Interactions News Wire
#44-05
2 June 2005
http://www.interactions.org*******************************************************************
Source:
PPARC
Content: Press Release
Date Issued: 2 June
2005
*******************************************************************
Millennium
Simulation - the largest ever model of the UniverseThe Virgo
consortium, an international group of astrophysicists from
the UK, Germany,
Canada and the USA has today (June 2nd) released first
results from the
largest and most realistic simulation ever of the
growth of cosmic structure
and the formation of galaxies and quasars.
In a paper published in Nature,
the Virgo Consortium shows how comparing
such simulated data to large
observational surveys can reveal the
physical processes underlying the
build-up of real galaxies and black
holes.
The "Millennium Simulation"
employed more than 10 billion particles of
matter to trace the evolution of
the matter distribution in a cubic
region of the Universe over 2 billion
light-years on a side. It kept the
principal supercomputer at the Max Planck
Society's Supercomputing
Centre in Garching, Germany occupied for more than a
month. By applying
sophisticated modelling techniques to the 25 Terabytes (25
million
Megabytes) of stored output, Virgo scientists are able to
recreate
evolutionary histories for the approximately 20 million galaxies
which
populate this enormous volume and for the supermassive black
holes
occasionally seen as quasars at their hearts.
Telescopes
sensitive to microwaves have been able to image the Universe
directly when it
was only 400,000 years old. The only structure at that
time was weak ripples
in an otherwise uniform sea of matter and
radiation. Gravitationally driven
evolution later turned these ripples
into the enormously rich structure we
see today. It is this growth which
the Millennium Simulation is designed to
follow, with the twin goals of
checking that this new paradigm for cosmic
evolution is indeed
consistent with what we see, and of exploring the complex
physics which
gave rise to galaxies and their central black
holes.
Recent advances in cosmology demonstrate that about 70 percent of
our
Universe currently consists of Dark Energy, a mysterious force
field
which is causing it to expand ever more rapidly. About one
quarter
apparently consists of Cold Dark Matter, a new kind of
elementary
particle not yet directly detected on Earth. Only about 5
percent is
made out of the ordinary atomic matter with which we are familiar,
most
of that consisting of hydrogen and helium. All these components
are
treated in the Millennium Simulation.
In their Nature article, the
Virgo scientists use the Millennium
Simulation to study the early growth of
black holes. The Sloan Digital
Sky Survey (SDSS) has discovered a number of
very distant and very
bright quasars which appear to host black holes at
least a billion times
more massive than the Sun at a time when the Universe
was less than a
tenth its present age.
"Many astronomers thought this
impossible to reconcile with the gradual
growth of structure predicted by the
standard picture", says Volker
Springel (Max Planck Institute for
Astrophysics, Garching) the leader of
the Millennium project and the first
author of the article, "Yet, when
we tried out our galaxy and quasar
formation modelling we found that a
few massive black holes do form early
enough to account for these very
rare SDSS quasars. Their galaxy hosts first
appear in the Millennium
data when the Universe is only a few hundred million
years old, and by
the present day they have become the most massive galaxies
at the
centres of the biggest galaxy clusters."
For Carlos Frenk
(Institute for Computational Cosmology, University of
Durham) the head of
Virgo in the UK, the most interesting aspect of the
preliminary results is
the fact that the Millennium Simulation
demonstrates for the first time that
the characteristic patterns
imprinted on the matter distribution at early
epochs and visible
directly in the microwave maps, should still be present
and should be
detectable in the observed distribution of galaxies. "If we can
measure
the baryon wiggles sufficiently well", says Frenk, "then they
will
provide us with a standard measuring rod to characterise the
geometry
and expansion history of the universe and so to learn about the
nature
of the Dark Energy."
"These simulations produce staggering
images and represent a
significant milestone in our understanding of how the
early Universe
took shape." said Professor Richard Wade, Chief Executive of
the
Particle Physics and Astronomy Research Council (PPARC), the
science
agency that funds UK involvement in the project. Professor Wade
added
"The Millennium Simulation is a brilliant example of the
interaction
between theory and experiment in astronomy as the latest
observations of
astronomical objects can be used to test the predictions of
theoretical
models of the Universe's history."
