Inflation, dark matter and dark energy in the string landscape

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dc.creatorLiddle, Andrew R
dc.creatorUreña-López, L Arturo
dc.date2006-05-09
dc.date2006-10-05
dc.date.accessioned2026-07-07T10:23:04Z
dc.date.available2026-07-07T10:23:04Z
dc.descriptionWe consider the conditions needed to unify the description of dark matter, dark energy and inflation in the context of the string landscape. We find that incomplete decay of the inflaton field gives the possibility that a single field is responsible for all three phenomena. By contrast, unifying dark matter and dark energy into a single field, separate from the inflaton, appears rather difficult.
dc.description4 pages RevTex4. Updated to include a toy model of reheating. Matches version accepted by Phys Rev Lett
dc.identifierhttps://arxiv.org/abs/astro-ph/0605205
dc.identifierhttp://arxiv.org/abs/astro-ph/0605205
dc.identifierPhys.Rev.Lett.97:161301,2006
dc.identifierdoi:10.1103/PhysRevLett.97.161301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175698
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleInflation, dark matter and dark energy in the string landscape
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