We describe a new efficient mechanism of reheating. Immediately after rolling down the rapidly moving inflaton field φ produces particles χ, which may be either bosons or fermions. This is a nonperturbative process which occurs almost instantly; no oscillations or parametric resonance is required. The effective masses of the χ particles may be very small at the moment when they are produced, but they “fatten” when the field φ increases. When the particles χ become sufficiently heavy, they rapidly decay to other, lighter particles. This leads to an almost instantaneous reheating accompanied by the production of particles with masses which may be as large as 1017–1018GeV. This mechanism works in the usual inflationary models where V(φ) has a ...
We investigate a possibility of reheating in a scenario of D-brane inflation in a warped deformed co...
We study how the universe reheats following an era of chaotic Dirac-Born-Infeld inflation, and compa...
Abstract We study models in which reheating happens only through non-perturbative processes. The ene...
We describe a new efficient mechanism of reheating. Immediately after rolling down the rapidly movin...
We perform a numerical study of the preheating mechanism of particle production in models of quintes...
We study inflationary models in which the effective potential of the inflaton field does not have a ...
We study particle production at the preheating era in inflation models with nonminimal coupling ξφ2R...
Different well-known ways to reheat the Universe, such as instant preheating, the creation of partic...
A numerical study of the non-oscillatory reheating mechanism in a quintessential inflation context s...
During the last ten years a detailed investigation of preheating was performed for chaotic inflation...
A new mechanism is presented which can reheat the Universe in non-oscillatory models of inflation, w...
In inflationary cosmology, the particles constituting the Universe are created after inflation in th...
A numerical study of the non-oscillatory reheating mechanism in a quintessential inflation context s...
International audienceWhereas preheating after chaotic and hybrid inflation models has been abundant...
Inflationary reheating via resonant production of non-minimally coupled scalar particles with only g...
We investigate a possibility of reheating in a scenario of D-brane inflation in a warped deformed co...
We study how the universe reheats following an era of chaotic Dirac-Born-Infeld inflation, and compa...
Abstract We study models in which reheating happens only through non-perturbative processes. The ene...
We describe a new efficient mechanism of reheating. Immediately after rolling down the rapidly movin...
We perform a numerical study of the preheating mechanism of particle production in models of quintes...
We study inflationary models in which the effective potential of the inflaton field does not have a ...
We study particle production at the preheating era in inflation models with nonminimal coupling ξφ2R...
Different well-known ways to reheat the Universe, such as instant preheating, the creation of partic...
A numerical study of the non-oscillatory reheating mechanism in a quintessential inflation context s...
During the last ten years a detailed investigation of preheating was performed for chaotic inflation...
A new mechanism is presented which can reheat the Universe in non-oscillatory models of inflation, w...
In inflationary cosmology, the particles constituting the Universe are created after inflation in th...
A numerical study of the non-oscillatory reheating mechanism in a quintessential inflation context s...
International audienceWhereas preheating after chaotic and hybrid inflation models has been abundant...
Inflationary reheating via resonant production of non-minimally coupled scalar particles with only g...
We investigate a possibility of reheating in a scenario of D-brane inflation in a warped deformed co...
We study how the universe reheats following an era of chaotic Dirac-Born-Infeld inflation, and compa...
Abstract We study models in which reheating happens only through non-perturbative processes. The ene...