Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity
From MaRDI portal
Publication:2946267
DOI10.1142/S0218271815500534zbMath1320.83036arXiv1409.0760MaRDI QIDQ2946267
Publication date: 16 September 2015
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1409.0760
Relativistic cosmology (83F05) 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 (8)
Irrotational-fluid cosmologies in fourth-order gravity ⋮ Chaplygin-gas solutions of f(R) gravity ⋮ Multifluid cosmology in f(G) gravity ⋮ Perturbations in the interacting vacuum ⋮ On f(R) gravity in scalar–tensor theories ⋮ A study of perturbations in scalar–tensor theory using 1 + 3 covariant approach ⋮ Cosmological perturbations in f(G) gravity ⋮ On multifluid perturbations in scalar–tensor cosmology
Cites Work
- \(f(R)\) theories
- A new type of isotropic cosmological models without singularity
- Extended theories of gravity and their cosmological and astrophysical applications
- Covariant gauge-invariant perturbations in multifluid f ( R ) gravity
- A new approach to reconstruction methods in f ( R ) gravity
- <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
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- INVERSE PROBLEM – RECONSTRUCTION OF DARK ENERGY MODELS
- Covariant analysis of gravitational waves in a cosmological context
- Anti-Newtonian cosmologies in f ( R ) gravity
- The cosmological constant problem
- Structure growth in f ( R ) theories of gravity with a dust equation of state
- Reconstruction and deceleration-acceleration transitions in modified gravity
This page was built for publication: Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity
