ESA Science & Technology - Puzzling X-rays point to dark matter

Perseus galaxy cluster. Credit: Chandra: NASA/CXC/SAO/E.Bulbul, et al.; XMM-Newton: ESA)

Although thought to be invisible, neither emitting nor absorbing light, dark matter can be detected through its gravitational influence on the movements and appearance of other objects in the Universe, such as stars or galaxies.

Based on this indirect evidence, astronomers believe that dark matter is the dominant type of matter in the Universe – yet it remains obscure.

Now a hint may have been found by studying galaxy clusters, the largest cosmic assemblies of matter bound together by gravity.

Galaxy clusters not only contain hundreds of galaxies, but also a huge amount of hot gas filling the space between them.

However, measuring the gravitational influence of such clusters shows that the galaxies and gas make up only about a fifth of the total mass – the rest is thought to be dark matter.

The gas is mainly hydrogen and, at over 10 million degrees celsius, is hot enough to emit X-rays. Traces of other elements contribute additional X-ray 'lines' at specific wavelengths.

Mysterious signal in the Perseus galaxy cluster. Credit: NASA/CXC/SAO/E.Bulbul, et al.

Examining observations by ESA's XMM-Newton and NASA's Chandra spaceborne telescopes of these characteristic lines in 73 galaxy clusters, astronomers stumbled on an intriguing faint line at a wavelength where none had been seen before.

"If this strange signal had been caused by a known element present in the gas, it should have left other signals in the X-ray light at other well-known wavelengths, but none of these were recorded," says Dr Esra Bulbul from the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, USA, lead author of the paper discussing the results.

"So we had to look for an explanation beyond the realm of known, ordinary matter."

The astronomers suggest that the emission may be created by the decay of an exotic type of subatomic particle known as a 'sterile neutrino', which is predicted but not yet detected.

Ordinary neutrinos are very low-mass particles that interact only rarely with matter via the so-called weak nuclear force as well as via gravity. Sterile neutrinos are thought to interact with ordinary matter through gravity alone, making them a possible candidate as dark matter.

"If the interpretation of our new observations is correct, at least part of the dark matter in galaxy clusters could consist of sterile neutrinos," says Dr Bulbul.

The surveyed galaxy clusters lie at a wide range of distances, from more than a hundred million light-years to a few billion light-years away. The mysterious, faint signal was found by combining multiple observations of the clusters, as well as in an individual image of the Perseus cluster, a massive structure in our cosmic neighbourhood.

The implications of this discovery may be far-reaching, but the researchers are being cautious. Further observations with XMM-Newton, Chandra and other high-energy telescopes of more clusters are needed before the connection to dark matter can be confirmed.

"The discovery of these curious X-rays was possible thanks to the large XMM-Newton archive, and to the observatory's ability to collect lots of X-rays at different wavelengths, leading to this previously undiscovered line," comments Norbert Schartel, ESA's XMM-Newton Project Scientist.

"It would be extremely exciting to confirm that XMM-Newton helped us find the first direct sign of dark matter.

"We aren't quite there yet, but we're certainly going to learn a lot about the content of our bizarre Universe while getting there."

More information

"Detection of an unidentified emission line in the stacked X-ray spectrum of galaxy clusters," by E. Bulbul et al. is published in the 1 July 2014 issue of the Astrophysical Journal.

For further information, please contact

Markus Bauer
ESA Science and Robotic Exploration Communication Officer
Tel: +31 71 565 6799
Mob: +31 61 594 3 954
Email: markus.baueresa.int

Esra Bulbul
Harvard-Smithsonian Center for Astrophysics
Cambridge, MA, USA
Phone: +1-617-496-7565
Email: ebulbulcfa.harvard.edu

Norbert Schartel
XMM-Newton Project Scientist
Tel: +34 91 8131 184
Email: Norbert.Schartelsciops.esa.int

(This article was originally published on ESA's Space Science Portal)