Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys

Abstract

We show that the measurement of the baryonic acoustic oscillations in large high redshift galaxy surveys offers a precision route to the measurement of dark energy. The cosmic microwave background provides the scale of the oscillations as a standard ruler that can be measured in the clustering of galaxies, thereby yielding the Hubble parameter and angular diameter distance as a function of redshift. This, in turn, enables one to probe dark energy. We use a Fisher matrix formalism to study the statistical errors for redshift surveys up to z=3 and report errors on cosmography while marginalizing over a large number of cosmological parameters including a time-dependent equation of state. With redshifts surveys combined with cosmic microwave background satellite data, we achieve errors of 0.037 on Omega_x, 0.10 on w(z=0.8), and 0.28 on dw(z)/dz for cosmological constant model. Models with less negative w(z) permit tighter constraints. We test and discuss the dependence of performance on redshift, survey conditions, and fiducial model. We find results that are competitive with the performance of future supernovae Ia surveys. We conclude that redshift surveys offer a promising independent route to the measurement of dark energy.

submitted to ApJ, 24 pages, LaTeX

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• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• A conventional approach to the dark-energy concept
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• A tachyonic scalar field with mutually interacting components
• Effects of Linear Redshift Space Distortions and Perturbation Theory on BAOs: A 3D Spherical Analysis
• Designer Cosmology
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• Topology of large scale structure as test of modified gravity
• Dark sectors of the Universe: A Euclid survey approach
• Quantifying the accuracy of the Alcock-Paczynski scaling of baryon acoustic oscillation measurements
• Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure
• Multi-tracer power spectra and bispectra: Formalism
• Consistency of LCDM with Geometric and Dynamical Probes
• Improving Fisher matrix forecasts for galaxy surveys: window function, bin cross-correlation, and bin redshift uncertainty
• Vacuum energy as dark matter
• Cosmological Constant and Local Gravity
• Imprints of deviations from the gravitational inverse-square law on the power spectrum of mass fluctuations
• Measuring the Hubble function with standard candle clustering
• On measuring the absolute scale of baryon acoustic oscillations
• 21 cm Intensity Mapping
• Testing extended Jordan-Brans-Dicke theories with future cosmological observations
• Cosmology from clustering of Lyman-alpha galaxies: breaking non-gravitational Lyman-alpha radiative transfer degeneracies using the bispectrum
• Weak Lensing of Baryon Acoustic Oscillations
• Characterizing unknown systematics in large scale structure surveys
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• Robust constraints on dark energy and gravity from galaxy clustering data
• Can $f(R)$ gravity relieve $H_0$ and ${\sigma }_8$ tensions?
• Model-Independent Measurements of Cosmic Expansion and Growth at z=0.57 Using the Anisotropic Clustering of CMASS Galaxies From the Sloan Digital Sky Survey Data Release 9
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Eigenmode Analysis of Galaxy Distributions in Redshift Space
• Dark Energy: The Observational Challenge
• Discrimination between Lambda-CDM, quintessence, and modified gravity models using wide area surveys
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Neutrinos and dark energy constraints from future galaxy surveys and CMB lensing information
• Combining spectroscopic and photometric surveys using angular cross-correlations II: Parameter constraints from different physical effects
• Constraints on dark energy models from radial baryon acoustic scale measurements
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• Probing the constancy of the speed of light with future galaxy survey: the case of SKA and Euclid
• Dilaton dominance in the early Universe dilutes Dark Matter relic abundances
• Primordial Power Spectrum features and $f_{NL}$ constraints
• Biases on cosmological parameters by general relativity effects
• The 6x2pt method: supernova velocities meet multiple tracers
• Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
• Constraining Cosmic Expansion and Gravity with Galaxy Redshift Surveys
• Combined constraints on deviations of dark energy from an ideal fluid from Euclid and Planck
• Forecasting neutrino masses from galaxy clustering in the Dark Energy Survey combined with the Planck Measurements
• Constraints on a scale-dependent bias from galaxy clustering
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• Large Scale Structure Forecast Constraints on Particle Production During Inflation
• Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
• Direct cosmological inference from three-dimensional correlations of the Lyman-$\alpha$ forest
• Measuring the Homogeneity of the Universe Using Polarization Drift
• Clustering with general photo-$z$ uncertainties: Application to Baryon Acoustic Oscillations
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Validating the Fisher approach for stage IV spectroscopic surveys
• On the amount of peculiar velocity field information in supernovae from LSST and beyond
• HIR4: cosmology from a simulated neutral hydrogen full sky using Horizon Run 4
• Bispectrum as Baryon Acoustic Oscillation Interferometer
• Path Integral Marginalization for Cosmology: Scale Dependent Galaxy Bias & Intrinsic Alignments
• Detecting Baryon Acoustic Oscillations
• Broadband Alcock-Paczynski test exploiting redshift distortions
• The D-material universe
• Cosmological Information Contents on the Light-Cone
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Delayed Recombination and Standard Rulers
• Cosmology with an Effective $\Lambda$-Term in Lyra Manifold
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• Spectro-Imaging Forward Model of Red and Blue Galaxies
• Emergent Universe in the Braneworld Scenario
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Recovering a redshift-extended VSL signal from galaxy surveys
• Distance Probes of Dark Energy
• An effective theory of accelerated expansion
• Understanding the Reconstruction of the Biased Tracer
• Searching for blue in the dark
• Describing variations of the Fisher-matrix across parameter space
• Constraints on Dark Energy Models Using Late Universe Probes
• Constraining Cosmic Inflation with Observations: Prospects for 2030
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• Measuring Baryon Acoustic Oscillations with Millions of Supernovae
• Is there a standard measuring rod in the Universe?
