From Dark Energy to Dark Matter via Non-Minimal Coupling

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dc.creatorBorowiec, A.
dc.date2008-12-23
dc.date.accessioned2026-07-07T12:21:23Z
dc.date.available2026-07-07T12:21:23Z
dc.descriptionToy cosmological models based on non-minimal coupling between gravity and scalar dilaton-like field are presented in the framework of Palatini formalism. They have the following property: preceding to a given cosmological epoch is a dark energy epoch with an accelerated expansion. The next (future) epoch becomes dominated by some kind of dark matter.
dc.description6 pages in revtex, contribution to the special volume "Problems of Modern Cosmology", TSPU publishing - in press
dc.identifierhttps://arxiv.org/abs/0812.4383
dc.identifierhttp://arxiv.org/abs/0812.4383
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/213348
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFrom Dark Energy to Dark Matter via Non-Minimal Coupling
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