Cosmic Complementarity: Joint Parameter Estimation from CMB Experiments and Redshift Surveys

Abstract

We study the ability of future CMB anisotropy experiments and redshift surveys to constrain a thirteen-dimensional parameterization of the adiabatic cold dark matter model. Each alone is unable to determine all parameters to high accuracy. However, considered together, one data set resolves the difficulties of the other, allowing certain degenerate parameters to be determined with far greater precision. We treat in detail the degeneracies involving the classical cosmological parameters, massive neutrinos, tensor-scalar ratio, bias, and reionization optical depth as well as how redshift surveys can resolve them. We discuss the opportunities for internal and external consistency checks on these measurements. Previous papers on parameter estimation have generally treated smaller parameter spaces; in direct comparisons to these works, we tend to find weaker constraints and suggest numerical explanations for the discrepancies.

Submitted to ApJ. LaTeX, 20 pages, emulateapj.sty and onecolfloat.sty. Minor errors in Table 8 corrected; reference added

References in corpus (27)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
• Baryonic Features in the Matter Transfer Function
• Power Spectra for Cold Dark Matter and its Variants
• Supernova Limits on the Cosmic Equation of State
• Weighing Neutrinos with Galaxy Surveys
• Structure Formation with Generalized Dark Matter
• Cosmic Confusion: Degeneracies among Cosmological Parameters Derived from Measurements of Microwave Background Anisotropies
• Semi-analytic modelling of galaxy evolution in the IR/submm range
• Cosmic Complementarity: H_0 and Omega_m from Combining CMB Experiments and Redshift Surveys
• Extragalactic Source Counts and Contributions to the Anisotropies of the Cosmic Microwave Background. Predictions for the Planck Surveyor mission
• Foreground separation methods for satellite observations of the cosmic microwave background
• Resolving the Cosmological Missing Energy Problem
• Extracting Primordial Density Fluctuations
• Constraints on the Effects of Locally-biased Galaxy Formation
• An Efficient Technique to Determine the Power Spectrum from Cosmic Microwave Background Sky Maps
• The Cosmic Microwave Background and Observational Convergence in the Omega_m - Omega_lambda Plane
• Removing point sources from CMB maps
• Do nuclear starbursts obscure the X-ray background?
• Cosmology in the Next Millennium: Combining MAP and SDSS Data to Constrain Inflationary Models
• Observationally Determining the Properties of Dark Matter
• Large Angular Scale Polarization of the Cosmic Microwave Background and the Feasibility of its Detection
• Small Scale Perturbations in a General MDM Cosmology
• Radio Sources in Galaxy Clusters at 28.5 GHz
• Gravitational lensing of cosmic microwave background anisotropies and cosmological parameter estimation
• Removing real-world foregrounds from CMB maps
• The Hubble Space Telescope Key Project to Measure the Hubble Constant

Cited by in corpus (267)

• Cosmological parameters from SDSS and WMAP
• The 3D power spectrum of galaxies from the SDSS
• Cosmological Constraints from the SDSS Luminous Red Galaxies
• In the Beginning: The First Sources of Light and the Reionization of the Universe
• 21-cm cosmology
• Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
• Cosmic Microwave Background Anisotropies
• Intrinsic alignment-lensing interference as a contaminant of cosmic shear
• Precision Determination of the Mass Function of Dark Matter Halos
• Probing the dark energy: methods and strategies
• micrOMEGAs: Version 1.3
• How exactly did the Universe become neutral?
