Inhomogeneous Cosmology, Inflation and Late-Time Accelerating Universe

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dc.creatorMoffat, J. W.
dc.date2006-06-06
dc.date2007-05-30
dc.date.accessioned2026-07-07T08:05:23Z
dc.date.available2026-07-07T08:05:23Z
dc.descriptionAn exact inhomogeneous solution of Einstein's field equations is shown to be able to inflate in a non-uniform way in the early universe and explain anomalies in the WMAP power spectrum data. It is also possible for the model to explain the accelerated expansion of the universe by late-time inhomogeneous structure.
dc.description10 pages, Latex file, no figures. Major revision of paper
dc.identifierhttps://arxiv.org/abs/astro-ph/0606124
dc.identifierhttp://arxiv.org/abs/astro-ph/0606124
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/130269
dc.subjectAstrophysics
dc.titleInhomogeneous Cosmology, Inflation and Late-Time Accelerating Universe
dc.typetext

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