  One of the firm predictions of inflationary cosmology is the consistency
relation between scalar and tensor spectra. It has been argued that such a
relation -if experimentally confirmed- would offer strong support for the idea
of inflation. We examine the possibility that trans-Planckian physics violates
the consistency relation in the framework of inflation with a cut-off proposed
in astro-ph/0009209. We find that despite the ambiguity that exists in choosing
the action, Planck scale physics modifies the consistency relation
considerably. It also leads to the running of the spectral index. For modes
that are larger than our current horizon, the tensor spectral index is
positive. For a window of k values with amplitudes of the same order of the
modes which are the precursor to structure formation, the behavior of tensor
spectral index is oscillatory about the standard Quantum Field theory result,
taking both positive and negative values. There is a hope that in the light of
future experiments, one can verify this scenario of short distance physics.
