An improved RF cavity search for halo axions
By S. Asztalos, R. Bradley, L. Duffy, C. Hagmann, D. Kinion, D. Moltz, L. Rosenberg, P. Sikivie, W. Stoeffl, N. Sullivan and 8 more. 2003
188 citations recorded by the source corpus.
The axion is a hypothetical elementary particle and cold dark matter candidate. In this RF cavity experiment, halo axions entering a resonant cavity immersed in a static magnetic field convert into microwave photons, with the resulting photons detected by a low-noise receiver. The ADMX Collaboration presents new limits on the axion-to-photon coupling and local axion dark matter halo mass density from a RF cavity axion search in the axion mass range 1.9-2.3 {micro}eV, broadening the search range to 1.9-3.3 {micro}eV. In addition, we report first results from an improved analysis technique.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/1cb213ab31dbd941b2d7876e44112354bc81f7fc
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In Nuclear and High Energy Physics
- J. Redondo
- Igor G. Irastorza
- Maurizio Giannotti
- G. Raffelt
- Luca Visinelli
- E. Nardi
- L. Luzio
- Edward Hardy
Citations in the corpus
- The landscape of QCD axion models (2020, background): “ABRACADABRA [291] A Broadband/Resonant Approach to Cosmic Axion Detection ADMX [505] Axion Dark Matter Experiment ALPS (II) [504] Any Light Particle Search (II) ARGUS [566] A Russian-German-United States-Swedish Collaboration ARIADNE [448] Axion Resonant InterAction Detection Experiment ATLAS [695] ”
- More axions from strings (2020, background): “We assume radiation domination in a spatially 18The existing experimental and observational bounds shown are from ADMX [61,62], earlier cavity experiments “UF/RBF” [63, 64], HAYSTACK [65], CAST [66], observations of horizontal branch starts “HB” [67], supernova 1987a “SN1987a” [68–70] (see however [”
- History of dark matter (2018, unknown): “In 2003, however, the ADMX Collaboration reported results that constrained realistic axion dark matter models, although only for a relatively narrow range of masses 1.9–3.3 μeV (Asztalos et al., 2004).”
- Towards a new generation axion helioscope (2011, methodology): “ADMX contemplates the exploration of the 1–10 µeV decade with sufficient sensitivity in gaγ to exclude or detect the QCD axion band, corresponding to gaγ in the approximate range 10 −17–10−14 GeV−1.”