We study the bulk flow of the local universe using Type Ia supernova data by
considering a class of cosmological model which is spatially flat,(FRW)
space-times and contains cold dark matter and Q component (QCDM models) of
the fluid as a scalar field, with self interactions determined by a potential
V(Q)=V0βExp(βΞ»Q) evolving in Universe. We use different cumulative
redshift slices of the Union 2 catalogue. A maximum-likelihood analysis of
peculiar velocities confirms that at low redshift 0.015<z<0.1, bulk flow is
moving towards the (l;b)=(302oΒ±20o;3oΒ±10o) direction with
vbulkβ=240Β±25kmsβ1 velocity. This direction is aligned with
direction of (SSC) and agreement with a number previous studies at
(1βΟ), however for high redshift 0.1<z<0.2, we get vbulkβ=1000Β±25kmsβ1 towards the (l;b)=(254β14o+16oβ;6β10o+7oβ). This indicates that for low redshift our results are
approximately consistent with the ΞCDM model with the latest WMAP best
fit cosmological parameters however for high redshift they are in disagreement
of ΞCDM and support the results of previous studies such as Kashlinsky
et. al, which report the large bulk flow for the Universe. We can conclude
that, in QCDM model, at small scales, fluctuations of the dark energy are
damped and do not enter in the evolution equation for the perturbations in the
pressureless matter, while at very large scales (βΌ>100hβ1Mpc), they
leaving an imprint on the microwave background anisotropy