One of the exact solutions of f(R) theories of gravity in the presence of
different forms of matter exactly mimics the LCDM solution of general
relativity at the background level. In this work we study the evolution of
scalar cosmological perturbations in the covariant and gauge-invariant
formalism and show that although the background in such a model is
indistinguishable from the standard LCDM cosmology, this degeneracy is broken
at the level of first-order perturbations. This is done by predicting different
rates of structure formation in LCDM and the f(R) model both in the complete
and quasi\hs static regimes.Comment: 17 pages, 19 figure