Topological invariant quintessence
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Publication:5251526
DOI10.1142/S0217732315500698zbMath1311.83040arXiv1411.7001WikidataQ63380413 ScholiaQ63380413MaRDI QIDQ5251526
Publication date: 20 May 2015
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1411.7001
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) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (4)
Noether symmetry approach for teleparallel-curvature cosmology ⋮ Dynamical analysis on $f(R, \mathcal{G})$ cosmology ⋮ Braneworld mimetic f(R) gravity ⋮ \(F(R,G)\) cosmology through Noether symmetry approach
Cites Work
- Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- On the \(\Lambda \)CDM universe in \(f(G)\) gravity
- Noether symmetry for Gauss-Bonnet dilatonic gravity
- Recovering the effective cosmological constant in extended gravity theories
- Energy conditions in \(f(R,G)\) gravity
- Extended theories of gravity and their cosmological and astrophysical applications
- THE GEODESIC MOTION NEAR HYPERSURFACES IN THE WARPED PRODUCTS SPACETIME
- SOME ASPECTS OF GENERALIZED MODIFIED GRAVITY MODELS
- Noether symmetry approach in Gauss–Bonnet cosmology
- Linear Growth of Matter Density Perturbations in Theories
- PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
- Inevitable Ghost and the Degrees of Freedom in f(R, ) Gravity
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Newtonian, Post-Newtonian and Parametrized Post-Newtonian limits of f(R, 𝒢) gravity
- ΛCDM epoch reconstruction from F ( R , G ) and modified Gauss–Bonnet gravities
- CURVATURE QUINTESSENCE
- On the stability of the cosmological solutions in f ( R , G ) gravity
- Reconstruction and deceleration-acceleration transitions in modified gravity
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