CROSSING OF PHANTOM DIVIDE IN F(R) GRAVITY

DOI10.1142/S0217732310000058zbMath1189.83091arXiv1003.0769MaRDI QIDQ3570743

Chao-Qiang Geng, Sergei D. Odintsov, Kazuharu Bamba, Shin'ichi Nojiri

Publication date: 28 June 2010

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1003.0769

zbMATH Keywords

cosmologydark energymodified theories of gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items

Phantom-like dark energy from quantum gravity ⋮ Barrow holographic phantom ⋮ FRW cosmology in f(Q,T) gravity ⋮ An exponential \(F(R)\) dark energy model ⋮ Thermodynamic properties of modified gravity theories ⋮ Smooth crossing of \(w_\Lambda=-1\) line in a single scalar field model ⋮ Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests ⋮ Exact solutions of Bianchi type \(V\) spacetime in \(f(R,T)\) gravity

Cites Work

• Cosmological constant -- the weight of the vacuum
• Extended theories of gravity and their cosmological and astrophysical applications
• The cosmological constant and dark energy
• DYNAMICS OF DARK ENERGY
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Consistent modified gravity: dark energy, acceleration and the absence of cosmic doomsday
• Oscillating Phantom in F(R) Gravity
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae