Structure growth in f ( R ) theories of gravity with a dust equation of state

DOI10.1088/0264-9381/26/23/235018zbMath1181.83152arXiv0809.3673OpenAlexW3125301318WikidataQ62562805 ScholiaQ62562805MaRDI QIDQ5850893

Peter K. S. Dunsby, Sante Carloni, Kishore N. Ananda

Publication date: 20 January 2010

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0809.3673

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (9)

Irrotational-fluid cosmologies in fourth-order gravity ⋮ Chaplygin-gas solutions of f(R) gravity ⋮ Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity ⋮ Multifluid cosmology in f(G) gravity ⋮ Reconstructing f(R) gravity from a Chaplygin scalar field in de Sitter spacetimes ⋮ Scalar–tensor f(R) gravity model for late-time universe ⋮ The role of initial conditions and parameters of the model in evolution of the universe. Case study: Brans-Dicke theory in Einstein frame ⋮ Cosmological perturbations in f(G) gravity ⋮ On multifluid perturbations in scalar–tensor cosmology

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