The most interesting
and far-reaching applications of the Millennium
Simulation are still to come
according to Simon White (Max Planck
Institute for Astrophysics) who heads
Virgo efforts in Germany. "New
observational campaigns are providing us with
information of
unprecedented precision about the properties of galaxies,
black holes
and the large-scale structure of our Universe," he notes. "Our
ability
to predict the consequences of our theories must reach a matching
level
of precision if we are to use these surveys effectively to learn
about
the origin and nature of our world. The Millennium Simulation is
a
unique tool for this. Our biggest challenge now is to make its
power
available to astronomers everywhere so that they can insert their
own
galaxy and quasar formation modelling in order to interpret their
own
observational surveys."
Notes for Editors
Virgo
Consortium
The Virgo Consortium is an international grouping of
scientists
carrying out supercomputer simulations of the formation of
galaxies,
galaxy clusters, large-scale structure, and of the evolution of
the
intergalactic medium. Although most of the members are based in
Britain
and at the MPA in Germany, there are important nodes in Japan,
Canada
and the United States. The primary platforms used by the consortium
are
the IBM supercomputer at the Computing Centre of the Max Planck
Society
in Garching and the Sun Microsystems "Cosmology Machine'' at
the
Institute for Computational Cosmology of Durham University.
Further
information about Virgo can be found at
http://www.virgo.dur.ac.uk/ Image
details
Images and animation files are available to download from
http://www.mpa-garching.mpg.de/galform/press/
Contact Details
Julia Maddock
PPARC Press Office
Tel +44
(0) 1793 442094
Email:
Julia.maddock@pparc.ac.uk
Professor Carlos Frenk FRS
Institute for Computational
Cosmology
Durham University
Tel: Direct line: 0191 334
3641
Secretary: 0191 334 3635
Mobile:
07808 726080
e-mail:
c.s.frenk@durham.ac.uk Available by
telephone until 27th May; thereafter by mobile or e-mail
Professor Simon
White FRS
Max-Planck Institute for Astrophysics
Tel: +49 89 30000
2211
Mobile: + 49 89-170-632-9225
Email
swhite@mpa-graching.mpg.de
Available by telephone until 30th May, thereafter by email or
mobile
only.
Dr Volker Springel
Max-Planck Institute for
Astrophysics
Tel: +49 89 30000 2238
Email
vspringel@mpa-graching.mpg.de
Available by telephone until 27th May, thereafter by email only.
The
Particle Physics and Astronomy Research Council (PPARC) is the
UK's strategic
science investment agency. It funds research,
education and public
understanding in four areas of science - particle
physics, astronomy,
cosmology and space science.
PPARC is government funded and provides
research grants and
studentships to scientists in British universities, gives
researchers
access to world-class facilities and funds the UK membership
of
international bodies such as the European Laboratory for
Particle
Physics (CERN), and the European Space Agency. It also contributes
money
for the UK telescopes overseas on La Palma, Hawaii, Australia and
in
Chile, the UK Astronomy Technology Centre at the Royal
Observatory,
Edinburgh and the MERLIN/VLBI National Facility, which includes
the
Lovell Telescope at Jodrell Bank observatory.
PPARC's Public
Understanding of Science and Technology Awards Scheme
funds both small local
projects and national initiatives aimed at
improving public understanding of
its areas of
science.
<Ends>
----------------------------------------------------
Julia
Maddock
Community Press Officer
Particle Physics & Astronomy
Research Council
Polaris House, North Star Avenue, Swindon, Wiltshire, SN2
1SZ, United
Kingdom
Tel +44 (0)1793 442094, Mobile 07901 514975
Fax +44
(0)1793 442002
Email:
julia.maddock@pparc.ac.uk Web:
www.pparc.ac.uk