Relic abundance of dark photon dark matter

Prateek Agrawal, Naoya Kitajima, Matthew Reece, Toyokazu Sekiguchi, Fuminobu Takahashi

研究成果: Article査読

70 被引用数 (Scopus)

抄録

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 10−20eV. 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, mγ /ma=O(10−3−1), 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.

本文言語English
論文番号135136
ジャーナルPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
801
DOI
出版ステータスPublished - 2020 2 10

ASJC Scopus subject areas

  • 核物理学および高エネルギー物理学

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