A nearby supernova could end the search for dark matter
Axion dark matter should be produced and converted to gamma rays during a supernova. Will we be lucky enough to see them?
Casey Reed, courtesy of Penn State; reproduction is permitted under a Creative Commons Attribution Non-Commercial 3.0 License
November 21, 2024
The 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.
“If we were to see a supernova, like supernova 1987A, with a modern gamma-ray telescope, we would be able to detect or rule out this QCD axion, this most interesting axion, across much of its parameter space — essentially the entire parameter space that cannot be probed in the laboratory, and much of the parameter space that can be probed in the laboratory, too,” said Benjamin Safdi, a UC Berkeley associate professor of physics and senior author of a paper that was published online Nov. 19 in the journal Physical Review Letters. “And it would all happen within 10 seconds.”
Benjamin Safdi, UC Berkeley
The researchers are anxious, however, that when the long-overdue supernova pops off in the nearby universe, we won’t be ready to see the gamma rays produced by axions. The scientists are now talking with colleagues who build gamma-ray telescopes to judge the feasibility of launching one or a fleet of such telescopes to cover 100% of the sky 24/7 and be assured of catching any gamma-ray burst. They have even proposed a name for their full-sky gamma-ray satellite constellation — the GALactic AXion Instrument for Supernova, or GALAXIS.
“I think all of us on this paper are stressed about there being a next supernova before we have the right instrumentation,” Safdi said. “It would be a real shame if a supernova went off tomorrow and we missed an opportunity to detect the axion — it might not come back for another 50 years.”
Safdi’s co-authors are graduate student Yujin Park and postdoctoral fellows Claudio Andrea Manzari and Inbar Savoray. All four are members of UC Berkeley’s physics department and the Theoretical Physics Group at Lawrence Berkeley National Laboratory.
QCD axions
Searches for dark matter originally focused on faint, massive compact halo objects (MACHOs) theoretically sprinkled throughout our galaxy and the cosmos, but when those didn’t materialize, physicists began to look for elementary particles that theoretically are all around us and should be detectable in Earth-bound labs. These weakly interacting massive particles (WIMPs) also failed to show up. The current best candidate for dark matter is the axion, a particle that fits nicely within the standard model of physics and solves several other outstanding puzzles in particle physics. Axions also fall neatly out of string theory, a hypothesis about the underlying geometry of the universe, and might be able to unify gravity, which explains interactions on cosmic scales, with the theory of quantum mechanics, which describes the infinitesimal.
Courtesy of Benjamin Safdi
“It seems almost impossible to have a consistent theory of gravity combined with quantum mechanics that does not have particles like the axion,” Safdi said.
The strongest candidate for an axion, called a QCD axion — named after the reigning theory of the strong force, quantum chromodynamics — theoretically interacts with all matter, though weakly, through the four forces of nature: gravity, electromagnetism, the strong force, which holds atoms together, and the weak force, which explains the breakup of atoms. One consequence is that, in a strong magnetic field, an axion should occasionally turn into an electromagnetic wave, or photon. The axion is distinctly different from another lightweight, weakly-interacting particle, the neutrino, which only interacts through gravity and the weak force and totally ignores the electromagnetic force.
Lab bench experiments — such as the ALPHA Consortium (Axion Longitudinal Plasma HAloscope), DMradio and ABRACADABRA, all of which involve UC Berkeley researchers — employ compact cavities that, like a tuning fork, resonate with and amplify the faint electromagnetic field or photon produced when a low-mass axion transforms in the presence of a strong magnetic field.
Alternatively, astrophysicists have proposed looking for axions produced inside neutron stars immediately after a core-collapse supernova, like 1987A. Until now, however, they’ve focused primarily on detecting gamma rays from these axions’ slow transformation into photons in the magnetic fields of galaxies. Safdi and his colleagues realized that that process is not very efficient at producing gamma rays, or at least not enough to detect from Earth.
Instead, they explored the production of gamma rays by axions in the strong magnetic fields around the very star that generated the axions. That process, supercomputer simulations showed, very efficiently creates a burst of gamma rays that is dependent on the mass of the axion, and the burst should occur simultaneously with a burst of neutrinos from inside the hot neutron star. That burst of axions, however, lasts a mere 10 seconds after the neutron star forms — after that, the production rate drops dramatically — though hours before the outer layers of the star explode.
“This has really led us to thinking about neutron stars as optimal targets for searching for axions as axion laboratories,” Safdi said. “Neutron stars have a lot of things going for them. They are extremely hot objects. They also host very strong magnetic fields. The strongest magnetic fields in our universe are found around neutron stars, such as magnetars, which have magnetic fields tens of billions of times stronger than anything we can build in the laboratory. That helps convert these axions into observable signals.”
Two years ago, Safdi and his colleagues put the best upper limit on the mass of the QCD axion at about 16 million electron volts, or about 32 times less than the mass of the electron. This was based on the cooling rate of neutron stars, which would cool faster if axions were produced along with neutrinos inside these hot, compact bodies.
In the current paper, the UC Berkeley team not only describes the production of gamma rays following core collapse to a neutron star, but also uses the non-detection of gamma rays from the 1987A supernova to put the best constraints yet on the mass of axion-like particles, which differ from QCD axions in that they do not interact via the strong force.
They predict that a gamma ray detection would allow them to identify the QCD axion mass if it is above 50 microelectron volts (micro-eV, or μeV), or about one 10-billionth the mass of the electron. A single detection could refocus existing experiments to confirm the mass of the axion, Safdi said. While a fleet of dedicated gamma-ray telescopes is the best option for detecting gamma rays from a nearby supernova, a lucky break with Fermi would be even better.
“The best-case scenario for axions is Fermi catches a supernova. It’s just that the chance of that is small,” Safdi said. “But if Fermi saw it, we’d be able to measure its mass. We’d be able to measure its interaction strength. We’d be able to determine everything we need to know about the axion, and we’d be incredibly confident in the signal because there’s no ordinary matter which could create such an event.”
The research was supported by funds from the U.S. Department of Energy.