• Power Spectrum Tomography with Weak Lensing
• Cosmological parameters from lensing power spectrum and bispectrum tomography
• The Clustering of Luminous Red Galaxies in the Sloan Digital Sky Survey Imaging Data
• The Reionization of the Universe by the First Stars and Quasars
• Foregrounds and Forecasts for the Cosmic Microwave Background
• Uncorrelated Modes of the Nonlinear Power Spectrum
• Improved forecasts for the baryon acoustic oscillations and cosmological distance scale
• Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and Three-Year Wilkinson Microwave Anisotropy Probe Observations
• The shape of the SDSS DR5 galaxy power spectrum
• Cosmology and the Bispectrum
• Joint Galaxy-Lensing Observables and the Dark Energy
• Probing Planckian physics: resonant production of particles during inflation and features in the primordial power spectrum
• Power Spectrum Correlations Induced by Non-Linear Clustering
• Probing cosmological parameters with the CMB: Forecasts from full Monte Carlo simulations
• Weak Lensing and Dark Energy
• Toward a Measurement of the Cosmological Geometry at z~2: Predicting Lyman-alpha Forest Correlation in Three Dimensions, and the Potential of Future Data Sets
• The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z=0.6
• The Baryonic Acoustic Feature and Large-Scale Clustering in the SDSS LRG Sample
• Redshifting Rings of Power
• Dark Synergy: Gravitational Lensing and the CMB
• Constraints on Omega_m, Omega_L, and Sigma_8, from Galaxy Cluster Redshift Distributions
• Determining Neutrino Mass from the CMB Alone
• What does inflation really predict?
• Reconstruction of the deceleration parameter and the equation of state of dark energy
• Large-Scale Anisotropic Correlation Function of SDSS Luminous Red Galaxies
• Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy
• The Impact of Non-Gaussian Errors on Weak Lensing Surveys
• Power spectrum normalization from the local abundance of rich clusters of galaxies
• Lensing Reconstruction with CMB Temperature and Polarization
• Constraining the unexplored period between reionization and the dark ages with observations of the global 21 cm signal
• Heating and Ionization of the Intergalactic Medium by an Early X-Ray Background
• Constraints on Warm Dark Matter from Cosmological Reionization
• How many dark energy parameters?
• Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies
• Is cosmology consistent?
• The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts
• Inflation and the Scale Dependent Spectral Index: Prospects and Strategies
• How to measure CMB polarization power spectra without losing information
• Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications
• Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest
• Probing the Reionization History of the Universe using the Cosmic Microwave Background Polarization
• Probing neutrino masses with CMB lensing extraction
• The Case for an Accelerating Universe from Supernovae
• Dark Energy and Matter Evolution from Lensing Tomography
• Cosmology with photometric redshift surveys
• Flux-averaging Analysis of Type Ia Supernova Data
• Probing neutrino masses with future galaxy redshift surveys
• Current cosmological bounds on neutrino masses and relativistic relics
• Probing dark energy with cluster counts and cosmic shear power spectra: including the full covariance
• Current cosmological constraints from a 10 parameter CMB analysis
• A Sudden Gravitational Transition
• Inflation, cold dark matter, and the central density problem
• CMB temperature and polarisation pseudo-Cl estimators and covariances
• The Age of the Universe and the Cosmological Constant Determined from Cosmic Microwave Background Anisotropy Measurements
• Information content of the non-linear matter power spectrum
• Tomography of lensing cross power spectra
• Constraining Neutrino Masses by CMB Experiments Alone
• Can luminosity distance measurements probe the equation of state of dark energy
• The impacts of dark matter particle annihilation on recombination and the anisotropies of the cosmic microwave background
• Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation
• Future Galaxy Cluster Surveys: The Effect of Theory Uncertainty on Constraining Cosmological Parameters
• Testing the Warm Dark Matter paradigm with large-scale structures
• Redshift space bias and beta from the halo model
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Prospects for determination of thermal history after inflation with future gravitational wave detectors
• Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
• Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test
• Probing Early Structure Formation with Far-Infrared Background Correlations
• Cosmological Information from Lensed CMB Power Spectra
• Measuring Time-Dependence of Dark Energy Density from Type Ia Supernova Data
• Cosmological implications of a Relic Neutrino Asymmetry
• Dark Energy Tomography
• CMB Polarization can constrain cosmology better than CMB temperature
• Voids as a Precision Probe of Dark Energy
• Improving measurements of H(z) and Da(z) by analyzing clustering anisotropies
• Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
• The 2dF Galaxy Redshift Survey: Wiener Reconstruction of the Cosmic Web
• Why multi-tracer surveys beat cosmic variance
• Foreground Model and Antenna Calibration Errors in the Measurement of the Sky-Averaged λ21 cm Signal at z~20
• Halo-model signatures from 380,000 SDSS Luminous Red Galaxies with photometric redshifts
• Measuring the metric: a parametrized post-Friedmanian approach to the cosmic dark energy problem
• A comparison of cosmological Boltzmann codes: are we ready for high precision cosmology?
