AbstractThe cosmological dynamics of minimally coupled scalar field that couple to the background matter with thermal interactions is investigated in exponential potential. The conditions for the existence and stability of various critical points as well as their cosmological implications are obtained. Although we show that the effects of thermal interaction such as depressing the equation-of-state parameter of quintessence, is only important at the early time, the evolution of equation-of-state parameter of quintessence is manifested. The upper bound is required on the coupling between quintessence and relativistic relic particles such as photons and neutrinos
We investigate the evolution of matter density perturbations and some properties of the peculiar vel...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
We consider the interacting holographic dark energy with new infrared cutoff (involving Hubble param...
AbstractThe cosmological dynamics of minimally coupled scalar field that couple to the background ma...
We present the dynamical analysis for interacting quintessence, considering linear cosmological pert...
We apply the tools of the dynamical system theory in order to revisit and uncover the structure of a...
We study a class of extended quintessence cosmologies where the scalar field playing the role of the...
We present general exact solutions for two classes of exponential potentials in a scalar field model...
We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark ma...
We study quintessence cosmologies in the context of scalar-tensor theories of gravity, where a scala...
A new component of the cosmic medium, a light scalar field or ''quintessence '', has been proposed r...
We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark ma...
In the light of the recent observations of type la supernovae (SNe Ia) suggesting an accelerating Un...
We study quintessence cosmologies in the context of scalar-tensor theories of gravity, where a scala...
Whereas the recent observations of type Ia supentovae (SNe Ia) reveal the universe is accelerating, ...
We investigate the evolution of matter density perturbations and some properties of the peculiar vel...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
We consider the interacting holographic dark energy with new infrared cutoff (involving Hubble param...
AbstractThe cosmological dynamics of minimally coupled scalar field that couple to the background ma...
We present the dynamical analysis for interacting quintessence, considering linear cosmological pert...
We apply the tools of the dynamical system theory in order to revisit and uncover the structure of a...
We study a class of extended quintessence cosmologies where the scalar field playing the role of the...
We present general exact solutions for two classes of exponential potentials in a scalar field model...
We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark ma...
We study quintessence cosmologies in the context of scalar-tensor theories of gravity, where a scala...
A new component of the cosmic medium, a light scalar field or ''quintessence '', has been proposed r...
We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark ma...
In the light of the recent observations of type la supernovae (SNe Ia) suggesting an accelerating Un...
We study quintessence cosmologies in the context of scalar-tensor theories of gravity, where a scala...
Whereas the recent observations of type Ia supentovae (SNe Ia) reveal the universe is accelerating, ...
We investigate the evolution of matter density perturbations and some properties of the peculiar vel...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
We consider the interacting holographic dark energy with new infrared cutoff (involving Hubble param...