ADMX-Orpheus First Search for 70 $\mu$eV Dark Photon Dark Matter: Detailed Design, Operations, and Analysis
Abstract
Dark matter makes up 85% of the matter in the universe and 27% of its energy density, but we do not know what comprises dark matter. It is possible that dark matter may be composed of either axions or dark photons, both of which can be detected using an ultra-sensitive microwave cavity known as a haloscope. The haloscope employed by ADMX consists of a cylindrical cavity operating at the TM mode and is sensitive to the QCD axion with masses of few eV. However, this haloscope design becomes challenging to implement for higher masses. This is because higher masses require smaller-diameter cavities, consequently reducing the detection volume which diminishes the detected signal power. ADMX-Orpheus mitigates this issue by operating a tunable, dielectrically-loaded cavity at a higher-order mode, allowing the detection volume to remain large. This paper describes the design, operation, analysis, and results of the inaugural ADMX-Orpheus dark photon search between 65.5 eV (15.8 GHz) and 69.3 eV (16.8 GHz), as well as future directions for axion searches and for exploring more parameter space.
Cite
@article{arxiv.2204.09475,
title = {ADMX-Orpheus First Search for 70 $\mu$eV Dark Photon Dark Matter: Detailed Design, Operations, and Analysis},
author = {R. Cervantes and G. Carosi and C. Hanretty and S. Kimes and B. H. LaRoque and G. Leum and P. Mohapatra and N. S. Oblath and R. Ottens and Y. Park and G. Rybka and J. Sinnis and J. Yang},
journal= {arXiv preprint arXiv:2204.09475},
year = {2022}
}
Comments
21 pages, 29 figures. To be submitted to Physical Review D. arXiv admin note: substantial text overlap with arXiv:2112.04542