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Limits from the FUNK experiment on the mixing strength of hidden-photon dark matter in the visible and near-ultraviolet wavelength range

Arnaud Andrianavalomahefa, Christoph M. Schäfer, Darko Veberič, R. Engel, Thomas Schwetz, Hermann-Josef Mathes, K. Daumiller, M. Roth, David Schmidt, R. Ulrich, Babette Döbrich, Joerg Jaeckel, M. Kowalski, A. Lindner, Javier Redondo, The FUNK Experiment

2020Physical review. D/Physical review. D.52 citationsDOIOpen Access PDF

Abstract

We present results from the FUNK experiment in the search for hidden-photon dark matter. Near the surface of a mirror, hidden photons may be converted into ordinary photons. These photons are emitted perpendicularly to the surface and have an energy equal to the mass of the dark matter hidden photon. Our experimental setup consists of a large, spherical mirror with an area of more than $14\text{ }\text{ }{\mathrm{m}}^{2}$, which concentrates the emitted photons into its central point. Using a detector sensitive to visible and near-UV photons, we can exclude a kinetic-mixing coupling of stronger than $\ensuremath{\chi}\ensuremath{\approx}{10}^{\ensuremath{-}12}$ in the mass range of 2.5 to 7 eV, assuming hidden photons comprise all of the dark matter. The experimental setup and analysis used to obtain this limit are discussed in detail.

Topics & Concepts

PhotonPhysicsDark matterRange (aeronautics)OpticsAstrophysicsMaterials scienceComposite materialDark Matter and Cosmic PhenomenaRandom lasers and scattering mediaCosmology and Gravitation Theories
Limits from the FUNK experiment on the mixing strength of hidden-photon dark matter in the visible and near-ultraviolet wavelength range | Litcius