Ruling out the Modified Chaplygin Gas cosmologies
| dc.contributor.author | OGOUYANDJOU, KOLADÉ SIMPLICE EPHREM CARLOS | |
| dc.date.accessioned | 2026-06-02T16:06:57Z | |
| dc.date.available | 2026-06-02T16:06:57Z | |
| dc.date.issued | 2011 | |
| dc.description.abstract | The 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.doi | 10.1016/j.physletb.2010.10.022 | |
| dc.identifier.other | BECDB-6777 | |
| dc.identifier.uri | https://dspace.uac.bj/handle/123456789/6138 | |
| dc.language.iso | fr | |
| dc.relation.ispartof | Physics Letters B | |
| dc.subject | Dark energy | |
| dc.subject | Unified models | |
| dc.subject | Cosmology | |
| dc.title | Ruling out the Modified Chaplygin Gas cosmologies | |
| dc.type | Article |
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