AbstractDynamics of the inflaton is studied when it interacts with boson and fermion fields and in minimal supersymmetric models. This encompasses multifield inflation models, such as hybrid inflation, and typical reheating models. For much of the parameter space conducive to inflation, the inflaton is found to dissipate adequate radiation to have observational effects on density perturbations and in cases to significantly affect inflaton evolution. Thus, for many inflation models, believed to yield exclusively isentropic inflation, the parameter space now divides into regimes of isentropic and nonisentropic inflation
We discuss inflaton decays and reheating in no-scale Starobinsky-like models of inflation, calculati...
An analytic means of studying the resonant decay of the inflaton field is developed for the case of ...
Our understanding of the state of the universe between the end of inflation and big bang nucleosynth...
AbstractDynamics of the inflaton is studied when it interacts with boson and fermion fields and in m...
We study inflationary models in which the effective potential of the inflaton field does not have a ...
Within the inflationary paradigm, our patch of the universe near the end of inflation is highly homo...
We study the perspectives to extract information about the microphysical parameters that govern the ...
A new mechanism is presented which can reheat the Universe in non-oscillatory models of inflation, w...
We discuss inflaton decays and reheating in no-scale Starobinsky-like models of inflation, calculati...
I present the production of matter and radiation during reheating after inflation, considering only ...
AbstractIn non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gr...
In quasi-single field inflation there are massive fields that interact with the inflaton field. If t...
We study models in which the inflaton is coupled to two otherwise decoupled sectors, and the effect ...
We show that inflation can naturally occur at a finite temperature T>H that is sustained by dissipat...
We discuss toy models where supersymmetry is broken due to non-vanishing time-varying vacuum expecta...
We discuss inflaton decays and reheating in no-scale Starobinsky-like models of inflation, calculati...
An analytic means of studying the resonant decay of the inflaton field is developed for the case of ...
Our understanding of the state of the universe between the end of inflation and big bang nucleosynth...
AbstractDynamics of the inflaton is studied when it interacts with boson and fermion fields and in m...
We study inflationary models in which the effective potential of the inflaton field does not have a ...
Within the inflationary paradigm, our patch of the universe near the end of inflation is highly homo...
We study the perspectives to extract information about the microphysical parameters that govern the ...
A new mechanism is presented which can reheat the Universe in non-oscillatory models of inflation, w...
We discuss inflaton decays and reheating in no-scale Starobinsky-like models of inflation, calculati...
I present the production of matter and radiation during reheating after inflation, considering only ...
AbstractIn non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gr...
In quasi-single field inflation there are massive fields that interact with the inflaton field. If t...
We study models in which the inflaton is coupled to two otherwise decoupled sectors, and the effect ...
We show that inflation can naturally occur at a finite temperature T>H that is sustained by dissipat...
We discuss toy models where supersymmetry is broken due to non-vanishing time-varying vacuum expecta...
We discuss inflaton decays and reheating in no-scale Starobinsky-like models of inflation, calculati...
An analytic means of studying the resonant decay of the inflaton field is developed for the case of ...
Our understanding of the state of the universe between the end of inflation and big bang nucleosynth...