Cosmological parameters derived from the final (PR4) Planck data release

Abstract

We present constraints on cosmological parameters using maps from the last Planck data release (PR4). In particular, we detail an upgraded version of the cosmic microwave background likelihood, HiLLiPoP, based on angular power spectra and relying on a physical modelling of the foreground residuals in the spectral domain. This new version of the likelihood retains a larger sky fraction (up to 75%) and uses an extended multipole range. Using this likelihood, along with low-l measurements from LoLLiPoP, we derive constraints on $\Lambda$CDM parameters that are in good agreement with previous Planck 2018 results, but with 10% to 20% smaller uncertainties. We demonstrate that the foregrounds can be accurately described in spectra domain with only negligible impact on $\Lambda$CDM parameters. We also derive constraints on single-parameter extensions to $\Lambda$CDM including $A_L$, ${\Omega }_K$, $N_{eff}$, and $\sum m_{\nu }$. Noteworthy results from this updated analysis include a lensing amplitude value of $A_L=1.039\pm 0.052$, which aligns more closely with theoretical expectations within the $\Lambda$CDM framework. Additionally, our curvature measurement, ${\Omega }_K=-0.012\pm 0.010$, now demonstrates complete consistency with a flat universe, and our measurement of $S_8$ is closer to the measurements derived from large-scale structure surveys (at the 1.6$\sigma$ level). We also add constraints from PR4 lensing, making the combination the most constraining data set that is currently available from Planck. Additionally we explore adding baryon acoustic oscillation data, which tightens limits on some particular extensions to the standard cosmology.

arXiv comment18 pages, 23 figures, 2 appendix pages. Add constraints with BAO and lensing

References in corpus (61)

• Planck 2015 results. XIII. Cosmological parameters
• Planck 2013 results. XVI. Cosmological parameters
• HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
• Efficient Computation of CMB anisotropies in closed FRW models
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Planck 2018 results. V. CMB power spectra and likelihoods
• BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
• MASTER of the CMB Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex CMB Data Sets
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• Cobaya: Code for Bayesian Analysis of hierarchical physical models
• Planck 2013 results. XV. CMB power spectra and likelihood
• Efficient sampling of fast and slow cosmological parameters
• CMB power spectrum parameter degeneracies in the era of precision cosmology
• Planck 2018 results. IV. Diffuse component separation
• Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
• Planck 2018 results. III. High Frequency Instrument data processing and frequency maps
• Planck intermediate results. LVII. Joint Planck LFI and HFI data processing
• Towards a precision calculation of $N_{\mathrm{eff}}$ in the Standard Model II: Neutrino decoupling in the presence of flavour oscillations and finite-temperature QED
• Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
• Joint Bayesian component separation and CMB power spectrum estimation
• Neutrino decoupling including flavour oscillations and primordial nucleosynthesis
• A precision calculation of relic neutrino decoupling
• The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz
• Improved limits on the tensor-to-scalar ratio using BICEP and Planck
• Likelihood Analysis of CMB Temperature and Polarization Power Spectra
• Parameter inference with estimated covariance matrices
• A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies
• Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
• CMB power spectra and cosmological parameters from Planck PR4 with CamSpec
• Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
• Planck 2013 results. IX. HFI spectral response
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• How to measure CMB polarization power spectra without losing information
• Xspect, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars
• Planck constraints on the tensor-to-scalar ratio
• Planck Early Results: Statistical properties of extragalactic radio sources in the Planck Early Release Compact Source Catalogue
• High--frequency predictions for number counts and spectral properties of extragalactic radio sources. New evidences of a break at mm wavelengths in spectra of bright blazar sources
• An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol Surveys
• CMB temperature and polarisation pseudo-Cl estimators and covariances
• Deconstructing the kinetic SZ Power Spectrum
• On the assumption of Gaussianity for cosmological two-point statistics and parameter dependent covariance matrices
• Predictions on high frequency polarization properties of extragalactic radio sources and implications for CMB polarization measurements
• Reionization on Large Scales III: Predictions for Low-ell Cosmic Microwave Background Polarization and High-ell Kinetic Sunyaev-Zel'dovich Observables
• Hybrid Estimation of CMB Polarization Power Spectra
• Cosmological constraints on the neutrino mass including systematic uncertainties
• Modelling the correlation between the thermal Sunyaev Zel'dovich effect and the cosmic infrared background
• Large-scale CMB temperature and polarization cross-spectra likelihoods
• The effect of aberration on partial-sky measurements of the cosmic microwave background temperature power spectrum
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• Super-Sample CMB Lensing
• QuickPol: Fast calculation of effective beam matrices for CMB polarization
• Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
• Relieving tensions related to the lensing of CMB temperature power spectra
• Neutrino Masses and Mass Hierarchy: Evidence for the Normal Hierarchy
• Cosmology with the CMB temperature-polarization correlation
• Quadratic estimator for CMB cross-correlation

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• DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
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• Scalar NSI: A unique tool for constraining absolute neutrino masses via $\nu$-oscillations
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• A glitch in gravity: cosmic Lorentz-violation from fiery Big Bang to glacial heat death
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• Dark energy constraints in light of theoretical priors
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Modeling optical systematics for the Taurus CMB experiment
• Constraints on the normal branch of DGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
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• Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario
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• Accurate and efficient likelihood modeling for large-scale CMB data