We extend the concept of quintessence to a flat nonminimally coupled scalar - tensor theories of gravity. By means of Noether's symmetries for the cosmological pointlike Lagrangian L, it is possible to exhibit exact solutions for a class of models depending on a free parameter s. This parameter comes out in the relationship existing between the coupling F(\phi) and the potential V(\phi) because of such a symmetry for L. When inverse power law potentials are taken in account, a whole family of exact solutions parametrized by such an s is proposed as a class of tracker fields, and some considerations are made about them
Scalar fields with inverse power-law effective potentials may provide a negative pressure component ...
The most recent cosmological data point in the direction of a cosmologicalconstant dominated univers...
A new component of the cosmic medium, a light scalar field or ''quintessence '', has been proposed r...
We extend the concept of quintessence to flat nonminimally coupled scalar-tensor theories of gravity...
We extend the concept of quintessence to flat nonminimally coupled scalar-tensor theories of gravity...
We extend the concept of quintessence to flat nonminimally coupled scalar-tensor theories of gravity...
We investigate the cosmological role of a tracking field φ in extended quintessence scenarios, where...
We investigate some aspects of quintessence models with a non-minimally coupled scalar field and in ...
We investigate the cosmological role of a tracking field \u3c6 in extended quintessence scenarios, w...
A generalized quintessence model is presented which corresponds to a richer vacuum structure that, b...
We study the cosmological role of a Tracking Field $\phi$ in Extended Quintessence scenarios (TEQ), ...
A substantial fraction of the energy density of the universe may consist of quintessence in the form...
We revise the stability of the tracking solutions and briefly review the potentials of quintessence ...
We investigate the evolution of matter density perturbations and some properties of the peculiar vel...
We study quintessence cosmologies in the context of scalar-tensor theories of gravity, where a scala...
Scalar fields with inverse power-law effective potentials may provide a negative pressure component ...
The most recent cosmological data point in the direction of a cosmologicalconstant dominated univers...
A new component of the cosmic medium, a light scalar field or ''quintessence '', has been proposed r...
We extend the concept of quintessence to flat nonminimally coupled scalar-tensor theories of gravity...
We extend the concept of quintessence to flat nonminimally coupled scalar-tensor theories of gravity...
We extend the concept of quintessence to flat nonminimally coupled scalar-tensor theories of gravity...
We investigate the cosmological role of a tracking field φ in extended quintessence scenarios, where...
We investigate some aspects of quintessence models with a non-minimally coupled scalar field and in ...
We investigate the cosmological role of a tracking field \u3c6 in extended quintessence scenarios, w...
A generalized quintessence model is presented which corresponds to a richer vacuum structure that, b...
We study the cosmological role of a Tracking Field $\phi$ in Extended Quintessence scenarios (TEQ), ...
A substantial fraction of the energy density of the universe may consist of quintessence in the form...
We revise the stability of the tracking solutions and briefly review the potentials of quintessence ...
We investigate the evolution of matter density perturbations and some properties of the peculiar vel...
We study quintessence cosmologies in the context of scalar-tensor theories of gravity, where a scala...
Scalar fields with inverse power-law effective potentials may provide a negative pressure component ...
The most recent cosmological data point in the direction of a cosmologicalconstant dominated univers...
A new component of the cosmic medium, a light scalar field or ''quintessence '', has been proposed r...