Constraining dark energy with Sunyaev-Zel'dovich cluster surveys
arXiv:astro-ph/0110353 · doi:10.1103/PhysRevLett.88.231301
Abstract
We discuss the prospects of constraining the properties of a dark energy component, with particular reference to a time varying equation of state, using future cluster surveys selected by their Sunyaev-Zel'dovich effect. We compute the number of clusters expected for a given set of cosmological parameters and propogate the errors expected from a variety of surveys. In the short term they will constrain dark energy in conjunction with future observations of type Ia supernovae, but may in time do so in their own right.
5 pages, 3 figures, 1 table, version accepted for publication in PRL
References in corpus (21)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- Cosmology and the Fate of Dilatation Symmetry
- Mass function of dark matter halos
- Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
- Using the Evolution of Clusters to Constrain Omega
- Cluster Abundance Constraints on Quintessence Models
- The Sunyaev-Zel'dovich Effect
- Prospects for probing the dark energy via supernova distance measurements
- Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys
- Quintessence and Supergravity
- The Most Massive Distant Clusters: Determining Omega and sigma_8
- The Cluster Abundance in Flat and Open Cosmologies
- Constraints on Omega_m, Omega_L, and Sigma_8, from Galaxy Cluster Redshift Distributions
- Limitations in using luminosity distance to determine the equation of state of the universe
- Power spectrum normalization from the local abundance of rich clusters of galaxies
- Opportunities for future supernova studies of cosmic acceleration
- Can luminosity distance measurements probe the equation of state of dark energy
- Expectations For an Interferometric Sunyaev-Zel'dovich Effect Survey for Galaxy Clusters
- Surveying the Sky with the Arcminute MicroKelvin Imager: Expected Constraints on Galaxy Cluster Evolution and Cosmology
Cited by in corpus (81)
- Toward a halo mass function for precision cosmology: the limits of universality
- Tracing cosmic evolution with clusters of galaxies
- Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts
- Euclid. I. Overview of the Euclid mission
- Sample Variance Considerations for Cluster Surveys
- Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample
- The halo mass function through the cosmic ages
- Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
- On the spherical collapse model in dark energy cosmologies
- Self Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum and Mass Measurements
- Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
- The Impact of Galaxy Formation on the Sunyaev-Zeldovich Effect of Galaxy Clusters
- Cosmology with the shear-peak statistics
- New constraints on dark energy from the observed growth of the most X-ray luminous galaxy clusters
- Importance of Cluster Structural Evolution in Using X-ray and SZE Galaxy Cluster Surveys to Study Dark Energy
- Constraining cosmological parameters using Sunyaev-Zel'dovich cluster surveys
- Probing Cosmology with Weak Lensing Peak Counts
- Cosmological Constraints from the Red-Sequence Cluster Survey
- Simultaneous Falsification of LCDM and Quintessence with Massive, Distant Clusters
- Probing dark energy with cluster counts and cosmic shear power spectra: including the full covariance
- Scaling Relations from Sunyaev-Zel'dovich Effect and Chandra X-ray measurements of high-redshift galaxy clusters
- Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
- Self-Consistency and Calibration of Cluster Number Count Surveys for Dark Energy
- Halo properties in models with dynamical Dark Energy
- Secondary anisotropies of the CMB
- Application of a Self-Similar Pressure Profile to Sunyaev-Zel'dovich Effect Data from Galaxy Clusters
- Constraining the Dark Energy Equation of State with Cosmic Voids
- The Atacama Cosmology Telescope Project: A Progress Report
- Cosmology with the Square Kilometre Array
- Precision cosmology with a wide area XMM cluster survey
- The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
- The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect
- Measuring cluster peculiar velocities with the Sunyaev-Zeldovich effects: scaling relations and systematics
- Bayesian joint analysis of cluster weak lensing and Sunyaev-Zel'dovich effect data
- Weak lensing analysis of RXC J2248.7-4431
- The Impact of Halo Properties, Energy Feedback and Projection Effects on the Mass-SZ Flux Relation
- Dark energy constraints from lensing-detected galaxy clusters
- Point sources in the context of future SZ surveys
- A high precision semi-analytic mass function
- Accurate Realizations of the Ionized Gas in Galaxy Clusters: Calibrating Feedback
- Microwave-Sky Simulations and Projections for Galaxy Cluster Detection with the Atacama Cosmology Telescope
- Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data
- On the implementation of the spherical collapse model for dark energy models
- The signature of dark energy perturbations in galaxy cluster surveys
- Number counts in homogeneous and inhomogeneous dark energy models
- Constraining Dark Energy Evolution with Gravitational Lensing by Large Scale Structures
- Cluster scaling relations from cosmological hydrodynamic simulations in dark energy dominated universe
- The most massive objects in the Universe
- Merging Galaxy Clusters: Offset Between the Sunyaev-Zel'dovich Effect and X-ray Peaks
- Galaxy Clustering and Dark Energy
- Apparent Clustering of Intermediate-redshift Galaxies as a Probe of Dark Energy
- Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey
- A Consistent Approach to Falsifying Lambda-CDM with Rare Galaxy Clusters
- Optimizing weak lensing mass estimates for cluster profile uncertainty
- Friends-of-Friends Groups and Clusters in the 2SLAQ Catalogue
- Constraints on the Energy Content of the Universe from a Combination of Galaxy Cluster Observables
- Optical & Sunyaev-Zel'dovich Observations of a New Sample of Distant Rich Galaxy Clusters in the ROSAT All Sky Survey
- Influence of Projection in Cluster Cosmology Studies
- The hybrid SZ power spectrum: Combining cluster counts and SZ fluctuations to probe gas physics
- Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
- Non-Gaussian Scatter in Cluster Scaling Relations
- Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
- Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
- Issues in joint SZ and optical cluster finding
- Precision cosmology with a combination of wide and deep Sunyaev-Zeldovich cluster surveys
- Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
- Dynamics of minimally coupled dark energy in spherical halos of dark matter
- Galaxy cluster scaling relations measured with APEX-SZ
- Constraining thawing and freezing models with cluster number counts
- Signatures of Light Massive Relics on nonlinear structure formation
- Using clusters in SZE + x-ray surveys as an ensemble of rulers to constrain cosmology
- Covariance of dark energy parameters and sound speed constraints from large HI surveys
- Cosmological constraints from a 2D SZ catalog
- An Evolving Entropy Floor in the Intracluster Gas?
- Stokes parameters spectral distortions due to the Sunyaev-Zel'dovich effect and an independent estimation of the CMB low multipoles
- Effects of tidal gravitational fields in clustering dark energy models
- Optimizing the yield of Sunyaev-Zel'dovich cluster surveys
- Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
- Polarization of the Sunyaev-Zel'dovich effect: relativistic imprint of thermal and non-thermal plasma
- Morphological Redshift Estimates for Galaxy Clusters in a Sunyaev-Zel'dovich Effect Survey
- Aemulus : Precision halo mass functions in wCDM cosmologies