Gravitational wave background from non-Abelian reheating after axion-like inflation

Abstract

A pseudoscalar inflaton $\phi$, coupled to the topological charge density $F\tilde{F}$ of a non-Abelian sector, can decay to gauge bosons ($\phi \to gg$), which may thermalize rapidly. The friction felt by $\phi$ is then increased by non-Abelian "strong sphalerons", leading to a self-amplifying process that can efficiently heat up the medium. We determine a lower bound for the gravitational wave production rate from such a process, originating via hydrodynamic fluctuations and particle collisions, in terms of a minimal number of parameters. Only a moderate fraction of energy density is converted to gravitational waves, suggesting that non-Abelian models may avoid the overproduction observed in some Abelian cases.

18 pages. v2: clarifications added

References in corpus (10)

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Cited by in corpus (2)

• Shape of the hot topological charge density spectral function
• Maximal temperature of strongly-coupled dark sectors