Dodecahedral topology fails to explain quadrupole-octupole alignment
arXiv:astro-ph/0611640 · doi:10.1088/0264-9381/24/7/011
Abstract
The CMB quadrupole and octupole, as well as being weaker than expected, align suspiciously well with each other. Non-trivial spatial topology can explain the weakness. Might it also explain the alignment? The answer, at least in the case of the Poincare dodecahedral space, is a resounding no.
5 pages, 1 figure
References in corpus (13)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- A high resolution foreground cleaned CMB map from WMAP
- Is the low-l microwave background cosmic?
- Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background
- Multipole Vectors--a new representation of the CMB sky and evidence for statistical anisotropy or non-Gaussianity at 2<=l<=8
- On Foreground Removal from the Wilkinson Microwave Anisotropy Probe Data by an Internal Linear Combination Method: Limitations and Implications
- Multipole vector anomalies in the first-year WMAP data: a cut-sky analysis
- Constraints on mode couplings and modulation of the CMB with WMAP data
- CMB Anisotropy of the Poincare Dodecahedron
- Cosmic microwave background multipole alignments in slab topologies
- CMB Alignment in Multi-Connected Universes
- Predicting the CMB power spectrum for binary polyhedral spaces
- Maxwell's Multipole Vectors and the CMB
Cited by in corpus (7)
- Large-scale alignments from WMAP and Planck
- A test of the Poincare dodecahedral space topology hypothesis with the WMAP CMB data
- Large scale alignment anomalies of CMB anisotropies: a new test for residuals applied to WMAP 5yr maps
- CMB Alignment in Multi-Connected Universes
- The spectral action and cosmic topology
- Topology beyond the horizon: how far can it be probed?
- Platonic topology and CMB fluctuations: Homotopy, anisotropy, and multipole selection rules