On the Suppression of Parametric Resonance and the Viability of Tachyonic Preheating after Multi-Field Inflation
arXiv:0904.2778 · doi:10.1103/PhysRevD.79.123510
Abstract
We investigate the feasibility of explosive particle production via parametric resonance or tachyonic preheating in multi-field 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 sub-dominant, we observe a slight enhancement of tachyonic preheating. Thus, in order for preheating after multi-field inflation to be efficient, one needs to ensure that three-leg interactions are present. If no tachyonic contributions exist, we expect the old theory of reheating to be applicable.
v2: reference added, identical with PRD version, 23 pages, 3 figures
References in corpus (17)
- String Cosmology: A Review
- Theory and Numerics of Gravitational Waves from Preheating after Inflation
- Multiple field inflation
- DEFROST: A New Code for Simulating Preheating after Inflation
- Energy Transfer in Multi Field Inflation and Cosmological Perturbations
- Gravitational Waves From the End of Inflation: Computational Strategies
- Attraction towards an inflection point inflation
- Large Volume Axionic Swiss-Cheese Inflation
- Preheating after N-flation
- Multi-field Inflation with a Random Potential
- Stochastic Backgrounds of Gravitational Waves from Cosmological Sources: Techniques and Applications to Preheating
- Cosmological Moduli Dynamics
- Reheating Closed String Inflation
- Multi-Field Inflation on the Landscape
- Direct/indirect detection signatures of nonthermally produced dark matter
- Study of the preheating phase of chaotic inflation
- Fine-tuning criteria for inflation and the search for primordial gravitational waves