Inflationary models, beside addressing the traditional problems
of big-bang cosmology, offer a mechanism to generate the
primordial perturbations that eventually formed galaxies and
shape the Cosmic Microwave Background anisotropies.
A crucial feature of the observed primordial spectrum of
perturbations is that its amplitude is very mildly dependent
on the wavelength (scale-invariance). In the simplest
inflationary models this is the result of a primordial phase
of quasi de-Sitter expansion.
In scalar field models where the Lagrangian is a generic function of the kinetic term and of the field itself, perturbations can travel at a velocity (the velocity of sound) different than the velocity of light.
With Justin Khoury I explored a generalization of the above mechanism. We showed that an adiabatic scale invariant spectrum is produced even if the expansion -- albeit still inflationary -- is far from exponential, provided the speed of sound varies appropriately. We also found a class of contracting (``ekpirotic”) cosmologies where this mechanism can be applied. Non-gaussianity can be large in both the expanding and the contracting cases. The most relevant feature of our model is perhaps that the amplitude of the three point function exhibits a strong running with the scale. The mechanism that protects the scale invariance of the two-point function cannot in fact forbid a running of the three-point function. The gravitational wave spectrum is also tilted.