  In this work we study the effects of field space curvature on scalar field
perturbations around an arbitrary background field trajectory evolving in time.
Non-trivial imprints of the 'heavy' directions on the low energy dynamics arise
when the vacuum manifold of the potential does not coincide with the span of
geodesics defined by the sigma model metric of the full theory. When the
kinetic energy is small compared to the potential energy, the field traverses a
curve close to the vacuum manifold of the potential. The curvature of the path
followed by the fields can still have a profound influence on the perturbations
as modes parallel to the trajectory mix with those normal to it if the
trajectory turns sharply enough. We analyze the dynamical mixing between these
non-decoupled degrees of freedom and deduce its non-trivial contribution to the
low energy effective theory for the light modes. We also discuss the
consequences of this mixing for various scenarios where multiple scalar fields
play a vital role, such as inflation and low-energy compactifications of string
theory.
