International audienceWe investigate the feasibility of explosive particle production via parametric resonance or tachyonic preheating in multifield inflationary models by means of lattice simulations. We observe a strong suppression of resonances in the presence of four-leg interactions between the inflaton fields and a scalar matter field, leading to insufficient preheating when more than two inflatons couple to the same matter field. This suppression is caused by a dephasing of the inflatons that increases the effective mass of the matter field. Including three-leg interactions leads to tachyonic preheating, which is not suppressed by an increase in the number of fields. If four-leg interactions are subdominant, we observe a slight enhan...
Tachyonic preheating is realized when the inflaton repeatedly returns to a convex region of the pote...
The Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Univers...
The parametric resonance responsible for preheating after inflation will end when self-interactions ...
International audienceWe investigate the feasibility of explosive particle production via parametric...
4 pages, proceedings for work presented at Cargese 2008, COSMO08 and UniverseNet second annual meeti...
We investigate the effects of bosonic trilinear interactions in preheating after chaotic inflation. ...
We study preheating after hilltop inflation where the inflaton couples to another scalar field, e.g....
We investigate the effects of bosonic trilinear interactions in preheating after chaotic inflation. ...
In inflationary cosmology, the particles constituting the Universe are created after inflation in th...
We study the postinflation dynamics of multifield models involving nonminimal couplings using lattic...
© 2020 American Physical Society. We have conducted extensive lattice simulations to study the posti...
We have conducted extensive lattice simulations to study the post-inflation dynamics of multifield m...
International audienceWhereas preheating after chaotic and hybrid inflation models has been abundant...
We study particle production at the preheating era in inflation models with nonminimal coupling ξφ2R...
We study preheating following Higgs inflation in the Palatini formulation of gravity. We numerically...
Tachyonic preheating is realized when the inflaton repeatedly returns to a convex region of the pote...
The Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Univers...
The parametric resonance responsible for preheating after inflation will end when self-interactions ...
International audienceWe investigate the feasibility of explosive particle production via parametric...
4 pages, proceedings for work presented at Cargese 2008, COSMO08 and UniverseNet second annual meeti...
We investigate the effects of bosonic trilinear interactions in preheating after chaotic inflation. ...
We study preheating after hilltop inflation where the inflaton couples to another scalar field, e.g....
We investigate the effects of bosonic trilinear interactions in preheating after chaotic inflation. ...
In inflationary cosmology, the particles constituting the Universe are created after inflation in th...
We study the postinflation dynamics of multifield models involving nonminimal couplings using lattic...
© 2020 American Physical Society. We have conducted extensive lattice simulations to study the posti...
We have conducted extensive lattice simulations to study the post-inflation dynamics of multifield m...
International audienceWhereas preheating after chaotic and hybrid inflation models has been abundant...
We study particle production at the preheating era in inflation models with nonminimal coupling ξφ2R...
We study preheating following Higgs inflation in the Palatini formulation of gravity. We numerically...
Tachyonic preheating is realized when the inflaton repeatedly returns to a convex region of the pote...
The Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Univers...
The parametric resonance responsible for preheating after inflation will end when self-interactions ...