Report of the Dark Energy Task Force
arXiv:astro-ph/0609591
Abstract
Dark energy appears to be the dominant component of the physical Universe, yet there is no persuasive theoretical explanation for its existence or magnitude. The acceleration of the Universe is, along with dark matter, the observed phenomenon that most directly demonstrates that our theories of fundamental particles and gravity are either incorrect or incomplete. Most experts believe that nothing short of a revolution in our understanding of fundamental physics will be required to achieve a full understanding of the cosmic acceleration. For these reasons, the nature of dark energy ranks among the very most compelling of all outstanding problems in physical science. These circumstances demand an ambitious observational program to determine the dark energy properties as well as possible.
The Dark Energy Task Force (DETF) was established by the Astronomy and Astrophysics Advisory Committee (AAAC) and the High Energy Physics Advisory Panel (HEPAP) as a joint sub-committee to advise the Department of Energy, the National Aeronautics and Space Administration, and the National Science Foundation on future dark energy research
Cited by in corpus (277)
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- SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
- Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
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- Observational Probes of Cosmic Acceleration
- KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
- Cosmology and Fundamental Physics with the Euclid Satellite
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
- Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
- CMB-S4 Science Case, Reference Design, and Project Plan
- Weak Gravitational Lensing and its Cosmological Applications
- Gravitational Lensing Analysis of the Kilo Degree Survey
- The DESI Experiment, a whitepaper for Snowmass 2013
- The Observed Growth of Massive Galaxy Clusters I: Statistical Methods and Cosmological Constraints
- CFHTLenS: Combined probe cosmological model comparison using 2D weak gravitational lensing
- Dark energy two decades after: Observables, probes, consistency tests
- How to measure redshift-space distortions without sample variance
- Cosmology and Astrophysics from Relaxed Galaxy Clusters II: Cosmological Constraints
- Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
- The DESI Experiment Part II: Instrument Design
- Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
- Theoretical Models of Dark Energy
- Measuring D_A and H at z=0.35 from the SDSS DR7 LRGs using baryon acoustic oscillations
- Putting the Precision in Precision Cosmology: How accurate should your data covariance matrix be?
- Dark Energy Survey Year 1 Results: Weak Lensing Shape Catalogues
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function
- Cosmology with the shear-peak statistics
- The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
- Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints
- The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
- The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts
- Measuring Baryon Acoustic Oscillations along the line of sight with photometric redshifs: the PAU survey
- The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release
- The ASTRO-H Mission
- LoCuSS: First Results from Strong-lensing Analysis of 20 Massive Galaxy Clusters at z~0.2
- The Tianlai project: a 21cm cosmology experiment
- The X-ray Cluster Normalization of the Matter Power Spectrum
- Automated Transient Identification in the Dark Energy Survey
- The abundance of voids and the excursion set formalism
- Taking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest
- Constraints on cosmic opacity and beyond the standard model physics from cosmological distance measurements
- A first application of the Alcock-Paczynski test to stacked cosmic voids
- Probing Gravity with Spacetime Sirens
- Testing the tidal alignment model of galaxy intrinsic alignment
- Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -II. Application to Simulations
- "Swiss-Cheese" Inhomogeneous Cosmology & the Dark Energy Problem
- Wide-Field InfraRed Survey Telescope (WFIRST) Final Report
- Power of Observational Hubble Parameter Data: a Figure of Merit Exploration
- Cosmological information in the redshift-space bispectrum
- Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys
- 3D Cosmic Shear: Cosmology from CFHTLenS
- Handbook for the GREAT08 Challenge: An image analysis competition for cosmological lensing
- Constraints on primordial non-Gaussianity from 800,000 photometric quasars
- Condensates in Quantum Chromodynamics and the Cosmological Constant
- The Evolution of Ly-alpha Emitting Galaxies Between z = 2.1 and z = 3.1
- Defining a weak lensing experiment in space
- Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
- Accounting for baryonic effects in cosmic shear tomography: Determining a minimal set of nuisance parameters using PCA
- Galaxy Shapes and Intrinsic Alignments in The MassiveBlack-II Simulation
- Super-Eddington accreting massive black holes as long-lived cosmological standards
- Constraints on Dark Energy from Supernovae, Gamma Ray Bursts, Acoustic Oscillations, Nucleosynthesis and Large Scale Structure and the Hubble constant
- The ASTRO-H X-ray Observatory
- Cosmic Shear Measurements with DES Science Verification Data
- Shape measurement biases from underfitting and ellipticity gradients
- Radio Continuum Surveys with Square Kilometre Array Pathfinders
- Measurement and Calibration of Noise Bias in Weak Lensing Galaxy Shape Estimation
- Cosmography by GRBs
- Findings of the Joint Dark Energy Mission Figure of Merit Science Working Group
- Cosmological Applications of Pade Approximant
