Cosmological perfect-fluids in f(R) gravity
arXiv:1810.03204 · doi:10.1142/S0219887819500087
Abstract
We show that an n-dimensional generalized Robertson-Walker (GRW) space-time with divergence-free conformal curvature tensor exhibits a perfect fluid stress-energy tensor for any f(R) gravity model. Furthermore we prove that a conformally flat GRW space-time is still a perfect fluid in both f(R) and quadratic gravity where other curvature invariants are considered.
arXiv comment13 pages, final version
References in corpus (21)
- f(R) Theories Of Gravity
- Extended Theories of Gravity
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Curvature Quintessence
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- Energy in Generic Higher Curvature Gravity Theories
- Dark energy and dark matter as curvature effects
- A simple characterization of generalized Robertson-Walker spacetimes
- Generalized Robertson-Walker space times, a survey
- On the theory and applications of modern cosmography
- Noether Symmetry Approach in Gauss-Bonnet Cosmology
- A condition for a perfect-fluid space-time to be a generalized Robertson-Walker space-time
- On the Weyl and Ricci tensors of Generalized Robertson-Walker space-times
- Global decomposition of a Lorentzian manifold as a Generalized Robertson-Walker space
- Newtonian, Post Newtonian and Parameterized Post Newtonian limits of f(R, G) gravity
- Weyl compatible tensors
- Connecting early and late universe by gravity
- Riemann compatible tensors
- Cosmic relic abundance and f(R) gravity
- Twisted Lorentzian manifolds, a characterization with torse-forming time-like unit vectors
Cited by in corpus (58)
- Study on anisotropic strange stars in gravity: An embedding approach under simplest linear functional of matter-geometry coupling
- Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
- Anisotropic compact stars in gravity
- Charged spherically symmetric black holes in gravity and their stability analysis
- Validation of Energy Conditions in Wormhole Geometry within Viable Gravity
- Unraveling the effective fluid approach for models in the subhorizon approximation
- Traversable wormholes in gravity with constant and variable redshift functions
- Non-Local Gravity Cosmology: an Overview
- Scalar induced gravitational waves from primordial black hole Poisson fluctuations in gravity
- Connecting early and late epochs by f(z)CDM cosmography
- Non-trivial black hole solutions in gravitational theory
- Unveiling cosmography from the dark energy equation of state
- Designing Horndeski and the effective fluid approach
- Cosmological perfect fluids in Gauss-Bonnet gravity
- Static Traversable Wormholes in Gravity
- A Panorama of Viable Gravity Dark Energy Models
- Cosmological perfect fluids in higher-order gravity
- Anisotropic compact stars in higher-order curvature theory
- Gravity Wormholes sourced by a Phantom Scalar Field
- Black holes of -dimensional gravity coupled to a scalar field
- Quasinormal modes and their anomalous behavior for black holes in gravity
- Noether Symmetry Approach in Energy-Momentum Squared Gravity
- Curvature Scalarization of Black Holes in f(R) Gravity
- Exact Solutions in Higher-Dimensional Lovelock and Chern-Simons Gravity
- Inflation Revisited and Dark Energy Corrections
- Cosmological constraints on non-adiabatic dark energy perturbations
- General properties of gravity vacuum solutions
- Almost pseudo-Ricci symmetric spacetime solutions in -gravity
- Estimation of Cosmological Parameters, Stability Analysis and Energy Conditions in Viable Modified Gravity
- Equivalence between Horndeski and beyond Horndeski theories and imperfect fluids
- Boson stars in extended theory of gravity
- Cosmological acceleration
- New rotating AdS/dS black holes in gravity
- On Curvature properties of Nariai Spacetimes
- Phantom energy dominated universe as a transient stage in cosmology
- Phantom energy supported wormhole model in gravity assuming conformal motion
- Specific neutral and charged black holes in gravitational theory
- Spherical doubly warped spacetimes for radiating stars and cosmology
- Uniqueness of non-trivial spherically symmetric black hole solution in special classes of F(R) gravitational theory
- FLRW-Cosmology in Generic Gravity Theories
- Friedmann equations in the Codazzi parametrization of Cotton and extended theories of gravity and the Dark Sector
- Wormhole modeling in gravity with linear trace term
- Black Holes with Electric and Magnetic Charges in Gravity
- The Effective Fluid approach for Modified Gravity and its applications
- Effective Actions for Loop Quantum Cosmology in Fourth-Order Gravity
- Bouncing Cosmology in Fourth-Order Gravity
- Generalized Ghost Dark Energy in DGP Model
- Palatini gravity and its Born-Infeld semblance
- w=1/3 to w=-1 evolution in a Robertson-Walker space-time with constant scalar curvature
- Gödel-type universes in energy-momentum-squared gravity
- Spinning (A)dS Black Holes with Slow-Rotation Approximation in Dynamical Chern-Simons Modified Gravity
- Cosmology from a running vacuum model driven by a scalar field
- Born - Infeld-type modified gravity
- Constraints on cosmological parameters and CMB first acoustic peak in conformal Killing gravity
- Causal cosmology with braneworld gravity including Gauss Bonnet coupling
- Exact charged black hole solutions in D-dimensions in f(R) gravity
- On Pseudo -symmetric spacetimes and gravity
- Polyakov-like approach to the modified gravity and other geometric theories