• Open Access

Probing dark photons with plasma haloscopes

Graciela B. Gelmini, Alexander J. Millar, Volodymyr Takhistov, and Edoardo Vitagliano
Phys. Rev. D 102, 043003 – Published 7 August 2020

Abstract

Dark photons (DPs) produced in the early Universe are well-motivated dark matter (DM) candidates. We show that the recently proposed tunable plasma haloscopes are particularly advantageous for DP searches. While in-medium effects suppress the DP signal in conventional searches, plasma haloscopes make use of metamaterials that enable resonant absorption of the DP by matching its mass to a tunable plasma frequency and thus enable efficient plasmon production. Using thermal field theory, we confirm the in-medium DP absorption rate within the detector. This scheme allows us to competitively explore a significant part of the DP DM parameter space in the DP mass range of 6400μeV. If a signal is observed, the observation of a daily or annual modulation of the signal would be crucial to clearly identify the signal as due to DP DM and could shed light on the production mechanism.

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  • Received 19 June 2020
  • Accepted 22 July 2020

DOI:https://doi.org/10.1103/PhysRevD.102.043003

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Graciela B. Gelmini1, Alexander J. Millar2,3, Volodymyr Takhistov1, and Edoardo Vitagliano1,*

  • 1Department of Physics and Astronomy, University of California, Los Angeles Los Angeles, California, 90095-1547, USA
  • 2The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, 10691 Stockholm, Sweden
  • 3Nordita, KTH Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, 10691 Stockholm, Sweden

  • *Corresponding author. edoardo@physics.ucla.edu

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Vol. 102, Iss. 4 — 15 August 2020

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