English

First search for dark photon dark matter with a MADMAX prototype

High Energy Physics - Experiment 2025-05-19 v2 Instrumentation and Methods for Astrophysics High Energy Physics - Phenomenology Instrumentation and Detectors

Abstract

We report the first result from a dark photon dark matter search in the mass range from 78.62{78.62} to 83.95 μeV/c283.95~\mathrm{\mu eV}/c^2 with a dielectric haloscope prototype for MADMAX (Magnetized Disc and Mirror Axion eXperiment). Putative dark photons would convert to observable photons within a stack consisting of three sapphire disks and a mirror. The emitted power of this system is received by an antenna and successively digitized using a low-noise receiver. No dark photon signal has been observed. Assuming unpolarized dark photon dark matter with a local density of ρχ=0.3 GeV/cm3\rho_{\chi}=0.3~\mathrm{GeV/cm^3} we exclude a dark photon to photon mixing parameter χ>2.7×1012\chi > 2.7 \times 10^{-12} over the full mass range and χ>1.1×1013\chi > 1.1 \times 10^{-13} at a mass of 80.57 μeV/c280.57~\mathrm{\mu eV}/c^2 with a 95\% confidence level. This is the first physics result from a MADMAX prototype and exceeds previous constraints on χ\chi in this mass range by up to almost three orders of magnitude.

Keywords

Cite

@article{arxiv.2408.02368,
  title  = {First search for dark photon dark matter with a MADMAX prototype},
  author = {J. Egge and D. Leppla-Weber and S. Knirck and B. Ary dos Santos Garcia and D. Bergermann and A. Caldwell and V. Dabhi and C. Diaconu and J. Diehl and G. Dvali and M. Ekmedžić and F. Gallo and E. Garutti and S. Heyminck and F. Hubaut and A. Ivanov and J. Jochum and P. Karst and M. Kramer and D. Kreikemeyer-Lorenzo and C. Krieger and C. Lee and A. Lindner and J. P. A. Maldonado and B. Majorovits and S. Martens and A. Martini and A. Miyazaki and E. Öz and P. Pralavorio and G. Raffelt and A. Ringwald and J. Redondo and S. Roset and N. Salama and J. Schaffran and A. Schmidt and F. Steffen and C. Strandhagen and I. Usherov and H. Wang and G. Wieching and G. Cancelo and M. Di Federico and G. Hoshino and L. Stefanazzi},
  journal= {arXiv preprint arXiv:2408.02368},
  year   = {2025}
}

Comments

v2 (Adapted to match published version. Fixed a mistake in the dark matter lineshape leading to a ~10% improvement in the limit)

R2 v1 2026-06-28T18:04:04.496Z