Stars fueled by the self-annihilation of dark matter might have been spotted for the first time by JWST
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Contrary to their name, dark stars could typically have glowed a billion times more luminously than the sun and grown to a million times its mass. Dark stars have never been definitively observed, but cosmological simulations suggest that they should have formed soon after the big bang from clouds of pure hydrogen and helium that collapsed at the centers of protogalaxies rich in dark matter.
Now researchers report in the Proceedings of the National Academy of Sciences USA that at least three far-off objects observed by the JWST and previously identified as galaxies could, in fact, each be single, supermassive dark stars. “If you find a new kind of star, that’s huge,” says study co-author Katherine Freese, an astrophysicist at the University of Texas at Austin.
The researchers can’t yet prove that the objects are dark stars—only that their characteristics are consistent with being either dark stars or galaxies populated by regular fusion-powered stars. JWST’s technology is sufficient to do that job, however, says study co-author Cosmin Ilie, an astrophysicist at Colgate University. All researchers need is more observation time. “We hope we are going to find one of these dark stars with the Webb within its lifetime,” Ilie says.
There are two possibilities for how the first stars in the universe formed. The conventional wisdom is that these early stars were “Population III” stars. Such stars would have been powered by nuclear fusion, like stars today, but they would have had very little to no metals in them—in astronomy, that means elements heavier than helium—because those elements had not yet formed in the early universe.
There is another possibility, though. In 2008 Freese and some of her colleagues proposed that the universe’s first stars could have been powered by dark matter. Dark matter is a mysterious form of matter that does not interact with electromagnetic forces; scientists only know it exists because of its gravitational effects, and they don’t know what it’s made of.
In the early universe, dark stars could have formed from the collapse of helium and hydrogen clouds made in the big bang. If dark matter particles are also their own antiparticles, as many dark matter theories posit, then within these collapsing clouds, those particles would have collided with each other and self-annihilated. The collision would have kicked off a chain of particle decay that ended with the production of photons, electron-positron pairs and neutrinos. Only the neutrinos would have really left the cloud, because they barely interact with matter. The other particles would have hit the hydrogen and helium and transferred their energy to this matter, which would have heated up the cloud and fueled the star’s formation and continued growth.
These stars would have formed at the center of “minihaloes,” which were early protogalaxies that existed 200 million years after the Big Bang before the advent of elements heavier than helium and hydrogen. These minihaloes consisted almost entirely of dark matter, making conditions ripe to power the dark stars. This high concentration of dark matter is why dark stars could form only in the early universe, Freese says.
Because the stars would have been relatively cool and would not have emitted the high-energy photons that nuclear-fusion-powered stars do, they could have kept adding mass, causing them to swell larger and larger over their lifetimes.
“Now you’ve got a weird thing,” Freese says. “It looks like the sun in terms of its surface temperature, but it’s a billion times as bright. It could be as bright as an entire galaxy of fusion-powered stars.”
At the end of their life spans, large dark stars would have collapsed into massive black holes. This could be a potential explanation for some of the ancient supermassive black holes observed in the universe, which seem too large to have formed so quickly from fusion-powered Population III stars, Ilie says.
To look for dark stars, Freese, Ilie and undergraduate student Jillian Paulin searched the catalogue of objects that the JWST has identified as being from the early universe, or from nearly 14 billion years ago. Only nine of those objects had enough data on their electromagnetic emissions to be useful for study. Of those nine, three were a good match to what a dark star would look like. These objects were high in redshift, meaning they emitted light skewed toward the red side of the electromagnetic spectrum, which is a sign of old and distant objects. They were also possibly from a single point source, such as a star, rather than a fuzzy galaxy, says Paulin, who will start graduate school at the University of Pennsylvania in the fall.
The researchers can’t say much else about the objects right now because they have only limited observations of them. The “smoking gun” for a dark star would be a particular hiccup in the electromagnetic spectrum where light is absorbed by a particular isotope of helium only in dark stars, not in galaxies. Finding that hiccup would take many months of observing these single objects, Ilie says, which is unrealistic given how many researchers are using the JWST to solve an array of astrophysics problems. The team can tell, however, that if the objects are dark stars, two of them would be about a million times the mass of the sun, and one would be about 500,000 times the mass of the sun.
The research team is now developing an automated method to search for more dark star candidates, some of which might require less observation time to confirm. “I’d expect there to be very many more candidates,” Paulin says.
Observing a dark star directly would be “off-the-charts” amazing, says Pearl Sandick, a theoretical particle physicist at the University of Utah who was not involved in the study. There are, however, other ways to look for dark stars, such as via their signatures in the cosmic microwave background—the faint glow of radiation left over from when our universe was hot and young. Finding a dark star would not only provide a new look into the early formation of the universe, Sandick says, but would also be a unique opportunity to directly observe dark matter interactions. “Observing that,” she says, “would really provide new insight about the nature of dark matter as a particle.”
ABOUT THE AUTHOR(S)
Stephanie Pappas is a freelance science journalist. She is based in Denver, Colo.