• Future CMB tests of dark matter: ultra-light axions and massive neutrinos
• Weighing Neutrinos with Galaxy Cluster Surveys
• Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
• The Real Space Power Spectrum of the PSCz Survey from 0.01 to 300 h/Mpc
• Observational evidence for stochastic biasing
• Neutrino Mass Spectrum and Future Beta Decay Experiments
• The Angular Power Spectrum of Galaxies from Early SDSS Data
• Probing primordial features with future galaxy surveys
• Probing Dark Energy with Supernovae: Exploiting Complementarity with the Cosmic Microwave Background
• Cosmological constraints from current CMB and SN 1a data: a brute force 8 parameter analysis
• A parametrization of the growth index of matter perturbations in various Dark Energy models and observational prospects using a Euclid-like survey
• The integrated Sachs-Wolfe Effect -- Large Scale Structure Correlation
• Non-linear Integrated Sachs-Wolfe Effect
• Formulae for Growth Factors In Expanding Universes Containing Matter and a Cosmological Constant
• Falsifying Paradigms for Cosmic Acceleration
• Primeval Corrections to the CMB Anisotropies
• Correlations in the Spatial Power Spectrum Inferred from Angular Clustering: Methods and Application to APM
• Measuring Angular Diameter Distances through Halo Clustering
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• Axion constraints in non-standard thermal histories
• Characterizing the Peak in the CMB Angular Power Spectrum
• The Case for Omega_M = 0.33 +/- 0.035
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• Model-independent constraints on the cosmological anisotropic stress
• What can the observation of nonzero curvature tell us?
• Constraining the helium abundance with CMB
• Non-Gaussian Aspects of Thermal and Kinetic Sunyaev-Zel'dovich Effects
• Contributions to the Power Spectrum of Cosmic Microwave Background from Fluctuations Caused by Clusters of Galaxies
• Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume
• New constraints on neutrino physics from Boomerang data
• CMB Observations and the Production of Chemical Elements at the End of the Dark Ages
• The last stand before MAP: cosmological parameters from lensing, CMB and galaxy clustering
• Precision cosmology with a wide area XMM cluster survey
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• Maximum Likelihood Estimates of the Two- and Three-Dimensional Power Spectra of the APM Galaxy Survey
• Introduction to Microwave Background Polarization
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• Can a galaxy redshift survey measure dark energy clustering?
• Weak Lensing of the CMB: Extraction of Lensing Information from the Trispectrum
• Gravitational Time Delay Effects on CMB Anisotropies
• Dark Energy Constraints from Baryon Acoustic Oscillations
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• Kinetic Sunyaev-Zel'dovich effect from halo rotation
• The cosmological information of shear peaks: beyond the abundance
• Reconstructing the inflationary power spectrum from CMBR data
• Optimized detection of shear peaks in weak lensing maps
• Probing the neutrino mass hierarchy with CMB weak lensing
• The road ahead of Horndeski: cosmology of surviving scalar-tensor theories
• The Hubble Constant and the Expansion Age of the Universe
• Bayesian `Hyper-Parameters' Approach to Joint Estimation: The Hubble Constant from CMB Measurements
• Prospects for Constraining Neutrino Mass Using Planck and Lyman-Alpha Forest Data
• Weak Lensing and CMB: Parameter forecasts including a running spectral index
• Characterising the Primordial Cosmic Perturbations
• Cross-correlation between cosmic microwave background lensing and galaxy intrinsic alignment as a contaminant to gravitational lensing cross-correlated probes of the universe
• Fourier analysis of multi-tracer cosmological surveys
• Constraining interacting dark energy with CMB and BAO future surveys
• Squared temperature-temperature power spectrum as a probe of the CMB bispectrum
• Cosmic Inversion: Reconstructing primordial spectrum from CMB anisotropy
• What can be learned from the lensed cosmic microwave background B-mode polarization power spectrum?
