Elements of dodecahedral cosmology

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dc.creatorBellon, Marc
dc.date2006-02-03
dc.date2006-10-26
dc.date.accessioned2026-07-07T06:57:11Z
dc.date.available2026-07-07T06:57:11Z
dc.descriptionA general method for the determination of the harmonics of quotients of the 3-sphere is given. They can all be deduced from three objects already known from Klein. We further show explicitly how these harmonics can be organized in irreducible representations of the holonomy group: this allows for the determination of the full correlation matrix of the Cosmic Microwave Background in the spherical harmonics basis.
dc.description18 pages, changed title and expanded explanations, to follow the published version. The results are unchanged
dc.identifierhttps://arxiv.org/abs/astro-ph/0602076
dc.identifierhttp://arxiv.org/abs/astro-ph/0602076
dc.identifierClassical and Quantum Gravity 23 (2006) 7029-7043
dc.identifierdoi:10.1088/0264-9381/23/23/025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/106876
dc.subjectAstrophysics
dc.subjectRepresentation Theory
dc.titleElements of dodecahedral cosmology
dc.typetext

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