A dissipative mechanism is presented, which emerges in generic interacting quantum field systems and which leads to robust warm inflation. An explicit example is considered, where using typical parameter values, it is shown that considerable radiation can be produced during inflation. The extension of our results to expanding spacetime also is discussed
AbstractThe amplitude of primordial curvature perturbations is enhanced when a radiation bath at a t...
An energetic justification of a thermal component during inflation is given. The thermal component c...
We show that, in warm inflation, the nearly constant Hubble rate and temperature lead to an adiabat...
AbstractA dissipative mechanism is presented, which emerges in generic interacting quantum field sys...
A quantum field theory warm inflation model is presented that solves the cosmological horizon/flatne...
The warm inflation scenario is an alternative mechanism which can explain the isotropic and homogene...
Warm inflation is examined in a multi-field model. Solutions are obtained for expansion e-folds and ...
We show that it is extremely difficult and perhaps even impossible to have inflation supported by th...
Warm inflation scenarios are studied with the dissipative coefficient computed in the equilibrium ap...
A quantum field theory warm inflation model is presented that solves the horizon/flatness problems. ...
Warm inflation presents an exceptional description of the early universe cosmology. It is a scenari...
A quantum field theory warm inflation model is presented that solves the horizon and flatness proble...
A quantum field theory warm inflation model is presented that solves the horizon and flatness proble...
We show that inflation can naturally occur at a finite temperature T>H that is sustained by dissipat...
The current status of early universe cosmology can be summarized as precision, but inherently limite...
AbstractThe amplitude of primordial curvature perturbations is enhanced when a radiation bath at a t...
An energetic justification of a thermal component during inflation is given. The thermal component c...
We show that, in warm inflation, the nearly constant Hubble rate and temperature lead to an adiabat...
AbstractA dissipative mechanism is presented, which emerges in generic interacting quantum field sys...
A quantum field theory warm inflation model is presented that solves the cosmological horizon/flatne...
The warm inflation scenario is an alternative mechanism which can explain the isotropic and homogene...
Warm inflation is examined in a multi-field model. Solutions are obtained for expansion e-folds and ...
We show that it is extremely difficult and perhaps even impossible to have inflation supported by th...
Warm inflation scenarios are studied with the dissipative coefficient computed in the equilibrium ap...
A quantum field theory warm inflation model is presented that solves the horizon/flatness problems. ...
Warm inflation presents an exceptional description of the early universe cosmology. It is a scenari...
A quantum field theory warm inflation model is presented that solves the horizon and flatness proble...
A quantum field theory warm inflation model is presented that solves the horizon and flatness proble...
We show that inflation can naturally occur at a finite temperature T>H that is sustained by dissipat...
The current status of early universe cosmology can be summarized as precision, but inherently limite...
AbstractThe amplitude of primordial curvature perturbations is enhanced when a radiation bath at a t...
An energetic justification of a thermal component during inflation is given. The thermal component c...
We show that, in warm inflation, the nearly constant Hubble rate and temperature lead to an adiabat...