Dark Energy in Practice
arXiv:1006.5694 · doi:10.1142/S0217751X10050743
Abstract
In this paper we review a part of the approaches that have been considered to explain the extraordinary discovery of the late time acceleration of the Universe. We discuss the arguments that have led physicists and astronomers to accept dark energy as the current preferable candidate to explain the acceleration. We highlight the problems and the attempts to overcome the difficulties related to such a component. We also consider alternative theories capable of explaining the acceleration of the Universe, such as modification of gravity. We compare the two approaches and point out the observational consequences, reaching the sad but foresightful conclusion that we will not be able to distinguish between a Universe filled by dark energy or a Universe where gravity is different from General Relativity. We review the present observations and discuss the future experiments that will help us to learn more about our Universe. This is not intended to be a complete list of all the dark energy models but this paper should be seen as a review on the phenomena responsible for the acceleration. Moreover, in a landscape of hardly compelling theories, it is an important task to build simple measurable parameters useful for future experiments that will help us to understand more about the evolution of the Universe.
Minor revisions; to appear in IJMPA
References in corpus (224)
- 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
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- Efficient Computation of CMB anisotropies in closed FRW models
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- f(R) Theories Of Gravity
- Cosmological parameters from SDSS and WMAP
- Cosmological Imprint of an Energy Component with General Equation of State
- de Sitter Vacua in String Theory
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- The Cosmological Constant
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- Weak Gravitational Lensing
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- Dark Energy and the Accelerating Universe
- k-Inflation
- The galileon as a local modification of gravity
- Essentials of k-essence
- Coupled Quintessence
- Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
- Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
- The 3D power spectrum of galaxies from the SDSS
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Constraints on the redshift dependence of the dark energy potential
- Quantization of Four-form Fluxes and Dynamical Neutralization of the Cosmological Constant
- Can the dark energy equation-of-state parameter w be less than -1?
- Quintessence and the Rest of the World
- Perturbations in k-inflation
- Causality, Analyticity and an IR Obstruction to UV Completion
- Inflation Dynamics and Reheating
- Quantum deSitter cosmology and phantom matter
- Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Brane cosmological evolution in a bulk with cosmological constant
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Cosmology on a Brane in Minkowski Bulk
- Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
- A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder
- Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
- Cosmic Growth History and Expansion History
- 1/R gravity and Scalar-Tensor Gravity
- The phantom menaced: constraints on low-energy effective ghosts
- Can dark energy evolve to the Phantom?
- Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
- The Anthropic Landscape of String Theory
- A glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3
- Interacting Quintessence
- Distributions of flux vacua
- Curvature quintessence matched with observational data
- Dark Matter and Dark Energy
- Are f(R) dark energy models cosmologically viable ?
- Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler
- Can the Chaplygin gas be a plausible model for dark energy?
- Is there Supernova Evidence for Dark Energy Metamorphosis ?
- On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter
- Quintessence as a run-away dilaton
- The end of unified dark matter?
- Very weak lensing in the CFHTLS Wide: Cosmology from cosmic shear in the linear regime
- Measuring the dark side (with weak lensing)
- Metastable Gravitons and Infinite Volume Extra Dimensions
- Dark Energy from structure: a status report
- Probing the Coupling between Dark Components of the Universe
- Quintessence and Supergravity
- Distances, ages, and epoch of formation of globular clusters
- Solar System constraints to general f(R) gravity
- Dark Energy Anisotropic Stress and Large Scale Structure Formation
- Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
- Confirmation of general relativity on large scales from weak lensing and galaxy velocities
- Probing dark energy perturbations: the dark energy equation of state and speed of sound as measured by WMAP
- The gravity lagrangian according to solar system experiments
- Phantom cosmologies
- Constructing Phantom Cosmologies from Standard Scalar Field Universes
- A New Cosmological Scenario in String Theory
- Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
- An inhomogeneous alternative to dark energy?
- Dynamics of interacting dark energy
- WMAP and the Generalized Chaplygin Gas
- The Robustness of Quintessence
- Generalized Chaplygin gas and CMBR constraints
- Constraints on the generalized Chaplygin gas from supernovae observations
- Accelerating Cosmologies from Compactification
- Joint Galaxy-Lensing Observables and the Dark Energy
- String Theory and Quintessence
- Baryonic Signatures in Large-Scale Structure
- The White Dwarf Cooling Sequence of the Globular Cluster Messier 4
- You need not be afraid of phantom energy
- K-Essential Phantom Energy: Doomsday around the corner?
