A nearby supernova could end the search for dark matter

November 21, 2024

Artist rendering of a black galaxy with stars and one large star, glowing red and black with blue lights shooting off of itThe search for the universe’s dark matter could end tomorrow — given a nearby supernova and a little luck.

The nature of dark matter has eluded astronomers for 90 years, since the realization that 85% of the matter in the universe is not visible through our telescopes. The most likely dark matter candidate today is the axion, a lightweight particle that researchers around the world are desperately trying to find.

Astrophysicists at the University of California, Berkeley, now argue that the axion could be discovered within seconds of the detection of gamma rays from a nearby supernova explosion. Axions, if they exist, would be produced in copious quantities during the first 10 seconds after the core collapse of a massive star into a neutron star, and those axions would escape and be transformed into high-energy gamma rays in the star’s intense magnetic field.

Such a detection is possible today only if the lone gamma-ray telescope in orbit, the Fermi Gamma-ray Space Telescope, is pointing in the direction of the supernova at the time it explodes. Given the telescope’s field of view, that is about one chance in 10.

Yet, a single detection of gamma rays would pinpoint the mass of the axion, in particular the so-called QCD axion, over a huge range of theoretical masses, including mass ranges now being scoured in experiments on Earth. The lack of a detection, however, would eliminate a large range of potential masses for the axion, and make most current dark matter searches irrelevant.

The problem is that, for the gamma rays to be bright enough to detect, the supernova has to be nearby — within our Milky Way galaxy or one of its satellite galaxies — and nearby stars explode only on average every few decades. The last nearby supernova was in 1987 in the Large Magellanic Cloud, one of the Milky Way’s satellites. At the time, a now defunct gamma-ray telescope, the Solar Maximum Mission, was pointing in the supernova’s direction, but it wasn’t sensitive enough to be able to detect the predicted intensity of gamma rays, according to the UC Berkeley team’s analysis.

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