  We construct the mechanism of formation of the scalar boson star (BS) having
a hierarchy of self-similar "lumps" of dark matter (DM) built into the
probability distribution function of allowed steps. It can ensure to study the
dynamics of the BS formation through the "cross-over" between the free scalar
DM and the compact condensate (CC) phase in one-dimensional model of the random
fluctuation walk. The main inputs are the random fluctuating weight $\lambda <
1$, the fundamental fluctuating length $\xi (\lambda)$ and the parameter $a >1$
of the spatial separation between the DM "lumps" inside the BS. The solution to
the functional equation for the characteristic probability to find the free
scalar DM and the CC phase is obtained. The time evolution of the probability
to form the DM "lump" (growth of the BS) is presented with the power-law
cascades expression depending on $\lambda$ and $a$. The special cases for
$\lambda$ in terms of the energy densities of the BS ($\rho_\star$) and the DM
($\rho_\odot$), as well as the Bose-Einstein correlation function for two
scalar DM particles, are considered. The lower bounds on the critical
temperature at the "cross-over" depending on $\rho_\odot$, $\rho_\star$, the
average multiplicities of the scalar DM particles and the parameters related to
the chaotically behaviour of the particles are obtained.
