Warm inflation with a heavy QCD axion

Abstract

We propose the first model of warm inflation in which the particle production emerges directly from coupling the inflaton to Standard Model particles. Warm inflation, an early epoch of sustained accelerated expansion at finite temperature, is a compelling alternative to cold inflation, with distinct predictions for inflationary observables such as the amplitude of fluctuations, the spectral tilt, the tensor-to-scalar ratio, and non-gaussianities. In our model a heavy QCD axion acts as the warm inflaton whose coupling to Standard Model gluons sources the thermal bath during warm inflation. Axion-like couplings to non-Abelian gauge bosons have been considered before as a successful microphysical theory with emerging thermal friction that can maintain finite temperature during inflation via sphaleron heating. However, the presence of light fermions charged under the non-Abelian group suppresses particle production, hindering a realization of warm inflation by coupling to QCD. We point out that the Standard Model quarks can be heavy during warm inflation if the Higgs field resides in a high-energy second minimum which restores efficient sphaleron heating. A subsequent large reheating temperature is required to allow the Higgs field to relax to its electroweak minimum. Exploring a scenario in which hybrid warm inflation provides the large reheating temperature, we show that future collider and beam dump experiments have discovery potential for a heavy QCD axion taking the role of the warm inflaton.

28 pages, 7 figures, fixed typos, matches journal version

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• Warm Inflation with the Standard Model
• Viability of warm inflation with standard model interactions
• WI2easy: warm inflation dynamics made easy
• Warm multi natural inflation
• No Warm Inflation From a Vanilla Axion
• Constraints on the Sharpness of the Curvature Power Spectrum
• On the prospects of thermalization of axion-SU(2) inflation
• Warm Inflation in $f(Q)$ gravity
• AliCPT Sensitivity to Cosmic Reheating
• Not So Minimal Warm Inflation
• Scalaron-driven Dark Matter during Warm Inflation via UV Freeze--in