No evidence for EDE from Planck data in extended scenarios
arXiv:2203.12930 · doi:10.1016/j.jheap.2023.05.002
Abstract
The latest data release from the ACT CMB experiment (in combination with previous WMAP data) shows evidence for an Early Dark Energy component at more than standard deviations. The same conclusion has been recently shown to hold when temperature data from the Planck experiment limited to intermediate angular scales () are included while it vanishes when the full Planck dataset is considered. However, it has been shown that the full Planck dataset exhibits an anomalous lensing component and a preference for a closed universe at the level of three standard deviation. It is therefore of utmost importance to investigate if these anomalies could anti-correlate with an early dark energy component and hide its presence during the process of parameter extraction. Here we demonstrate that extended parameters choices as curvature, equation of state of dark energy and lensing amplitude have no impact on the Planck constraints on EDE. In practice, EDE does not solve Planck angular spectra anomalies. This indicates that current CMB evidence for an EDE component comes essentially from the ACT-DR4 dataset.
arXiv comment6 pages, 3 Figures
References in corpus (29)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Planck 2015 results. XIII. Cosmological parameters
- Efficient Computation of CMB anisotropies in closed FRW models
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
- In the Realm of the Hubble tension a Review of Solutions
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- Tensions between the Early and the Late Universe
- Planck 2018 results. V. CMB power spectra and likelihoods
- Early Dark Energy Can Resolve The Hubble Tension
- Planck 2018 results. VIII. Gravitational lensing
- The Hubble Hunter's Guide
- The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
- Planck evidence for a closed Universe and a possible crisis for cosmology
- Efficient sampling of fast and slow cosmological parameters
- Cosmology Intertwined II: The Hubble Constant Tension
- Early dark energy, the Hubble-parameter tension, and the string axiverse
- Curvature tension: evidence for a closed universe
- Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
- Early Dark Energy Does Not Restore Cosmological Concordance
- Cosmic Microwave Weak lensing data as a test for the dark universe
- Early dark energy is not excluded by current large-scale structure data
- A Lockdown Perspective on the Hubble Tension (with comments from the SH0ES team)
- Quantifying the global parameter tensions between ACT, SPT and Planck
Cited by in corpus (4)
- Challenges for CDM: An update
- Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
- Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
- Early dark energy constraints with late-time expansion marginalization