Constraints On The Topology Of The Universe From The WMAP First-Year Sky Maps
arXiv:astro-ph/0404400 · doi:10.1086/432861
Abstract
We compute the covariance expected between the spherical harmonic coefficients of the cosmic microwave temperature anisotropy if the universe had a compact topology. For fundamental cell size smaller than the distance to the decoupling surface, off-diagonal components carry more information than the diagonal components (the power spectrum). We use a maximum likelihood analysis to compare the Wilkinson Microwave Anisotropy Probe first-year data to models with a cubic topology. The data are compatible with finite flat topologies with fundamental domain times the distance to the decoupling surface at 95% confidence. The WMAP data show reduced power at the quadrupole and octopole, but do not show the correlations expected for a compact topology and are indistinguishable from infinite models.
16 pages, 5 figures
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- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Planck 2013 results. XXVI. Background geometry and topology of the Universe
- Planck 2015 results. XVIII. Background geometry & topology
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- Constraints on the topology of the Universe derived from the 7-year WMAP data
- Imprints of spherical non-trivial topologies on the CMB
- A test of the Poincare dodecahedral space topology hypothesis with the WMAP CMB data
- The Topology and Size of the Universe from CMB Temperature and Polarization Data
- The Topology and Size of the Universe from the Cosmic Microwave Background
- Promise of Future Searches for Cosmic Topology
- Cosmic microwave anisotropies in an inhomogeneous compact flat universe
- On Axial and Plane--Mirror Inhomogeneities in the WMAP3 Cosmic Microwave Background Maps
- Cosmic Topology : Twenty Years After
- Orbifold Line Topology and the Cosmic Microwave Background
- A spatial-correlation analysis of the cubic 3-torus topology based on the Planck 2013 data
- Searching for Stringy Topologies in the Cosmic Microwave Background