Stability of the scale parameter: Hu-Sawicki model
  The evolution of the scale parameter in the Hu-Sawicki model is examined. We
search the parameter area for instabilities. It turns out the parameter area of
physically meaningful evolution is non-existent. For greater stability a
stabilising term such as R^2 should be added. With the addition, the area
mainly coincides with phantom models. We also find that the evolution of the
scale parameter can be examined through a linear expansion and not only in the
Hu-Sawicki case. The oscillatory behaviour found in the evolution raises
questions of the physicality of the model. The behaviour can also cause current
observations of the Hubble parameter to be misleading.
  This paper has been withdrawn by the authords due to a critical error in
equation (10)
