In astrophysics, dark flow is a theoretical non-random component of the peculiar velocity of galaxy clusters. The actual measured velocity is the sum of the velocity predicted by Hubble's Law plus a possible small and unexplained (or dark) velocity flowing in a common direction.
According to standard cosmological models, the motion of galaxy clusters with respect to the cosmic microwave background should be randomly distributed in all directions. However, analyzing the three-year Wilkinson Microwave Anisotropy Probe (WMAP) data using the kinematic Sunyaev-Zel'dovich effect, astronomers Alexander Kashlinsky, F. Atrio-Barandela, D. Kocevski and H. Ebeling found evidence of a "surprisingly coherent" 600–1000 km/s flow of clusters toward a 20-degree patch of sky between the constellations of Centaurus and Vela.
The researchers had suggested that the motion may be a remnant of the influence of no-longer-visible regions of the universe prior to inflation. Telescopes cannot see events earlier than about 380,000 years after the Big Bang, when the universe became transparent (the cosmic microwave background); this corresponds to the particle horizon at a distance of about 46 billion (4.6×1010) light years. Since the matter causing the net motion in this proposal is outside this range, it would in a certain sense be outside our visible universe; however, it would still be in our past light cone.
The results appeared in the October 20, 2008, issue of Astrophysical Journal Letters. In 2013, data from the Planck space telescope showed no evidence of "dark flow" on that sort of scale, discounting the claims of evidence for either gravitational effects reaching beyond the visible universe or existence of a multiverse. However, in 2015 Kashlinsky et al claim to have found support for its existence using both Planck and WMAP data.
Location
Panoramic
view of galaxies beyond Milky Way, with Norma cluster & Great
Attractor shown by a long blue arrow at the bottom-right in image near
the disk of the Milky Way.
The dark flow was determined to be flowing in the direction of the Centaurus and Hydra constellations. This corresponds with the direction of the Great Attractor,
which is a gravitational mystery originally discovered in 1973.
However, the source of the Great Attractor's attraction was thought to
originate from a massive cluster of galaxies called the Norma Cluster, located about 250 million light-years away from Earth.
In a study from March 2010, Kashlinsky extended his work from
2008, by using the 5-year WMAP results rather than the 3-year results,
and doubling the number of galaxy clusters observed from 700. The team
also sorted the cluster catalog into four "slices" representing
different distance ranges. They then examined the preferred flow
direction for the clusters within each slice. While the size and exact
position of this direction display some variation, the overall trends
among the slices exhibit remarkable agreement.
"We detect motion along this axis, but right now our data cannot state
as strongly as we'd like whether the clusters are coming or going,"
Kashlinsky said.
The team has so far catalogued the effect as far out as 2.5
billion light-years, and hopes to expand its catalog out further still
to twice the current distance.
The dark flow.
The colored dots are clusters within one of
four distance ranges, with
redder colors indicating greater
distance. Colored ellipses show the
direction of bulk motion
for the clusters of the corresponding color.
Images of representative
galaxy clusters in each distance slice are also
shown
Criticisms
Astrophysicist Ned Wright posted an online response to the study arguing that its methods are flawed.
The authors of the "dark flow" study released a statement in return,
refuting three of Wright's five arguments and identifying the remaining
two as a typo and a technicality that do not affect the measurements and
their interpretation.
A more recent statistical work done by Ryan Keisler
claims to rule out the possibility that the dark flow is a physical
phenomenon because Kashlinsky et al. did not consider the primary anisotropies of the cosmic microwave background (CMB) to be as important as they are.
NASA's Goddard Space Flight Center considered that this could be
the effect of a sibling universe or a region of space-time fundamentally
different from the observable universe. Data on more than 1,000 galaxy
clusters have been measured, including some as distant as 3 billion
light-years. Alexander Kashlinsky claims these measurements show the
universe's steady flow is clearly not a statistical fluke. Kashlinsky
said: "At this point we don't have enough information to see what it is,
or to constrain it. We can only say with certainty that somewhere very
far away the world is very different than what we see locally. Whether
it's 'another universe' or a different fabric of space-time we don't
know." Laura Mersini-Houghton
and Rich Holman observe that some anisotropy is predicted both by
theories involving interaction with another universe, or when the frame
of reference of the CMB does not coincide with that of the universe's
expansion.
In 2013, data from the European Space Agency's Planck satellite was claimed to show no statistically significant evidence of existence of dark flow.
However, another analysis by a member of the Planck collaboration,
Fernando Atrio-Barandela, suggested the data were consistent with the
earlier findings from WMAP.
Popular media continued to be interested in the idea, with
Mersini-Houghton claiming the Planck results support existence of a
multiverse.
