NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
2012/12/31 by G. Hinshaw, D. Larson, E. Komatsu +18 · 5,118 citations
Computer Science · Physics and Astronomy · #Amplitude #CMB cold spot #Computational Physics and Python Applications #Cosmic background radiation #Cosmic microwave background #Cosmology #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Hubble's law #Neutrino #Planck #Primordial fluctuations #astro-ph.CO
paper · pdf · doi:10.1088/0067-0049/208/2/19
published in The Astrophysical Journal Supplement Series 208(2), 19 (Institute of Physics) · 32 pages, 12 figures, v3: Version accepted to Astrophysical Journal Supplement Series. Includes improvements in response to referee and community; corrected 3 entries in Table 10, (w0 & wa model). See the Legacy Archive for Microwave Background Data Analysis (LAMBDA): http://lambda.gsfc.nasa.gov/product/map/current/ for further detail
arxiv created 2013/06/04 · openalex publication_date 2013/09/20 · arxiv updated 2015/06/12 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
Abstract
We present cosmological parameter constraints based on the final nine-year Wilkinson Microwave Anisotropy Probe ( WMAP ) data, in conjunction with a number of additional cosmological data sets. The WMAP data alone, and in combination, continue to be remarkably well fit by a six-parameter ΛCDM model. When WMAP data are combined with measurements of the high- l cosmic microwave background anisotropy, the baryon acoustic oscillation scale, and the Hubble constant, the matter and energy densities, Ω b h 2 , Ω c h 2 , and Ω Λ , are each determined to a precision of ∼1.5%. The amplitude of the primordial spectrum is measured to within 3%, and there is now evidence for a tilt in the primordial spectrum at the 5σ level, confirming the first detection of tilt based on the five-year WMAP data. At the end of the WMAP mission, the nine-year data decrease the allowable volume of the six-dimensional ΛCDM parameter space by a factor of 68,000 relative to pre- WMAP measurements. We investigate a number of data combinations and show that their ΛCDM parameter fits are consistent. New limits on deviations from the six-parameter model are presented, for example: the fractional contribution of tensor modes is limited to r < 0.13 (95% CL); the spatial curvature parameter is limited to ; the summed mass of neutrinos is limited to ∑ m ν < 0.44 eV (95% CL); and the number of relativistic species is found to lie within N eff = 3.84 ± 0.40, when the full data are analyzed. The joint constraint on N eff and the primordial helium abundance, Y He , agrees with the prediction of standard big bang nucleosynthesis. We compare recent Planck measurements of the Sunyaev–Zel'dovich effect with our seven-year measurements, and show their mutual agreement. Our analysis of the polarization pattern around temperature extrema is updated. This confirms a fundamental prediction of the standard cosmological model and provides a striking illustration of acoustic oscillations and adiabatic initial conditions in the early universe.