- Extending cosmological tests of General Relativity with the Square Kilometre Array
- Strong near-infrared carbon in the Type Ia supernova iPTF13ebh
- Hubble parameter measurement constraints on dark energy
- Intrinsic alignments of galaxies in the MassiveBlack-II simulation: analysis of two-point statistics
- Dark energy equation of state parameter and its variation at low redshifts
- Cross-Correlation of spectroscopic and photometric galaxy surveys: cosmology from lensing and redshift distortions
- Using neural networks to estimate redshift distributions. An application to CFHTLenS
- General Requirements on Matter Power Spectrum Predictions for Cosmology with Weak Lensing Tomography
- Gamma Rays from Clusters and Groups of Galaxies: Cosmic Rays versus Dark Matter
- The cosmological analysis of X-ray cluster surveys: II- Application of the CR-HR method to the XMM archive
- Near-Infrared Properties of Type Ia Supernovae
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- Star/galaxy separation at faint magnitudes: Application to a simulated Dark Energy Survey
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- Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
- Cosmology with the Large Synoptic Survey Telescope: an Overview
- Testing Low-Redshift Cosmic Acceleration with Large-Scale Structure
- Model-independent constraints on the cosmological anisotropic stress
- Galaxy shapes and alignments in the MassiveBlack-II hydrodynamic and dark matter-only simulations
- Cosmological parameter inference with Bayesian statistics
- Cosmography beyond standard candles and rulers
- Intrinsic alignments of disk and elliptical galaxies in the MassiveBlack-II and Illustris simulations
- Precision cosmology with a wide area XMM cluster survey
- A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies
- Dark degeneracy I: Dynamical or interacting dark energy?
- The High Redshift Integrated Sachs-Wolfe Effect
- Effects of the neutrino mass splitting on the non-linear matter power spectrum
- Image Analysis for Cosmology: Results from the GREAT10 Star Challenge
- Growth factor and galaxy bias from future redshift surveys: a study on parametrizations
- Dark Energy Survey Year 1 Results: The Impact of Galaxy Neighbours on Weak Lensing Cosmology with im3shape
- VIS: the visible imager for Euclid
- 3D Photometric Cosmic Shear
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- Simulations of Wide-Field Weak Lensing Surveys II: Covariance Matrix of Real Space Correlation Functions
- Dark matter and halo bispectrum in redshift space: theory and applications
- Observational constraints on thawing quintessence models
- Response function of the large-scale structure of the universe to the small scale inhomogeneities
- Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
- Precise Measurements of Primordial Power Spectrum with 21 cm Fluctuations
- Anisotropy of Cosmic Acceleration
- Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
- Testing general relativity with the multipole spectra of the SDSS luminous red galaxies
- Modelling the Transfer Function for the Dark Energy Survey
- What Lies Beneath: Using p(z) to Reduce Systematic Photometric Redshift Errors
- Cosmological Systematics Beyond Nuisance Parameters : Form Filling Functions
- Toward More Realistic Forecasting of Dark Energy Constraints from Galaxy Redshift Surveys
- Constraining warm dark matter with cosmic shear power spectra
- Early Dark Energy at High Redshifts: Status and Perspectives
- Constraints on growth index parameters from current and future observations
- Photometric redshift estimation based on data mining with PhotoRApToR
- Probing dark energy and neutrino mass from upcoming lensing experiments of CMB and galaxies
- Lensing and Supernovae: Quantifying The Bias on the Dark Energy Equation of State
- : Estimating Transient Discovery Rates for the Zwicky Transient Facility
- Cosmology with the cluster mass function: mass estimators and shape systematics in large weak lensing surveys
- A step towards testing general relativity using weak gravitational lensing and redshift surveys
- Self calibration of photometric redshift scatter in weak lensing surveys
- Measuring dark energy spatial inhomogeneity with supernova data
- Using a phenomenological model to test the coincidence problem of dark energy
- The signature of dark energy perturbations in galaxy cluster surveys
- SKA Weak Lensing III: Added Value of Multi-Wavelength Synergies for the Mitigation of Systematics
- The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
- Sérsic galaxy models in weak lensing shape measurement: model bias, noise bias and their interaction
- Cosmological test of gravity using weak lensing voids
- Cluster X-ray luminosity-temperature relation at z>~1.5
- The Dark UNiverse Explorer (DUNE): Proposal to ESA's Cosmic Vision
- Fast full N-body simulations of generic modified gravity: conformal coupling models
- The Cosmological Constant Problem, Dark Energy, and the Landscape of String Theory
- Optimised angular power spectra for spectroscopic galaxy surveys
- Cosmological perturbations in SFT inspired non-local scalar field models
- Comparison of Recent SnIa datasets
- Extending the Hubble diagram by gamma ray bursts
- Classical tests in brane gravity
- Localization of nonlocal cosmological models with quadratic potentials in the case of double roots
- Center-Excised X-ray Luminosity as an Efficient Mass Proxy for Future Galaxy Cluster Surveys
- Cosmological Constraints on Higgs-Dilaton Inflation
- Fast full -body simulations of generic modified gravity: derivative coupling models
- I. Apples to apples : realistic galaxy simulated catalogs and photometric redshift predictions for next-generation surveys
- Precision cosmology in muddy waters: Cosmological constraints and N-body codes
- Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?
