Anomalies in the topology of the temperature fluctuations in the cosmic microwave background: An analysis of the and data releases
arXiv:2111.15427 · doi:10.1051/0004-6361/202140291
Abstract
We present a multi-scale topological analysis of the temperature fluctuation maps from the NPIPE and FFP10 datasets, invoking relative homology to account for the analysis in the presence of masks. For the topological components, we detect a deviation between the observations and simulations at , for the FFP10 dataset. For the topological loops, we observe a high deviation between the observation and simulations in the number of loops at , at a low dimensionless threshold , for the NPIPE dataset. Under a Gaussian assumption, this would amount to a deviation of . However, the distribution in this bin is manifestly non-Gaussian and does not obey Poisson statistics either. In the absence of a true theoretical understanding, we simply note that the significance is higher than what may be resolved by simulations. The FFP10 dataset, indicates a deviation at this resolution and threshold. The Euler characteristic reflects the deviations in the components and loops. To assess the significance of combined levels for a given scale, we employed the empirical and theoretical versions of the test as well as the nonparametric Tukey depth test. Although all statistics exhibit a stable distribution, we favor the empirical version of the test in the final interpretation, as it indicates the most conservative differences. Even though both datasets exhibit mild to significant discrepancies, they also exhibit contrasting behaviors at various instances. Therefore, we do not find it feasible to convincingly accept or reject the null hypothesis. Disregarding the large-scale anomalies that persist at similar scales in WMAP and Planck, observations of the cosmic microwave background are largely consistent with the standard cosmological model within .
arXiv comment16 figures, 2 tables. Matches accepted version in A&A. arXiv admin note: substantial text overlap with arXiv:2101.02237
References in corpus (36)
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- Asymmetries in the CMB anisotropy field
- Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
- Planck 2018 results. VII. Isotropy and Statistics of the CMB
- Planck 2015 results. XVI. Isotropy and statistics of the CMB
- Planck 2018 results. IV. Diffuse component separation
- CMB Anomalies after Planck
- Planck intermediate results. LVII. Joint Planck LFI and HFI data processing
- Minkowski Functionals used in the Morphological Analysis of Cosmic Microwave Background Anisotropy Maps
- Non-Gaussian Signatures in the Temperature Fluctuation Observed by the Wilkinson Microwave Anisotropy Probe
- Testing for Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe Data: Minkowski Functionals and the Length of the Skeleton
- The Topology of the Cosmic Web in Terms of Persistent Betti Numbers
- The BOOMERanG experiment and the curvature of the Universe
- Analytic Minkowski Functionals of the Cosmic Microwave Background: Second-order Non-Gaussianity with Bispectrum and Trispectrum
- Large-scale alignments from WMAP and Planck
- Felix: A Topology based Framework for Visual Exploration of Cosmic Filaments
- Non Gaussianity and Minkowski Functionals: forecasts for Planck
- Topology and Geometry of Gaussian random fields I: on Betti Numbers, Euler characteristic and Minkowski functionals
- Non-Gaussian Minkowski functionals & extrema counts in redshift space
- Betti numbers of Gaussian fields
- Doppler Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: A Fingerprint of Topological Defects
- Finding cosmic voids and filament loops using topological data analysis
- The invariant joint distribution of a stationary random field and its derivatives: Euler characteristic and critical point counts in 2 and 3D
- Persistent homology in cosmic shear: constraining parameters with topological data analysis
- The Persistence of Large Scale Structures I: Primordial non-Gaussianity
- Stochastic Homology of Gaussian vs. non-Gaussian Random Fields: Graphs towards Betti Numbers and Persistence Diagrams
- Persistent homology of the cosmic web. I: Hierarchical topology in CDM cosmologies
- Unexpected Topology of the Temperature Fluctuations in the Cosmic Microwave Background
- Modeling and replicating statistical topology, and evidence for CMB non-homogeneity
- Filaments and Pancakes in the IRAS 1.2 Jy Redshift Catalogue
- Tensor Minkowski Functionals for random fields on the sphere
- Cosmological Applications of the Gaussian Kinematic Formula
- Cosmological Parameter Estimation from the Two-Dimensional Genus Topology -- Measuring the Shape of the Matter Power Spectrum
- A Study on the Baryon Acoustic Oscillation with Topological Data Analysis
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- Homology reveals significant anisotropy in the cosmic microwave background
- Betti Functionals as a Probe for Cosmic Topology