Forthcoming missions probing the absolute intensity of the CMB are expected to be able to measure
spectral distortions, which are deviations from its blackbody distribution. As cosmic inflation can induce spectral
distortions, these experiments offer a possibility to further test the various promising inflationary
proposals, whose predictions need to be carefully determined. After numerically fitting all inflationary
observables to match current observations, we compute the predicted spectral distortions of
various promising single and multifield inflationary models. The predictions of single-field
inflationary models display deviations between 0.5% and 20% with respect to the standard cosmological
model in the observable window, where multi-natural and axion-monodromy inflation stand out in this respect.
In the case of multifield inflation, we observe a richer structure of the power spectrum, which, in
the case of so-called hybrid attractors, yields spectral distortions about 100 times more intense than
the standard signal. These observations open up questions about the relation among our results
and other cosmological observables that are also to be probed soon, such as the production of
primordial black holes and gravitational waves.