IceCube Results for Diffuse Muon Neutrinos

Recent results from the IceCube Neutrino Observatory provide evidence for high energy astrophysical neutrinos in an analysis using events whose interactions occurred within the detector volume. In this talk I will show the results of a complimentary analysis using neutrino-induced muon events which enter the detector from outside, with a focus on the region of energies around 100 TeV where the hypothetical best-fit astrophysical flux corresponding to the contained event data begins to dominate over the conventional atmospheric muon neutrino flux.