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Nonlinear Dynamics of Preheating after Multifield Inflation with Nonminimal Couplings
Rachel Nguyen1, Jorinde van de Vis2, Evangelos I Sfakianakis2,3
1Department of Physics, Kenyon College, Gambier, Ohio 43022, USA.
We studied multifield models with nonminimal couplings using lattice simulations. Large couplings cause rapid preheating, suppressing multifield signatures and aligning predictions with cosmic microwave background observations.
Area of Science:
- Cosmology
- Theoretical Physics
- Particle Physics
Background:
- Postinflationary dynamics in multifield models are crucial for understanding the early universe.
- Nonminimal couplings introduce nonlinear effects that require advanced simulation techniques.
- Understanding thermalization and preheating is key to connecting theory with observational data.
Purpose of the Study:
- To investigate the postinflationary dynamics of multifield models with nonminimal couplings.
- To capture nonlinear effects such as backreaction and rescattering using lattice simulations.
- To determine the impact of nonminimal couplings on preheating, thermalization timescales, and primordial observables.
Main Methods:
- Utilized lattice simulations to model multifield dynamics with nonminimal couplings.
- Measured the effective equation of state and timescales for thermalization.
- Analyzed the influence of varying nonminimal coupling constants on particle production and attractor behavior.
Main Results:
- Identified efficient particle production and nearly instantaneous preheating for large nonminimal coupling constants.
- Observed the persistence of strong single-field attractor behavior throughout preheating.
- Found that multifield signatures are suppressed, leading to predictions consistent with observations.
Conclusions:
- Nonminimal couplings significantly impact early universe dynamics, leading to rapid preheating.
- The observed suppression of multifield signatures ensures that model predictions align with cosmic microwave background anisotropy data.
- These findings refine our understanding of primordial perturbation spectra in multifield cosmological models.
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