DARK MATTER AND DARK ENERGY AS EFFECTS OF MODIFIED GRAVITY

DOI10.1142/S0219887807001898zbMath1112.83043arXivastro-ph/0607639OpenAlexW2953390569WikidataQ117553812 ScholiaQ117553812MaRDI QIDQ3435123

Marek Szydłowski, Andrzej Zdzisław Borowiec, Włodzimierz Godłowski

Publication date: 25 April 2007

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0607639

zbMATH Keywords

dark mattermodified gravitydark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items

New class of hybrid metric-Palatini scalar-tensor theories of gravity ⋮ Modified gravity theories on a nutshell: inflation, bounce and late-time evolution ⋮ An alternative \(f(R,T)\) gravity theory and the dark energy problem ⋮ Energy conditions in higher derivative f(R,□R,T) gravity ⋮ Comparison of energy conditions in general relativity and modified theories of gravity ⋮ Geodesic motion in Schwarzschild spacetime surrounded by quintessence ⋮ An exponential \(F(R)\) dark energy model ⋮ Higher-derivative f(R,□R,T) theories of gravity ⋮ Geodesic deviation equation in \(f(R)\) gravity ⋮ ACCELERATION OF THE UNIVERSE DRIVEN BY THE CASIMIR FORCE ⋮ Energy conditions in \(f(R,G)\) gravity ⋮ Impact of the running gravitational constant on the extensive thermodynamics of galaxies ⋮ USING GLOBAL POSITIONING SYSTEMS TO TEST EXTENSIONS OF GENERAL RELATIVITY ⋮ PALATINI FORMULATION OF MODIFIED GRAVITY WITH A NON-MINIMAL CURVATURE-MATTER COUPLING ⋮ Constraining f(T) gravity by dynamical system analysis ⋮ Dynamics of relativistic fluids with structure scalars and \(\epsilon R^2\) cosmology

Cites Work

• Unnamed Item
• Which cosmological model-with dark energy or modified FRW dynamics?
• Estimating the dimension of a model
• Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
• \(f(R)\) theories of gravity in the Palatini approach matched with observations
• Higher-order gravity theories and scalar–tensor theories
• CURVATURE QUINTESSENCE
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• A new look at the statistical model identification