- Density perturbations in an Universe dominated by the Chaplygin gas
- Cosmological consequences of a Chaplygin gas dark energy
- Why the Universe is Just So
- deSitter brane universeinduced by phantom and quantum effects
- Structure formation in the DGP cosmological model
- The foundations of observing dark energy dynamics with the Wilkinson Microwave Anisotropy Probe
- Crossing of the w=-1 Barrier by D3-brane Dark Energy Model
- Models of dynamical supersymmetry breaking and quintessence
- Confronting Lemaitre-Tolman-Bondi models with Observational Cosmology
- Dark Energy versus Modified Gravity
- More on ghosts in DGP model
- Likely Values of the Cosmological Constant
- Cosmic distance-duality as probe of exotic physics and acceleration
- Accelerating Cosmologies from S-Branes
- The cluster gas mass fraction as a cosmological probe: a revised study
- Dust of Dark Energy
- The Dynamics of Quintessence, The Quintessence of Dynamics
- Self-Accelerating Universe in Galileon Cosmology
- Baryonic acoustic oscillations in simulated galaxy redshift surveys
- B-Inflation
- A new view of k-essence
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: observational constraints
- Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy
- f(R) actions, cosmic acceleration and local tests of gravity
- Growing Matter
- Testing the Cosmic Coincidence Problem and the Nature of Dark Energy
- The Acceleration of the Universe, a Challenge for String Theory
- Crossing the Phantom Divide Barrier with Scalar Tensor Theories
- Generalized phantom energy
- Cosmological Effects of a Class of Fluid Dark Energy Models
- A Single Scalar Field Model of Dark Energy with Equation of State Crossing -1
- String or M theory axion as a quintessence
- Observational constraints on self-accelerating cosmology
- Dark-Energy Evolution Across the Cosmological-Constant Boundary
- Quintessence: a mini-review
- Acoustic oscillations in the SDSS DR4 Luminous Red Galaxy sample power spectrum
- Are there ghosts in the self-accelerating brane universe?
- Challenges to the DGP Model from Horizon-Scale Growth and Geometry
- Cascading Gravity and Degravitation
- Parametrization of Quintessence and Its Potential
- Cosmological structure formation in a homogeneous dark energy background
- Parametrizations of the Dark Energy Density and Scalar Potentials
- On likely values of the cosmological constant
- Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys
- Density perturbations in f(R) gravity theories in metric and Palatini formalisms
- Generalizing the generalized Chaplygin gas
- K-essence and the coincidence problem
- Crossing the Phantom Divide
- De Sitter Space in Supergravity and M Theory
- Dark energy from a quintessence (phantom) field rolling near potential minimum (maximum)
- A Quintessential Axion
- Quintessence models in Supergravity
- Looking the void in the eyes - the kSZ effect in LTB models
- Constraining Dark Energy Anisotropic Stress
- SUSY QCD and Quintessence
- The cosmological constant and the time of its dominance
- No-go theorem for k-essence dark energy
- Phantom cosmology with general potentials
- Cosmological Constraints on DGP Braneworld Gravity with Brane Tension
- Power-laws f(R) theories are cosmologically unacceptable
- Interacting models of soft coincidence
- Constraints on the Sound Speed of Dynamical Dark Energy
- Supersymmetric Large Extra Dimensions and the Cosmological Constant: An Update
- Supergravity, Dark Energy and the Fate of the Universe
- Gauged Supergravities, de Sitter Space and Cosmology
- Axion Phantom Energy
- A Dynamical Approach to the Cosmological Constant
- Constraining the cosmic equation of state from old galaxies at high redshift
- Quintessence from M-Theory
- Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
- Fingerprinting dark energy
- Ages of globular clusters: a new approach
- Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
- Quintessence Axion Potential Induced by Electroweak Instanton Effects
- A k-essence Model Of Inflation, Dark Matter and Dark Energy
- Baryon oscillations
- Attractor Behavior of Phantom Cosmology
- Bulk Singularities and the Effective Cosmological Constant for Higher Co-dimension Branes
- Slow-roll k-essence
- Generalized Chaplygin Gas Models tested with SNIa
- Distance, Growth Factor, and Dark Energy Constraints from Photometric Baryon Acoustic Oscillation and Weak Lensing Measurements
- K-essential Leptogenesis
- A Brane World Solution to the Cosmological Constant Problem
- Affine equation of state from quintessence and k-essence fields
- Structure formation in modified gravity models alternative to dark energy
- Dark energy equation of state and anthropic selection
- Skewness as a test of the equivalence principle
- Constraints on early dark energy from CMB lensing and weak lensing tomography
- Large-scale inhomogeneities in modified Chaplygin gas cosmologies
- Dark Energy and Right-Handed Neutrinos
- Viscous dissipative Chaplygin gas dominated homogenous and isotropic cosmological models
- Chaplygin gas with non-adiabatic pressure perturbations
- Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
- Supernova data may be unable to distinguish between quintessence and k-essence
- Cascading Cosmology
- Scalar phantom energy as a cosmological dynamical system
- On the estimation of the current value of the cosmological constant
- Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
- Constraints on dark energy from the lookback time versus redshift test
- Domain Walls As Probes Of Gravity
- A cosmological constant from degenerate vacua
- Fingerprinting Dark Energy II: weak lensing and galaxy clustering tests
- Stability of FRW Cosmology with Generalized Chaplygin Gas
- Induced gravity on intersecting brane-worlds Part I: Maximally symmetric solutions
- Can we live in a self-tuning universe?
