Unified Model for Inflation and the Dark Side of the Universe

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dc.creatorZsembinszki, Gabriel
dc.date2007-01-12
dc.date.accessioned2026-07-07T07:40:18Z
dc.date.available2026-07-07T07:40:18Z
dc.descriptionWe present a model with a complex and a real scalar fields and a potential whose symmetry is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe and for the period of acceleration of the late universe or for the dark matter, depending on the smallness of the explicit breaking.
dc.descriptionContribution to the proceedings of International Workshop on the Dark Side of the Universe (DSU2006), Madrid, Spain, 20-24 Jun 2006; 7 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0701369
dc.identifierhttp://arxiv.org/abs/astro-ph/0701369
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121735
dc.subjectAstrophysics
dc.titleUnified Model for Inflation and the Dark Side of the Universe
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