Late time cosmology in f(R,G) -gravity with interacting fluids
DOI10.1088/1361-6382/ac4b97zbMath1487.83049OpenAlexW4205582175MaRDI QIDQ5066831
A. Chanda, Sunil D. Maharaj, Aroonkumar Beesham, Bikash Chandra Paul
Publication date: 30 March 2022
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/1361-6382/ac4b97
Navier-Stokes equations for incompressible viscous fluids (76D05) Other elementary particle theory in quantum theory (81V25) Geometrodynamics and the holographic principle (83E05) Statistical mechanics of superconductors (82D55) Nonlinear higher-order PDEs (35G20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Liquid-liquid two component flows (76T06)
Cites Work
- Do consistent \(F(R)\) models mimic general relativity plus \(\Lambda\)?
- On the growth of perturbations in interacting dark energy and dark matter fluids
- Swampland implications of GW170817-compatible Einstein-Gauss-Bonnet gravity
- Emergent universe scenario in the Einstein-Gauss-Bonnet gravity with dilaton
- Towards a non-singular pre-big bang cosmology
- \(1/R\) gravity and scalar-tensor gravity
- Avoidance of naked singularities in dilatonic brane world scenarios with a Gauss-Bonnet term
- Dynamics of inflation and dark energy from \(F(R, \mathcal{G})\) gravity
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- A new type of isotropic cosmological models without singularity
- \(f(R)\) theories of gravity in the Palatini approach matched with observations
- Emergent universe with interacting fluids and the generalized second law of thermodynamics
- PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- The cosmological constant and dark energy
- Constraining f ( R ) gravity in the Palatini formalism
- Newtonian, Post-Newtonian and Parametrized Post-Newtonian limits of f(R, đą) gravity
- Dynamical analysis on $f(R, \mathcal{G})$ cosmology
- The realistic models of relativistic stars in f â( R ) = R + αR 2 gravity
- Dynamics of relativistic interacting gases: from a kinetic to a fluid description
- Cosmic history of viable exponential gravity: equation of state oscillations and growth index from inflation to dark energy era
- Connecting early and late epochs by f(z)CDM cosmography
- Late-time cosmology of scalar-coupled f(R,G) gravity
- Measurements of Ω and Î from 42 HighâRedshift Supernovae
- Cosmological constraints on f(R) gravity theories within the Palatini approach
- The Einstein Tensor and Its Generalizations
- The cosmological constant
This page was built for publication: Late time cosmology in f(R,G) -gravity with interacting fluids