- Matter Power Spectrum for the Generalized Chaplygin Gas Model: The Newtonian Approach
- Observational constraints on generalized Chaplygin gas model
- Bias and the power spectrum beyond the turn-over
- Multiple kinetic k-essence, phantom barrier crossing and stability
- Atypical k-essence cosmologies
- Tracking quintessence and k-essence in a general cosmological background
- Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
- MSLED, Neutrino Oscillations and the Cosmological Constant
- Instability of Chaplygin gas trajectories in unified dark matter models
- Vacuum Energy: "If Not Now, Then When?"
- Constraints on Dark Energy and Modified Gravity models by the Cosmological Redshift Drift test
- Vacuum Energy: If Not Now, Then When?
- Microwave Background Anisotropies Induced by Global Scalar Fields: The Large N Limit
- Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
- Brane-world cosmology
- Slow-roll Extended Quintessence
- Transient acceleration from a hybrid Chaplygin gas
- Rigidity of cosmic acceleration in a class of k-essence cosmologies
- Quintessence as k-essence
- Current lookback time-redshift bounds on dark energy
- Dynamical vacuum energy via adjustment mechanism
- An Approach to the Cosmological Constant Problem(s)
- Covariance of dark energy parameters and sound speed constraints from large HI surveys
- Dark Energy Phenomenology
Cited by in corpus (36)
- Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
- Dark Energy
- Curvature vs Distances: testing the FLRW cosmology
- The phenomenological approach to modeling the dark energy
- Internal Robustness of Growth Rate data
- A parametrization of the growth index of matter perturbations in various Dark Energy models and observational prospects using a Euclid-like survey
- Constraints on dark energy from H II starburst galaxy apparent magnitude versus redshift data
- Anisotropic stress and stability in modified gravity models
- Galaxy cluster number count data constraints on cosmological parameters
- Null tests of the standard model using the linear model formalism
- Fingerprinting Dark Energy III: distinctive marks of viscosity
- Massive and modified gravity as self-gravitating media
- Exact nonlinear inhomogeneities in CDM cosmology
- Can dark energy viscosity be detected with the Euclid survey?
- Consistency check of ΛCDM phenomenology
- A novel null test for the CDM model with growth-rate data
- The traces of anisotropic dark energy in light of Planck
- Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
- Observational constraints on scalar field models of dark energy with barotropic equation of state
- Present accelerated expansion of the universe from new Weyl-Integrable gravity approach
- Quintessence versus phantom dark energy: the arbitrating power of current and future observations
- Cosmological dark fluid from five-dimensional vacuum
- Revisiting a model-independent dark energy reconstruction method
- Reconstruction of the null-test for the matter density perturbations
- Dark energy homogeneity in general relativity: Are we applying it correctly?
- Forecasting cosmological parameter constraints from near-future space-based galaxy surveys
- Constraints on a gravity dark energy model with early scaling evolution
- The Distinguishability of Interacting Dark Energy from Modified Gravity
- Comparison of piecewise-constant methods for dark energy
- Comparing Dark Energy models with Hubble versus Growth Rate data
- Gravitational waves during inflation from a 5D large-scale repulsive gravity model
- Linear dark energy equation of state revealed by supernovae?
- Dark energy from a renormalization group flow
- Study of branes with variable tension
- Cosmological constraints from galaxy multi-tracers in the nearby Universe
- Dark Energy Simulations