Evolution of the universe in inverse and \(\ln f(R)\) gravity

DOI10.1007/S10509-012-1169-4zbMath1286.83115OpenAlexW2027591968MaRDI QIDQ2448640

Yanyan Li

Publication date: 2 May 2014

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-012-1169-4

zbMATH Keywords

modified gravitydark energy

Mathematics Subject Classification ID

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

Related Items (14)

Thermodynamics in \(f(T)\) gravity with nonminimal coupling to matter ⋮ Dynamics of an anisotropic universe in \(f(R, T)\) theory ⋮ Thermodynamics in \(f(\mathcal{G}, T)\) gravity ⋮ Functional form of \(f(R)\) with power-law expansion in anisotropic model ⋮ Quintessence and holographic dark energy in \(f(T)\) gravity ⋮ Self-similar cosmological solutions in f(R,T) gravity theory ⋮ Wormholes solutions in f(R,T) gravity with photon sphere at the throat ⋮ Energy constraints for static wormholes in f(ℛ,𝒯 ) gravity ⋮ LRS Bianchi type-I cosmological model with constant deceleration parameter in f(R,T) gravity ⋮ Stable traversable wormholes in f(Q) gravity ⋮ Analysis of \(f(R)\) theory corresponding to NADE and NHDE ⋮ Inflationary constraints in teleparallel gravity theory ⋮ Inflation in \(f(R, \phi)\) gravity with exponential model ⋮ Power law f(𝒢,T) gravity models supporting wormhole solutions

Cites Work

• Unnamed Item
• Modified gravity with ln \(R\) terms and cosmic acceleration
• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• de Sitter brane universe induced by phantom and quantum effects
• Can modified gravity explain accelerated cosmic expansion?
• \(1/R\) gravity and scalar-tensor gravity
• Where new gravitational physics comes from: M-theory?
• The force of gravity from a Lagrangian containing inverse powers of the Ricci scalar
• Quantum de Sitter cosmology and phantom matter
• Cosmological constant -- the weight of the vacuum
• A new type of isotropic cosmological models without singularity
• Dark energy and gravity
• EFFECTS OF ELECTROMAGNETIC FIELD ON THE DYNAMICS OF BIANCHI TYPE VI₀UNIVERSE WITH ANISOTROPIC DARK ENERGY
• The cosmological constant and dark energy
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• INVERSE PROBLEM – RECONSTRUCTION OF DARK ENERGY MODELS
• Cosmological evolution in 1/ R -gravity theory
• Consistent modified gravity: dark energy, acceleration and the absence of cosmic doomsday
• 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
• The cosmological constant problem
• Curvature-driven acceleration: a utopia or a reality?
• Cosmological dynamics of R ⁿ gravity
• The cosmological constant
• An alternative to quintessence

This page was built for publication: Evolution of the universe in inverse and \(\ln f(R)\) gravity