Add to ORKGA quantum field theory warm inflation model is presented that solves the horizon/flatness problems. The model obtains, from the elementary dynamics of particle physics, cosmological scale factor trajectories that begin in a radiation dominated regime, enter an inflationary regime and then smoothly exit back into a radiation dominated regime, with nonnegligible radiation throughout the evolution
We show that it is extremely difficult and perhaps even impossible to have inflation supported by th...
Warm inflation presents an exceptional description of the early universe cosmology. It is a scenari...
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 and flatness proble...
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 cosmological horizon/flatne...
Warm inflation is examined in a multi-field model. Solutions are obtained for expansion e-folds and ...
A dissipative mechanism is presented, which emerges in generic interacting quantum field systems and...
We show that inflation can naturally occur at a finite temperature T>H that is sustained by dissipat...
During cosmological inflation, it has been suggested that fields coupled to the inflaton can be exci...
We propose a model for early universe cosmology without the need for fundamental scalar fields. Cosm...
The warm inflation scenario is an alternative mechanism which can explain the isotropic and homogene...
We propose a model for early universe cosmology without the need for fundamental scalar fields. Cosm...
We explore the dynamics and observational predictions of the warm little inflaton scenario, presentl...
We propose a model for early universe cosmology without the need for fundamental scalar fields. Cosm...
We show that it is extremely difficult and perhaps even impossible to have inflation supported by th...
Warm inflation presents an exceptional description of the early universe cosmology. It is a scenari...
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 and flatness proble...
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 cosmological horizon/flatne...
Warm inflation is examined in a multi-field model. Solutions are obtained for expansion e-folds and ...
A dissipative mechanism is presented, which emerges in generic interacting quantum field systems and...
We show that inflation can naturally occur at a finite temperature T>H that is sustained by dissipat...
During cosmological inflation, it has been suggested that fields coupled to the inflaton can be exci...
We propose a model for early universe cosmology without the need for fundamental scalar fields. Cosm...
The warm inflation scenario is an alternative mechanism which can explain the isotropic and homogene...
We propose a model for early universe cosmology without the need for fundamental scalar fields. Cosm...
We explore the dynamics and observational predictions of the warm little inflaton scenario, presentl...
We propose a model for early universe cosmology without the need for fundamental scalar fields. Cosm...
We show that it is extremely difficult and perhaps even impossible to have inflation supported by th...
Warm inflation presents an exceptional description of the early universe cosmology. It is a scenari...
Warm inflation scenarios are studied with the dissipative coefficient computed in the equilibrium ap...