New exact solutions for inflationary cosmological perturbations

From a general ansatz for the effective potential of cosmological perturbations we find new, exact solutions in single-scalar-field inflation: a three parameter family of exact inflationary solutions that encompasses all exact solutions that have been known previously (power-law inflation, Eastherʹs model, and a generalised version of Starobinskyʹs solution). The main feature of this new family is that the spectral indices are scale dependent.