In the framework of chaotic inflation we study the case of a massive scalar field using a semiclassical approach. We derive the energy density fluctuations in the infrared sector generated by matter field and gauge-invariant metric fluctuations by means of a different method. We find that the super Hubble density fluctuations increase during inflation for a massive scalar field, in agreement with the result obtained in a previous work in which a power-law expanding universe was considered
Recently multi-field inflation models that can produce large scalar fluctuations on small scales hav...
We consider inflation driven by the energy density of a conventional scalar field minimally coupled ...
The energy and time scales during the inflationary stage of the universe calls for an out of equilib...
In the framework of inflationary cosmology I study some aspects of nonequilibrium thermodynamics for...
We consider the effect of quantizing the homogeneous mode of a scalar field on inflation. It is show...
After a brief review of the theory of cosmological perturbations, I highlight some recent progress i...
We study chaotic inflation driven by a real, massive, homogeneous minimally coupled scalar field in ...
The physics of the inflationary universe requires the study of the out of equilibrium evolution of q...
We investigate the cosmological perturbation of two-scalar field model during the reheating phase af...
A calculation of the one-mode occupation numbers for vacuum fluctuations of massive fields in De Sit...
The physics during the inflationary stage of the universe is of quantum nature involving extremely h...
An analysis of the decoherence of quantum fluctuations shows that production of classical adiabatic ...
We investigate the scalar perturbation produced at the pre-inflationary stage driven by a massive sc...
We investigate the scalar perturbation of the inflation model driven by a massive scalar field in Ed...
We discuss metric perturbations produced during a period of inflation in the early universe where tw...
Recently multi-field inflation models that can produce large scalar fluctuations on small scales hav...
We consider inflation driven by the energy density of a conventional scalar field minimally coupled ...
The energy and time scales during the inflationary stage of the universe calls for an out of equilib...
In the framework of inflationary cosmology I study some aspects of nonequilibrium thermodynamics for...
We consider the effect of quantizing the homogeneous mode of a scalar field on inflation. It is show...
After a brief review of the theory of cosmological perturbations, I highlight some recent progress i...
We study chaotic inflation driven by a real, massive, homogeneous minimally coupled scalar field in ...
The physics of the inflationary universe requires the study of the out of equilibrium evolution of q...
We investigate the cosmological perturbation of two-scalar field model during the reheating phase af...
A calculation of the one-mode occupation numbers for vacuum fluctuations of massive fields in De Sit...
The physics during the inflationary stage of the universe is of quantum nature involving extremely h...
An analysis of the decoherence of quantum fluctuations shows that production of classical adiabatic ...
We investigate the scalar perturbation produced at the pre-inflationary stage driven by a massive sc...
We investigate the scalar perturbation of the inflation model driven by a massive scalar field in Ed...
We discuss metric perturbations produced during a period of inflation in the early universe where tw...
Recently multi-field inflation models that can produce large scalar fluctuations on small scales hav...
We consider inflation driven by the energy density of a conventional scalar field minimally coupled ...
The energy and time scales during the inflationary stage of the universe calls for an out of equilib...