Towards a refined cosmic concordance model: joint 11-parameter constraints from CMB and large-scale structure
arXiv:astro-ph/0008167 · doi:10.1103/PhysRevD.63.043007
Abstract
We present a method for calculating large numbers of power spectra C_l and P(k) that accelerates CMBfast by a factor around 10^3 without appreciable loss of accuracy, then apply it to constrain 11 cosmological parameters from current Cosmic Microwave Background (CMB) and Large Scale Structure (LSS) data. While the CMB alone still suffers from several degeneracies, allowing, e.g., closed models with strong tilt and tensor contributions, the shape of the real space power spectrum of galaxies from the IRAS Point Source Catalogue Redshift (PSCz) survey breaks these degeneracies and helps place strong constraints on most parameters. At 95% confidence, the combined CMB and LSS data imply a baryon density 0.020 < omega_b < 0.037, dark matter density 0.10 < omega_d < 0.32 with a neutrino fraction f_nu < 38%, vacuum density Omega_Lambda < 0.76, curvature -0.19 < Omega_k < 0.10, scalar tilt 0.86 < n_s < 1.16 and reionization optical depth tau < 0.44. These joint constraints are quite robust, changing little when we impose priors on the Hubble parameter, tilt, flatness, gravity waves or reionization. Adding nucleosynthesis and neutrino priors on the other hand tightens parameters considerably, requiring Omega_Lambda > 0.49 and a red-tilt. The analysis allows a number of consistency tests to be made, all of which pass. At the 95% level, the flat scalar ``concordance model'' with Omega_Lambda=0.62, omega_d=0.13, omega_b=0.02, f_nu~0, n_s=0.9, tau=0.1, h=0.63 is consistent with external constraints. The inferred PSCz bias b~1.2 agrees with the value estimated independently from redshift space distortions. The inferred cosmological constant value agrees with the one independently derived from SN 1a studies. Cosmology seems to be on the right track.
Replaced with accepted version. Improved accuracy, more refs; 15 pages, 13 figs. Power spectrum movies at http://www.hep.upenn.edu/~max/concordance.html or from [email protected]
References in corpus (14)
- The PSCz Catalogue
- Measuring Cosmological Parameters from the Evolution of Cluster X-ray Temperatures
- Current cosmological constraints from a 10 parameter CMB analysis
- New CMB constraints on the cosmic matter budget: trouble for nucleosynthesis?
- Non equilibrium spectra of degenerate relic neutrinos
- The Cosmic Microwave Background Radiation
- New Constraints on inflation from the Cosmic Microwave Background
- New constraints on neutrino physics from Boomerang data
- Testing Standard and Degenerate Big Bang Nucleosynthesis with BOOMERanG and MAXIMA-1
- The standard and degenerate primordial nucleosynthesis versus recent experimental data
- Remarks on the Boomerang results, the baryon density and the leptonic asymmetry
- A Younger Age for the Universe
- Decaying neutrino and a high cosmological baryon density
- The Optical Depth to Reionization as a Probe of Cosmological and Astrophysical Parameters
Cited by in corpus (101)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Cosmological parameters from SDSS and WMAP
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
- Cosmic Microwave Background Anisotropies
- Probing the dark energy: methods and strategies
- Cosmological Parameter Extraction from the First Season of Observations with DASI
- Evidence for a non-zero Lambda and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and Cosmic Microwave Background Anisotropies
- Cosmological implications of the MAXIMA-I high resolution Cosmic Microwave Background anisotropy measurement
- Supernovae, CMB, and Gravitational Leakage into Extra Dimensions
- Feedback from Galaxy Formation: Production and Photodissociation of Primordial Molecular Hydrogen
- The power spectrum of galaxies in the 2dF 100k redshift survey
- What Is The BBN Prediction for the Baryon Density and How Reliable Is It?
- Is cosmology consistent?
- How to measure CMB polarization power spectra without losing information
- CDM and Strong Lensing: Concord or Conflict?
- Separating the Early Universe from the Late Universe: cosmological parameter estimation beyond the black box
- Current constraints on the dark energy equation of state
- Constraining neutrino physics with BBN and CMBR
- Correlated perturbations from inflation and the cosmic microwave background
- The Age of the Universe and the Cosmological Constant Determined from Cosmic Microwave Background Anisotropy Measurements
- Friedmann cosmology with decaying vacuum density
- Redshift space bias and beta from the halo model
- Scaling Laws in the Distribution of Galaxies
- A late-time transition in the cosmic dark energy?
