The Search for the Cosmological Axion -- A New Refined Narrow Mass Window and Detection Scheme
This paper proposes a refined search strategy targeting a narrow axion mass window of 78.6 to 79.6 micro-eV (18.99–19.01 GHz) using a resonant cavity detection scheme based on the inverse Primakoff effect, supported by recent simulations and novel experimental designs involving Josephson Parametric Amplifiers and Resonant Tunneling Diodes.