Upgrading the existing Haloscope-type detector for sensitive axion detection

Haloscope is one of the typical installations to detect the electromagnetic responses (EMRs) of axion field in radio-frequency (rf) band. Given what the detection by the existing Haloscope-type detector (HTD) biased only by a high stationary magnetic field, is just the second axion-photon energy converted effect and thus the detectable signal is still significantly weak, here we propose a feasible approach to upgrade the existing HTD by additionally applying a transverse rf modulated magnetic field for generating the first-order axion-photon energy converted signal. Accordingly, we argue that the detection sensitivity of the upgrading HTD (UHTD) could be enhanced feasibly by a few orders of magnitude, compared with those achieved by the existing HTDs. The feasibility of the proposed UHTD is also discussed.
Comment: 22 pages,3 figures