Topological Lensing in Spherical Spaces

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dc.creatorGausmann, Evelise
dc.creatorLehoucq, Roland
dc.creatorLuminet, Jean-Pierre
dc.creatorUzan, Jean-Philippe
dc.creatorWeeks, Jeffrey
dc.date2001-06-11
dc.date.accessioned2026-07-07T10:51:48Z
dc.date.available2026-07-07T10:51:48Z
dc.descriptionThis article gives the construction and complete classification of all three-dimensional spherical manifolds, and orders them by decreasing volume, in the context of multiconnected universe models with positive spatial curvature. It discusses which spherical topologies are likely to be detectable by crystallographic methods using three-dimensional catalogs of cosmic objects. The expected form of the pair separation histogram is predicted (including the location and height of the spikes) and is compared to computer simulations, showing that this method is stable with respect to observational uncertainties and is well suited for detecting spherical topologies.
dc.description32 pages, 26 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0106033
dc.identifierhttp://arxiv.org/abs/gr-qc/0106033
dc.identifierClass.Quant.Grav.18:5155-5186,2001
dc.identifierdoi:10.1088/0264-9381/18/23/311
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184945
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleTopological Lensing in Spherical Spaces
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