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- W3104729907 abstract "When the density parameter is close to unity, the universe has a large curvature radius independent of its being hyperbolic or spherical, or in the limiting case of an infinite curvature radius, flat. Whatever the curvature, the universe may have either a simply connected or a multiply connected topology. In the flat case, the topology scale is arbitrary, and there is no a priori reason for this scale to be of the same order as the size of the observable universe. In the hyperbolic case, any nontrivial topology would almost surely be on a length scale too large to detect. In the spherical case, in contrast, the topology could easily occur on a detectable scale. The present paper shows how, in the spherical case, the assumption of a nearly flat universe simplifies the algorithms for detecting a multiply connected topology, but also reduces the amount of topology that can be seen. This is of primary importance for the upcoming cosmic microwave background data analysis." @default.
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- W3104729907 date "2003-03-28" @default.
- W3104729907 modified "2023-10-10" @default.
- W3104729907 title "Detecting topology in a nearly flat spherical universe" @default.
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- W3104729907 doi "https://doi.org/10.1088/0264-9381/20/8/309" @default.
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