First potential signs of “interacting” dark matter suggest it is not completely dark after all
(15 April 2015)
Astronomers believe they might have observed the first potential signs of dark matter interacting with a force other than gravity.
An international team of scientists, led by researchers at Durham University, UK, made the discovery by using the Hubble Space Telescope to view the simultaneous collision of four distant galaxies at the centre of a galaxy cluster 1.3 billion light years away from Earth.
Writing in the journal Monthly Notices of the Royal Astronomical Society today (Wednesday, April 15, 2015), the researchers said one dark matter clump appeared to be lagging behind the galaxy it surrounds.
They said the clump was currently offset from its galaxy by 5,000 light years (50,000 million million km) – a distance it would take NASA’s Voyager spacecraft 90 million years to travel.
Such an offset is predicted during collisions if dark matter interacts, even very slightly, with forces other than gravity. Computer simulations show that the extra friction from the collision would make the dark matter slow down, and eventually lag behind.
Scientists believe that all galaxies exist inside clumps of dark matter – called “dark” because it is thought to interact only with gravity, therefore making it invisible.
Nobody knows what dark matter is, but it is believed to make up about 85 per cent of the Universe’s mass. Without the constraining effect of its extra gravity, galaxies like our Milky Way would fling themselves apart as they spin.
In the latest study, the researchers were able to “see” the dark matter clump because of the distorting effect its mass has on the light from background galaxies - a technique called gravitational lensing.
The researchers added that their finding potentially rules out the standard theory of Cold Dark Matter, where dark matter interacts only with gravity.
Lead author Dr Richard Massey, Royal Society Research Fellow, in Durham University’s Institute for Computational Cosmology, said: “We used to think that dark matter sits around, minding its own business.
“But if it slowed down during this collision, this could be the first dynamical evidence that dark matter notices the world around it.
“Dark matter may not be completely ‘dark’ after all.”
The researchers note that while they appear to have observed the offsetting of dark matter, more investigation will be needed into other potential effects that could also produce a lag between the dark matter and the galaxy it hosts. Similar observations of more galaxies and computer simulations of galaxy collisions are under way to confirm the interpretation.
Team member Professor Liliya Williams of the University of Minnesota said: “Our observation suggests that dark matter might be able to interact with more forces than just gravity.
“The parallel Universe going on around us has just got interesting. The dark sector could contain rich physics and potentially complex behaviour.”
Last month, Dr Massey and colleagues published observations showing that dark matter interacted very little during 72 collisions between galaxy clusters (each containing up to 1,000 galaxies).
Today’s latest research concerns the motion of individual galaxies. Researchers say that the collision between these galaxies could have lasted longer than the collisions observed in the previous study – allowing even a small frictional force to build up over time .
Taken together, the two results bracket the behaviour of dark matter for the first time. Dark matter interacts more than this, but less than that.
Dr Massey, who is also a member of Durham’s Centre for Extragalactic Astronomy, added: “We are finally homing in on dark matter from above and below – squeezing our knowledge from two directions.
“Dark matter, we’re coming for you.”
The research was funded by the Royal Society, the Science and Technology Facilities Council and The Leverhulme Trust.
 The main uncertainty in the result is the timespan for the collision: the friction that slowed the dark matter could have been a very weak force over acting over about a billion years, or a relatively stronger force acting for “only” 100 million years.