Cosmic microwave background anomalies viewed via Gumbel Statistics
arXiv:0908.1931 · doi:10.1111/j.1365-2966.2009.15503.x
Abstract
We describe and discuss the application of Gumbel statistics, which model extreme events, to WMAP 5-year measurements of the cosmic microwave background. We find that temperature extrema of the CMB are well modelled by the Gumbel formalism and describe tests for Gaussianity that the approach can provide. Comparison to simulations reveals Gumbel statistics to have only weak discriminatory power for the conventional statistic: , though it may probe other regimes of non-Gaussianity. Tests based on hemispheric cuts reveal interesting alignment with other reported CMB anomalies. The approach has the advantage of model independence and may find further utility with smaller scale data.
5 pages, 8 figures, accepted for publication in MNRAS. This version: added references
References in corpus (5)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence
- The Axis of Evil revisited
- A high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets
- The Hot and Cold Spots in Five-Year WMAP Data
Cited by in corpus (9)
- Most massive halos with Gumbel Statistics
- Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
- Exact Extreme Value Statistics and the Halo Mass Function
- Extreme value statistics of smooth random Gaussian fields
- Are the 2dFGRS superstructures a problem for hierarchical models?
- Isotropy statistics of CMB hot and cold spots
- TDCOSMO XV: Population Analysis of Lines of Sight of 25 Strong Galaxy-Galaxy Lenses with Extreme Value Statistics
- Is GN-z11 powered by a super-Eddington massive black hole?
- Extreme value statistics of CMB lensing deflection angles