English

Superconducting Radio Frequency Cavities as Axion Dark Matter Detectors

High Energy Physics - Phenomenology 2013-01-22 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment

Abstract

A modification of the cavity technique for axion dark matter detection is described in which the cavity is driven with input power instead of being permeated by a static magnetic field. A small fraction of the input power is pumped by the axion field to a receiving mode of frequency ω1\omega_1 when the resonance condition ω1=ω0±ma\omega_1 = \omega_0 \pm m_a is satisfied, where ω0\omega_0 is the frequency of the input mode and mam_a the axion mass. The relevant form factor is calculated for any pair of input and output modes in a cylindrical cavity. The overall search strategy is discussed and the technical challenges to be overcome by an actual experiment are listed.

Keywords

Cite

@article{arxiv.1009.0762,
  title  = {Superconducting Radio Frequency Cavities as Axion Dark Matter Detectors},
  author = {P. Sikivie},
  journal= {arXiv preprint arXiv:1009.0762},
  year   = {2013}
}

Comments

4 pages, 1 figure. The new version gives a more realistic discussion of the challenges involved in carrying out the proposed experiment