- Halo properties in models with dynamical Dark Energy
- Detection of cosmic filaments using the Candy model
- Measuring the metric: a parametrized post-Friedmanian approach to the cosmic dark energy problem
- The Real Space Power Spectrum of the PSCz Survey from 0.01 to 300 h/Mpc
- Evolving Spectra of Pop III Stars: Consequences for Cosmological Reionization
- Neutrino Mass Spectrum and Future Beta Decay Experiments
- Primordial Nucleosynthesis with CMB Inputs: Probing the Early Universe and Light Element Astrophysics
- On the APM power spectrum and the CMB anisotropy: Evidence for a phase transition during inflation?
- Probing the Friedmann equation during recombination with future CMB experiments
- Modeling Dynamical Dark Energy
- Reproducing Cosmic Microwave Background anisotropies with mixed isocurvature perturbations
- Scale Dependent Spectral Index in Slow Roll Inflation
- The last stand before MAP: cosmological parameters from lensing, CMB and galaxy clustering
- Right-Handed Sneutrinos as Curvatons
- Adventures in Friedmann Cosmology: An Educationally Detailed Expansion of the Cosmological Friedmann Equations
- Mass bounds for compact spherically symmetric objects in generalized gravity theories
- Update of the direct detection of dark matter and the role of the nuclear spin
- Possible Detection of Baryonic Fluctuations in the Large-Scale Structure Power Spectrum
- New CMBR data and the cosmic neutrino background
- Probing the power spectrum bend with recent CMB data
- Dynamics of Cosmological Perturbations in Position Space
- Holography and the large number hypothesis
- Position-Space Description of the Cosmic Microwave Background and Its Temperature Correlation Function
- Acoustic peaks and dips in the CMB power spectrum: observational data and cosmological constraints
- Model Independent Primordial Power Spectrum from Maxima, Boomerang, and DASI Data
- Dark Matter and Dark Energy from a single scalar field and CMB data
- Cluster Ellipticities as a Cosmological Probe
- Brane inflation driven by noncanonical scalar field
- Anisotropic cosmologies containing isotropic background radiation
- Computational Cosmology: from the Early Universe to the Large Scale Structure
- Constraints on Resonant Particle Production during Inflation from the Matter and CMB Power Spectra
- Principal Component Analysis of the Cosmic Microwave Background Anisotropies: Revealing The Tensor Degeneracy
- CMBfit: Rapid WMAP likelihood calculations with normal parameters
- On astrophysical bounds of the cosmological constant
- Physics with Supernovae
- Large Distance Modification of Newtonian Potential and Structure Formation in Universe
- Strong Gravitational Lensing and Dynamical Dark Energy
- How is the Reionization Epoch Defined?
- Light of Planck-2015 on Non-Canonical Inflation
- A framework for the next generation of stationary cosmological models
- Global fits for the spectral index of the cosmological curvature perturbation
- The minimum mass of a charged spherically symmetric object in dimensions, its implications for fundamental particles, and holography
- Cluster arc statistics
- Comparing and combining the Saskatoon, QMAP and COBE CMB maps
- Tracing the Nature of Dark Energy with Galaxy Distribution
- The CMB power spectrum at l=30-200 from QMASK
- The lepton asymmetry: the last chance for a critical-density cosmology?
- Reproducing the observed Cosmic microwave background anisotropies with causal scaling seeds
- Cosmological parameters from complementary observations of the Universe
- Mutual Constraints Between Reionization Models and Parameter Extraction From Cosmic Microwave Background Data
- Fast Parameter Estimation from the CMB Power Spectrum
- Constraining Cosmological Models by the Cluster Mass Function
- On the primordial helium content: CMB and stellar constraints
- Recent CMB Observations and the Ionization History of the Universe
- Expanding Universe and Dynamical Compactification Using Yang-Mills Instantons
- Inflationary scenarios with scale-invariant spectral tensorial index
- Local Supercluster Dynamics: External Tidal Impact of the PSCz sample traced by Optimized Numerical Least Action Method
- Searches for Particle Dark Matter: An Introduction
- Inflation with a constant ratio of scalar and tensor perturbation amplitudes
- The Pioneer anomaly and the holographic scenario
- Towards a quantum universe
- Implications to CMB from Model Independent evolution of w and Late Time Phase Transition
- The effect of reionization on the COBE normalization
- GUT, Neutrinos, and Baryogenesis
- Mapping the Cosmological Confidence Ball Surface
- Statistical evaluation of the observational information on and
- Role of Spatial Curvature in a Dark Energy Interacting Model
- Numerical Analysis of the Primordial Power Spectrum for (Small Field) Inflationary Potentials
- Power Spectrum Estimation II. Linear Maximum Likelihood
- The Effects of Spatial Curvature on Cosmic Evolution
- A robust assessment of the local anisotropy of the Hubble constant
- Cosmology from Large Scale Structure
- Has the density of sources of gamma-ray burts been constant over the last ten billion years ?
- Dark 2002 and Beyond