The slow-roll approximation to inflation is ultimately justified by the presence of inflationary attractors for the orbits of the solutions of the dynamical equations in phase space. There are many indications that the inflaton field couples nonminimally to the spacetime curvature: the existence of attractor points for inflation with nonminimal coupling is demonstrated, subject to a condition on the inflaton potential and the value of the coupling constant
We consider inflation in a universe with a positive cosmological constant and a nonminimally coupled...
The inflationary scenario is nowadays the most natural and simple way to solve the problems of the s...
AbstractWe explore an effective 4D cosmological model for the universe where the variable cosmologic...
We comment on the choice of the quintessence potential, examining the slow-roll approximation in a m...
The slow roll approximation is studied for cosmological models in Hyperextended Scalar-Tensor Theori...
The spectrum of curvature perturbation generated during inflation is studied in the case the inflati...
Inflation predicts the generation of cosmological perturbations. Usually, the power spectra for the ...
Results of a general study on the dynamics of cosmological scalar fields with arbitrary potentials a...
We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly...
AbstractThe spectrum of curvature perturbation generated during inflation is studied in the case the...
We study the stability of a scalar inflaton field and analyze its point attractors in the phase spac...
We demonstrate that the latest constraints on inflationary observables, namely the tensor-to-scalar ...
The possibility of mass in the context of scale-invariant, generally covariant theories, is discusse...
Using the nonlinear $\delta N$ formalism, we consider a simple exactly soluble model of multi-compon...
We consider inflation in a universe with a positive cosmological constant and a nonminimally coupled...
We consider inflation in a universe with a positive cosmological constant and a nonminimally coupled...
The inflationary scenario is nowadays the most natural and simple way to solve the problems of the s...
AbstractWe explore an effective 4D cosmological model for the universe where the variable cosmologic...
We comment on the choice of the quintessence potential, examining the slow-roll approximation in a m...
The slow roll approximation is studied for cosmological models in Hyperextended Scalar-Tensor Theori...
The spectrum of curvature perturbation generated during inflation is studied in the case the inflati...
Inflation predicts the generation of cosmological perturbations. Usually, the power spectra for the ...
Results of a general study on the dynamics of cosmological scalar fields with arbitrary potentials a...
We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly...
AbstractThe spectrum of curvature perturbation generated during inflation is studied in the case the...
We study the stability of a scalar inflaton field and analyze its point attractors in the phase spac...
We demonstrate that the latest constraints on inflationary observables, namely the tensor-to-scalar ...
The possibility of mass in the context of scale-invariant, generally covariant theories, is discusse...
Using the nonlinear $\delta N$ formalism, we consider a simple exactly soluble model of multi-compon...
We consider inflation in a universe with a positive cosmological constant and a nonminimally coupled...
We consider inflation in a universe with a positive cosmological constant and a nonminimally coupled...
The inflationary scenario is nowadays the most natural and simple way to solve the problems of the s...
AbstractWe explore an effective 4D cosmological model for the universe where the variable cosmologic...