• Probing violation of the Copernican principle via the integrated Sachs-Wolfe effect
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• Fundamental Uncertainty in the BAO Scale from Isocurvature Modes
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• Geometric and dynamic distortions in anisotropic galaxy clustering
• Probing Dark Energy with the Kunlun Dark Universe Survey Telescope
• Parametrization for the Scale Dependent Growth in Modified Gravity
• Evolution of Spherical Overdensity in Thawing Dark energy Models
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
• Prospects in Constraining the Dark Energy Potential
• Fast calculation of the Fisher matrix for cosmic microwave background experiments
• Predictions for BAO distance estimates from the cross-correlation of the Lyman-alpha forest and redshifted 21-cm emission
• Redshift space distortions in the presence of non-minimally coupled dark matter
• Implications of JLA data for $k-$essence model of dark energy with given equation of state
• Detecting baryon acoustic oscillations by 3d weak lensing
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Fisher matrix for multiple tracers: model independent constraints on the redshift distortion parameter
• Cosmological Model of Interacting Tachyon Field
• Emergent Cosmos in Einstein-Cartan Theory
• The role of $T_0$ in CMB anisotropy measurements
• The sensitivity of BAO Dark Energy Constraints to General Isocurvature Perturbations
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• Forecasts on neutrino mass constraints from the redshift-space two-point correlation function
• ProtoDESI: First On-Sky Technology Demonstration for the Dark Energy Spectroscopic Instrument
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Locating the Baryon Acoustic Peak
• Dilaton dominance relaxes LHC and cosmological constraints in supersymmetric models
• Probing Neutrinos from Planck and Forthcoming Galaxy Redshift Surveys
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Skewness as a probe of Baryon Acoustic Oscillations
• Non-Gaussian error bars in galaxy surveys -- II
• An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• Coherent Combination of Baryon Acoustic Oscillation Statistics and Peculiar Velocity Measurements from Redshift Survey
• Neutrino Masses, Scale-Dependent Growth, and Redshift-Space Distortions
• Gravitational Lensing Effects on the Baryonic Acoustic Oscillation Signature in the Redshift-Space Correlation Function
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Parametrizing growth in dark energy and modified gravity models
• A potentially pure test of cosmic geometry: galaxy clusters and the real space Alcock-Paczynski test
• Compact objects and the swampland
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• Perturbations in Tachyon Dark Energy and their Effect on Matter Clustering
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Large-Distance Lens Uncertainties and Time-Delay Measurements of $H_0$
• Cosmological test of local position invariance from the asymmetric galaxy clustering
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Detecting galaxy-21-cm cross-correlation during reionization
• Cosmological implications of different baryon acoustic oscillation data
• Simultaneous constraints on bias, normalization and growth index through power spectrum measurements
• An Evolving Entropy Floor in the Intracluster Gas?
