Experimental Searches for the Axion and Axion-Like Particles

Author:

Graham Peter W.1,Irastorza Igor G.2,Lamoreaux Steven K.3,Lindner Axel4,van Bibber Karl A.5

Affiliation:

1. Stanford Institute for Theoretical Physics, Stanford University, Stanford, California 94305;

2. Laboratorio de Física Nuclear y Astropartículas, Departamento de Física Teórica, Universidad de Zaragoza, 50009 Zaragoza, Spain

3. Department of Physics, Yale University, New Haven, Connecticut 06511

4. DESY, 22607 Hamburg, Germany

5. Department of Nuclear Engineering, University of California, Berkeley, California 94720

Abstract

Four decades after its prediction, the axion remains the most compelling solution to the strong-CP problem and a well-motivated dark matter candidate, inspiring a host of elegant and ultrasensitive experiments based on axion–photon mixing. This article reviews the experimental situation on several fronts. The microwave cavity experiment is making excellent progress in the search for dark matter axions in the μeV range and may plausibly be extended up to 100 μeV. Within the past several years, however, researchers have realized that axions are pervasive throughout string theories, but with masses that fall naturally in the neV range, for which an NMR-based search is under development. Both searches for axions emitted from the Sun's burning core and purely laboratory experiments based on photon regeneration have recently made great progress, with ambitious projects proposed for the coming decade. Each of these campaigns has pushed the state of the art in technology, enabling large gains in sensitivity and mass reach. Furthermore, each modality has been exploited in order to search for more generalized axion-like particles, which we also discuss in this review. We are hopeful, even optimistic, that the next review of the subject will concern the discovery of the axion, its properties, and its exploitation as a probe of early universe cosmology and structure formation.

Publisher

Annual Reviews

Subject

Nuclear and High Energy Physics

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