• Structure Formation in Modified Gravity Scenarios
• Likelihood methods for the combined analysis of CMB temperature and polarisation power spectra
• Cosmological parameters after WMAP5: forecasts for Planck and future galaxy surveys
• Lensing Corrections to Features in the Angular Two-Point Correlation Function and Power Spectrum
• Cosmological parameters from cluster abundances, CMB and IRAS
• Reconstructing the radial profiles of gas density and temperature in clusters of galaxies from high-resolution X-ray and radio observations
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• Stochastic optimization methods for extracting cosmological parameters from CMBR power spectra
• Measuring primordial non-Gaussianity with weak-lensing surveys
• Constraining the initial conditions of the Universe using large scale structure
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• Revisiting the Constraint on the Helium Abundance from CMB
• Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data
• Detectability of Microwave Background Polarization
• The full Fisher matrix for galaxy surveys
• Constraining Inflation
• Baryogenesis and Gravitino Dark Matter in Gauge-Mediated Supersymmetry-Breaking Models
• A ring accelerator? Unusual jet dynamics in the IceCube candidate PKS 1502+106
• Umbrella sampling: a powerful method to sample tails of distributions
• Probing Primordial Magnetism with Off-Diagonal Correlators of CMB Polarization
• Cosmological Implications of Neutrinos
• Precision cosmology in muddy waters: Cosmological constraints and N-body codes
• Approximate Analytic Spectra of Reionized CMB Anisotropies and Polarization generated by Relic Gravitational Waves
• Self-Calibration for 3-point Intrinsic Alignment Auto-Correlations in Weak Lensing Surveys
• Disentangling Dark Physics with Cosmic Microwave Background Experiments
• Self-Calibration Technique for 3-point Intrinsic Alignment Correlations in Weak Lensing Surveys
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• How sound are our ultra-light axion approximations?
• Exploring Large-scale Structure with Billions of Galaxies
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Galaxy surveys, inhomogeneous reionization, and dark energy
• J-PAS: forecasts on dark energy and modified gravity theories
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• 3D Weak Gravitational Lensing of the CMB and Galaxies
• The information content of cosmic microwave background anisotropies
• Determining neutrino properties using future galaxy redshift surveys
• Optimal Binning of the Primordial Power Spectrum
• Effects of halo substructure on the power spectrum and bispectrum
• Constraints on Inflation
• Constraining the Variation of G by Cosmic Microwave Background Anisotropies
• Relic gravitational waves: latest revisions and preparations for new data
• Impact of Uncertainties in the Cosmological Parameters on the Measurement of Primordial non-Gaussianity
• K-mouflage Imprints on Cosmological Observables and Data Constraints
• What do cluster counts really tell us about the Universe?
