The implementation of a Planck-scale high frequency and short wavelength cu
toff in quantum theories on expanding backgrounds may have potentially nont
rivial implications, such as the breaking of local Lorentz invariance and t
he existence of a yet unknown mechanism for the creation of vacuum modes. I
n scenarios where inflation begins close to the cutoff scale, these effects
could have observable consequences as trans-Planckian modes are redshifted
to cosmological scales. In close analogy with similar studies of Hawking r
adiation, st simple theory of a minimally coupled scalar field in de Sitter
space is studied, with a high frequency cutoff imposed by a nonlinear disp
ersion relation. Under certain conditions the model predicts deviations fro
m the standard inflationary scenario. We also comment on the difficulties i
n generalizing fluid models of Hawking radiation to cosmological space-time
s.