Anisotropic stress and stability in modified gravity models
@article{Saltas2010AnisotropicSA, title={Anisotropic stress and stability in modified gravity models}, author={Ippocratis D. Saltas and Martin Kunz}, journal={Physical Review D}, year={2010}, volume={83}, pages={064042} }
The existence of anisotropic stress of a purely geometrical origin seems to be a characteristic of higher order gravity models, and has been suggested as a probe to test these models observationally, for example, in weak lensing experiments. In this paper, we seek to find a class of higher order gravity models of f(R,G) type that would give us a zero anisotropic stress and study the consequences for the viability of the actual model. For the special case of a de Sitter background, we identify a…
31 Citations
Nonlinear cosmological consistency relations and effective matter stresses
- Physics
- 2012
We propose a fully nonlinear framework to construct consistency relations for testing generic cosmological scenarios using the evolution of large scale structure. It is based on the covariant…
On the stability of the cosmological solutions in f(R, G) gravity
- Physics
- 2012
Modified gravity is one of the most promising candidates for explaining the current accelerating expansion of the Universe, and even its unification with the inflationary epoch. Nevertheless, the…
Anisotropic stress as a signature of nonstandard propagation of gravitational waves.
- Physics, GeologyPhysical review letters
- 2014
It is shown that in cosmological solutions of very general classes of models extending gravity-all scalar-tensor theories, Einstein-aether models, and bimetric massive gravity-a direct correspondence exists between perfect fluids apparently carrying anisotropic stress and a modification in the propagation of gravitational waves.
Model-independent constraints on the cosmological anisotropic stress
- Physics
- 2014
= / is a key variable in the characterisation of the physical origin of the dark energy, as it allows to test for a non-minimal coupling of the dark sector to gravity in the Jordan frame. It is…
Effects of anisotropic stress in interacting dark matter – dark energy scenarios
- PhysicsMonthly Notices of the Royal Astronomical Society
- 2018
We study a novel interacting dark energy − dark matter scenario where the anisotropic stress of the large-scale inhomogeneities is considered. The dark energy has a constant equation of state and the…
Consistent perturbations in an imperfect fluid
- Physics
- 2013
We present a new prescription for analysing cosmological perturbations in a more-general class of scalar-field dark-energy models where the energy-momentum tensor has an imperfect-fluid form. This…
Consistent perturbations in an imperfect fluid
- Physics
- 2013
We present a new prescription for analysing cosmological perturbations in a more-general class of scalar-field dark-energy models where the energy-momentum tensor has an imperfect-fluid form. This…
Thermal relic abundance and anisotropy due to modified gravity
- Physics
- 2014
Alternative cosmologies, based on extensions of General Relativity, predict modified thermal histories in the early universe during the pre Big Bang Nucleosynthesis (BBN) era. When the expansion rate…
General relativistic N -body simulations in the weak field limit
- Physics
- 2013
We develop a formalism for general relativistic $N$-body simulations in the weak field regime, suitable for cosmological applications. The problem is kept tractable by retaining the metric…
References
SHOWING 1-10 OF 77 REFERENCES
Matter instabilities in general Gauss-Bonnet gravity
- Physics
- 2010
We study the evolution of cosmological perturbations in f(G) gravity, where the Lagrangian is the sum of a Ricci scalar R and an arbitrary function f in terms of a Gauss-Bonnet term G. We derive the…
Disappearing cosmological constant in f(R) gravity
- Physics
- 2007
For higher-derivative f(R) gravity, where R is the Ricci scalar, a class of models is proposed, which produce viable cosmology different from the ACDM at recent times and satisfy cosmological, Solar…
Singularity problem with f(R) models for dark energy.
- PhysicsPhysical review letters
- 2008
There is a curvature singularity problem appearing on the nonlinear level that generally plagues f(R) models that modify Einstein gravity in the infrared, and the viability of many f( R) models in the current literature will have to be reevaluated.
Dark energy cosmology from higher-order, string-inspired gravity, and its reconstruction
- Physics
- 2006
In this paper we investigate the cosmological effects of modified gravity with string curvature corrections added to the Einstein-Hilbert action in the presence of a dynamically evolving scalar field…
A Parameterized Post-Friedmann Framework for Modified Gravity
- Physics
- 2007
We develop a parametrized post-Friedmann (PPF) framework which describes three regimes of modified gravity models that accelerate the expansion without dark energy. On large scales, the evolution of…
Ghosts, instabilities, and superluminal propagation in modified gravity models
- Mathematics
- 2006
We consider modified gravity models involving inverse powers of fourth order curvature invariants. Using these models’ equivalence to the theory of a scalar field coupled to a linear combination of…
Solar system constraints on f(G) gravity models
- Physics, Geology
- 2009
We discuss solar system constraints on f(G) gravity models, where f is a function of the Gauss-Bonnet term G. We focus on cosmologically viable f(G) models that can be responsible for late-time…
f(R) Theories Of Gravity
- Physics
- 2010
Modified gravity theories have received increased attention lately due to combined motivation coming from high-energy physics, cosmology, and astrophysics. Among numerous alternatives to Einstein's…