Kinetic equilibration of particles produced by broad resonance preheating after inflation is almost instantaneous on the Hubble time, with an e-fold duration of about 4.4 for benchmark parameters.
Theory and applications of Mathieu equations
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Kinetic Equilibration after Preheating
Kinetic equilibration of particles produced by broad resonance preheating after inflation is almost instantaneous on the Hubble time, with an e-fold duration of about 4.4 for benchmark parameters.