2006/01/31 by Guido Cognola, E. Elizalde, Emilio Elizalde +4 · 22 citations
Physics and Astronomy · #Acceleration #Astrophysics #Black Holes and Theoretical Physics #Classical mechanics #Cosmological constant #Cosmology #Cosmology and Gravitation Theories #Dark energy #De Sitter universe #Galaxies: Formation, Evolution, Phenomena #General relativity #Hierarchy problem #Lambda-CDM model #Mathematical physics #Metric expansion of space #Physics #Quantum gravity #Quantum mechanics #Quintessence #Theoretical physics #Universe #astro-ph #f(R) gravity #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1103/physrevd.73.084007
published as Phys.Rev.D73:084007,2006 · LaTeX file 20 pages, new subsections are added
arxiv created 2006/03/01 · openalex publication_date 2006/04/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
Dark energy cosmology is considered in a modified Gauss-Bonnet (GB) model of gravity where an arbitrary function of the GB invariant, f(G), is added to the general relativity action. We show that a theory of this kind is endowed with a quite rich cosmological structure: it may naturally lead to an effective cosmological constant, quintessence, or phantom cosmic acceleration, with a possibility for the transition from deceleration to acceleration. It is demonstrated in the paper that this theory is perfectly viable, since it is compliant with the solar system constraints. Specific properties of f(G) gravity in a de Sitter (dS) universe, such as dS and SdS solutions, their entropy, and its explicit one-loop quantization are studied. The issue of a possible solution of the hierarchy problem in modified gravities is also addressed.