Broadband interferometry-based searches for photon-axion conversion in vacuum

A novel experiment is introduced to detect photon-axion conversion independent of the dark-matter hypothesis in a broad mass-range called WISP Interferometer (WINTER). The setup consists of a free-space Mach-Zehnder-type interferometer incorporating an external magnetic field and vacuum in one of the arms, where photon-axion mixing occurs via the Primakoff effect and is detected through changes in amplitude. The expected axion-induced signal is then modulated by polarization changes. The experiment is designed to integrate a Fabry-Pérot cavity with a finesse of 10 5 that will be operated in a vacuum environment, significantly enhancing the sensitivity. It is projected to reach the Dine-Fischler-Srednicki-Zhitnitsky theoretical line with photon-axion coupling sensitivities down to g a γ γ ≃ 3.7 × 10 − 14 GeV − 1 for axion masses up to 380 μeV.