Constraints on the Topology of the Universe: Extension to General Geometries
arXiv:1206.2939 · doi:10.1103/PhysRevD.86.083526
Abstract
We present an update to the search for a non-trivial topology of the universe by searching for matching circle pairs in the cosmic microwave background using the WMAP 7 year data release. We extend the exisiting bounds to encompass a wider range of possible topologies by searching for matching circle pairs with opening angles 10 degree < α< 90 degree and separation angles 11 degree < θ< 180 degree. The extended search reveal two small anomalous regions in the CMB sky. Numerous pairs of well-matched circles are found where both circles pass through one or the other of those regions. As this is not the signature of any known manifold, but is a likely consequence of contamination in those sky regions, we repeat the search excluding circle pairs where both pass through either of the two regions. We then find no statistically significant pairs of matched circles, and so no hints of a non-trivial topology. The absence of matched circles increases the lower limit on the length of the shortest closed null geodesic that self-intersects at our location in the universe (equivalently the injectivity radius at our location) to 98.5% of the diameter of the last scattering surface or approximately 26 Gpc. It extends the limit to any manifolds in which the intersecting arcs of said geodesic form an angle greater than 10^o.
11 pages, 11 figures
References in corpus (4)
Cited by in corpus (36)
- CMB Anomalies after Planck
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- Planck 2015 results. XVIII. Background geometry & topology
- The Status of Cosmic Topology after Planck Data
- Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
- Proper Size of the Visible Universe in FRW Metrics with Constant Spacetime Curvature
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- Promise of Future Searches for Cosmic Topology
- A search for cosmic topology in the final WMAP data
- Topology beyond the horizon: how far can it be probed?
- Cosmic topology. Part I. Limits on orientable Euclidean manifolds from circle searches
- The variance of the CMB temperature gradient: a new signature of a multiply connected Universe
- Cosmic topology. Part IIa. Eigenmodes, correlation matrices, and detectability of orientable Euclidean manifolds
- Electromagnetic vacuum fluctuations and topologically induced motion of a charged particle
- On the question of measuring spatial curvature in an inhomogeneous universe
- A small Universe
- Exploring suppressed long-distance correlations as the cause of suppressed large-angle correlations
- Limits of the circles-in-the-sky searches in the determination of cosmic topology of nearly flat universes
- The Hantzsche-Wendt Manifold in Cosmic Topology
- Cosmic Topology of Polyhedral Double-Action Manifolds
- Cosmic topology. Part IIIa. Microwave background parity violation without parity-violating microphysics
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- Global monopoles can change Universe's topology
- Cosmic Topology : Twenty Years After
- Cosmic topology. Part IVa. Classification of manifolds using machine learning: a case study with small toroidal universes
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- Orbifold Line Topology and the Cosmic Microwave Background
- Searching for Stringy Topologies in the Cosmic Microwave Background
- Gravitational Interaction in the Chimney Lattice Universe
- Cosmic topology. Part Ic. Limits on lens spaces from circle searches
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- Gravitational potentials and forces in the Lattice Universe: a slab
- Cosmic topology. Part IIIb. Eigenmodes and correlation matrices of spin-2 perturbations in orientable Euclidean manifolds
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- Wada Boundaries on a Hyperbolic Pair of Pants
- The Universe Originating from an Empty Planck-Size Torus