Gravitational production of hidden photon dark matter in light of the XENON1T excess

研究成果: Article査読

22 被引用数 (Scopus)

抄録

Recently, the XENON1T experiment has reported an excess in the electronic recoil events. The excess is consistent with the interpretation of absorption of 3 keV bosonic dark matter, for example, hidden photon dark matter with kinetic mixing of the order of 10−15. We point out that the minimally gravitational production provides a viable mechanism for obtaining a correct relic hidden photon abundance. We present parameter dependence of the hidden photon dark matter abundance on the inflationary scale Hinf and also the reheating temperature TR. We show that the inflationary Hubble scale and reheating temperature are both bounded from below, Hinf≳7×1011 GeV,TR≳102 GeV. In particular, the high-scale inflation is consistent with 3 keV hidden photon dark matter.

本文言語English
論文番号135977
ジャーナルPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
811
DOI
出版ステータスPublished - 2020 12月 10
外部発表はい

ASJC Scopus subject areas

  • 核物理学および高エネルギー物理学

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