Counterexample to Claimed COBE Constraints on Compact Toroidal Universe Models

dc.contributor.authorRoukema, B. F.
dc.date.accessioned2012-03-12T11:16:20Z
dc.date.available2012-03-12T11:16:20Z
dc.date.issued2000-03-12
dc.description.abstractIt has been suggested that if the Universe satisfies a flat, multiply connected, perturbed Friedmann- Lemaˆıtre model, then cosmic microwave back- ground data from the COBE satellite implies that the minimum size of the injectivity diameter (shortest closed spatial geodesic) must be larger than about two fifths of the horizon diameter. To show that this claim is misleading, a simple T2×R universe model of injectivity diameter a quarter of this size, i.e. a tenth of the horizon diameter, is shown to be consistent with COBE four year ob- servational maps of the cosmic microwave back- ground. This is done using the identified circles principle.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1261
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;30/00
dc.subjectClaimed COBE Constraintsen_US
dc.subjectCompact Toroidal Universe Modelsen_US
dc.titleCounterexample to Claimed COBE Constraints on Compact Toroidal Universe Modelsen_US
dc.typePreprinten_US

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