Citations
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- A bias in VLBI measurements of the core shift effect in AGN jets
- Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
- Constraints from high-precision measurements of the cosmic microwave background: the case of disintegrating dark matter with Λ or dynamical dark energy
- IDCS J1426.5+3508: WEAK LENSING ANALYSIS OF A MASSIVE GALAXY CLUSTER AT z = 1.75
- Parity-violating and anisotropic correlations in pseudoscalar inflation
- Measuring polarized emission in clusters in the CMB S4 era
- Search for the Effect of Massive Bodies on Atomic Spectra and Constraints on Yukawa-Type Interactions of Scalar Particles
- Observing the Dark Sector
- Detecting Intermediate-mass Black Holes Using Quasar Microlensing
- Constraining violations of the weak equivalence principle Using CHIME FRBs
- Z-portal dark matter
- Clustering, cosmology and a new era of black hole demographics– II. The conditional luminosity functions of Type 2 and Type 1 active galactic nuclei
- Clustering, cosmology and a new era of black hole demographics– I. The conditional luminosity function of active galactic nuclei
- The impact of photometric redshift errors on lensing statistics in ray-tracing simulations
- A Limit on the Warm Dark Matter Particle Mass from the Redshifted 21 cm Absorption Line
- Coupled scalar fields in the late Universe: the mechanical approach and the late cosmic acceleration
- The XXL Survey
- Understanding the muon anomalous magnetic moment in light of a flavor symmetry-based Minimal Supersymmetric Standard Model
- The simplest non-minimal matter–geometry coupling in the f(R, T) cosmology
- Baryon-Interacting Dark Matter: heating dark matter and the emergence of galaxy scaling relations
- Collider signatures of hylogenesis
- Redshift-space distortions in massive neutrino and evolving dark energy cosmologies
- C osmo++: An object-oriented C++ library for cosmology
- Scalar warm inflation in holographic cosmology
- Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel’dovich effect
- Universal upper bound on the inflationary energy scale from the trans-Planckian censorship conjecture
- Future CMB constraints on cosmic birefringence and implications for fundamental physics
- Suite of hydrodynamical simulations for the Lyman-αforest with massive neutrinos
- The MUSE 3D view of feedback in a high-metallicity radio galaxy at z = 2.9
- NMSSM with a singlino LSP: possible challenges for searches for supersymmetry at the LHC
- The generalized second law of thermodynamics for interacting f(R) gravity
- Low-mass galaxy formation and the ionizing photon budget during reionization
- Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
- Probing gravitational lensing of the CMB with SDSS-IV quasars
- Impact of massive binary star and cosmic evolution on gravitational wave observations I: black hole–neutron star mergers
- CMB distortion anisotropies due to the decay of primordial magnetic fields
- Dark-matter-spin effects at future e+e− colliders
- Inflation in Non-de Sitter Background with Coherent States
- Large angular scale CMB anisotropy from an excited initial mode
- Effects of long-lived 10 MeV-scale sterile neutrinos on primordial elemental abundances and the effective neutrino number
- Search for dark matter produced in association with a single top quark in √(s)=13 TeV pp collisions with the ATLAS detector
- The VIMOS Public Extragalactic Redshift Survey (VIPERS)
- One-loop Type II seesaw neutrino model with stable dark matter candidates
- Cosmological simulations for combined-probe analyses: covariance and neighbour-exclusion bias
- Galaxy Zoo: morphological classifications for 120 000 galaxies inHSTlegacy imaging
- Is a Higgs vacuum instability fatal for high-scale inflation?
- Conformal frame dependence of inflation
- Correcting Type Ia Supernova Distances for Selection Biases and Contamination in Photometrically Identified Samples
- Cosmology from a running vacuum model driven by a scalar field
- COSMIC SHEAR RESULTS FROM THE DEEP LENS SURVEY. II. FULL COSMOLOGICAL PARAMETER CONSTRAINTS FROM TOMOGRAPHY
- Cosmological wave maps
- Pattern universes
- Phenomenology of baryogenesis from lepton-doublet mixing
- Kinematic model-independent reconstruction of Palatini f(R) cosmology
- Whether Lyra’s Manifold Itself is aHidden Source of Dark Energy
- Reconstructing af(R) theory from the α-Attractors
- Testing the dark energy consistency with geometry and growth
- Canadian Hydrogen Intensity Mapping Experiment (CHIME) pathfinder
- Power-law cosmology, SN Ia, and BAO
- Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
- Spatially homogeneous Einstein-aether cosmological models: scalar fields with a generalized harmonic potential
- TheSwiftX-ray Telescope Cluster Survey
- Warm brane inflation with an exponential potential: A consistent realization away from the swampland
- The first Hubble diagram and cosmological constraints using superluminous supernovae
- Dark energy at early times, the Hubble parameter, and the string axiverse
- Halo and subhalo demographics with Planck cosmological parameters: Bolshoi–Planck and MultiDark–Planck simulations
- Dark QCD matters
- Interplay of the LHC and non-LHC dark matter searches in the effective field theory approach
- Higher-derivative f(R,□R,T) theories of gravity
- The Cosmology Large Angular Scale Surveyor
- A More Accurate and Competitive Estimative of H0 in Intermediate Redshifts
- Global stability analysis for cosmological models with nonminimally coupled scalar fields
- K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≈ 0.2–0.6
- Hubble Constant from LSST Strong-lens Time Delays with Microlensing Systematics
- New reaction rates for improved primordialD/Hcalculation and the cosmic evolution of deuterium
- Type IIn supernova light-curve properties measured from an untargeted survey sample
- Reconstruction of scalar field theories realizing inflation consistent with the Planck and BICEP2 results
- Probing the scotogenic model with lepton flavor violating processes
- Asymmetric dark matter and the scalar-tensor model
- Dynamical Analysis of Scalar Field Cosmologies with Spatial Curvature
- Sensitivity of primordial black hole abundance on the reheating phase
- Impact of a complex singlet: Electroweak baryogenesis and dark matter
- BICEP2, non-Bunch–Davies and entanglement
- Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
- Foreground biases on primordial non-Gaussianity measurements from the CMB temperature bispectrum: Implications forPlanckand beyond
- Time-dependent diffusive interactions between dark matter and dark energy in the context of k -essence cosmology
- Joint Analysis of Constraints on f(R) Parametrization from Recent Cosmological Observations
- The dynamical state of bars in cluster dwarf galaxies: The cases of NGC 4483 and NGC 4516
- The Quantum Primordial Black Holes, Dimensionless Small Parameter, Inflationary Cosmology and Non-Gaussianity
- Inflationary universe from perfect fluid andF(R)gravity and its comparison with observational data
- Recovering \LambdaCDM model from a cosmographic study
- Dark matter, dark energy, and alternate models: A review
- BRIGHT AND FAINT ENDS OF Lyα LUMINOSITY FUNCTIONS AT z = 2 DETERMINED BY THE SUBARU SURVEY: IMPLICATIONS FOR AGNs, MAGNIFICATION BIAS, AND ISM H I EVOLUTION
- Gödel-type solutions in cubic Galileon gravity
- Natural NMSSM after LHC Run I and the Higgsino dominated dark matter scenario
- Skewness as a Probe of Gravity: Real and Redshift Space Counts-In-Cells
- Matter power spectra in viablef(R)gravity models with massive neutrinos
- New parametrization for unified dark matter and dark energy
- Large fluctuations in the hydrogen-ionizing background and mean free path following the epoch of reionization
- Minimal semi-annihilating ℤNscalar dark matter
- SPIDERS: selection of spectroscopic targets using AGN candidates detected in all-sky X-ray surveys
- SU(2)CMB at high redshifts and the value of H0
- Late-Time Power-Law Stages of Cosmological Evolution in Teleparallel Gravity with Nonminimal Coupling
- Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
- Double-Disk Dark Matter
- The Structure and Formation Histories of Low-Mass Quiescent Galaxies in the Abell 2744 Cluster Environment
- Emergence of inflationary perturbations in the CSL model
- The cosmic merger rate of stellar black hole binaries from the Illustris simulation
- Holographic dark energy in Gauss-Bonnet gravity with Granda-Oliveros cut-off
- Cluster–galaxy weak lensing
- Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons
- New quantum phase of the Universe before inflation and its cosmological and dark energy implications
- Strict renormalizability as a paradigm for fundamental physics
- UNCOVER/MegaScience: No Evidence of Environmental Quenching in a z∼2.6 Proto-cluster
- AI-Driven Reconstruction of Large-Scale Structure from Combined Photometric and Spectroscopic Surveys
- COSMIC MICROWAVE BACKGROUND LIKELIHOOD APPROXIMATION FOR BANDED PROBABILITY DISTRIBUTIONS
- The MassiveBlack-II simulation: the evolution of haloes and galaxies to z ∼ 0
- Physical cosmology [wikipedia]
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