Operation of a ferromagnetic axion haloscope at $$m_a=58\,\upmu \mathrm {eV}$$ ma=58μeV

• Main Authors: N. Crescini, D. Alesini, C. Braggio, G. Carugno, D. Di Gioacchino, C. S. Gallo, U. Gambardella, C. Gatti, G. Iannone, G. Lamanna, C. Ligi, A. Lombardi, A. Ortolan, S. Pagano, R. Pengo, G. Ruoso, C. C. Speake, L. Taffarello
• Format: Article
• Language: English
• Published: SpringerOpen 2018-09-01
• Series: European Physical Journal C: Particles and Fields
• Online Access: http://link.springer.com/article/10.1140/epjc/s10052-018-6163-8

Abstract Axions, originally proposed to solve the strong CP problem of quantum chromodynamics, emerge now as leading candidates of WISP dark matter. The rich phenomenology associated to the light and stable QCD axion can be described as an effective magnetic field that can be experimentally investigated. For the QUAX experiment, dark matter axions are searched by means of their resonant interactions with electronic spins in a magnetized sample. In principle, axion-induced magnetization changes can be detected by embedding a sample in an rf cavity in a static magnetic field. In this work we describe the operation of a prototype ferromagnetic haloscope, with a sensitivity limited by thermal fluctuations and receiver noise. With a preliminary dark matter search, we are able to set an upper limit on the coupling constant of DFSZ axions to electrons $$g_{aee}<4.9\times 10^{-10}$$ gaee<4.9×10-10 at 95% C.L. for a mass of $$58\,\upmu $$ 58μ eV (i. e. 14 GHz). This is the first experimental result with an apparatus exploiting the coupling between cosmological axions and electrons.