After sifting through reams of X-ray data, scientists believe they could have identified the signal of a particle of dark matter.
This substance, which up to now has been purely hypothetical, is run by none of the standard models of physics other than through the gravitational force.
When physicists study the dynamics of galaxies and the movement of stars, they are confronted with a mystery.
If they only take visible matter into account, their equations simply don't add up: the elements that can be observed are not sufficient to explain the rotation of objects and the existing gravitational forces.
Called "dark matter," this substance appears to make up at least 80 per cent of the Universe.
Two groups have recently announced that they have detected the much sought after signal.
One of them, led by Ecole Polytechnique Federale de Lausanne scientists Oleg Ruchayskiy and Alexey Boyarsky, also a professor at Leiden University in the Netherlands, found it by analysing X-rays emitted by two celestial objects - the Perseus galaxy cluster and the Andromeda galaxy.
The signal appears in the X-ray spectrum as a weak, atypical photon emission that could not be attributed to any known form of matter.
"The signal's distribution within the galaxy corresponds exactly to what we were expecting with dark matter, that is, concentrated and intense in the centre of objects and weaker and diffuse on the edges," said Ruchayskiy.
"With the goal of verifying our findings, we then looked at data from our own galaxy, the Milky Way, and made the same observations," said Boyarsky.
If the discovery is confirmed, it will open up new avenues of research in particle physics. Apart from that, "It could usher in a new era in astronomy," said Ruchayskiy.
"Confirmation of this discovery may lead to construction of new telescopes specially designed for studying the signals from dark matter particles," Boyarsky added.
The study appears in the journal Physical Review Letters.
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