We bring together the physics of preheating, following a period of inflation, and the dynamics of non-topological solitons, namely oscillons. We show that the oscillating condensate that makes up an oscillon can be an efficient engine for producing heavy fermions, just as a homogeneous condensate is known for doing the same. This then allows heavy fermions to be produced when the energy scale of the Universe has dropped below the scale naturally associated to the fermions
We describe a new efficient mechanism of reheating. Immediately after rolling down the rapidly movin...
Large amplitude oscillation of cosmic field that may occur right after inflation and in the decay pr...
We discuss toy models where supersymmetry is broken due to non-vanishing time-varying vacuum expecta...
We bring together the physics of preheating, following a period of inflation, and the dynamics of no...
Coherent oscillations of the inflaton field at the end of inflation can parametrically excite fermio...
We present a complete computation of the inflaton decay into very massive fermions during preheating...
Oscillons are long-lived, localized excitations of nonlinear scalar fields which may be copiously pr...
At the end of inflation, the coherent oscillations of the inflation field may resonantly amplify the...
Fermion creation during preheating in the presence of multiple scalar fields exhibits a range of int...
Non-perturbative production of fermions after chaotic inflation has been the object of several studi...
We study inflationary models in which the effective potential of the inflaton field does not have a ...
We present a complete computation of the inflaton decay into very massive fermions during preheating...
We study the production of gravitinos during the preheating era after inflation by means of the non-...
AbstractParticle production in the background of an external classical oscillating field is a key pr...
Certain inflation models undergo pre-heating, in which inflaton oscillations can drive parametric re...
We describe a new efficient mechanism of reheating. Immediately after rolling down the rapidly movin...
Large amplitude oscillation of cosmic field that may occur right after inflation and in the decay pr...
We discuss toy models where supersymmetry is broken due to non-vanishing time-varying vacuum expecta...
We bring together the physics of preheating, following a period of inflation, and the dynamics of no...
Coherent oscillations of the inflaton field at the end of inflation can parametrically excite fermio...
We present a complete computation of the inflaton decay into very massive fermions during preheating...
Oscillons are long-lived, localized excitations of nonlinear scalar fields which may be copiously pr...
At the end of inflation, the coherent oscillations of the inflation field may resonantly amplify the...
Fermion creation during preheating in the presence of multiple scalar fields exhibits a range of int...
Non-perturbative production of fermions after chaotic inflation has been the object of several studi...
We study inflationary models in which the effective potential of the inflaton field does not have a ...
We present a complete computation of the inflaton decay into very massive fermions during preheating...
We study the production of gravitinos during the preheating era after inflation by means of the non-...
AbstractParticle production in the background of an external classical oscillating field is a key pr...
Certain inflation models undergo pre-heating, in which inflaton oscillations can drive parametric re...
We describe a new efficient mechanism of reheating. Immediately after rolling down the rapidly movin...
Large amplitude oscillation of cosmic field that may occur right after inflation and in the decay pr...
We discuss toy models where supersymmetry is broken due to non-vanishing time-varying vacuum expecta...