The Accelerated Expansion of the Universe Challenged by an Effect of the Inhomogeneities. A Review

dc.creatorCélérier, Marie-Noëlle
dc.date2007-02-15
dc.date2007-06-07
dc.date.accessioned2026-07-07T08:04:23Z
dc.date.available2026-07-07T08:04:23Z
dc.descriptionSince its decovery during the late 90's, the dimming of distant SN Ia apparent luminosity has been mostly ascribed to the influence of a mysterious dark energy component. Formulated in a Friedmannian cosmological modelling framework based upon the cosmological ``principle'' hypothesis, this interpretation has given rise to the ``concordance'' model. However, a caveat of such a reasoning is that the cosmological ``principle'' derives from a philosophical Copernican assumption and has never been tested. Furthermore, a weakness of its conclusion, i. e., the existence of a negative-pressure fluid or a cosmological constant, is that it would have profound implications for the current theories of physics. This is why we have proposed a more conservative explanation, ascribing the departure of the observed universe from an Einstein-de Sitter model to the influence of inhomogeneities. This idea has been independently developed by other authors and further enlarged to the reproduction of different cosmological data. We review here the main proposals which have been put forward to deal with this purpose and present some prospects for future developments.
dc.description21 pages, minor changes to match the final published version
dc.identifierhttps://arxiv.org/abs/astro-ph/0702416
dc.identifierhttp://arxiv.org/abs/astro-ph/0702416
dc.identifierNew Advances in Physics 1, 29 (2007)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/129937
dc.subjectAstrophysics
dc.titleThe Accelerated Expansion of the Universe Challenged by an Effect of the Inhomogeneities. A Review
dc.typetext

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