non-minimally coupled scalar from the equivalence of the Einstein and Jordan frames