2008/01/09 by K. Atazadeh, Mehrdad Farhoudi, M. Farhoudi +2 · 4 citations
Mathematics · Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Curvature #Galaxies: Formation, Evolution, Phenomena #Geometry #Mathematics #Physics #Universe #astro-ph #gr-qc #hep-th
paper · pdf · doi:10.1016/j.physletb.2007.12.057
published as Phys.Lett.B660:275-281,2008 · 9 pages, 1 figure, to appear in PLB
arxiv created 2008/01/09 · openalex publication_date 2008/01/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We study a 5-dimensional f(R) brane gravity within the framework of scalar-tensor type theories. We show that such a model predicts, for a certain choice of f(R) and a spatially flat universe, an exponential potential, leading to an accelerated expanding universe driven solely by the curvature of the bulk space. This result is consistent with the observational data in the cosmological scale.