Dark Photons from Perturbative Decay of a Misaligned Higgs Field

Abstract

We reconsider the production of dark photons $A^{\prime }$ as dark matter, from the perturbative decay of a dark Higgs field $h$, that is stochastically misaligned from the minimum of its potential during inflation. This is a simple and predictive framework for generating the $A^{\prime }$ relic abundance. It is constrained by structure formation, since the $A^{\prime }$ are initially boosted, and inflationary isocurvature fluctuations, which require small quartic couplings $\lambda h^4$. We identify $A^{\prime }$ masses between 100 eV and 1 GeV and gauge couplings $g\sim 10^{-15}-10^{-10}$ that are consistent in this scenario, and which become more tightly constrained if a generic level of kinetic mixing is present. The favored parameter region could be tested through future CMB or Lyman-$\alpha$ observations, and, in the presence of kinetic mixing, by direct detection experiments or diffuse soft gamma-ray searches.

Comments: 14 pages, 3 figures