  Although IceCube has discovered a diffuse astrophysical neutrino flux, the
underlying sources of these neutrinos remain unknown. Transient astrophysical
objects, such as fast radio bursts (FRBs), could explain a large percentage of
the measured flux. We present the analysis techniques of IceCube searches for
MeV to TeV neutrinos from FRBs. As no significant correlation between IceCube
neutrinos and FRBs has been found, we present the first limit on MeV neutrino
emission from FRBs and the most constraining limits for neutrinos with GeV to
TeV energies. We also describe the prospects for future IceCube neutrino
searches coinciding with FRB detections from next generation radio
interferometers.
