  Neutron star mergers provide a unique laboratory for the study of
strong-field gravity coupled to Quantum Chromodynamics in extreme conditions.
The frequencies and amplitudes of the resulting gravitational waves encode
invaluable information about the merger. Simulations to date have shown that
these frequencies lie in the kilo-Hertz range. They have also shown that, if
Quantum Chromodynamics possesses a first-order phase transition at high baryon
density, then this is likely to be accessed during the merger dynamics. Here we
show that this would result in the nucleation of superheated and/or
supercompressed bubbles whose subsequent dynamics would produce gravitational
waves in the Mega-Hertz range. We estimate the amplitude of this signal and
show that it may fall within the expected sensitivity of future superconducting
radio-frequency cavity detectors for mergers at distances up to tens of
Mega-parsecs.
