Assessing consistency between CMB temperature and polarization measurements, with application to Planck, ACT and SPT

International audience Planck's Cosmic Microwave Background temperature and polarization observations are the premier dataset for constraining cosmological models. Cosmic variance limited temperature at large and intermediate scales today dominates the constraints; polarization provides additio...

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Bibliographic Details
Published in:Physical Review D
Main Authors: La Posta, Adrien, Natale, Umberto, Calabrese, Erminia, Garrido, Xavier, Louis, Thibaut
Other Authors: Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Cardiff University, European Project: 849169,ERC-2019-STG
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2023
Subjects:
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Lambda
South Pole
South pole
Online Access:https://hal.science/hal-03644852
https://doi.org/10.1103/physrevd.107.023510
Description
Summary:International audience Planck's Cosmic Microwave Background temperature and polarization observations are the premier dataset for constraining cosmological models. Cosmic variance limited temperature at large and intermediate scales today dominates the constraints; polarization provides additional constraining power and further scrutiny of the models. To complete this picture from Planck, ground-based experiments, such as the Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT) continue to add temperature and polarization measurements at small scales, allowing for the extraction of competitive cosmological constraints from the $TE$ and $EE$ power spectra. Matching at the same time all these stringent probes is a key challenge and validation step for any cosmological model. In particular, $\Lambda$CDM requires a tight consistency between the temperature and polarization measurements. In this paper, we present a number of methods to identify and quantify possible inconsistencies between temperature and polarization, we apply them to the latest Planck, ACT and SPT data and find no evidence for a deviation from $\Lambda$CDM. Application of these methods will have increased importance for future, more constraining CMB data.

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