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Axion dark matter detection by superconducting resonant frequency conversion

Journal Article · · Journal of High Energy Physics (Online)
 [1];  [2];  [3];  [3];  [3];  [3];  [3];  [3];  [3]
  1. New York Univ. (NYU), NY (United States). Center for Cosmology and Particle Physics
  2. Univ. Paris-Saclay, Gif-sur-Yvette (France). Inst. de Physique Theorique, CEA
  3. SLAC National Accelerator Lab., Menlo Park, CA (United States)

We propose an approach to search for axion dark matter with a specially designed superconducting radio frequency cavity, targeting axions with masses ma ≲ 10-6 eV. Our approach exploits axion-induced transitions between nearly degenerate resonant modes of frequency ~ GHz. A scan over axion mass is achieved by varying the frequency splitting between the two modes. Compared to traditional approaches, this allows for parametrically enhanced signal power for axions lighter than a GHz. The projected sensitivity covers unexplored parameter space for QCD axion dark matter for 10-8 eV ≲ ma ≲ 10-6 eV and axion-like particle dark matter as light as ma~ 10-14 eV.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC); National Science Foundation (NSF); Swiss National Science Foundation; German Research Foundation (DFG)
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1656591
Journal Information:
Journal of High Energy Physics (Online), Journal Name: Journal of High Energy Physics (Online) Journal Issue: 7 Vol. 2020; ISSN 1029-8479
Publisher:
Springer BerlinCopyright Statement
Country of Publication:
United States
Language:
English

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