English

ADMX SLIC: Results from a Superconducting LC Circuit Investigating Cold Axions

Cosmology and Nongalactic Astrophysics 2020-07-01 v1 Instrumentation and Methods for Astrophysics Instrumentation and Detectors

Abstract

Axions are a promising cold dark matter candidate. Haloscopes, which use the conversion of axions to photons in the presence of a magnetic field to detect axions, are the basis of microwave cavity searches such as the Axion Dark Matter eXperiment (ADMX). To search for lighter, low frequency axions in the sub 2×1072\times10^{-7} eV (50 MHz) range, a tunable lumped-element LC circuit has been proposed. For the first time, through ADMX SLIC (Superconducting Lc circuit Investigating Cold axions), a resonant LC circuit was used to probe this region of axion mass-coupling space. The detector used a superconducting LC circuit with piezoelectric driven capacitive tuning. The axion mass and corresponding frequency range 1.74981.7519×1071.7498 -1.7519 \times10^{-7} eV (42.31 -- 42.36 MHz), 1.77341.7738×1071.7734 - 1.7738 \times10^{-7} eV (42.88 -- 42.89 MHz), and 1.80071.8015×1071.8007 - 1.8015 \times10^{-7} eV (43.54 -- 43.56 MHz) was covered at magnetic fields of 4.5 T, 5.0 T, and 7.0 T respectively. Exclusion results from the search data, for coupling below 1012GeV110^{-12} \text{GeV}^{-1} are presented.

Keywords

Cite

@article{arxiv.1911.05772,
  title  = {ADMX SLIC: Results from a Superconducting LC Circuit Investigating Cold Axions},
  author = {N. Crisosto and G. Rybka and P. Sikivie and N. S. Sullivan and D. B. Tanner and J. Yang},
  journal= {arXiv preprint arXiv:1911.05772},
  year   = {2020}
}