Supercomputer predicts disk of 'dark matter' in Milky Way Galaxy
New research raises the exciting prospect that the dark disk — and dark matter — could be directly detected in the very near future.
September 16, 2008
Provided by the Royal Astronomical Society, United Kingdom
September 16, 2008
A composite image of the dark matter disk (red contours) and the Atlas Image mosaic of the Milky Way obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
Photo by J. Read & O. Agertz
An international team of scientists predicts that our galaxy, the Milky Way, contains a disk of 'dark matter.' In a paper published in Monthly Notices of the Royal Astronomical Society, astronomers Dr. Justin Read, Professor George Lake and Oscar Agertz of the University of Zurich, and Dr. Victor Debattista of the University of Central Lancashire use the results of a supercomputer simulation to deduce the presence of this disk. They explain how it could allow physicists to directly detect and identify the nature of dark matter for the first time.
Unlike the familiar 'normal' matter that makes up stars, gas and dust, 'dark' matter is invisible, but its presence can be inferred through its gravitational influence on its surroundings. Physicists believe that it makes up 23 percent of the mass of the universe (compared with the 5 percent of normal matter and 72 percent comprising the mysterious 'dark energy'). But, despite its pervasive influence, no one is sure what dark matter consists of.
Prior to this work, it was thought that dark matter forms in roughly spherical lumps called 'halos', one of which envelopes the Milky Way. But this 'standard' theory is based on supercomputer simulations that model the gravitational influence of the dark matter alone. The new work includes the gravitational influence of the stars and gas that also make up our galaxy.
Stars and gas are thought to have settled into disks very early on in the life of the universe and this affected how smaller dark matter halos formed. The team's results suggest that most lumps of dark matter in our locality merged to form a halo around the Milky Way. The largest lumps were preferentially dragged towards the galactic disk and were then torn apart, creating a disk of dark matter within the galaxy.
"The dark disk only has about half of the density of the dark matter halo, which is why no one has spotted it before," said lead author Justin Read. "However, despite its low density, if the disk exists it has dramatic implications for the detection of dark matter here on Earth."
Earth and the Sun move at some 136.7 miles per second along a nearly circular orbit about the center of our galaxy. Since the dark matter halo does not rotate, from an Earth-based perspective it feels as if we have a 'wind' of dark matter flowing towards us at great speed. By contrast, the 'wind' from the dark disk is much slower than from the halo because the disk co-rotates with Earth.
"It's like sitting in your car on the highway moving at a hundred kilometers an hour," said team member Dr. Victor Debattista. "It feels like all of the other cars are stationary because they are moving at the same speed."
This abundance of low-speed dark matter particles could be a real boon for researchers because they are more likely to excite a response in dark matter detectors than fast-moving particles.
"Current detectors cannot distinguish these slow moving particles from other background 'noise'," said Prof. Laura Baudis, a collaborator at the University of Zurich and one of the lead investigators for the XENON direct detection experiment, which is located at the Gran Sasso Underground Laboratory in Italy. "But the XENON100 detector that we are turning on right now is much more sensitive. For many popular dark matter particle candidates, it will be able to see something if it's there."