MOND can explain dark matter ‘clincher’

MOND can explain dark matter ‘clincher’

This week– Dimmer outlook for dark matter MARCUS CHOWN THOUGH we can’t see it, dark matter is supposed to make up 22 per cent of the universe. Now i...

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This week–

Dimmer outlook for dark matter MARCUS CHOWN

THOUGH we can’t see it, dark matter is supposed to make up 22 per cent of the universe. Now it turns out it might not exist at all. Earlier this year, the discovery of a ring-like astronomical feature, invisible except for the way its gravity distorts background galaxies, was hailed as proof for the existence of dark matter and the death knell for a rival theory known as modified Newtonian dynamics (MOND). Not so, claims the father of MOND. “MOND perfectly explains the ring,” says Mordehai Milgrom

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of the Weizmann Institute of Science in Rehovot, Israel. “In fact, it explains it more naturally than dark matter.” The ring-like feature is in a galaxy cluster called CL0024+17. It showed up when a team led by Myungkook James Jee, now at the University of California, Davis, observed the distortion of background galaxies by the cluster’s gravity. This revealed an ill-defined ring with a radius of about 1.2 million light years. Jee’s team interpreted it as a ring of invisible dark matter. According to Jee and his colleagues, CL0024+17 is in fact two

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clusters, one hidden behind the other, and the ring of dark matter was created when the clusters collided sometime in the past. Think of the dark matter ring as like a smoke ring that formed at the collision point and grew outwards. Our view today is just a snapshot of this still-expanding ring. This doesn’t convince Milgrom and his colleague Bob Sanders of the Kapteyn Institute at the University of Groningen in the Netherlands. They now say that MOND provides a simpler explanation of the ring, which does not require any collision. “It’s a natural feature of MONDian gravity,” Milgrom says. In MOND, gravity changes from a form which weakens in the way Newton predicted to a stronger form that weakens more slowly. “In the transition region, gravity will shift to being stronger than Newtonian,” says Milgrom.

“Stronger gravity will bend the light of background galaxies more markedly, which is exactly the effect that led to the discovery of the ring.” Jee’s team dismissed the MOND explanation because they thought it predicts that there should be no enhanced gravity without visible matter to do the enhancing. “This

“MOND explains things naturally whereas dark matter proponents have to propose the existence of cold molecular gas” is a common misconception,” says Milgrom. “In fact, in MOND there does not necessarily have to be visible matter there to boost gravity – it is naturally boosted in the transition region.” No one knows what physics may underpin such a transition. “I am interested to hear that the

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transition between the Newtonian and MONDian regime also gives rise to a ring,” says Jee. “In general, I am happy whenever there comes a theory which is simpler but can explain more observations.” According to Milgrom, MOND predicts the rough location of the ring in CL0024+17, which dark matter does not. It also predicts that such rings will be observed in other galaxy clusters and in spiral galaxies (www.arxiv.org/ abs/0709.2561). The crucial requirement is that a cluster be compact enough for the transition to MOND to occur outside where most of the cluster mass is concentrated, so its effect is clearly visible. This is the case in CL0024+17. “If such rings are found in all compact clusters it will strengthen the case for MOND, since the dark matter explanation requires –What holds it together?– collisions, which are relatively

rare,” Milgrom says. Milgrom and Sanders claim that the MOND transition will also be visible in compact single galaxies known as “high surface brightness galaxies”. They say there is tentative evidence of the transition in two such galaxies: UGC 3456 and UGC 11670. Stronger evidence may be found in three dwarf galaxies which were formed in galactic collisions near the galaxy NGC 5291, discovered this year by a team led by Frederic Bournaud of the French Atomic Energy Commission in Paris. “The collision should have stripped the galaxies of all their dark matter yet they still have enhanced gravity,” says Milgrom. “MOND explains things naturally whereas dark matter proponents have to propose the existence of yet another type of dark matter – cold molecular gas.” ●

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