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arxiv: hep-ph/9904409 · v4 · submitted 1999-04-20 · ✦ hep-ph · astro-ph· gr-qc· hep-th

Warm Inflation in the Adiabatic Regime- a Model, an Existence Proof for Inflationary Dynamics in Quantum Field Theory

classification ✦ hep-ph astro-phgr-qchep-th
keywords modelregimeadiabaticdynamicsdensitye-foldsequilibriumexpansion
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Warm inflation is examined in a multi-field model. Solutions are obtained for expansion e-folds and scalar density perturbations. Nonequilibrium dynamics is restricted to a regime that is displaced only slightly from thermal equilibrium and in which all macroscopic motion is adiabatic. In such a regime, nonequilibrium dynamics is well defined, provided macroscopic motions that displace the thermal equilibrium state occur sufficiently slow. The solution has adjustable parameters that permit observational consistency with respect to expansion e-folds and density perturbations in the full adiabatic regime, thus insuring a valid solution regime. For particle physics, the model is nonstandard since it requires a large number of fields, $> 10^4$. A particle physics/string interpretation of the model and solutions is discussed, which can accommodate the large field number requirement.

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  1. Warm Inflation with Pseudo-scalar Couplings

    hep-ph 2025-05 unverdicted novelty 7.0

    Warm inflation models with pseudo-scalar couplings require inclusion of induced chemical potentials that make the thermal friction-fluctuation relation model-dependent rather than universal.