341 research outputs found
-essence non-minimally coupled with Gauss-Bonnet invariant for inflation
In this paper, we investigated inflationary solutions for a subclass of
Horndeski models where a scalar field is non-minimally coupled with the
Gauss-Bonnet invariant. Examples of canonical scalar field and -essence to
support the early-time acceleration are considered. The formalism to calculate
the perturbations in FRW universe and to derive the spectral index and the
tensor-to-scalar ratio is furnished.Comment: final version, accepted in Symmetry 14 page
Intermediate inflation or late time acceleration?
The expansion rate of `Intermediate inflation' lies between the exponential
and power law expansion but corresponding accelerated expansion does not start
at the onset of cosmological evolution. Present study of `Intermediate
inflation' reveals that it admits scaling solution and has got a natural exit
form it at a later epoch of cosmic evolution, leading to late time
acceleration. The corresponding scalar field responsible for such feature is
also found to be a tracker field for both gravity with canonical and some
non-canonical form of kinetic term. Thus the so called Intermediate inflation
should be considered as yet another dark energy model with asymptotic de-Sitter
expansion.Comment: 10 page
Dark energy from scalar field with Gauss Bonnet and non-minimal kinetic coupling
We study a model of scalar field with a general non-minimal kinetic coupling
to itself and to the curvature, and additional coupling to the Gauss Bonnet
4-dimensional invariant. The model presents rich cosmological dynamics and some
of its solutions are analyzed. A variety of scalar fields and potentials giving
rise to power-law expansion have been found. The dynamical equation of state is
studied for two cases, with and without free kinetic term . In both cases
phenomenologically acceptable solutions have been found. Some solutions
describe essentially dark energy behavior, and and some solutions contain the
decelerated and accelerated phases.Comment: 21 page
Modified Gravity and Cosmology
In this review we present a thoroughly comprehensive survey of recent work on
modified theories of gravity and their cosmological consequences. Amongst other
things, we cover General Relativity, Scalar-Tensor, Einstein-Aether, and
Bimetric theories, as well as TeVeS, f(R), general higher-order theories,
Horava-Lifschitz gravity, Galileons, Ghost Condensates, and models of extra
dimensions including Kaluza-Klein, Randall-Sundrum, DGP, and higher
co-dimension braneworlds. We also review attempts to construct a Parameterised
Post-Friedmannian formalism, that can be used to constrain deviations from
General Relativity in cosmology, and that is suitable for comparison with data
on the largest scales. These subjects have been intensively studied over the
past decade, largely motivated by rapid progress in the field of observational
cosmology that now allows, for the first time, precision tests of fundamental
physics on the scale of the observable Universe. The purpose of this review is
to provide a reference tool for researchers and students in cosmology and
gravitational physics, as well as a self-contained, comprehensive and
up-to-date introduction to the subject as a whole.Comment: 312 pages, 15 figure
On Bouncing and Nonsingular Solutions in Einstein-scalar-Gauss-Bonnet Cosmology
It is generically believed that higher-order curvature corrections to the
Einstein-Hilbert action might cure the curvature singularities that plague
general relativity. Here we consider Einstein-scalar-Gauss-Bonnet gravity, the
only four-dimensional, ghost-free theory with quadratic curvature terms. For
any choice of the coupling function and of the scalar potential, we show that
the theory does not allow for bouncing solutions in the flat and open Friedmann
universe. For the case of a closed universe, using a reverse-engineering
method, we explicitly provide a bouncing solution which is nevertheless
linearly unstable in the scalar gravitational sector. Moreover, we show that
the expanding, singularity-free, early-time cosmologies allowed in the theory
are unstable. These results rely only on analyticity and finiteness of
cosmological variables at early times.Comment: 9 pages, 4 figures; references and discussion added; further minor
revision, accepted to PR
Smooth crossing of line in a single scalar field model
Smooth double crossing of the phantom divide line has been
found possible with a single minimally coupled scalar field for the most simple
form of generalized k-essence cosmological model, in the presence of background
cold dark matter. Such crossing is a sufficiently late time transient phenomena
and does not have any pathological behaviour.Comment: 9 pages, 6 figure
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