Axion Inflation with a Massive Abelian Gauge Field

Abstract

An axial coupling between an inflaton and an Abelian gauge field can trigger the tachyonic amplification of one gauge-field helicity. For a massless vector, modes with physical momentum $k/a\sim |\xi|H$ are enhanced by approximately $\exp(\pi|\xi|)$, and sufficiently efficient production can provide substantial friction for the homogeneous inflaton. We extend this mechanism to a vector of mass $m$. The instability is present only for $|\xi|>\bar m\equiv m/H$, and in the heavy regime the mode amplitude scales as $\exp[\pi(|\xi|-\bar m)]$. Because the amplified modes remain well inside the Hubble radius when $\bar m\gg1$, their contribution to long-wavelength curvature perturbations is power-law suppressed at fixed background backreaction. In the weak-backreaction regime we obtain ${\cal P}^{\rm id}_{\zeta} \propto \bar m^{-2}$, while including the gauge-induced friction of scalar perturbations gives the scaling ${\cal P}^{\rm id}_{\zeta}\propto \bar{m}^{-3}$. These estimates indicate that ${\cal P}^{\rm id}_{\zeta}\lesssim 10^{-9}$ on CMB scales should be compatible with gauge field backreaction for $\bar{m}$ larger than order a few hundred. We test the analytical mode functions and backreaction estimates with the first lattice simulations based on a massive-vector extension of the \texttt{Pencil Code}, including simulations in the strongly backreacting regime.