f(R) GRAVITY AND ITS COSMOLOGICAL IMPLICATIONS

DOI10.1142/S0218271811019529zbMath1263.83139arXiv1101.0716OpenAlexW2072344789WikidataQ57731827 ScholiaQ57731827MaRDI QIDQ4914570

Hayato Motohashi, Alexei A. Starobinsky, Jun'ichi Yokoyama

Publication date: 15 April 2013

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

Full work available at URL: https://arxiv.org/abs/1101.0716

zbMATH Keywords

equation of stategrowth indexdark energy\(f(R)\) gravity

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) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (5)

A dynamical system approach to Bianchi III cosmology for Hu-Sawicki type \(f(R)\) gravity ⋮ Reconstruction of an observationally constrained f(R,T) gravity model ⋮ Strange stars in energy–momentum-conserved f(R,T) gravity ⋮ Domestic corpuscular inflaton ⋮ Observational constraints on models of the universe with time variable gravitational and cosmological constants along MOG

Cites Work

• Do consistent \(F(R)\) models mimic general relativity plus \(\Lambda\)?
• A new type of isotropic cosmological models without singularity
• Matter Power Spectrum in f(R) Gravity with Massive Neutrinos
• ANALYTIC SOLUTION FOR MATTER DENSITY PERTURBATIONS IN A CLASS OF VIABLE COSMOLOGICAL f(R) MODELS
• Phantom Boundary Crossing and Anomalous Growth Index of Fluctuations in Viable f(R) Models of Cosmic Acceleration
• Inflationary universe: A possible solution to the horizon and flatness problems

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