• Non-Gaussian Covariance of CMB B-modes of Polarization and Parameter Degradation
• The large-scale polarization of the microwave background and foreground
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• The power spectrum of the CfA/SSRS UZC galaxy redshift survey
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Color Tomography
• Detecting relic gravitational waves in the CMB: Comparison of different methods
• A Beginner's Guide to the Theory of CMB Temperature and Polarization Power Spectra in the Line-of-Sight Formalism
• Weak Lensing of the CMB: Power Spectrum Covariance
• Constraints on Neutrino Mixing Parameters By Observation of Neutrinoless Double Beta Decay
• Late time sky as a probe of steps and oscillations in primordial Universe
• Cosmological measurement of neutrino mass in the presence of leptonic asymmetry
• Dark energy, curvature, and cosmic coincidence
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• Testing cosmological models and understanding cosmological parameter determinations with metaparameters
• Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy
• Neutrinos and dark energy constraints from future galaxy surveys and CMB lensing information
• The Optical Depth to Reionization as a Probe of Cosmological and Astrophysical Parameters
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• Future CMB ISW-Lensing bispectrum constraints on modified gravity in the Parameterized Post-Friedmann formalism
• Small-Scale Cosmic Microwave Background Polarization from Reionization
• Observational Tests of FRW World Models
• Mutual Constraints Between Reionization Models and Parameter Extraction From Cosmic Microwave Background Data
• On the degree of scale invariance of inflationary perturbations
• Cosmological constraints on sterile neutrino oscillations from Planck
• Probing a panoply of curvaton-decay scenarios using CMB data
• Predicted Constraints on Cosmic String Tension from Planck and Future CMB Polarization Measurements
• ECLIPSE: a fast Quadratic Maximum Likelihood estimator for CMB intensity and polarization power spectra
• Dimensionless cosmology
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• CMB-Normalized Predictions for Sunyaev-Zel'dovich effect fluctuations
• Eccentricity Evolution in Simulated Galaxy Clusters
• The role of $T_0$ in CMB anisotropy measurements
• Sunyaev-Zel'dovich power spectrum with decaying cold dark matter
• Reionization Constraints on the Contribution of Primordial Compact Objects to Dark Matter
• Cosmological constraints from a 2D SZ catalog
• A study on the Clustering Properties of Radio-Selected sources in the Lockman Hole Region at 325 MHz
• Probing Neutrinos from Planck and Forthcoming Galaxy Redshift Surveys
• On the coupling between different species during recombination
• Constraining the mass-concentration relation through weak lensing peak function
• `Hyper Parameters' Approach to Joint Estimation: Applications to Cepheid-Calibrated Distances and X-Ray Clusters
• Detectable Data-driven Features in the Primordial Scalar Power Spectrum
• Cosmological parameter determination from Planck and SDSS data in LambdaCHDM cosmologies
• Impact of a Warm Dark Matter late-time velocity dispersion on large-scale structures
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• The Fisher gAlaxy suRvey cOde ($\text{FARO}$)
• Constraints on cosmic birefringence using $E$-mode polarisation
• Cosmic opacity to CMB photons and polarization measurements
• Applications of High Resolution High Sensitivity Observations of the CMB
• The Effects of Relativistic Corrections on Cosmological Parameter Estimations from SZE Cluster Surveys
• Constraining the reionization history with large angle CMB polarization
• On the Determination of Neutrino Masses and Dark Energy Evolution from the Cross Correlation of CMB and LSS
• Accurate method for ultralight axion CMB and matter power spectra
• Simulated Versus Observed Cluster Eccentricity Evolution
• Overconstrained dynamics in galaxy redshift surveys
• Nonparametric Forecasts of the CMB Angular Power Spectra for the Planck Mission
• Measuring lensing ratios with future cosmological surveys
• Sterile Neutrinos in astrophysical and cosmological sauce
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Estimators for the cross-pairwise kSZ effect: forecasts for the dark energy and modified gravity parameters with Simons Observatory and CMB-S4
• Analytic expressions for the background evolution of massive neutrinos and dark matter particles
• Cosmological Constraints on Radion Evolution in the Universal Extra Dimension Model
• CMB Constraint on Radion Evolution in the Brane World Scenario
• Massive black hole binaries in LISA: constraining cosmological parameters at high redshifts
• Forecasting isocurvature models with CMB lensing information: axion and curvaton scenarios
• Cosmic Microwave Background: Past, Future, and Present