Relic Abundance of Dark Photon Dark Matter
Abstract
We present a new mechanism for producing the correct relic abundance of dark photon dark matter over a wide range of its mass, extending down to . The dark matter abundance is initially stored in an axion which is misaligned from its minimum. When the axion starts oscillating, it efficiently transfers its energy into dark photons via a tachyonic instability. If the dark photon mass is within a few orders of magnitude of the axion mass, , then dark photons make up the dominant form of dark matter today. We present a numerical lattice simulation for a benchmark model that explicitly realizes our mechanism. This mechanism firms up the motivation for a number of experiments searching for dark photon dark matter.
Keywords
Cite
@article{arxiv.1810.07188,
title = {Relic Abundance of Dark Photon Dark Matter},
author = {Prateek Agrawal and Naoya Kitajima and Matthew Reece and Toyokazu Sekiguchi and Fuminobu Takahashi},
journal= {arXiv preprint arXiv:1810.07188},
year = {2019}
}
Comments
5 pages + supplementary material, 4 figures