High resolution search for dark-matter axions
By L. Duffy, P. Sikivie, D. Tanner, S. Asztalos, C. Hagmann, D. Kinion, L. Rosenberg, K. Bibber, D. Yu, R. Bradley. 2006
182 citations recorded by the source corpus.
We have performed a high resolution search for galactic halo axions in cold flows using a microwave cavity detector. The analysis procedure and other details of this search are described. No axion signal was found in the mass range 1.98-2.17 micro-eV. We place upper limits on the density of axions in local discrete flows based on this result.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/45dd8be8f8c157d888a032f8a664ee02bc990933
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In Nuclear and High Energy Physics
Citations in the corpus
- Axions and the Strong CP Problem (2008, methodology): “Results from a high resolution search have probed further into coupling space over a smaller mass range, 1.98-2.17 µeV [149, Duffy et al. (2006)].”
- Axion dark matter, solitons and the cusp–core problem (2015, background): “This question is of more than theoretical importance and can greatly affect the direct detection prospects for the axion, for example by Axion Dark Matter Experiment (ADMX; Duffy et al. 2006; Hoskins et al. 2011).”
- Dark matter and fundamental physics with the Cherenkov Telescope Array (2012, methodology): “The photon/ALP mixing is indeed the main signature used at present in ALP searches, such as those carried out by CAST [133–136] or ADMX [137], but it could also have important implications for astronomical observations.”
- Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles (2014, background): “o search for generic ALPs in light-shining-through-the-wall experiments (e.g. ALPS [14], CROWS [15], and OSQAR [16]), and for ALP dark matter [17] in micro-wave cavity experiments (for instance, ADMX [18]). Photon{ALP oscillations would also lead to peculiar signatures in astrophysical and cosmologi”
- Radio for hidden-photon dark matter detection (2014, methodology): “Axion detectors such as ADMX [5, 6] and the proposed CASPEr [7] are examples of this type of strategy.”
- Dark Matter: A Primer (2010, background): “Although the axion has never been observed directly, several experiments such as ADMX and CARRACK are continuing the search and setting new limits on axion parameters [45, 46].”