Abstract
It is well known that a canonical scalar field with an exponential potential can drive power law inflation (PLI).However, the tensor-to-scalar ratio in such models turns out to be larger than the stringent limit set by recent Planck results.We propose a new model of power law inflation for which the scalar spectra index, the tensor-to-scalar ratio and the non-gaussianity parameter fNLequil are in excellent agreement with Planck results. Inflation, in this model, is driven by a non-canonical scalar field with an inverse power law potential. The Lagrangian for our model is structurally similar to that of a canonical scalar field and has a power law form for the kinetic term. A simple extension of our model resolves the graceful exit problem which usually afflicts models of power law inflation.
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