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Darkish matter doesn’t defy gravity, examine suggests

November 3, 2025
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Darkish matter doesn’t defy gravity, examine suggests
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Dark matter does not defy gravity
Map of the distribution of galaxies noticed by the DESI collaboration, from which it’s attainable to precisely measure the velocities of galaxies. Credit score: Claire Lamman/DESI collaboration; customized colormap bundle by cmastro.

Does darkish matter observe the identical legal guidelines as odd matter? The thriller of this invisible and hypothetical part of our universe—which neither emits nor displays mild—stays unsolved. A staff involving members from the College of Geneva (UNIGE) got down to decide whether or not, on a cosmological scale, this matter behaves like odd matter or whether or not different forces come into play.

Their findings, published in Nature Communications, recommend the same habits, whereas leaving open the opportunity of an as-yet-unknown interplay. This breakthrough sheds just a little extra mild on the properties of this elusive matter, which is 5 instances extra ample than odd matter.

Odd matter obeys 4 well-identified forces: gravity, electromagnetism, and the sturdy and weak forces on the atomic stage. However what about darkish matter? Invisible and elusive, it could possibly be topic to the identical legal guidelines or ruled by a fifth, as but unknown pressure.

To unravel this thriller, a staff led by UNIGE got down to decide whether or not, on a cosmic scale, darkish matter falls into gravitational wells in the identical manner as odd matter. Below the affect of huge celestial our bodies, the house occupied by our universe is distorted, creating wells. Odd matter—planets, stars and galaxies—falls into these wells based on well-established bodily legal guidelines, together with Einstein’s idea of basic relativity and Euler’s equations. However what about darkish matter?

“To reply this query, we in contrast the velocities of galaxies throughout the universe with the depth of gravitational wells,” explains Camille Bonvin, affiliate professor within the Division of Theoretical Physics at UNIGE’s College of Science and co-author of the examine.

“If darkish matter will not be topic to a fifth pressure, then galaxies—that are principally product of darkish matter—will fall into these wells like odd matter, ruled solely by gravity. However, if a fifth pressure acts on darkish matter, it would affect the movement of galaxies, which might then fall into the wells otherwise. By evaluating the depth of the wells with the galaxies’ velocities, we are able to due to this fact check for the presence of such a pressure.”

Euler’s equations nonetheless legitimate

Making use of this method to present cosmological information, the analysis staff concluded that darkish matter falls into gravitational wells in the identical manner as odd matter, thus obeying Euler’s equations.

“At this stage, nevertheless, these conclusions don’t but rule out the presence of an unknown pressure. But when such a fifth pressure exists, it can’t exceed 7% of the energy of gravity—in any other case it might have already got appeared in our analyses,” says Nastassia Grimm, first writer of the examine and former postdoctoral researcher on the Division of Theoretical Physics at UNIGE’s College of Science who has just lately joined the Institute of Cosmology and Gravitation on the College of Portsmouth.

These preliminary outcomes mark a significant step ahead in characterizing darkish matter. The following problem will probably be to find out whether or not a fifth pressure governs it.

“Upcoming information from the latest experiments, equivalent to LSST and DESI, will probably be delicate to forces as weak as 2% of gravity. They need to due to this fact permit us to be taught much more concerning the habits of darkish matter,” concludes Isaac Tutusaus, researcher at ICE-CSIC and IEEC and affiliate professor at IRAP, Midi-Pyrénées observatory, College of Toulouse, co-author of the examine.

Extra data:
Nastassia Grimm et al, Evaluating the movement of darkish matter and customary mannequin particles on cosmological scales, Nature Communications (2025). DOI: 10.1038/s41467-025-65100-8

Supplied by
College of Geneva


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