Ruling out the Modified Chaplygin Gas cosmologies

dc.contributor.authorOGOUYANDJOU, KOLADÉ SIMPLICE EPHREM CARLOS
dc.date.accessioned2026-06-02T16:06:57Z
dc.date.available2026-06-02T16:06:57Z
dc.date.issued2011
dc.description.abstractThe Modified Chaplygin Gas (MCG) model belongs to the class of a unified models of dark energy (DE) and dark matter (DM). It is characterized by an equation of state (EoS) p c = B ρ − A / ρ α , where the case B = 0 corresponds to the Generalized Chaplygin Gas (GCG) model. Using a perturbative analysis and power spectrum observational data we show that the MCG model is not a successful candidate for the cosmic medium unless B = 0. In this case, it reduces to the usual GCG model.
dc.identifier.doi10.1016/j.physletb.2010.10.022
dc.identifier.otherBECDB-6777
dc.identifier.urihttps://dspace.uac.bj/handle/123456789/6138
dc.language.isofr
dc.relation.ispartofPhysics Letters B
dc.subjectDark energy
dc.subjectUnified models
dc.subjectCosmology
dc.titleRuling out the Modified Chaplygin Gas cosmologies
dc.typeArticle

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