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Unified and Consistent Structure Growth Measurements from Joint ACT, SPT, and Planck CMB Lensing

0Citations signalées — pas une note de qualité
77Institutions déclarées
15Pays d’affiliation déclarés

Résumé fourni par la source

We present the tightest cosmic microwave background (CMB) lensing constraints to date on the growth of structure by combining CMB lensing measurements from the Atacama Cosmology Telescope (ACT), the South Pole Telescope (SPT) and \textit{Planck}. Each of these surveys individually provides lensing measurements with similarly high statistical power, achieving signal-to-noise ratios of approximately 40. The combined lensing bandpowers represent the most precise CMB lensing power spectrum measurement to date with a signal-to-noise ratio of 61 and an amplitude of $A_\mathrm{lens}^\mathrm{recon} = 1.025 \pm 0.017$ with respect to the theory prediction from the best-fit CMB \textit{Planck}-ACT cosmology. The bandpowers from all three lensing datasets, analyzed jointly, yield a $1.6\%$ measurement of the parameter combination $S_8^\mathrm{CMBL} \equiv σ_8\,(Ω_m/0.3)^{0.25} = 0.825^{+0.015}_{-0.013}$. Including Dark Energy Spectroscopic Instrument (DESI) Baryon Acoustic Oscillation (BAO) data improves the constraint on the amplitude of matter fluctuations to $σ_8 = 0.829 \pm 0.009$ (a $1.1\%$ determination). When combining with uncalibrated supernovae from \texttt{Pantheon+}, we present a $4\%$ sound-horizon-independent estimate of $H_0=66.4\pm2.5\,\mathrm{km\,s^{-1}\,Mpc^{-1}} $. The joint lensing constraints on structure growth and present-day Hubble rate are fully consistent with a $Λ$CDM model fit to the primary CMB data from \textit{Planck} and ACT. While the precise upper limit is sensitive to the choice of data and underlying model assumptions, when varying the neutrino mass sum within the $Λ\mathrm{CDM}$ cosmological model, the combination of primary CMB, BAO and CMB lensing drives the probable upper limit for the mass sum towards lower values, comparable to the minimum mass prior required by neutrino oscillation experiments.

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Contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé, mais le titre doit être comparé manuellement.

Titre Crossref
Unified and Consistent Structure Growth Measurements from Joint ACT, SPT, and <i>Planck</i> CMB Lensing
Date Crossref
14/01/2026
Éditeur
American Physical Society (APS)
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude et ne compte pas comme une seconde source scientifique indépendante.

Institutions déclarées

Kavli Institute for Particle Astrophysics and CosmologyMenlo SchoolNetherlands Institute for Radio AstronomyUniversity of California, DavisSLAC National Accelerator LaboratoryUniversity of CambridgeInstitute of AstronomyCalifornia University of PennsylvaniaPhiladelphia UniversityFermi National Accelerator LaboratoryAstrobiology CenterMelbourne HealthThe University of MelbourneCanadian Institute for Theoretical AstrophysicsUniversity of ChicagoInstitut d'Astrophysique de ParisSt. Joseph Medical CenterCentre National de la Recherche ScientifiqueCornell UniversityLaboratoire AstroParticule et CosmologieSorbonne UniversitéAgence Parisienne du ClimatArgonne National LaboratoryElectronics for Imaging (United States)Reproductive Medicine InstituteCardiff UniversityUniversity of WalesUniversity of GenevaUniversity of California, RiversideUniversity of California, BerkeleyUrbana UniversityUniversity of Illinois Urbana-ChampaignUniversité Paris CitéUniversité Paris-SaclayGeneva CollegeHigh Energy Accelerator Research OrganizationAdvanced Science Research CenterCanadian Institute for Advanced ResearchMcGill UniversityMax Planck Institute of Quantum OpticsMax Planck Computing and Data FacilityPrinceton UniversityMax Planck Institute for AstrophysicsInstitute of Astrophysics and Space SciencesUniversity of Colorado SystemPlanetary Science InstituteJoint Institute for Laboratory AstrophysicsLawrence Berkeley National LaboratoryCommissariat à l'Énergie Atomique et aux Énergies AlternativesAstrophysique, Instrumentation et ModélisationUniversity of Illinois SystemMichigan State UniversityUniversity of California, Los AngelesStony Brook UniversityUniversity of PennsylvaniaNorthwestern UniversityStanford UniversityNorthwestern UniversityColumbia UniversityCentre for Research in Astrophysics of QuébecUniversity of the WitwatersrandUniversity of KwaZulu-NatalCase Western Reserve UniversityUniversity of PittsburghScience OxfordLaboratoire de Physique des 2 Infinis Irène Joliot-CurieSouthern Methodist UniversityKavli Institute for the Physics and Mathematics of the UniverseIndian Institute of AstrophysicsPontificia Universidad Católica de ChilePontificia Universidad Católica de ValparaísoPontificial Catholic University of ValparaisoFlatiron Health (United States)Harvard UniversityCenter for Astrophysics Harvard & SmithsonianArizona State UniversityGoddard Space Flight Center

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Sujets associés

Astronomy and Astrophysical ResearchParticle Accelerators and Free-Electron LasersParticle physics theoretical and experimental studies

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