Çiftçi, Dilek K.Faraoni, Valerio2022-05-112022-05-1120180003-49161096-035Xhttps://doi.org/10.1016/j.aop.2018.02.002https://hdl.handle.net/20.500.11776/7040Brans-Dicke cosmology with an (inverse) power-law potential is revisited in the light of modern quintessence and inflation models. A simple ansatz relating scale factor and scalar field recovers most of the known solutions and generates new ones. A phase space interpretation of the ansatz is provided and these universes are mapped into solutions off (R) cosmology. (C) 2018 Elsevier Inc. All rights reserved.en10.1016/j.aop.2018.02.002info:eu-repo/semantics/openAccessBrans-Dicke cosmologyf (R) cosmologyScalar-tensor gravityExact solutionsScalar-Tensor CosmologyExtended InflationN-GravityDark EnergyQualitative-AnalysisMachs PrincipleF(R) GravityUniverseModelsFieldArticle3916582Q2WOS:0004300381000062-s2.0-85042449638Q1