Experimental Searches for the Axion and Axion-Like Particles
By P. Graham, Igor G. Irastorza, S. Lamoreaux, A. Lindner, K. Bibber. 2015
700 citations recorded by the source corpus.
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 m...
Subfields: Materials Chemistry, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ca4c7738dbb50239c72601858052ed6d9e9c810f
How researchers see this paper
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In Nuclear and High Energy Physics
- J. Redondo
- Igor G. Irastorza
- G. Raffelt
- Edward Hardy
- P. Fierlinger
- J. Singh
- Timothy E. Chupp
- Dmitry Budker
Citations in the corpus
- Recent Progress in the Physics of Axions and Axion-Like Particles (2020, background): “New ideas for axion search in laboratory experiments have been proposed [21–23] which can probe a wide range of axion mass and couplings that were not accessible before.”
- Axions from strings: the attractive solution (2018, background): “g or in development. These will be sensitive to a substantial proportion of the relevant parameter space, and, if an axion is discovered, they could measure its mass and couplings precisely (see e.g. [11,12]). The dynamics by which QCD axion DM is produced, and its nal relic abundance, depends on th”
- Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter (2017, unknown): “For reviews see Raffelt (2008); Graham et al. (2015).”
- New experimental approaches in the search for axion-like particles (2018, background): “The experimental landscape is rapidly evolving, so relatively recent reviews are quickly becoming obsolete [47,48].”
- Search for axion-like dark matter with spin-based amplifiers (2021, background): “This section presents three other possible couplings between bosonic dark matter fields and nuclear spins [8, 10, 11, 16, 17]: the quadratic wind coupling with the axions, the couplings to dark electric field and magnetic field mediated by spin-1 bosons such as dark photons [8, 10].”
- Current Status and Future Prospects of the SNO+ Experiment (2015, background): “An axion-like particle (ALP) is defined as a neutral pseudoscalar particle that exists as an extension to the QCD Lagrangian [81].”
- Electric dipole moments of atoms, molecules, nuclei, and particles (2017, background): “The axion proposal has been very compelling and has spawned a number of experimental endeavors summarized, for example by Graham et al. (2015).”