- A Technique for Weak Lensing with Velocity Maps: Eliminating Ellipticity Noise in HI Radio Observations
- Constraining cosmology with shear peak statistics: tomographic analysis
- Tomographic weak lensing shear spectra from large N-body and hydrodynamical simulations
- A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
- The Three Faces of Omega_m: Testing Gravity with Low and High Redshift SN Ia Surveys
- A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
- Null Energy Condition Violation and Classical Stability in the Bianchi I Metric
- The Absolute Magnitude of RRc Variables From Statistical Parallax
- Future dark energy constraints from measurements of quasar parallax: Gaia, SIM and beyond
- Non-linear weak lensing forecasts
- A new cosmic shear function: Optimised E-/B-mode decomposition on a finite interval
- The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
- 3D Weak Gravitational Lensing of the CMB and Galaxies
- The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
- Model independent constraints on mass-varying neutrino scenarios
- Non-parametric Dark Energy Degeneracies
- Constraining Scale-Dependent Non-Gaussianity with Future Large-Scale Structure and the CMB
- Modified Gravity: the CMB, Weak Lensing and General Parameterisations
- Parameter estimation with Sandage-Loeb test
- A one-parameter formula for testing slow-roll dark energy: observational prospects
- Optimizing baryon acoustic oscillation surveys II: curvature, redshifts, and external datasets
- Cosmic shear without shape noise
- Complementary constraints on dark energy equation of state from strongly lensed gravitational wave
- The Accelerating Universe
- Intrinsic uncertainty on the nature of dark energy
- Velocity and mass bias in the distribution of dark matter halos
- Seeing in the dark -- I. Multi-epoch alchemy
- Testing cosmic acceleration for parameterizations using measurements in galaxy clusters
- Sources of contamination to weak lensing tomography: redshift-dependent shear measurement bias
- Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure
- The scale of cosmic homogeneity as a standard ruler
- An Accurate Cluster Selection Function for the J-PAS Narrow-Band wide-field survey
- Non-Gaussian isocurvature perturbations in dark radiation
- Observational Bounds on Modified Gravity Models
- Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
- BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures
- Tension between SN and BAO: current status and future forecasts
- Effects of overlapping sources on cosmic shear estimation: Statistical sensitivity and pixel-noise bias
- Confronting Tracker Field Quintessence with Data
- The Impact of Non-Gaussianity upon Cosmological Forecasts
- Cold dark energy constraints from the abundance of galaxy clusters
- Exploring the NRO Opportunity for a Hubble-sized Wide-field Near-IR Space Telescope -- NEW WFIRST
- Testing dark energy using pairs of galaxies in redshift space
- First simultaneous optical/near-infrared imaging of an X-ray selected, high-redshift cluster of galaxies with GROND: the galaxy population of XMMU J0338.7+0030 at z=1.1
- Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
- Breaking through the high redshift bottleneck of Observational Hubble parameter Data: The Sandage-Loeb signal Scheme
- On the measurement of cosmological parameters
- Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
- Modelling the shapes of the largest gravitationally bound objects
- Path Integral Marginalization for Cosmology: Scale Dependent Galaxy Bias & Intrinsic Alignments
- Detecting Baryon Acoustic Oscillations
- The self similarity of weak lensing peaks
- Space-quality data from balloon-borne telescopes: the High Altitude Lensing Observatory (HALO)
- Simultaneous Constraints on Cosmology and Photometric Redshift Bias from Weak Lensing and Galaxy Clustering
- Reconstruction of HI power spectra with radio-interferometers to study dark energy
- The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
- Instrumental systematics and weak gravitational lensing
- The impact of cosmic variance on simulating weak lensing surveys
- Optimal void finders in weak lensing maps
- Parameter constraints from weak lensing tomography of galaxy shapes and cosmic microwave background fluctuations
