Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence

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dc.creatorLindesay, James V.
dc.creatorNoyes, H. Pierre
dc.date2004-10-07
dc.date2004-10-25
dc.date.accessioned2026-07-07T02:14:58Z
dc.date.available2026-07-07T02:14:58Z
dc.descriptionStandard cosmology connects the scale generated at late times by the cosmological constant with that generated in early times by the energy dynamics. Assuming dark energy de-coherence occurs during early times when the scale parameter expansion rate is no longer supra-luminal specifies a class of cosmological models in which the cosmic microwave background fluctuation amplitude at last scattering is approximately $10^{-5}$.
dc.description9 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0410217
dc.identifierhttp://arxiv.org/abs/astro-ph/0410217
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8339
dc.subjectAstrophysics
dc.titleCosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence
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