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

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 grav...

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Main Authors: Kazunori Nakayama, Yong Tang
Format: Article
Language:English
Published: Elsevier 2020-12-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269320307802
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author Kazunori Nakayama
Yong Tang
author_facet Kazunori Nakayama
Yong Tang
author_sort Kazunori Nakayama
collection DOAJ
description 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.
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spelling doaj.art-21599f34ed9d49e8b9dcd6fdbb8709492022-12-21T20:28:57ZengElsevierPhysics Letters B0370-26932020-12-01811135977Gravitational production of hidden photon dark matter in light of the XENON1T excessKazunori Nakayama0Yong Tang1Department of Physics, Faculty of Science, The University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan; Kavli IPMU (WPI), The University of Tokyo, Kashiwa, Chiba 277-8583, Japan; Corresponding author.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences (UCAS), Beijing, China; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China; School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, UCAS, Hangzhou 310024, ChinaRecently, 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.http://www.sciencedirect.com/science/article/pii/S0370269320307802
spellingShingle Kazunori Nakayama
Yong Tang
Gravitational production of hidden photon dark matter in light of the XENON1T excess
Physics Letters B
title Gravitational production of hidden photon dark matter in light of the XENON1T excess
title_full Gravitational production of hidden photon dark matter in light of the XENON1T excess
title_fullStr Gravitational production of hidden photon dark matter in light of the XENON1T excess
title_full_unstemmed Gravitational production of hidden photon dark matter in light of the XENON1T excess
title_short Gravitational production of hidden photon dark matter in light of the XENON1T excess
title_sort gravitational production of hidden photon dark matter in light of the xenon1t excess
url http://www.sciencedirect.com/science/article/pii/S0370269320307802
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