- A new framework for numerical simulations of structure formation
- The Angular-Diameter-Distance-Maximum and Its Redshift as Constraints on FLRW Models
- Nontrivial Geometries: Bounds on the Curvature of the Universe
- -attractor dark energy in view of next-generation cosmological surveys
- Fisher Matrix Stability
- Prospects in Constraining the Dark Energy Potential
- Constraints on Generalized Dark Energy from Recent Observations
- Unravelling the Dark Matter - Dark Energy Paradigm
- A Precise Photometric Ratio via Laser Excitation of the Sodium Layer I: One-photon Excitation Using 342.78 nm Light
- Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
- Information Content in the Angular Power Spectrum of Weak Lensing: Wavelet Method
- Dark Energy Perturbations Revisited
- Multi-scalar field cosmology from SFT: an exactly solvable approximation
- A Quantum Cosmology: No Dark Matter, Dark Energy nor Accelerating Universe
- An Inhomogeneous Model Universe Behaving Homogeneously
- Measuring cosmic distances with galaxy clusters
- Self-accelerating solutions of scalar-tensor gravity
- Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
- Reducing Zero-point Systematics in Dark Energy Supernova Experiments
- The sensitivity of BAO Dark Energy Constraints to General Isocurvature Perturbations
- Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
- Cosmological constraints from multiple tracers in spectroscopic surveys
- Interpreting Internal Consistency of DES Measurements
- The Distinguishability of Interacting Dark Energy from Modified Gravity
- Constraints on Dark Energy state equation with varying pivoting redshift
- The SDSS Coadd: Cross-Correlation Weak Lensing and Tomography of Galaxy Clusters
- Impacts on Cosmological Constraints from Degeneracies
- Fisher matrix forecasts for astrophysical tests of the stability of the fine-structure constant
- Type Ia Supernovae Selection and Forecast of Cosmology Constraints for the Dark Energy Survey
- Beyond the Standard Model of Physics with Astronomical Observations
- Observational constraints to a unified cosmological model
- Constraints on Dark Energy from New Observations including Pan-STARRS
- Parameters and pitfalls in dark energy models with time varying equation of state
- Image Analysis for Cosmology: Shape Measurement Challenge Review & Results from the Mapping Dark Matter Challenge
- Cosmic Reionization Study : Principle Component Analysis After Planck
- Constraints on dark energy evolution
- Testing and selecting cosmological models with ultra-compact radio quasars
- Self calibration of galaxy bias in spectroscopic redshift surveys of baryon acoustic oscillations
- Quantum Yang-Mills Condensate Dark Energy Models
- The expansion of the universe observed with supernovae
- Testing the Origin of the CMB Large-Angle Correlation Deficit with a Galaxy Imaging Survey
- The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview
- DECam integration tests on telescope simulator
- Cosmological parameters from lenses distance ratio
- A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
- Constraints on Decaying Dark Matter
- CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
- Cosmic Shear Bias and Calibration in Cosmic Shear Studies
- Dark Energy and Hubble Constant From the Latest SNe Ia, BAO and SGL
- Satellite-Mounted Light Sources as Photometric Calibration Standards
- An Analysis of DES Cluster Simulations through the IMCAT and Shapelets Weak Lensing Pipelines
- Cosmological singularities in FLRW spacetimes
- aTmcam: A Simple Atmospheric Transmission Monitoring Camera For Sub 1% Photometric Precision
- Evaluating Systematic Dependencies of Type Ia Supernovae
- Precision Cosmology and the Landscape
- One more fitting (D=5) of Supernovae redshifts
- Great Surveys of the Universe
- Analytic Photometric Redshift Estimator for Type Ia Supernovae From the Large Synoptic Survey Telescope
- Dark Energy and CMB
- Conference Summary: HI Science in the Next Decade
- Lookback time and Chandra constrains on cosmological parameters
- Closing the cosmological loop with the redshift drift
- Lossy compression of weak lensing data
- SPOKES: an End-to-End Simulation Facility for Spectroscopic Cosmological Surveys
- Precision Calibration via Artificial Light Sources Above the Atmophere