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• The Alcock Paczynski test with 21cm intensity field
• Study on the mapping of halo clustering from real space to redshift space
• Uncalibrated Cosmic Standards as a Robust Test on Late-Time Cosmological Models
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• Cosmological Models with a Varying $\Lambda$ -Term in Lyra's Geometry
• Cosmological Leverage from the Matter Power Spectrum in the Presence of Baryon and Nonlinear Effects
• Unveiling the Universe with Emerging Cosmological Probes
• A forecast for the detection of the power asymmetry from galaxy surveys
• Power Spectrum Precision for Redshift Space Distortions
• Cosmology at high redshift -- a probe of fundamental physics
• Representation learning for automated spectroscopic redshift estimation
• Local measurement of Λ using pulsar timing arrays
• Beyond the Standard Model of Physics with Astronomical Observations
• The evolution of Luminous Red Galaxies in the Sloan Digital Sky Survey 7th data release
• Model-Independent Dark Energy Measurements from DESI DR2 and Planck 2015 Data
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys
• Complementarity of Future Dark Energy Probes
• Improved Cosmological Parameter Constraints from CMB and H(z) Data
• Baryon acoustic oscillations with the cross-correlation of spectroscopic and photometric samples
• A proposal to improve the accuracy of cosmological observables and address the Hubble tension problem
• Dark Energy with a Fine-toothed Comb
• Gravitational Wave Detection Using Redshifted 21-cm Observations
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Deep learning for cosmological parameter inference from a dark matter halo density field
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Squeezing Full-Shape Dynamical Dark Energy Constraints with Galaxy Alignments
• Survey design for Spectral Energy Distribution fitting: a Fisher Matrix approach
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• Measurement of the baryonic acoustic oscillation scale in 21 cm intensity fluctuations during the reionisation era
• Power Spectrum Analysis of the 2dF QSO Sample Revisited
• On the propagation of gravitational waves in a $\Lambda$CDM universe
• Optimizing BAO measurements with non-linear transformations of Lyman-alpha forest
• Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Constraining primordial non-Gaussianity by combining photometric galaxy and 21cm intensity mapping surveys
• Bias-Limited Extraction of Cosmological Parameters
• Information content in anisotropic cosmological fields: Impact of different multipole expansion scheme for galaxy density and ellipticity correlations
• Optimizing the Recovery of Fisher Information in the Dark Matter Power Spectrum
• On the origin of the BAOtr-DESI tension
• Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys
• Non-Linearity-Free prediction of the growth-rate $f{\sigma }_8$ using Convolutional Neural Networks
• Measuring $H_0$ with pulsar timing arrays
• The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
• Experimental evaluation of complete safe coordination of astrobots for Sloan Digital Sky Survey V
• Reconstructing the Cosmic Expansion History with a Monotonicity Prior
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Testing for gravitational preferred directions with galaxy and lensing surveys
• Illuminating the dark universe with a very high density galaxy redshift survey over a wide area
• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• The expansion of the universe observed with supernovae
• Angular Diameter Distance Measurement with Galaxy Clustering in the Multipole Space
• Cosmological constraints from galaxy multi-tracers in the nearby Universe
• Squeezing information from radio surveys to probe the primordial Universe
• Photo-z optimization for measurements of the BAO radial direction
• Cosmological Constraints on Neutrino Masses in a Second-Order CPL Dark Energy Model
• A cosmic speed-trap: a gravity-independent test of cosmic acceleration using baryon acoustic oscillations
• Direct Determination of Expansion History Using Redshift Distortions
• Constraint on the growth factor of the cosmic structure from the damping of the baryon acoustic oscillation signature
• Constraining cosmology with N-body simulations for future spectroscopic galaxy surveys at $2\le z\le 3$
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Cosmology with Type II Supernovae
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• Observational signatures of dark energy produced in an ancestor vacuum: Forecast for galaxy surveys
• Accelerating BAO Scale Fitting Using Taylor Series
• Comparing LambdaCDM, wCDM, and w0waCDM models with DESI DR2 BAO: Redshift-Resolved Diagnostics and the Role of rd
• Fluids in cosmology
• Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Probing Interacting Dark Sectors with upcoming Post-Reionization and Galaxy Surveys
• Cosmology of Cubic Poincaré Gauge gravity
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• Investigating the Constraints on Primordial Features with Future Cosmic Microwave Background and Galaxy Surveys
• Iterative reconstruction excursions for Baryon Acoustic Oscillations and beyond
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Cosmological constraints from the density gradient weighted correlation function
• Multivariate analysis of cosmic void characteristics
• J-PAS: forecast on the primordial power spectrum reconstruction
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Constraining effective neutrino species with bispectrum of large scale structures
• Effect of the cosmological parameters on gravitational waves: general analysis
• VADER - A Satellite Mission Concept For High Precision Dark Energy Studies
• Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space
• Can accelerated expansion of the universe be due to spacetime vorticity?