Models to explain the formation of structures in the universe take shape
THE big bang cosmological model is one
of the most successful models of our
universe. Its efficacy in predicting the
temperature of the cosmic microwave
background radiation and the profusion
of light elements in the universe (like
helium and lithium) remains unsurpassed by any of the competing cosmological models (Nature, Vol 377,September 7, 1995).
Successful as it is, the big bang
model has its own share of problems.
Outstanding among them is that of the
formation of structure in the universe.
The universe is made up of stars
which group into galaxies. Galaxies in
their turn, get together in clusters. For
instance, our sun is a part of the Milky
Way galaxy (which has some
100 billion other stars). The
Milky Way is part of another
system, a cluster of galaxies
called the Local Group. The big
bang model offers no natural
way in which these structures
could have been formed.
To create a clearer picture,
we can incorporate another
class of models called the inflationary universe models into
the big bang scenario.
According to these models, the
universe - after the initial big
bang - undergoes a phase of
tremendous expansion. But we
are still far from having a complete and satisfactory theory of
understanding how matter in
the universe groups into galaxies and
dusters.
Now a group of researchers have
ftported a new sample of clusters of
pi"es which could shed some light on
the formation and evolution of
kqescale structure in the universe,
Cknters of galaxies are visible as regions
of extended x-ray emission.
Thus, one could identify clusters by
etamining photographic plates and
ksAing for associated galaxies. This,
boonever, is not very reliable since there
could be an artificial enhancement
along the line of sight of the telescope
(objects far apart could appear to be
closer to each other). Observation of xray emission is far more trustworthy.
When th@- clusters collapse under their
gravitation, the inter-cluster gas is compressed and heated. The clusters' gravitation pull confines the hot gas and thus
x-ray emission can be correlated to the
presence of clusters.
Using the Rosat International x-ray
Optical Survey (RLXOS), a project aimed
at cataloguing some 400 x-ray sources,
the team of scientists from England,
Germany, Spain and Finland have concluded from their studies of clusters that
in the recent past there were few high
mass (and thus high luminosity, luminosity being a measure of the energy
given out by an object) objects. In cosmology, one can look into the past by
looking into the distant. This conclusion is significant because it implies that
the dusters - the largest gravitationally
bound systems in the universe - are
forming now (compared to galaxies
which formed long ago).
The x-ray emission from a cluster is
also dependent on the temperature and
density of the hot gas from which it is
coming. Thus x-ray luminosity can be
used to study the history of the 'seeds'
from which the cluster grew as well as
the evolution of the hot gas. Several
models have been proposed to under-
stand x-ray emission and its correlation
with the history of the hot gas; an
important finding of the recent study
has been to rule out some of these
models as being inconsistent with data.
Though the study is a significant
step towards understanding the formation and evolution of structure in the
universe, several questions remain
unanswered. One of the foremost concerns the amount of matter in the universe and its composition. The nature of
the matter in the universe - whether it
is the well known ordinary baryonic
matter or something more exotic like
wimps (weakly interacting massive particles) which comprise the dark matter
- necessarily influences the formation
of structure.
In any case, with better observational facilities (from satellites and the
Hubble Space Telescope) as well as
more sophisticated computer simulations, we are gradually moving towards
determining how the universe became
what it is.
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