Key points are not available for this paper at this time.
The shear dynamics in Bianchi I cosmological model on the brane with a perfect fluid (the equation of state is p= (\-1) \) is studied. It is shown that for 1 < \ < 2 the shear parameter has maximum at some moment during a transition period from nonstandard to standard cosmology. An exact formula for the matter density \ in the epoch of maximum shear parameter as a function of the equation of state is obtained.
A. V. Toporensky (Wed,) studied this question.