  Inflationary dynamics solves several cosmological problems at a classical
level. If in addition one considers quantum perturbations, inflation can also
explain the observed temperature anisotropies in the cosmic microwave
background (CMB) radiation. The predictions for the amplitude and spectral
index of the comoving curvature perturbation of theoretically well motivated
inflationary models are in perfect agreement with the recent Planck data. In
this work we study the corrections induced by dynamical collapse models, which
phenomenologically solve the measurement problem of quantum mechanics, to the
inflationary observables. We compute the leading order correction to the power
spectrum of the comoving curvature perturbation during inflation and the
radiation dominated era. For the reference values of the phenomenological
parameters of the Continuous Spontaneous Localization (CSL) model, we find that
these corrections are negligible with respect to the observed values.
